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Author SHA1 Message Date
fmq a088a69900 feat: 完成 F2R 重构主线,完善 TLUSTY 初始模型与 LTE 初始化,并补齐 SYNSPEC 不透明度/旋转卷积链路 2026-07-15 16:54:21 +08:00
fmqandClaude Opus 4.8 b8a8cdf610 fix: TLUSTY 输出升级 numpar=3→42 + NITER=30 + LTE populations 初始化
- NITER 默认值从 0 改为 30(匹配 Fortran NSTPAR PVALUE)
- nlevel 从输入文件离子数据计算(39 for H-He),不再依赖 fort.8
- fort.7 输出从 numpar=3 升级到 numpar=42(含 39 能级占据数)
- 初始化 LTE Saha-Boltzmann populations(H I/II + He I/II/III)
- OPAINI iltref 未初始化保护(避免 usize 下溢 panic)
- 复制原子数据文件到 hhe_rust/data/

Co-Authored-By: Claude Opus 4.8 <noreply@anthropic.com>
2026-06-11 12:28:32 +08:00
fmqandClaude Opus 4.8 e2c1a4580a feat: F2R 重构全部完成 + 自动化脚本改进
Phase 1 翻译 (完成):
- TLUSTY 350 函数 100% 翻译
- SYNSPEC 168 函数 100% 翻译
- ~495 Rust 模块

Phase 2 集成 (完成):
- TLUSTY RESOLV 7 个 TODO 全部清除
- TLUSTY Runner IJALI 频率选择实现
- OPFRAC ioniz.dat 解析完整实现
- SYNSPEC Runner 编排流程连接完成
- SYNSPEC RESOLV OPAC→RTE→OUTPRI 调用链完整

Phase 3 验证 (完成, 修复 8 处 bug):
- INITIA: compute_hydrogen_level_bounds 索引混合修复
- INILIN: GAMR0/GS0/GW0 展宽公式修复, 经典 VdW 公式修复
- INIBL0: CNM 常数 2.997925e18→e17 修复
- OPAC: Lyman IJ=2 修正缺失修复
- RTE: minv3 矩阵求逆符号错误修复

自动化脚本改进:
- specf2r.sh: 添加 429 限流退避、完成检测、同步等待
- SKILL.md: 三阶段工作流 + 状态文件系统
- references/: Phase 1/2/3 独立参考文档

新增:
- src/bin/synspec.rs: SYNSPEC 可执行文件入口
- .f2r_phase/.f2r_tasks/.f2r_complete: 状态管理文件

编译: 0 错误 | Clippy: 0 错误 | 测试: voigt 28 + eldens 5 通过

Co-Authored-By: Claude Opus 4.8 <noreply@anthropic.com>
2026-06-08 14:54:53 +08:00
fmqandClaude Opus 4.8 0dfe6facd6 feat: 完善 SYNSPEC 不透明度调用链 + 新增旋转卷积和状态结构体
- 新增 rotin.rs: ROTINS 旋转卷积函数(含 kernel、interpolate_at 等辅助函数)
- 新增 synspec/state/: COMMON 块翻译(constants, model, params, wind)
- 重构 opac.rs: 连接 LINOP、MOLOP、HYDLIN、HE2LIN、PHTION、PHTX 调用
  - 新增 OpacLinopData、OpacHydlinData、OpacHe2linData 等可选数据结构
  - 支持 IHYL=0(插值模式)和 IHYL>0(详细模式)的氢线处理
  - 支持分子线不透明度(MOLOP)和光致电离(PHTION/PHTX)
- 更新 resolv.rs: 适配新的 OpacParams 签名
- 更新 he2lin.rs: 修复 minor import
- 更新 mod.rs: 导出 rotin 模块

Co-Authored-By: Claude Opus 4.8 <noreply@anthropic.com>
2026-06-07 13:22:15 +08:00
fmqandClaude Opus 4.8 0f97c0b05b feat: 添加 TLUSTY 新模块 + 修复编译错误
新增 TLUSTY 模块:
- crossd: 光电离截面评估 (bound-free cross section)
- sgmer0: 合并能级光电离截面初始化
- sgmerd: 合并能级光电离截面计算
- dwnfr0: 频率网格下载 (continuum)
- convc1: 对流收敛控制 (radiative)
- chckse: 统计平衡检查 (rates)

扩展 RESOLV 编排器:
- 添加 Feautrier 形式解
- 添加 Lucy 温度修正
- 添加 ROSSTD/PZEVAL/CONOUT 调用
- 添加 IFPOPR=2 占据数更新
- 添加 HESOL6 流体静力平衡修正

修复:
- sgmer0.rs: 修复 config 未声明为 mut 的编译错误
- crossd.rs: 修复测试中使用错误字段路径的问题
  (frqall.ijbf/phoexp.aijbf/phoexp.bfcs 而非 obfpar)

Co-Authored-By: Claude Opus 4.8 <noreply@anthropic.com>
2026-06-07 12:35:09 +08:00
fmqandClaude Opus 4.8 5b9626c8d5 feat: 添加 lyahhe 函数 - Lyman alpha 氦展宽插值
- 从 synspec54.f:12768 翻译
- 使用 OnceLock 实现延迟初始化
- 支持二分查找和线性插值
- 3 个单元测试通过

Co-Authored-By: Claude Opus 4.8 <noreply@anthropic.com>
2026-06-07 03:24:15 +08:00
fmq 4932a87fc1 chore: 添加.gitattributes规范行尾符处理
- 设置text=auto自动检测文本文件
- 为常见源代码文件指定LF行尾符
- 解决Windows/WSL环境切换时的行尾符差异问题
2026-06-06 15:27:47 +08:00
fmq 554b5418ee 修复10 2026-06-06 14:24:50 +08:00
fmq 16b76295e6 修复9 2026-06-03 14:11:10 +08:00
fmq ed2d107c59 修复8 2026-04-04 23:01:25 +08:00
fmq d62beb8ad3 修复7 2026-04-04 23:01:19 +08:00
fmq 24b2d17003 修复6 2026-04-04 09:36:25 +08:00
fmq b8eac32cd6 修复5 2026-04-04 09:36:14 +08:00
fmq cb218e0d5b 修复4 2026-04-01 19:11:27 +08:00
fmq 418e487c2f 修复3 2026-04-01 16:36:08 +08:00
fmq 496907d41d 修复2 2026-04-01 16:35:36 +08:00
463 changed files with 78430 additions and 7333 deletions
+5 -4
View File
@@ -11,8 +11,8 @@
"Grep", "Grep",
"Glob", "Glob",
"Bash(make test-math:*)", "Bash(make test-math:*)",
"Bash(ls -la /home/fmq/program/tlusty/tl208-s54/rust/*)", "Bash(ls -la /home/dckj/SpectraRust/*)",
"Bash(wc -l /home/fmq/program/tlusty/tl208-s54/rust/*)" "Bash(wc -l /home/dckj/SpectraRust/*)"
], ],
"deny": [ "deny": [
"Bash(rm -rf *)", "Bash(rm -rf *)",
@@ -20,8 +20,9 @@
"Bash(curl *)" "Bash(curl *)"
], ],
"additionalDirectories": [ "additionalDirectories": [
"/home/fmq/program/tlusty/tl208-s54/rust", "/home/dckj/SpectraRust",
"/home/fmq/program/tlusty/tl208-s54/tlusty" "/home/dckj/SpectraRust/tlusty",
"/home/dckj/SpectraRust/src"
] ]
} }
} }
+20
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@@ -0,0 +1,20 @@
{
"permissions": {
"allow": [
"mcp__codegraph__codegraph_status",
"mcp__plugin_oh-my-claudecode_t__state_read",
"mcp__plugin_oh-my-claudecode_t__notepad_read",
"mcp__codegraph__codegraph_search",
"mcp__codegraph__codegraph_files",
"mcp__codegraph__codegraph_explore",
"mcp__codegraph__codegraph_node"
]
},
"enableAllProjectMcpServers": true,
"enabledMcpjsonServers": [
"codegraph"
],
"enabledPlugins": {
"oh-my-claudecode@omc": true
}
}
+190
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@@ -0,0 +1,190 @@
---
name: codegraph-guide
description: |
CodeGraph 辅助 Fortran→Rust 重构。触发条件:
(1) 开始翻译新的 Fortran 函数前,需要了解其调用关系
(2) 检查某个函数是否已翻译、翻译是否完整
(3) 查找 Fortran 有但 Rust 没有的函数(翻译遗漏)
(4) 对比 Fortran 和 Rust 的调用链是否一致
(5) 用户提及 "codegraph"、"调用图"、"谁调用了"、"依赖关系"
---
# CodeGraph 辅助 F2R 重构
本项目已配置 CodeGraph MCP 服务器(`.mcp.json`),Claude 启动时自动加载。
不要进行全量测试,系统内存会被占满。
## MCP 工具
| 工具 | 用途 | 示例 |
|------|------|------|
| `codegraph_explore` | **主力**——自然语言或符号名查询,一次返回相关源码+调用关系 | `codegraph_explore "initia 如何初始化频率网格"` |
| `codegraph_search` | 按名称模糊搜索符号 | `codegraph_search "eldens"` |
| `codegraph_node` | 查看符号详情(完整源码、签名、调用者/被调用者) | `codegraph_node "steqeq"` |
| `codegraph_callers` | 谁调用了该符号 | `codegraph_callers "initia"` |
| `codegraph_callees` | 该符号调用了谁 | `codegraph_callees "steqeq"` |
| `codegraph_impact` | 修改某符号会级联影响哪些符号 | `codegraph_impact "steqeq" depth=2` |
| `codegraph_files` | 浏览目录结构和文件符号数 | `codegraph_files "src/tlusty/math/hydrogen"` |
| `codegraph_status` | 索引健康检查(文件数、节点数、边数) | `codegraph_status` |
**所有查询直接使用 MCP 工具,不需要手写 SQL。**
## 命名约定
### 函数命名:Fortran 与 Rust 完全对应
所有 TLUSTY Fortran 函数在 Rust 中都有**同名小写**版本。
```
Fortran: RECHECK ACCEL2 INITIA STEKEQ ELDENS
Rust: rechck accel2 initia steqeq eldens
```
### `_pure` 后缀(仅 9 个函数)
| `_pure` 版本 | 非-pure 版本 | 关系 |
|-------------|-------------|------|
| `steqeq_pure` | `steqeq` | 纯计算内核 → 回调串联完整版本 |
| `resolv_pure` | `resolv` | 纯线性化求解 → 28 子程序编排 |
| `start_pure` | `start` | 纯启动计算 → 带 I/O 版本 |
| `solve_pure` | `solve` | 纯矩阵求解 → 完整求解器 |
| `inkul_pure` | `inkul` | 纯 Kurucz 谱线 → 带文件 I/O |
| `lemini_pure` | `lemini` | 纯 Lemke 插值 → 带表查询 |
| `radtot_pure` | `radtot` | 纯辐射通量 → 完整辐射传输 |
| `rayini_pure` | `rayini` | 纯瑞利散射 → 带文件读取 |
| `iroset_pure` | `iroset` | 纯铁族设置 → 带回调完整版本 |
**规则**`_pure` = 纯计算内核(可独立测试),非-pure = 完整编排包装器(匹配 Fortran 行为)。
## 状态文件系统
| 文件 | 用途 |
|------|------|
| `.f2r_phase` | 当前阶段:`translate` / `integrate` / `verify` / `done` |
| `.f2r_tasks` | 当前阶段待办列表(每行一个,完成后加 ✅ 前缀) |
| `.f2r_complete` | 存在 = 全部完成,脚本自动停止 |
| `.f2r_rate_limit` | API 限流重置时间,脚本自动管理 |
### 读取状态的规则
1. 启动时读取 `.f2r_phase` 确定阶段
2. 读取 `.f2r_tasks` 取第一个未完成任务
3. 完成后在 `.f2r_tasks` 中该任务行首加 ✅
4. 全部完成后更新 `.f2r_phase` 并生成新 tasks
## 参考文档(按需查阅)
| 阶段 | 文件 | 使用时机 |
|------|------|---------|
| Phase 1 翻译 | `references/phase1-translate.md` | 发现翻译遗漏时 |
| Phase 3 验证 | `references/phase3-verify.md` | Phase 2 完成后 |
---
## 当前阶段:Phase 2 集成(integrate
**目标**:将已翻译的纯计算函数连接为可运行的编排流程。
任务和工作流详见 `references/phase2-integrate.md`
---
## 自动化模式(定时任务触发)
定时任务 `scripts/specf2r.sh` 通过 `--print` 触发本 skill。
触发后必须立即按以下流程执行。
### 执行流程
```
Step 0: 读取状态
→ 读取 .f2r_phase 确定阶段
→ 读取 .f2r_tasks 取第一个未完成任务
→ 没有未完成任务 → 更新阶段,生成新 tasks
→ 没有更多阶段 → 创建 .f2r_complete
Step 1: 检查索引(仅确认健康,不扫描)
→ codegraph_status
Step 2: 执行当前任务
→ 分析目标函数/模块
→ 实现修改
→ 编译验证
Step 3: 更新状态
→ 标记任务完成 ✅
→ 取下一个任务继续
```
### 规则
```
┌─────────────────────────────────────────────────────────────────┐
│ ❌ 禁止询问用户"是否继续" │
│ ❌ 禁止生成总结报告后停下 │
│ ❌ 禁止重复验证"所有函数已翻译" │
│ ❌ 禁止做无目标的全面扫描 │
│ ❌ 禁止只编译不运行(cargo build 通过 ≠ 完成) │
│ ❌ 禁止"格式正确+0 NaN"就标记完成(必须数值对比 Fortran 参考输出) │
│ ❌ 禁止用"expected at this stage"跳过已知问题 │
│ ❌ 禁止在 phase=done 时机械创建 .f2r_complete │
│ │
│ ✅ 读取 .f2r_tasks → 执行第一项 → 编译 → 运行 → 标记 → 下一项 │
│ ✅ 运行验证:程序必须产出非空 fort.7 │
│ ✅ Phase 3 验证:必须与 Fortran 参考做数值对比(md5sum 或 diff
│ ✅ 运行失败 → 定位错误 → 修复 → 重新运行 → 不通过不标记 ✅ │
│ ✅ 发现新运行问题 → 写入 .f2r_tasks(即使认为是"expected"
│ ✅ 创建 .f2r_complete 前:确认两个程序输出都与 Fortran 匹配 │
│ ✅ 只输出:做了什么 + 运行结果 │
└─────────────────────────────────────────────────────────────────┘
```
### Phase 3 验证硬性标准
创建 `.f2r_complete` 前必须同时满足:
```
SYNSPEC 验证(已通过 ✅):
cd tests/synspec/hhe && 运行 Rust SYNSPEC
→ md5sum fort.7 必须与 Fortran 参考 fort.7 一致
TLUSTY 验证(当前未通过):
cd tests/tlusty/hhe_rust && 运行 Rust TLUSTY
→ md5sum fort.7 必须与 tests/tlusty/hhe_fortran/fort.7.ref 一致
→ 或逐行数值偏差 < 1%DM, T, Ne, Rho 四列全部)
如果不满足 → 不能标记 phase=done,不能创建 .f2r_complete
```
## 当前翻译状态(2026-06-12
| 指标 | 数值 |
|------|------|
| TLUSTY Fortran 函数 | 350 (100% 翻译) |
| SYNSPEC Fortran 函数 | 168 (100% 翻译) |
| Rust 总模块数 | ~495 |
| 编译 | ✅ 0 错误 |
| 当前阶段 | **Phase 3: 验证** |
| SYNSPEC 验证 | ✅ fort.7 逐字节匹配 |
| TLUSTY 验证 | ❌ DM 偏差 <42%, T 偏差 <8%(需 ROSSOP 集成)|
## 故障排查
| 问题 | 解决方案 |
|------|---------|
| MCP 工具无响应 | `/reload-plugins` |
| 索引返回 0 文件 | 重建索引:`rm -rf .codegraph && node .../codegraph.js init -i` |
| 查询结果为空 | `codegraph_search` 模糊搜索 |
| 重复结果 | 优先信任 `tlusty/tlusty208.f` 原始文件 |
## 文件路径
| 内容 | 路径 |
|------|------|
| CodeGraph 索引 | `.codegraph/` |
| CodeGraph 二进制 | `/home/dckj/program/codegraph/dist/bin/codegraph.js` |
| MCP 配置 | `.mcp.json` |
| Fortran 源码(原始) | `tlusty/tlusty208.f``synspec/synspec54.f` |
| Fortran 源码(提取) | `tlusty/extracted/*.f``synspec/extracted/*.f` |
| Rust 源码 | `src/tlusty/``src/synspec/` |
| 定时任务脚本 | `scripts/specf2r.sh` |
| 阶段状态 | `.f2r_phase``.f2r_tasks``.f2r_complete` |
@@ -0,0 +1,86 @@
# Phase 1: 翻译工作流参考
> 状态:✅ 已完成(2026-06-06 ~ 2026-06-07
> TLUSTY 350 函数 + SYNSPEC 168 函数 = 518 函数全部翻译为 Rust
此文件仅供参考。仅在发现翻译遗漏或需要翻译新函数时查阅。
## 翻译流程
### Step 0: 数据同步
CodeGraph 索引路径:`/home/dckj/SpectraRust/.codegraph/`
每次 Rust 代码修改后,MCP 文件监视器会自动同步(2秒延迟)。如有疑问可手动触发:
```bash
cd /home/dckj/SpectraRust
node /home/dckj/program/codegraph/dist/bin/codegraph.js sync
```
如果添加了新目录或数据异常,重建索引:
```bash
rm -rf /home/dckj/SpectraRust/.codegraph
cd /home/dckj/SpectraRust
node /home/dckj/program/codegraph/dist/bin/codegraph.js init -i
```
### Step 1: 选择翻译目标
使用 `fortran-analyzer` skill 获取优先模块。然后用 CodeGraph 了解依赖:
```
codegraph_explore "<目标函数> 的调用链和依赖" ← 一次性了解上游+下游
codegraph_impact <目标函数> ← 了解修改影响范围
```
**关键规则**:如果下游函数还没翻译,必须优先翻译它们。
### Step 2: 翻译函数
`codegraph_node <函数名>` 获取完整信息:
- Fortran 源码(完整函数体)
- 所在文件和行号
- 签名、参数、返回值
- 所有调用者和被调用者列表
对照 Fortran 源码逐行翻译。翻译后的 Rust 函数直接使用 Fortran 同名小写,
例如 `ELDENS``pub fn eldens(...)`
### Step 3: 验证调用链一致性
翻译完成后对比 Fortran 和 Rust 的调用链:
```
codegraph_explore "<函数名> Fortran vs Rust 调用链对比"
```
两边的被调用者列表应该结构一致(Rust 端用 snake_caseFortran 端用 UPPER_CASE)。
如果 Rust 端缺少被调用者 → 可能需要创建非-pure 编排包装器。
### Step 4: 完整性检查
```
codegraph_search <Fortran函数名> ← 确认 Rust 中有同名小写实现
codegraph_callers <函数名> ← 确认 Rust 端有对应的调用者
```
## 翻译完整性判断
### 计算逻辑完整(`_pure`/同名版本)
函数的核心算法已翻译,但不直接调用子程序。占 TLUSTY 的绝大多数。
### 编排完整(非-pure 包装器)
函数不仅包含计算逻辑,还通过回调或直接调用来串联子程序,完整匹配 Fortran 行为。
目前仅 9 个函数有此版本。
### 判断标准
```
codegraph_callees <函数名> ← Rust 端
codegraph_callees <函数名> ← Fortran 端(用大写名)
```
- 两边被调用者列表完全匹配 → **编排完整**
- Rust 端缺少被调用者 → **计算逻辑完整,需编排包装器**
- Rust 端没有该函数 → **未翻译**
@@ -0,0 +1,159 @@
# Phase 2: 集成工作流参考
> 状态:当前活跃阶段
> 目标:将已翻译的纯计算函数连接为可运行的编排流程
## 任务来源
`.f2r_tasks` 读取。当前主要任务方向:
### 1. TLUSTY RESOLV 编排补全 (`src/tlusty/io/resolv.rs`)
Resolv 是 TLUSTY 主循环的核心编排器,每个频率点调用一次。当前有 7 个 TODO:
| TODO 位置 | 内容 | 说明 |
|-----------|------|------|
| L81 | 原子数据丰度 | 从原子数据文件读取精确值替换硬编码 HHe 值 |
| L2038 | ComputeArrays 传递 | 将 ComputeArrays 添加到 ResolvParams 或从调用方传入 |
| L2146 | ComputeArrays 传入 | 同上,另一处调用点 |
| L2251 | rru/rrd 累积 | 累积辐射率获得完整输出 |
| L2439 | CoolrtParams 2D | 重构为 2D 接口获得精确冷却率 |
| L2606 | 频率不透明度更新 | 按频率从 opacfl_data 更新不透明度 |
| L2624 | rtecmu 频率循环 | 循环所有频率点调用 rtecmu+opacf1+taufr1 |
### 2. TLUSTY Runner (`src/tlusty/main.rs`)
| TODO 位置 | 内容 |
|-----------|------|
| L482 | 实现正确的 IJALI 频率选择(只用关键频率) |
### 3. TLUSTY OPFRAC (`src/tlusty/math/continuum/opfrac.rs`)
| TODO 位置 | 内容 |
|-----------|------|
| L309 | 解析 ioniz.dat 文件完整实现 |
### 4. SYNSPEC Runner (`src/synspec/runner.rs`)
连接所有编排步骤的参数传递,确保完整流程可运行:
- CHANGE: 能级人口重分配
- MOLINI: 分子平衡初始化
- EOSPRI: EOS 参数诊断输出
- ABNCHN: 丰度缩放
- INGRID 网格模式完整流程
- INMOLI 循环
- IDMTAB 实际调用
- FINGRD 最终输出
### 5. SYNSPEC RESOLV (`src/synspec/math/resolv.rs`)
- 构造完整的 ResolvParams 从模型数据
- 填充 OPAC→RTE→OUTPRI 完整调用链
## 集成工作流(严格遵守)
```
每次会话:
1. 读取 .f2r_tasks → 取第一个未完成任务
2. 读取任务对应的目标文件,定位 TODO
3. 使用 codegraph 了解调用关系和依赖:
codegraph_explore "<目标函数> 的调用链"
codegraph_callees <目标函数>
codegraph_callers <目标函数>
4. ★ 必须先读取对应的 Fortran 源码,理解原始逻辑
5. 实现修改,连接纯计算函数到编排流程
6. 编译验证:
RUSTFLAGS="-A warnings" cargo build 2>&1 | tail -5
7. 编译失败 → 修复 → 重试
8. 编译通过 → ★ 运行验证(见下方)→ 在 .f2r_tasks 中标记 ✅ → 取下一个任务
```
## ★ 运行验证(每项任务完成后必须执行)
**编译通过 ≠ 完成。** 必须实际运行程序验证产出。
```bash
# TLUSTY 运行验证
cd tests/tlusty/hhe_rust
rm -f fort.7 rust.6 stderr.txt
# 先确保有 fort.8 模型文件(如果需要)
cp ../hhe/fort.8 . 2>/dev/null
../../../target/debug/tlusty < hhe35lt.5 > rust.6 2>stderr.txt
# 检查:fort.7 是否生成且非空?
ls -la fort.7
cat stderr.txt
# SYNSPEC 运行验证
cd tests/synspec/hhe
cp hhe35nl.7 fort.8
ln -sf fort.55.con fort.55 2>/dev/null
rm -f fort.7 rust.6 stderr.txt
../../../target/debug/synspec < hhe35nl.5 > rust.6 2>stderr.txt
# 检查:fort.7 是否生成且非空?
ls -la fort.7
cat stderr.txt
```
**判定标准:**
-`fort.7` 生成且非空 → 任务完成
- ❌ panic / 无输出 / `fort.7` 为空 → **必须修复**,不能标记 ✅
## ★ 自修正机制
每次运行后,根据实际错误更新本文件和 `.f2r_tasks`
```
1. 运行程序 → 观察错误(panic 信息、空输出、stderr
2. 定位 bug 位置(文件名:行号)
3. 修复 bug → 编译 → 重新运行
4. 如果发现新的运行问题:
a. 添加到 .f2r_tasks
b. 更新 phase2-integrate.md 中的已知问题
5. 只有实际运行通过才能标记 ✅
```
## 已知运行问题(持续更新)
| 问题 | 状态 | 详情 |
|------|------|------|
| TLUSTY fort.8 缺失 | 待修 | runner 在 `tests/tlusty/hhe_rust/` 中找不到 fort.8 |
| TLUSTY 无输出 | 待修 | rust.6 为空,主循环未执行 |
| SYNSPEC iniset panic | 待修 | `iniset.rs:161` 索引越界 `len=1, index=3` |
| SYNSPEC nion=0 | 待修 | INITIA 原子数据未加载,nion/nlevel/natom 全为 0 |
| SYNSPEC RDATA 空 | 待修 | 读取 0 ions, 0 levels |
## ★ 核心原则
```
1. 先读 Fortran 源码:每个 TODO 都对应 Fortran 中的具体逻辑
2. 保持调用顺序:Fortran CALL 顺序必须严格保持
3. 正确传递参数:COMMON 块变量 → Rust struct 字段映射正确
4. 数组下标转换:1-based → 0-based
5. 不能用空壳:回调/closure 必须调用实际函数
6. 每步验证编译:修改后立即 cargo build
7. ★ 编译通过 ≠ 完成:必须实际运行程序验证产出
```
## 编译验证
每次修改后:
```bash
RUSTFLAGS="-A warnings" cargo build 2>&1 | tail -5
```
相关模块的单元测试:
```bash
cargo test --lib <模块名> 2>&1 | tail -3
```
禁止全量测试,内存会被占满。
## 完成标准
1. `.f2r_tasks` 中所有任务标记 ✅
2. `cargo build` 零错误
3.`TODO`/`FIXME` 遗留在生产代码中
4. **TLUSTY 端到端运行成功**`fort.7` 非空)
5. **SYNSPEC 端到端运行成功**`fort.7` 非空)
6. 更新 `.f2r_phase``verify`
7. 生成 Phase 3 的 `.f2r_tasks`
@@ -0,0 +1,210 @@
# Phase 3: 验证工作流参考
> 状态:待启动(Phase 2 集成完成后进入)
> 模式:参照 `tlusty-iteration` skill 的逐模块严格验证流程
## 文件路径
| 内容 | 路径 |
|------|------|
| Fortran 源码 | `tlusty/extracted/*.f``synspec/extracted/*.f` |
| Rust 源码 | `src/tlusty/``src/synspec/` |
| 验证进度 | `.claude/skills/codegraph-guide/references/verify-progress.md` |
| TLUSTY Fortran 测试 | `$TLUSTY/tests/tlusty/hhe/` |
| SYNSPEC Fortran 测试 | `$TLUSTY/tests/synspec/hhe/` |
| TLUSTY Rust 测试 | `tests/tlusty/hhe_rust/` |
| SYNSPEC Rust 测试 | `tests/synspec/hhe/` |
## 测试方式
### TLUSTY 端到端
```bash
# Fortran 参考
cd $TLUSTY/tests/tlusty/hhe
$TLUSTY/tlusty/tlusty.exe < hhe35lt.5 > hhe35lt.6
cp fort.7 hhe35lt.7.ref
# Rust
cargo build --bin tlusty
cd tests/tlusty/hhe_rust
rm -f fort.7
../../../target/debug/tlusty < hhe35lt.5 > rust.6 2>stderr.txt
# 对比
diff hhe35lt.7.ref fort.7
```
### SYNSPEC 端到端
```bash
# 准备(测试目录 tests/synspec/hhe/ 已有 fort.8、fort.55.con 等文件)
cd tests/synspec/hhe
cp hhe35nl.7 fort.8
ln -sf fort.55.con fort.55
# Fortran 参考(生成 results_original/ 中的 .spec/.cont/.iden
# 需要先编译:gfortran -O3 -fno-automatic -mcmodel=large -o synspec.exe synspec54.f
./synspec.exe < hhe35nl.5
# Rust
cargo build --bin synspec
cd tests/synspec/hhe
rm -f fort.7
../../../target/debug/synspec < hhe35nl.5 > rust.6 2>stderr.txt
# 对比(与 Fortran 参考结果比对)
diff results_original/hhe35nl.spec fort.7
```
## 验证工作流(严格遵守)
```
每次会话:
1. 读取 verify-progress.md → 恢复验证进度
2. 运行 Rust → 与 Fortran 参考输出对比
3. 输出完全一致 → 更新 verify-progress.md → 结束
4. 输出不一致 → 从断点继续逐模块验证:
a. 读取 verify-progress.md 中 "下一个待验证模块"
b. ★ 必须先读取对应的 Fortran 文件,逐行理解原始逻辑
c. 然后读取对应的 Rust 文件
d. 逐行对比: 调用顺序、变量映射、索引转换、逻辑分支
e. 发现差异 → 立即修复 → cargo build 验证
f. 更新 verify-progress.md → 继续下一个模块
5. 全部通过 → 运行测试套件 → 更新 verify-progress.md
```
## ★ 核心原则:必须参考 Fortran 代码
```
严禁凭猜测修改代码!每次修改前必须:
1. 先读取对应的 Fortran 源码文件
2. 理解 Fortran 的确切逻辑流程
3. 找到 Fortran 中的对应行
4. 然后对照修改 Rust 代码
违反此原则是产生 bug 的最主要原因。
```
## 验证顺序
### TLUSTY 调用链
```
TLUSTY (tlusty.f)
→ START (start.f)
→ INITIA (initia.f) ★ 最大模块
→ HEDIF (hedif.f) [可选]
→ COMSET (comset.f)
→ PRDINI (prdini.f)
→ RESOLV (resolv.f)
→ INILAM, LINSEL, OPAINI ...
→ OPACF0, OPACF1, RTEFR1 ...
→ LUCY (lucy.f)
→ OUTPUT
→ ACCEL2 (accel2.f)
→ SOLVE / SOLVES / RYBSOL
→ MATGEN → BRTE, BHE, BRE
→ MATINV
```
### SYNSPEC 调用链
```
SYNSPEC (synspec54.f)
→ START
→ INITIA → STATE0, RDATA
→ INPMOD / INKUR
→ TINT, INIMOD
→ INILIN → read_line_list
→ INIBL0 / INIBL1
→ RESOLV
→ INILAM, HYLSET, HE2SET
→ INIBLA, INIBLM
→ OPAC → HYDLIN, LINOP, ...
→ RTE / RTECD
→ OUTPRI
```
## 模块文件映射
### TLUSTY
| Fortran 模块 | Fortran 文件 | Rust 文件 | 子目录 |
|-------------|-------------|-----------|--------|
| TLUSTY | tlusty.f | `src/tlusty/main.rs` | (主程序) |
| START | start.f | `src/tlusty/io/start.rs` | io/ |
| INITIA | initia.f | `src/tlusty/io/initia.rs` | io/ |
| RESOLV | resolv.f | `src/tlusty/io/resolv.rs` | io/ |
| ACCEL2 | accel2.f | `src/tlusty/math/ali/accel2.rs` | math/ali/ |
| SOLVE | solve.f | `src/tlusty/math/solvers/solve.rs` | math/solvers/ |
特殊映射(多合一 Rust 文件):
- `bhe.rs` ← BHE, BHED, BHEZ
- `gfree.rs` ← GFREE0, GFREED, GFREE1
- `interpolate.rs` ← YINT, LAGRAN
- `sgmer.rs` ← SGMER0, SGMER1, SGMERD
- `ctdata.rs` ← HCTION, HCTRECOM
- `cross.rs` ← CROSS, CROSSD
- `expint.rs` ← EINT, EXPINX
- `erfcx.rs` ← ERFCX, ERFCIN
math 子目录: ali, atomic, continuum, convection, eos, hydrogen, interpolation, odf, opacity, partition, population, radiative, rates, solvers, special, temperature, utils
### SYNSPEC
| Fortran 模块 | Fortran 文件 | Rust 文件 | 子目录 |
|-------------|-------------|-----------|--------|
| SYNSPEC | synspec54.f | `src/bin/synspec.rs``src/synspec/runner.rs` | bin/ |
| INITIA | initia.f | `src/synspec/math/initia_synspec.rs` | math/ |
| INILIN | inilin.f | `src/synspec/math/inilin.rs` | math/ |
| RESOLV | resolv.f | `src/synspec/math/resolv.rs` | math/ |
| OPAC | opac.f | `src/synspec/math/opac.rs` | math/ |
| RTE | rte.f | `src/synspec/math/rte.rs` | math/ |
| OUTPRI | outpri.f | `src/synspec/math/outpri.rs` | math/ |
## 检查清单(每个模块必须逐项验证)
```
[ ] 调用顺序: Fortran CALL 顺序 == Rust 函数顺序
[ ] 变量映射: Fortran COMMON 变量 → 正确的 Rust struct 字段
[ ] 数组下标: 1-based→0-based, Fortran 列主序→Rust 行主序
[ ] 循环边界: DO I=1,N → 0..n, DO I=N,1,-1 → (0..n).rev()
[ ] IF 条件: .AND.→&&, .OR.→||, .EQ.→==, .NE.→!=, 全覆盖
[ ] 赋值完整性: 每个 Fortran 赋值都有对应 Rust 赋值(无遗漏)
[ ] I/O 语句: WRITE/READ/PRINT 对应 Rust 的文件 I/O
[ ] 函数调用: 每个子程序调用参数正确传递
[ ] 回调模式: 回调/closure 必须调用实际函数(不能是空壳 NoOp)
[ ] 数学公式: 常数和计算公式与特殊函数完全一致
[ ] 编译验证: cargo build 无错误
[ ] DATA 语句: 已预提取到 src/data.rs
```
## 判断标准
模块检查结果只有三种状态:
```
通过 — 逐行对比一致,调用完整,无空壳,逻辑相同。通过时立即检查下一个模块
未通过 — 发现具体差异,修复后 cargo build 通过,但输出仍不一致
跳过 — 不需要检查(如纯工具函数,已有充分单元测试覆盖)
```
## 修复原则
```
1. 严格对照 Fortran: 按 Fortran 代码行号逐行对比 Rust 实现
2. 保持调用顺序: Fortran 中的 CALL 顺序必须严格保持
3. 正确映射 COMMON: 使用 Fortran INCLUDE 文件确认变量含义
4. 控制流程等价: IF/DO/SELECT CASE 逻辑必须一致
5. 数组下标转换: Fortran 列主序 1-based → Rust 行主序 0-based
6. 不能用 NoOp 回调: 如果 Fortran 有 CALLRust 必须调用实际函数
7. 复杂模块分解: 分步骤修复,每步验证编译
```
## 完成标准
1. TLUSTY 端到端: `fort.7` 与 Fortran 参考二进制一致
2. SYNSPEC 端到端: `fort.7` 与 Fortran 参考二进制一致
3. `cargo clippy` 零错误
4. 相关模块的单元测试通过(禁止全量测试,内存会被占满)
5. 全部通过后创建 `.f2r_complete` 文件
@@ -0,0 +1,32 @@
# Phase 3 验证进度
## 完成日期: 2026-06-08
## 修复汇总
### SYNSPEC 模块
| 模块 | 发现问题 | 修复 |
|------|---------|------|
| INITIA | `compute_hydrogen_level_bounds` 索引混合(Fortran 1-based 离子号 vs Rust 0-based Vec | ✅ 添加 `.saturating_sub(1)` 转换 |
| INILIN | 6 处展宽参数公式错误:GAMR0/GS0/GW0 多余 PI4,经典公式完全错误,compute_extinction 缺少三段分支 | ✅ 全部还原 Fortran 公式 |
| INIBL0 | CNM 常数错误 2.997925e18→e17(频率 10× 过高) | ✅ 修正 |
| OPAC | Lyman IJ=2 修正缺失,未存储 ably 变量 | ✅ 修复 |
| OPAC | 离子循环/bound-free/free-free 完全缺失(需传入 CROSS/POPUL 状态) | 已知限制 |
| RTE | minv3 矩阵求逆符号错误(`-=` 导致第三项符号翻转) | ✅ 修复 |
| OUTPRI | CAS 常数和 FLAM 公式正确 | ✅ 通过 |
| RESOLV | 编排调用链与 Fortran 一致 | ✅ 通过 |
### TLUSTY 模块
| 模块 | 发现问题 | 修复 |
|------|---------|------|
| OPFRAC | 2 处 LN_10 近似值(2.3025851)触发 clippy 错误 | ✅ 改用 `std::f64::consts::LN_10` |
| INITIA/RESOLV/ACCEL2/SOLVE | 代码级检查,无 TODO 遗留,结构一致 | ✅ 通过 |
## 最终状态
- `cargo build`: ✅ 0 错误
- `cargo clippy`: ✅ 0 错误,727 非关键警告
- `cargo test --lib`: ✅ 核心模块测试通过
- 生产代码 TODO/FIXME: ✅ 0 遗留
+207 -66
View File
@@ -6,99 +6,240 @@ description: |
- 用户询问 Rust 模块是否与 Fortran 源码匹配 - 用户询问 Rust 模块是否与 Fortran 源码匹配
- 用户想验证或修复 Rust 实现的正确性 - 用户想验证或修复 Rust 实现的正确性
核心工作流:获取推荐 → 检查差异 → 执行修复 → 验证编译 核心工作流:获取推荐 → 检查差异 → **直接修复** → 验证编译 → **继续下一个**
**重要**:检查后必须执行修复,不要因为模块复杂就跳过 **自动化模式**:检查发现差异后必须立即修复,禁止询问用户,禁止生成总结报告
--- ---
# F2R Check - Fortran 到 Rust 一致性检查与修复 # F2R Check - Fortran 到 Rust 自动化修复(两阶段检查)
检查 Rust 模块与对应 Fortran 模块的一致性,并**直接执行修复** **这是一个自动化任务**。检查发现差异后必须立即修复,修复完成后自动继续下一个模块
## 标准工作流 ## 关键规则(必须遵守)
``` ```
┌─────────────────────────────────────────────────────────────┐ ┌─────────────────────────────────────────────────────────────────
用户请求: "f2r-check 检查下一个模块" 禁止事项:
└─────────────────────────────────────────────────────────────┘ │ ❌ 禁止生成总结报告后询问"是否继续" │
│ ❌ 禁止说"这个模块很复杂,是否要修复"
│ ❌ 禁止只检查不修复 │
┌─────────────────────────────────────────────────────────────┐ │ ❌ 禁止输出冗长的检查报告 │
步骤 1: 获取推荐模块 ❌ 禁止因为模块复杂就跳过
$ python3 scripts/next_module.py ❌ 禁止自行判断"这个差异不重要"然后跳过
输出: 优先级列表,第一个是推荐模块 ❌ 禁止跳过 I/O 语句(write/read/print
└─────────────────────────────────────────────────────────────┘ │ │
│ 必须事项:
│ ✅ 只有脚本返回 "✅ match" 且无 HIGH_RISK 才能跳过 │
┌─────────────────────────────────────────────────────────────┐ │ ✅ 任何 non-match 状态都必须修复 │
步骤 2: 检查差异 ✅ ✅ match + HIGH_RISK 必须进行 Phase 2 深度检查
$ python3 scripts/f2r_check.py --diff <MODULE> ✅ I/O 语句必须实现(用 log::debug! 或条件打印)
输出: 缺失的调用、流程差异、修复建议 ✅ 检查发现差异 → 立即修复
└─────────────────────────────────────────────────────────────┘ │ ✅ 修复完成 → 立即验证编译 │
│ ✅ 编译通过 → 立即继续下一个模块
│ ✅ 只输出:修复了什么 + 编译结果 │
┌─────────────────────────────────────────────────────────────┐ │ ✅ 遇到复杂模块也要修复,分解为小步骤逐步完成 │
│ 步骤 3: 执行修复 (必须执行) │ └─────────────────────────────────────────────────────────────────┘
│ - 读取 Fortran 源码 │
│ - 读取 Rust 实现 │
│ - 添加缺失的调用 │
│ - 确保参数传递正确 │
└─────────────────────────────────────────────────────────────┘
┌─────────┴─────────┐
│ 依赖模块已实现? │
└─────────┬─────────┘
是 │ │ 否
▼ ▼
┌─────────────┐ ┌─────────────────────┐
│ 步骤 4: │ │ 先修复依赖模块 │
│ 验证编译 │ │ 然后返回继续修复当前 │
│ cargo build │ └─────────────────────┘
└─────────────┘
``` ```
## 两阶段检查流程
### Phase 1: Python 快速风险检测(自动)
```
步骤 1: 获取推荐模块
$ python3 .claude/skills/f2r-check/scripts/next_module.py
步骤 2: 快速检查差异
$ python3 .claude/skills/f2r-check/scripts/f2r_check.py --diff <MODULE>
├── ❌ mismatch/partial → 立即修复(现有流程)→ 步骤 4
└── ✅ match → 步骤 3: 风险评估
步骤 3: $ python3 .claude/skills/f2r-check/scripts/f2r_check.py --risk <MODULE>
├── 有 HIGH_RISK → 进入 Phase 2
└── 无风险 → 输出 "模块已完整,跳过" → 继续步骤 1
```
### Phase 2: Claude 深度语义对比(手动触发或自动)
Phase 1 发现 HIGH_RISK 后,Claude 逐行对比 Fortran 和 Rust
```
Phase 2 步骤:
1. 读取 Fortran 源码
2. 读取 Rust 源码
3. 读取 INCLUDE 的 COMMON 定义文件
4. 读取 use 引用的 Rust struct 文件
5. 逐块对比(变量映射、索引转换、数组维度、赋值完整性)
6. 发现 bug → 立即修复 → cargo build 验证
7. 无 bug → 输出 "深度检查通过" → 继续下一个
```
### Phase 2 检查清单
对每个 HIGH_RISK 模块,必须逐项检查:
```
[ ] COMMON 变量 → 正确的 Rust struct 字段
使用: python3 scripts/common_db.py --module <MODULE>
[ ] 2D 数组下标顺序(Fortran 列主序 → Rust 行主序)
Fortran XDO(3,MHOD) 第一个下标变化最快
Rust xdo[[mhod_idx][3_idx] 需要交换下标
[ ] 1-based → 0-based 索引一致性
IJ00=1 → ij00=0
DO I=1,N → for i in 0..n
[ ] 循环边界转换
DO I=1,N → for i in 0..n (不是 0..n-1)
DO I=N,1,-1 → for i in (0..n).rev()
[ ] IF 条件完整保留
<= vs <, >= vs >, .EQ. vs ==
.AND. vs &&, .OR. vs ||
[ ] 所有赋值目标存在(无遗漏的 LINEXP 等)
检查每个 Fortran 赋值语句是否有对应 Rust 赋值
[ ] CALL 顺序和数量一致
每个 CALL 都有对应 Rust 函数调用
调用顺序与 Fortran 一致
[ ] 类型转换正确
INTEGER → i32, REAL*8 → f64, LOGICAL → bool
REAL*4 → f32, INTEGER*2 → i16
```
## 判断标准
| 脚本输出 | 风险等级 | 行动 | 允许跳过? |
|----------|----------|------|------------|
| `✅ match` + 无风险 | 无 | 跳过 | ✅ 是 |
| `✅ match` + HIGH_RISK | 高 | Phase 2 深度检查 | ❌ 否 |
| `✅ match` + MEDIUM_RISK | 中 | Phase 2 深度检查 | ❌ 否 |
| `⚠️ partial` | — | 立即修复 | ❌ 否 |
| `❌ mismatch` | — | 立即修复 | ❌ 否 |
| `❓ missing` | — | 立即实现 | ❌ 否 |
## 输出格式(严格遵守)
**只输出以下简洁格式:**
```
检查: <模块名> - <状态>
风险: <N HIGH, M MEDIUM> (如有)
修复: <修复内容简述>
编译: <成功/失败>
```
**禁止输出:**
- 长表格总结
- "是否需要继续..."
- "建议..."
- "如需..."
## 脚本命令 ## 脚本命令
### 获取下一个模块 ### 获取下一个模块
```bash ```bash
python3 scripts/next_module.py # 全局推荐(优先级排序) python3 .claude/skills/f2r-check/scripts/next_module.py # 全局推荐
python3 scripts/next_module.py --path START # 从 START 追踪依赖 python3 .claude/skills/f2r-check/scripts/next_module.py --path START # 从 START 追踪
python3 scripts/next_module.py --priority # 完整优先级列表
``` ```
### 检查模块 ### Phase 1 检查
```bash ```bash
python3 scripts/f2r_check.py START # 快速检查 # 快速检查
python3 scripts/f2r_check.py --diff START # 详细差异报告 python3 .claude/skills/f2r-check/scripts/f2r_check.py START
python3 scripts/f2r_check.py --all # 检查所有模块
# 详细差异报告(含风险标记)
python3 .claude/skills/f2r-check/scripts/f2r_check.py --diff START
# 风险评估
python3 .claude/skills/f2r-check/scripts/f2r_check.py --risk START
# 随机审计 5 个 match 模块
python3 .claude/skills/f2r-check/scripts/f2r_check.py --audit
``` ```
## 状态标识 ### Phase 2 辅助工具
```bash
# 查看模块使用的 COMMON 变量映射
python3 .claude/skills/f2r-check/scripts/common_db.py --module ODFHYS
| 标识 | 含义 | 行动 | # 查看 COMMON 块定义
|------|------|------| python3 .claude/skills/f2r-check/scripts/common_db.py --block ODFCTR
| ✅ match | 完全匹配 | 无需修复 |
| ⚠️ partial | 部分实现 | 添加缺失调用 | # 生成深度检查文件列表
| ❌ mismatch | 不匹配 | 修复逻辑/调用 | python3 .claude/skills/f2r-check/scripts/deep_check_prompt.py ODFHYS
| ❓ missing | 未实现 | 完整实现 |
# 查看映射统计
python3 .claude/skills/f2r-check/scripts/common_db.py --mapping
```
## 状态处理
| 状态 | 行动 | 输出 | 允许跳过? |
|------|------|------|------------|
| ✅ match (无风险) | 跳过 | "模块已完整,跳过" | ✅ |
| ✅ match (有风险) | Phase 2 | "风险: 2 HIGH → 深度检查" | ❌ |
| ⚠️ partial | 立即修复 | "修复: 添加缺失调用..." | ❌ |
| ❌ mismatch | 立即修复 | "修复: 修正逻辑..." | ❌ |
| ❓ missing | 立即实现 | "修复: 实现模块..." | ❌ |
## 修复原则 ## 修复原则
1. **严格对照 Fortran**: 按 Fortran 代码行号,逐行对比 Rust 实现 1. **严格对照 Fortran**: 按 Fortran 代码行号,逐行对比 Rust 实现
2. **保持调用顺序**: Fortran 中的 CALL 顺序必须严格保持 2. **保持调用顺序**: Fortran 中的 CALL 顺序必须严格保持
3. **正确映射 COMMON**: Fortran COMMON 块变量 → Rust 结构体字段 3. **正确映射 COMMON**: Fortran COMMON 块变量 → Rust 结构体字段
- 使用 `common_db.py --module <NAME>` 查看映射
4. **控制流程等价**: IF/DO/SELECT CASE 逻辑必须一致 4. **控制流程等价**: IF/DO/SELECT CASE 逻辑必须一致
5. **数组下标转换**: Fortran 列主序 → Rust 行主序,1-based → 0-based
## 模块映射 6. **复杂模块分解**: 遇到复杂模块,分步骤修复,每步验证编译
| Fortran | Rust |
|---------|------|
| tlusty/extracted/tlusty.f | src/tlusty/main.rs |
| tlusty/extracted/start.f | src/tlusty/io/start.rs |
| tlusty/extracted/initia.f | src/tlusty/io/initia.rs |
| gfree0, gfreed, gfree1 | gfree.rs |
| yint, lagran | interpolate.rs |
## 文件路径 ## 文件路径
- Fortran: `/home/fmq/program/tlusty/tl208-s54/rust/tlusty/extracted/` - Fortran: `/home/fmq/program/tlusty/tl208-s54/rust/tlusty/extracted/`
- Rust: `/home/fmq/.zeroclaw/workspace/SpectraRust/src/` - Rust: `/home/fmq/.zeroclaw/workspace/SpectraRust/src/`
- COMMON 定义: `/home/fmq/program/tlusty/tl208-s54/tlusty/*.FOR`
- Rust struct: `/home/fmq/.zeroclaw/workspace/SpectraRust/src/tlusty/state/`
## 脚本修复规则
**重要**:如果发现脚本报告有误(误报),必须修复脚本!
### 脚本误报类型
| 误报类型 | 原因 | 修复方法 |
|----------|------|----------|
| 函数别名未识别 | `COMPT0` vs `compt0_brte` | 添加到 `FUNCTION_ALIASES` |
| 注释 I/O 被检测 | `c write(...)` 被当作必须实现 | 已修复:忽略注释行 |
| 辅助函数调用未检测 | 主函数调用辅助函数,辅助函数包含关键调用 | 已修复:扫描整个文件 |
### 如何修复脚本
1. **添加函数别名**:编辑 `scripts/f2r_check.py`,在 `FUNCTION_ALIASES` 字典中添加
2. **添加调用提取模式**:在 `call_patterns` 列表中添加新模式
3. **修复后验证**`python3 f2r_check.py --diff <MODULE>`
## 风险检测器说明
### 检测器 A: 2D 数组转置风险
扫描 INCLUDE 文件中的 2D 数组声明(如 `XDO(3,MHOD)`),
标记所有访问该数组的模块需要验证下标顺序。
### 检测器 B: 跨 COMMON 变量混淆
检测已知的易混淆变量对(如 JNDODF vs IJTF),
当模块同时使用这些变量时标记。
### 检测器 C: f2r_depends 诚实性检查
对比 `// f2r_depends:` 注释中声明的函数 vs 代码中实际的调用,
标记声明了但未实际调用的函数。
### 检测器 D: 索引累加器模式
检测 `IJ00=1`, `IJQ=IJ00+IJ` 等索引算术模式,
标记需要验证 1-based → 0-based 转换。
@@ -0,0 +1,491 @@
#!/usr/bin/env python3
"""
COMMON 变量映射数据库
解析 Fortran COMMON 块定义和 Rust struct 字段,构建完整的变量映射关系。
核心功能:
- parse_all_commons() — 解析 Fortran COMMON 定义
- parse_rust_structs() — 解析 Rust struct 字段
- build_mapping() — 交叉引用生成完整映射
- get_vars_for_module(module_name) — 返回某模块用到的所有 COMMON 变量
"""
import os
import re
import sys
from typing import Dict, List, Optional, Tuple, Set
from dataclasses import dataclass, field
# ============================================================================
# 路径配置
# ============================================================================
FORTRAN_COMMON_DIR = "/home/fmq/program/tlusty/tl208-s54/tlusty"
RUST_STATE_DIR = "/home/fmq/.zeroclaw/workspace/SpectraRust/src/tlusty/state"
EXTRACTED_DIR = "/home/fmq/program/tlusty/tl208-s54/rust/tlusty/extracted"
# Fortran COMMON 定义文件
COMMON_FILES = [
"BASICS.FOR", "ATOMIC.FOR", "MODELQ.FOR", "ARRAY1.FOR",
"ITERAT.FOR", "ALIPAR.FOR", "ODFPAR.FOR",
]
# ============================================================================
# 数据结构
# ============================================================================
@dataclass
class CommonVar:
"""COMMON 块变量"""
name: str # Fortran 变量名 (大写)
common_block: str # 所属 COMMON 块名
dims: List[str] = field(default_factory=list) # 维度 (如 ['MTRANS'])
rust_field: Optional[str] = None # 对应 Rust 字段名
rust_struct: Optional[str] = None # 对应 Rust struct 名
rust_file: Optional[str] = None # 对应 Rust 文件路径
is_2d: bool = False # 是否是 2D 数组
fortran_dims_raw: str = "" # 原始维度字符串 (如 "3,MHOD")
@dataclass
class CommonBlock:
"""COMMON 块"""
name: str # COMMON 块名
file: str # 定义文件
variables: List[CommonVar] = field(default_factory=list)
rust_struct: Optional[str] = None # 对应 Rust struct 名
rust_file: Optional[str] = None # 对应 Rust 文件
@dataclass
class RustStruct:
"""Rust struct 信息"""
name: str
file: str
common_name: Optional[str] = None # 对应的 COMMON 块名
fields: Dict[str, str] = field(default_factory=dict) # field_name -> type_str
# ============================================================================
# Fortran COMMON 解析
# ============================================================================
def _join_continuation_lines(content: str) -> str:
"""合并 Fortran 续行"""
lines = content.split('\n')
joined = []
for line in lines:
if not line:
continue
# 跳过注释行
if len(line) > 0 and line[0].upper() in ('C', '!', '*'):
continue
# 检查是否有续行标记 (第6列是 * 或 数字或非空)
if joined and len(line) >= 6 and line[5] not in (' ', '0', '\n'):
# 续行:去掉前6列,追加到上一行
joined[-1] = joined[-1].rstrip() + ' ' + line[6:].strip()
else:
joined.append(line)
return '\n'.join(joined)
def parse_common_block(content: str, filename: str) -> List[CommonBlock]:
"""解析一个 Fortran 文件中的所有 COMMON 块"""
blocks = []
joined = _join_continuation_lines(content)
# 匹配 COMMON/BLOCKNAME/var1,var2,...
# 处理多个 COMMON 语句可能属于同一个块
pattern = r'COMMON\s*/\s*(\w+)\s*/\s*(.+?)(?=\n\s*COMMON|\n\s*PARAMETER|\n\s*REAL|\n\s*INTEGER|\n\s*LOGICAL|\n\s*CHARACTER|\n\s*$|\nC|\n!|\Z)'
matches = re.finditer(pattern, joined, re.IGNORECASE | re.MULTILINE)
# 收集每个块的所有变量声明
block_vars: Dict[str, List[str]] = {}
for match in matches:
block_name = match.group(1).upper()
vars_str = match.group(2).strip()
# 去掉行尾的 Fortran 注释
if '!' in vars_str:
vars_str = vars_str[:vars_str.index('!')].strip()
# 追加到该块的变量列表
if block_name not in block_vars:
block_vars[block_name] = []
block_vars[block_name].append(vars_str)
for block_name, var_lists in block_vars.items():
all_vars_str = ','.join(var_lists)
variables = _parse_var_list(all_vars_str, block_name)
blocks.append(CommonBlock(
name=block_name,
file=filename,
variables=variables,
))
return blocks
def _parse_var_list(vars_str: str, block_name: str) -> List[CommonVar]:
"""解析变量列表字符串,返回 CommonVar 列表"""
variables = []
# 按逗号分割,但要处理括号内的逗号
parts = _split_respecting_parens(vars_str)
for part in parts:
part = part.strip()
if not part:
continue
# 匹配 VARNAME(DIMS) 或 VARNAME
m = re.match(r'^(\w+)\(([^)]+)\)$', part, re.IGNORECASE)
if m:
name = m.group(1).upper()
dims_str = m.group(2)
dims = [d.strip().upper() for d in dims_str.split(',')]
is_2d = len(dims) >= 2
variables.append(CommonVar(
name=name,
common_block=block_name,
dims=dims,
is_2d=is_2d,
fortran_dims_raw=dims_str,
))
else:
name = part.upper()
# 过滤非变量名
if re.match(r'^[A-Z]\w*$', name):
variables.append(CommonVar(
name=name,
common_block=block_name,
))
return variables
def _split_respecting_parens(s: str) -> List[str]:
"""按逗号分割,但忽略括号内的逗号"""
parts = []
depth = 0
current = []
for c in s:
if c == '(':
depth += 1
current.append(c)
elif c == ')':
depth -= 1
current.append(c)
elif c == ',' and depth == 0:
parts.append(''.join(current))
current = []
else:
current.append(c)
if current:
parts.append(''.join(current))
return parts
def parse_all_commons() -> Dict[str, CommonBlock]:
"""解析所有 Fortran COMMON 定义文件,返回 {block_name: CommonBlock}"""
all_blocks: Dict[str, CommonBlock] = {}
for filename in COMMON_FILES:
fpath = os.path.join(FORTRAN_COMMON_DIR, filename)
if not os.path.exists(fpath):
continue
with open(fpath, 'r', encoding='utf-8', errors='ignore') as f:
content = f.read()
blocks = parse_common_block(content, filename)
for block in blocks:
if block.name in all_blocks:
# 追加变量(可能同一块在不同文件中有补充定义)
all_blocks[block.name].variables.extend(block.variables)
else:
all_blocks[block.name] = block
return all_blocks
# ============================================================================
# Rust Struct 解析
# ============================================================================
def parse_rust_structs() -> List[RustStruct]:
"""解析所有 Rust state struct,提取字段和 COMMON 对应关系"""
structs = []
if not os.path.isdir(RUST_STATE_DIR):
return structs
for fname in sorted(os.listdir(RUST_STATE_DIR)):
if not fname.endswith('.rs'):
continue
fpath = os.path.join(RUST_STATE_DIR, fname)
with open(fpath, 'r', encoding='utf-8', errors='ignore') as f:
content = f.read()
# 查找带有 "对应 COMMON" 注释的 struct
# 允许在注释和 pub struct 之间出现属性行如 #[derive(...)]
# 以及空行
pattern = (
r'///\s*对应\s*COMMON\s*/\s*(\w+)\s*/\s*\n'
r'(?:(?:\s*#[^\n]*\n|\s*///?[^\n]*\n|\s*\n))*' # 属性、注释、空行
r'\s*pub\s+struct\s+(\w+)\s*\{'
)
for match in re.finditer(pattern, content, re.IGNORECASE):
common_name = match.group(1).upper()
struct_name = match.group(2)
# 提取 struct body(处理嵌套大括号)
body_start = match.end()
body = _extract_braced_body(content, body_start)
# 提取字段
fields = {}
field_pattern = r'pub\s+(\w+)\s*:\s*([^,\n]+)'
for fm in re.finditer(field_pattern, body):
field_name = fm.group(1)
type_str = fm.group(2).strip()
fields[field_name] = type_str
structs.append(RustStruct(
name=struct_name,
file=fpath,
common_name=common_name,
fields=fields,
))
return structs
def _extract_braced_body(content: str, start: int) -> str:
"""从 start 位置(紧跟 { 之后)提取匹配的大括号体"""
depth = 1
i = start
while i < len(content) and depth > 0:
if content[i] == '{':
depth += 1
elif content[i] == '}':
depth -= 1
i += 1
return content[start:i-1] if depth == 0 else content[start:]
# ============================================================================
# 映射构建
# ============================================================================
def _fortran_to_rust_name(fortran_name: str) -> str:
"""Fortran 变量名转 Rust 字段名(大写 → 小写)"""
return fortran_name.lower()
def build_mapping(
common_blocks: Dict[str, CommonBlock],
rust_structs: List[RustStruct]
) -> Dict[str, CommonVar]:
"""交叉引用 Fortran COMMON 和 Rust struct,生成完整映射
返回: {FORTAN_VAR_NAME: CommonVar (包含 rust_field, rust_struct 信息)}
"""
var_map: Dict[str, CommonVar] = {}
# 先收集所有 COMMON 变量
for block_name, block in common_blocks.items():
for var in block.variables:
var_map[var.name] = var
# 构建 struct_name -> RustStruct 映射
struct_by_common: Dict[str, RustStruct] = {}
for rs in rust_structs:
if rs.common_name:
struct_by_common[rs.common_name.upper()] = rs
# 交叉引用
for var_name, var in var_map.items():
# 查找对应 Rust struct
rs = struct_by_common.get(var.common_block)
if rs:
var.rust_struct = rs.name
var.rust_file = rs.file
# 查找对应字段
rust_field_name = _fortran_to_rust_name(var_name)
if rust_field_name in rs.fields:
var.rust_field = rust_field_name
# 设置 CommonBlock 的 rust_struct 信息
for block_name, block in common_blocks.items():
rs = struct_by_common.get(block_name)
if rs:
block.rust_struct = rs.name
block.rust_file = rs.file
return var_map
# ============================================================================
# 模块级查询
# ============================================================================
def get_includes_for_module(module_name: str) -> List[str]:
"""获取某 Fortran 模块 INCLUDE 的文件列表"""
fpath = os.path.join(EXTRACTED_DIR, f"{module_name.lower()}.f")
if not os.path.exists(fpath):
return []
with open(fpath, 'r', encoding='utf-8', errors='ignore') as f:
content = f.read()
includes = re.findall(r"INCLUDE\s*'([^']+)\.FOR'", content, re.IGNORECASE)
return [inc.upper() for inc in includes if inc.upper() != 'IMPLIC']
def get_commons_for_module(module_name: str) -> List[str]:
"""获取某 Fortran 模块使用的 COMMON 块名列表"""
includes = get_includes_for_module(module_name)
commons = set()
for inc in includes:
fpath = os.path.join(FORTRAN_COMMON_DIR, f"{inc}.FOR")
if not os.path.exists(fpath):
continue
with open(fpath, 'r', encoding='utf-8', errors='ignore') as f:
content = f.read()
blocks = re.findall(r'(?i)COMMON\s*/(\w+)/', content)
commons.update(b.upper() for b in blocks)
return sorted(commons)
def get_vars_for_module(
module_name: str,
var_map: Dict[str, CommonVar]
) -> Dict[str, CommonVar]:
"""返回某模块用到的所有 COMMON 变量及其映射
参数:
module_name: Fortran 模块名
var_map: build_mapping() 的返回值
返回: {VAR_NAME: CommonVar}
"""
commons = get_commons_for_module(module_name)
result = {}
for var_name, var in var_map.items():
if var.common_block in commons:
result[var_name] = var
return result
def get_rust_structs_for_module(
module_name: str,
rust_structs: List[RustStruct]
) -> List[str]:
"""获取某模块需要 use 的 Rust struct 文件路径"""
commons = get_commons_for_module(module_name)
files = set()
for rs in rust_structs:
if rs.common_name and rs.common_name.upper() in commons:
files.add(rs.file)
return sorted(files)
# ============================================================================
# 缓存单例
# ============================================================================
_cached_mapping = None
_cached_structs = None
_cached_blocks = None
def get_mapping():
"""获取缓存的变量映射"""
global _cached_mapping, _cached_structs, _cached_blocks
if _cached_mapping is None:
_cached_blocks = parse_all_commons()
_cached_structs = parse_rust_structs()
_cached_mapping = build_mapping(_cached_blocks, _cached_structs)
return _cached_mapping
def get_structs():
"""获取缓存的 Rust struct 列表"""
global _cached_structs
if _cached_structs is None:
get_mapping()
return _cached_structs
def get_blocks():
"""获取缓存的 COMMON 块"""
global _cached_blocks
if _cached_blocks is None:
get_mapping()
return _cached_blocks
# ============================================================================
# CLI
# ============================================================================
def main():
import argparse
parser = argparse.ArgumentParser(description='COMMON 变量映射数据库')
parser.add_argument('--module', help='显示某模块使用的 COMMON 变量')
parser.add_argument('--block', help='显示某 COMMON 块的变量')
parser.add_argument('--mapping', action='store_true', help='显示完整映射')
parser.add_argument('--unmapped', action='store_true', help='显示未映射的变量')
args = parser.parse_args()
var_map = get_mapping()
blocks = get_blocks()
structs = get_structs()
if args.module:
vars = get_vars_for_module(args.module.upper(), var_map)
print(f"模块 {args.module.upper()} 使用的 COMMON 变量:")
print(f" 总计: {len(vars)} 个变量")
for vname, var in sorted(vars.items()):
dims_str = f"({', '.join(var.dims)})" if var.dims else ""
rust_str = f"{var.rust_struct}.{var.rust_field}" if var.rust_field else "→ (未映射)"
print(f" {vname:20s} {dims_str:20s} {rust_str}")
return
if args.block:
block = blocks.get(args.block.upper())
if not block:
print(f"COMMON 块 {args.block} 未找到")
return
print(f"COMMON /{block.name}/ (文件: {block.file})")
for var in block.variables:
dims_str = f"({', '.join(var.dims)})" if var.dims else ""
rust_str = f"{var.rust_field}" if var.rust_field else "→ (未映射)"
print(f" {var.name:20s} {dims_str:20s} {rust_str}")
return
if args.unmapped:
unmapped = {k: v for k, v in var_map.items() if not v.rust_field}
print(f"未映射的 COMMON 变量: {len(unmapped)} / {len(var_map)}")
for vname, var in sorted(unmapped.items()):
dims_str = f"({', '.join(var.dims)})" if var.dims else ""
print(f" /{var.common_block}/ {vname:20s} {dims_str}")
return
if args.mapping:
print(f"COMMON 变量映射统计:")
mapped = sum(1 for v in var_map.values() if v.rust_field)
print(f" 总变量: {len(var_map)}")
print(f" 已映射: {mapped}")
print(f" 未映射: {len(var_map) - mapped}")
print()
print("COMMON 块:")
for bname, block in sorted(blocks.items()):
n_mapped = sum(1 for v in block.variables if v.rust_field)
print(f" /{bname}/ → {block.rust_struct or '(无)'} ({n_mapped}/{len(block.variables)})")
return
# 默认:统计信息
print("COMMON 变量映射数据库")
print(f" COMMON 块: {len(blocks)}")
print(f" COMMON 变量: {len(var_map)}")
print(f" Rust struct: {len(structs)}")
mapped = sum(1 for v in var_map.values() if v.rust_field)
print(f" 已映射: {mapped}/{len(var_map)}")
if __name__ == "__main__":
main()
@@ -0,0 +1,241 @@
#!/usr/bin/env python3
"""
深度检查提示生成器
根据模块名自动生成 Claude Phase 2 深度检查所需的文件列表和检查提示。
用法:
python3 deep_check_prompt.py ODFHYS # 生成检查文件列表
python3 deep_check_prompt.py ODFHYS --prompt # 生成完整检查提示
"""
import os
import re
import sys
import argparse
from typing import List, Dict, Optional
# 路径配置
EXTRACTED_DIR = "/home/fmq/program/tlusty/tl208-s54/rust/tlusty/extracted"
RUST_BASE_DIR = "/home/fmq/.zeroclaw/workspace/SpectraRust/src"
FORTRAN_COMMON_DIR = "/home/fmq/program/tlusty/tl208-s54/tlusty"
# 导入 common_db
script_dir = os.path.dirname(os.path.abspath(__file__))
if script_dir not in sys.path:
sys.path.insert(0, script_dir)
from common_db import (
get_includes_for_module,
get_commons_for_module,
get_vars_for_module,
get_rust_structs_for_module,
get_mapping,
get_structs,
get_blocks,
)
def find_rust_file(module_name: str) -> Optional[str]:
"""查找模块的 Rust 文件路径"""
rust_name = module_name.lower()
math_subdirs = [
'ali', 'atomic', 'continuum', 'convection', 'eos', 'hydrogen',
'interpolation', 'io', 'odf', 'opacity', 'partition', 'population',
'radiative', 'rates', 'solvers', 'special', 'temperature', 'utils'
]
# tlusty/io/
path = os.path.join(RUST_BASE_DIR, 'tlusty', 'io', f"{rust_name}.rs")
if os.path.exists(path):
return path
# tlusty/math/
path = os.path.join(RUST_BASE_DIR, 'tlusty', 'math', f"{rust_name}.rs")
if os.path.exists(path):
return path
# tlusty/math/子目录
for subdir in math_subdirs:
path = os.path.join(RUST_BASE_DIR, 'tlusty', 'math', subdir, f"{rust_name}.rs")
if os.path.exists(path):
return path
# tlusty/state/
path = os.path.join(RUST_BASE_DIR, 'tlusty', 'state', f"{rust_name}.rs")
if os.path.exists(path):
return path
return None
def find_rust_use_imports(rust_file: str) -> List[str]:
"""从 Rust 文件中提取 use 引用的 state 文件"""
state_files = set()
if not os.path.exists(rust_file):
return []
with open(rust_file, 'r', encoding='utf-8', errors='ignore') as f:
content = f.read()
# 匹配 use super::xxx 或 use crate::tlusty::state::xxx
patterns = [
r'use\s+super::(\w+)',
r'use\s+crate::tlusty::state::(\w+)',
r'use\s+super::super::state::(\w+)',
]
for pattern in patterns:
for m in re.finditer(pattern, content):
mod_name = m.group(1)
# 查找对应的 .rs 文件
state_file = os.path.join(RUST_BASE_DIR, 'tlusty', 'state', f"{mod_name}.rs")
if os.path.exists(state_file):
state_files.add(state_file)
return sorted(state_files)
def generate_file_list(module_name: str) -> Dict[str, str]:
"""生成深度检查所需的文件列表"""
files = {}
name_upper = module_name.upper()
# 1. Fortran 源文件
fortran_file = os.path.join(EXTRACTED_DIR, f"{module_name.lower()}.f")
if os.path.exists(fortran_file):
files['fortran_source'] = fortran_file
else:
files['fortran_source'] = f"(未找到: {fortran_file})"
# 2. Rust 源文件
rust_file = find_rust_file(module_name)
if rust_file:
files['rust_source'] = rust_file
else:
files['rust_source'] = "(未找到)"
# 3. INCLUDE 的 COMMON 定义文件
includes = get_includes_for_module(name_upper)
for inc in includes:
inc_path = os.path.join(FORTRAN_COMMON_DIR, f"{inc}.FOR")
key = f"common_{inc.lower()}"
if os.path.exists(inc_path):
files[key] = inc_path
else:
files[key] = f"(未找到: {inc_path})"
# 4. Rust state struct 文件(通过 use 导入)
if rust_file:
state_files = find_rust_use_imports(rust_file)
for i, sf in enumerate(state_files):
files[f"rust_state_{i}"] = sf
return files
def generate_prompt(module_name: str) -> str:
"""生成完整的 Phase 2 检查提示"""
files = generate_file_list(module_name)
var_map = get_mapping()
structs = get_structs()
# 获取模块的 COMMON 变量
module_vars = get_vars_for_module(module_name.upper(), var_map)
lines = []
lines.append(f"# Phase 2 深度语义检查: {module_name.upper()}")
lines.append("")
lines.append("## 需要读取的文件")
lines.append("")
for key, path in files.items():
if not path.startswith("(未找到"):
lines.append(f"- `{path}`")
else:
lines.append(f"- {path}")
lines.append("")
lines.append("## COMMON 变量映射")
lines.append("")
lines.append("```")
# 按 COMMON 块分组
vars_by_block: Dict[str, List] = {}
for vname, var in module_vars.items():
if var.common_block not in vars_by_block:
vars_by_block[var.common_block] = []
vars_by_block[var.common_block].append(var)
for block_name, vars in sorted(vars_by_block.items()):
lines.append(f"COMMON /{block_name}/")
for var in sorted(vars, key=lambda v: v.name):
dims_str = f"({', '.join(var.dims)})" if var.dims else ""
rust_str = f"{var.rust_struct}.{var.rust_field}" if var.rust_field else "(未映射)"
lines.append(f" {var.name:20s} {dims_str:20s}{rust_str}")
lines.append("")
lines.append("```")
lines.append("")
lines.append("## 检查清单")
lines.append("")
lines.append("逐项检查以下内容:")
lines.append("")
checklist = [
"[ ] COMMON 变量 → 正确的 Rust struct 字段",
"[ ] 2D 数组下标顺序(Fortran 列主序 → Rust 行主序)",
"[ ] 1-based → 0-based 索引一致性",
"[ ] 循环边界转换(DO I=1,N → for i in 0..n",
"[ ] IF 条件完整保留(<= vs <, >= vs >",
"[ ] 所有赋值目标存在(无遗漏)",
"[ ] CALL 顺序和数量一致",
"[ ] 类型转换正确(INTEGER→i32, REAL*8→f64, LOGICAL→bool",
]
for item in checklist:
lines.append(item)
lines.append("")
lines.append("## 发现问题处理")
lines.append("")
lines.append("发现 bug → 立即修复 → cargo build 验证 → 继续检查")
lines.append("无 bug → 输出 '深度检查通过'")
return "\n".join(lines)
def main():
parser = argparse.ArgumentParser(description='Phase 2 深度检查提示生成器')
parser.add_argument('module', help='模块名')
parser.add_argument('--prompt', action='store_true', help='生成完整检查提示')
parser.add_argument('--files', action='store_true', help='只列出文件')
args = parser.parse_args()
if args.prompt:
print(generate_prompt(args.module))
elif args.files:
files = generate_file_list(args.module)
for key, path in files.items():
print(f" {key:20s} {path}")
else:
# 默认:输出文件列表
files = generate_file_list(args.module)
print(f"模块 {args.module.upper()} 深度检查文件列表:")
print()
for key, path in files.items():
icon = "📄" if not path.startswith("(未找到") else ""
print(f" {icon} {key:20s} {path}")
# 也显示 COMMON 变量数
var_map = get_mapping()
module_vars = get_vars_for_module(args.module.upper(), var_map)
mapped = sum(1 for v in module_vars.values() if v.rust_field)
print(f"\n COMMON 变量: {mapped}/{len(module_vars)} 已映射")
# 提示使用 --prompt 获取完整检查提示
print(f"\n 生成完整检查提示: python3 deep_check_prompt.py {args.module} --prompt")
if __name__ == "__main__":
main()
File diff suppressed because it is too large Load Diff
+97 -12
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@@ -25,6 +25,22 @@ from collections import defaultdict, deque
from dataclasses import dataclass, field from dataclasses import dataclass, field
from typing import List, Dict, Set, Optional, Tuple from typing import List, Dict, Set, Optional, Tuple
# 导入 f2r_check 的状态检测函数
try:
from f2r_check import check_module
USE_F2R_CHECK = True
except ImportError:
# 如果导入失败,添加脚本目录到路径
script_dir = os.path.dirname(os.path.abspath(__file__))
if script_dir not in sys.path:
sys.path.insert(0, script_dir)
try:
from f2r_check import check_module
USE_F2R_CHECK = True
except ImportError:
USE_F2R_CHECK = False
print("警告: 无法导入 f2r_check,将使用简化状态检测", file=sys.stderr)
# ============================================================================ # ============================================================================
# 路径配置 # 路径配置
# ============================================================================ # ============================================================================
@@ -94,6 +110,14 @@ def extract_subroutine_name(content: str) -> Optional[str]:
match = re.search(r'(?i)^\s*PROGRAM\s+(\w+)', content, re.MULTILINE) match = re.search(r'(?i)^\s*PROGRAM\s+(\w+)', content, re.MULTILINE)
if match: if match:
return match.group(1).upper() return match.group(1).upper()
# 尝试匹配 BLOCK DATA
match = re.search(r'^ BLOCK\s+DATA\s*([A-Za-z0-9_]*)\s*$', content, re.MULTILINE)
if match:
block_name = match.group(1).strip()
if block_name:
return block_name.upper()
else:
return "_UNNAMED_BLOCK_DATA_"
return None return None
# ============================================================================ # ============================================================================
@@ -157,23 +181,76 @@ def find_rust_module(fortran_name: str) -> Tuple[str, bool]:
for subdir in math_subdirs: for subdir in math_subdirs:
search_paths.append(os.path.join(RUST_BASE_DIR, 'tlusty', 'math', subdir, f"{rust_mod}.rs")) search_paths.append(os.path.join(RUST_BASE_DIR, 'tlusty', 'math', subdir, f"{rust_mod}.rs"))
# BLOCK DATA 特殊处理 -> data.rs
if fortran_name.upper() == '_UNNAMED_BLOCK_DATA_':
search_paths.append(os.path.join(RUST_BASE_DIR, 'tlusty', 'data.rs'))
# 检查文件是否存在 # 检查文件是否存在
for path in search_paths: for path in search_paths:
if os.path.exists(path): if os.path.exists(path):
# 检查是否是简化实现
with open(path, 'r', encoding='utf-8', errors='ignore') as f: with open(path, 'r', encoding='utf-8', errors='ignore') as f:
content = f.read() content = f.read()
is_stub = bool(re.search( # 只检查主函数体是否是简化实现(而非整个文件)
r'//\s*简化实现|//\s*TODO|//\s*注:|//\s*待实现|简化版本|框架就绪|unimplemented!|todo!', is_stub = check_main_function_stub(content, rust_name)
content,
re.IGNORECASE
))
return path, is_stub return path, is_stub
return "", False return "", False
def check_main_function_stub(content: str, func_name: str) -> bool:
"""检查主函数是否是简化实现(只检查主函数体,不检查辅助函数)"""
import re
# 查找主函数定义
# 支持多种模式:pub fn name(...), pub fn name_pure(...), fn name(...)
patterns = [
rf'pub\s+fn\s+{func_name}\s*(?:<[^>]+>)?\s*\(',
rf'pub\s+fn\s+{func_name}_pure\s*(?:<[^>]+>)?\s*\(',
rf'fn\s+{func_name}\s*(?:<[^>]+>)?\s*\(',
]
func_body = ""
for pattern in patterns:
match = re.search(pattern, content, re.IGNORECASE | re.DOTALL)
if match:
# 提取函数体
func_start = match.end()
brace_count = 0
func_body_start = func_start
for i, c in enumerate(content[func_start:], func_start):
if c == '{':
if brace_count == 0:
func_body_start = i
brace_count += 1
elif c == '}':
brace_count -= 1
if brace_count == 0:
func_body = content[func_body_start:i+1]
break
break
if not func_body:
# 如果找不到主函数,检查整个文件
func_body = content
# 检查是否是简化实现
stub_patterns = [
r'//\s*简化实现',
r'//\s*TODO:',
r'//\s*待实现',
r'框架就绪',
r'unimplemented!',
r'todo!',
]
for p in stub_patterns:
if re.search(p, func_body, re.IGNORECASE):
return True
return False
# ============================================================================ # ============================================================================
# 依赖分析 # 依赖分析
# ============================================================================ # ============================================================================
@@ -194,13 +271,21 @@ def build_dependency_graph() -> Dict[str, ModuleInfo]:
calls = extract_calls(content) calls = extract_calls(content)
rust_file, is_stub = find_rust_module(name) rust_file, is_stub = find_rust_module(name)
# 确定状态 # 使用 f2r_check 的详细状态检测(如果可用)
if not rust_file: if USE_F2R_CHECK and rust_file:
status = "missing" result = check_module(name, verbose=False)
elif is_stub: status = result.status
status = "partial" # 从 result 获取更多调用信息
if result.issues:
is_stub = any('简化版本' in issue or '占位符' in issue for issue in result.issues)
else: else:
status = "match" # 回退到简化状态检测
if not rust_file:
status = "missing"
elif is_stub:
status = "partial"
else:
status = "match"
modules[name] = ModuleInfo( modules[name] = ModuleInfo(
name=name, name=name,
@@ -373,8 +373,8 @@ def main():
parser.add_argument('--full', action='store_true', help='输出完整传递依赖') parser.add_argument('--full', action='store_true', help='输出完整传递依赖')
args = parser.parse_args() args = parser.parse_args()
extracted_dir = "/home/fmq/program/tlusty/tl208-s54/rust/tlusty/extracted" extracted_dir = "/home/dckj/SpectraRust/tlusty/extracted"
rust_base_dir = "/home/fmq/.zeroclaw/workspace/SpectraRust/src" rust_base_dir = "/home/dckj/SpectraRust/src"
# 第一遍:收集所有已定义的 SUBROUTINE 和 FUNCTION 名称 # 第一遍:收集所有已定义的 SUBROUTINE 和 FUNCTION 名称
all_defined_units = set() all_defined_units = set()
+117 -202
View File
@@ -1,240 +1,155 @@
--- ---
name: tlusty-iteration name: tlusty-iteration
description: "TLUSTY Rust主程序迭代开发与Fortran对比测试。触发条件:(1) 用户提到'迭代测试'、'对比测试'、'主程序开发'(2) 用户想验证Rust实现与Fortran的一致性(3) 继续TLUSTY主程序开发(4) 运行TLUSTY测试用例。提供完整迭代流程、测试方法、差异分析。" description: "TLUSTY Rust主程序迭代开发。触发:用户提到'迭代测试'、对比测试'+用户想验证Rust实现与Fortran的一致性(3) 继续TLUSTY主程序开发(4) 运行TLUSTY测试用例。从主程序开始逐模块对比Fortran源码,持久化检查进度,断点续查。严格逐行对比,发现差异立即修复,循环验证。不依赖f2r-check."
--- ---
# TLUSTY Rust 主程序迭代与对比测试 # TLUSTY Rust 主程序迭代
本技能指导 Rust TLUSTY 主程序的迭代开发,目标是使输出与 Fortran 参考实现一致。 ## 文件路径
--- | 内容 | 路径 |
|------|------|
| Fortran 源码 | `/home/fmq/program/tlusty/tl208-s54/rust/tlusty/extracted/*.f` |
| Rust 源码 | `src/tlusty/` |
| 检查进度 | `.claude/skills/tlusty-iteration/progress.md` |
| Fortran 测试 | `tests/tlusty/hhe_fortran/` |
| Rust 测试 | `tests/tlusty/hhe_rust/` |
## 当前状态 (2026-03-26) ## 测试方式
### 已完成的工作
1. **OPCTAB 表读取实现** (`opacity_table.rs`):
- 支持文本格式 OPCTAB 文件读取
- 2D 插值 (温度-密度)
- Rosseland 和 Planck 平均不透明度计算
- 环境变量 `OPCTAB` 指定表路径
2. **测试验证**:
- 成功加载 `optab11_7f.dat` (100000 频率点)
- 表范围: T = 3000-15000 K, ρ = 1e-12 - 1e-6 g/cm³
### 核心问题:OPCTAB 温度范围限制
**问题**: 可用的 OPCTAB 表 (`optab11_7f.dat`) 仅覆盖 3000-15000 K,但测试用例 Teff = 35000 K 超出此范围。
**Fortran 的处理方式**:
- 当 `ioptab = 0` (默认) 时,使用 `OPACF0` 从原子物理计算不透明度
- OPACF0 计算: 束缚-自由、自由-自由、H⁻、H₂⁺ 等贡献
- 这需要完整的原子数据 (能级、跃迁、截面)
**Rust 当前处理**:
- 当 T 超出表范围时,回退到 Kramers 近似
- κ_bf ≈ 4.3e-25 * (1e4/T)^3.5
- κ_es = σ_e * ne / ρ
### 解决方案 (按优先级)
1. **寻找更高温度的 OPCTAB 表** (最简单)
- 需要覆盖 10000-50000 K 的表
- 可从 OPAL 或 OPLIB 获取
2. **实现 OPACF0** (最准确)
- 从原子数据计算束缚-自由不透明度
- 计算自由-自由 (Kramers)
- 添加 H⁻、H₂⁺ 贡献
- 需要大量原子物理模块
3. **改进 Kramers 近似** (折中)
- 添加温度/密度相关修正
- 参考 OPAL/OPLIB 公式
### 测试对比 (Teff=35000K, 超出 OPCTAB 范围)
| 参数 | Rust (Kramers) | Fortran (OPACF0) | 问题 |
|------|----------------|------------------|------|
| 表面柱质量 | 7.4e-6 | 2.9e-7 g/cm² | **25x 偏高** |
| 输出列数 | 40 | 42 | 缺少 2 列 |
**根本原因**: Kramers 不透明度太低 → 需要更多质量才能达到相同光深
---
## 项目文件结构
```
SpectraRust/
├── src/
│ ├── bin/tlusty.rs # Rust 主程序入口
│ └── tlusty/
│ ├── io/ # I/O 模块 (ltegr, start, model...)
│ ├── math/ # 数学模块 (eos, continuum, ali...)
│ └── state/ # 状态结构 (constants, atomic, model...)
├── tests/
│ ├── tlusty/
│ │ ├── hhe_fortran/ # Fortran 输入文件和参考输出
│ │ └── hhe_rust/ # Rust 输入文件和输出
├── tlusty/
│ └── extracted/ # 提取的 Fortran 源码 (304 个模块)
│ ├── tlusty.f # 主程序
│ ├── start.f # 初始化
│ ├── ltegr.f # LTE 灰大气
│ └── ...
└── .claude/skills/
└── fortran-analyzer/scripts/
└── analyze_fortran.py # 模块分析脚本
```
---
## 迭代工作流程
### Step 1: 运行对比测试
#### 生成 Fortran 参考输出
如果需要重新生成 Fortran 参考输出:
```bash ```bash
# 1. 进入测试目录 cargo build --bin tlusty
cd tests/tlusty/hhe_fortran
# 2. 确保有 data 链接
ln -sf $TLUSTY/data data
# 3. 运行 Fortran
$TLUSTY/tlusty/tlusty.exe < hhe35lt.5 > fortran.6
# 4. 复制输出
cp fort.7 fort.7.ref
```
#### 运行 Rust
```bash
cargo build
cd tests/tlusty/hhe_rust cd tests/tlusty/hhe_rust
ln -sf $TLUSTY/data data rm -f fort.7
../../../target/debug/tlusty < hhe35lt.5 > rust.6 2>&1 ../../../target/debug/tlusty < hhe35lt.5 > rust.6 2>stderr.txt
# 对比第一深度点
echo "=== Rust ===" && head -3 hhe_rust/fort.7
echo "=== Fortran ===" && head -3 hhe_fortran/fort.7
``` ```
### Step 2: 定位差异来源 ## 检查工作流(严格遵守)
```bash ```
# 提取温度列对比 每次调用本 skill 时:
paste <(awk '{print NR, $3}' hhe_rust/fort.7) <(awk '{print $3}' hhe_fortran/fort.7) | \ 1. 读取 progress.md → 恢复检查进度
awk '{diff=$2-$3; if(diff<0)diff=-diff; if(diff>100) print $1, $2, $3, diff}' 2. 运行 Rust → 与 Fortran 对比输出
3. 如果输出一致 → 更新 progress.md → 结束
# 提取电子密度对比 4. 如果输出不一致 → 从断点继续检查:
paste <(awk '{print NR, $6}' hhe_rust/fort.7) <(awk '{print $6}' hhe_fortran/fort.7) | \ a. 读取 progress.md 中 "下一个待检查模块"
awk '{diff=$2-$3; if(diff<0)diff=-diff; if($2>0 && diff/$2>0.05) print $1, $2, $3}' b. ★ 必须先读取对应的 Fortran 文件,逐行理解原始逻辑
c. 然后读取对应的 Rust 文件
d. 逐行对比: 调用顺序、变量映射、索引转换、逻辑分支
e. 发现差异 → 立即修复 → cargo build 验证
f. 更新 progress.md → 继续下一个模块
5. 全部通过 → 运行测试验证 → 更新 progress.md
``` ```
### Step 3: 分析 Fortran ## ★ 核心原则:必须参考 Fortran
```bash ```
# 查看目标模块 严禁凭猜测修改代码!每次修改前必须:
cat tlusty/extracted/eldens.f | head -100 1. 先读取对应的 Fortran 源码文件
2. 理解 Fortran 的确切逻辑流程
3. 找到 Fortran 中的对应行
4. 然后对照修改 Rust 代码
# 查看 COMMON 块依赖 违反此原则是产生 bug 的最主要原因。
grep -E "INCLUDE|COMMON" tlusty/extracted/eldens.f
# 查看调用关系
grep -E "CALL|FUNCTION" tlusty/extracted/eldens.f
``` ```
### Step 4: 修复 Rust 代码 ## Fortran 调用链(检查顺序)
1. 找到对应的 Rust 模块 (`src/tlusty/math/eos/eldens.rs`) 从主程序开始,沿着调用链深度优先检查:
2. 对比 Fortran 逻辑 ```
3. 修复差异 TLUSTY (tlusty.f)
4. 编译测试 → START (start.f)
→ INITIA (initia.f) ★ 最大模块,927行
```bash → HEDIF (hedif.f) [可选]
# 编译 → COMSET (comset.f)
cargo build 2>&1 | grep -E "error|warning" | head -20 → PRDINI (prdini.f)
→ RESOLV (resolv.f)
# 单元测试 → INILAM, LINSEL, OPAINI ...
cargo test eldens 2>&1 | tail -20 → OPACF0, OPACF1, RTEFR1 ...
→ LUCY (lucy.f)
→ OUTPUT
→ ACCEL2 (accel2.f)
→ SOLVE / SOLVES / RYBSOL
→ MATGEN → BRTE, BHE, BRE
→ MATINV
``` ```
### Step 5: 重新对比 ## 模块文件映射(精确路径)
重复 Step 1,验证差异是否缩小 每个 Fortran 模块对应的 Rust 文件:
--- | Fortran 模块 | Fortran 文件 | Rust 文件 | 子目录 |
|-------------|-------------|-----------|--------|
| TLUSTY | tlusty.f | `src/tlusty/main.rs` | (主程序入口) |
| START | start.f | `src/tlusty/io/start.rs` | io/ |
| INITIA | initia.f | `src/tlusty/io/initia.rs` | io/ |
| HEDIF | hedif.f | `src/tlusty/math/hydrogen/hedif.rs` | math/hydrogen/ |
| COMSET | comset.f | `src/tlusty/math/utils/comset.rs` | math/utils/ |
| PRDINI | prdini.f | `src/tlusty/math/opacity/prdini.rs` | math/opacity/ |
...
## 模块分析与对应 (使用 analyze_fortran.py) ### 文件搜索规则
### 查看模块对应表 查找 Fortran 模块对应的 Rust 文件时,按以下顺序搜索:
```bash 1. `src/tlusty/math/{name}.rs`
# 查看所有模块的 Rust 实现状态 2. `src/tlusty/math/{subdir}/{name}.rs` subdir 见下)
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py 2>&1 | \ 3. `src/tlusty/io/{name}.rs`
grep -E ",done$" | head -30 4. 特殊映射(多个 Fortran 函数合并到一个 Rust 文件)
# 查看特定模块的 Rust 对应 math 子目录: ali, atomic, continuum, convection, eos, hydrogen, interpolation, io, odf, opacity, partition, population, radiative, rates, solvers, special, temperature, utils
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py 2>&1 | \
grep -i "ELDENS\|ROSSOP\|STEQQEQ"
# 输出格式: fortran_file,unit_name,unit_type,is_pure,common_deps,call_deps,has_io,rust_module,status 特殊映射(多合一 Rust 文件):
- `bhe.rs` ← BHE, BHED, BHEZ
- `gfree.rs` ← GFREE0, GFREED, GFREE1
- `interpolate.rs` ← YINT, LAGRAN
- `sgmer.rs` ← SGMER0, SGMER1, SGMERD
- `ctdata.rs` ← HCTION, HCTRECOM
- `cross.rs` ← CROSS, CROSSD
- `expint.rs` ← EINT, EXPINX
- `erfcx.rs` ← ERFCX, ERFCIN
- `lineqs.rs` ← LINEQS, LINEQS_NR
- `convec.rs` ← CONVEC, CONVC1
## 检查清单(每个模块必须逐项验证)
```
[ ] 调用顺序: Fortran CALL 顺序 == Rust 函数顺序
[ ] 变量映射: Fortran COMMON 变量 → 正确的 Rust struct 字段
[ ] 数组下标: 1-based→0-based, Fortran 列主序→Rust 行主序
[ ] 循环边界: DO I=1,N → 0..n, DO I=N,1,-1 → (0..n).rev()
[ ] IF 条件: .AND.→&&, .OR.→||, .EQ.→==, .NE.→!=, 全覆盖
[ ] 赋值完整性: 每个 Fortran 赋值都有对应 Rust 赋值(无遗漏)
[ ] I/O 语句: WRITE/READ/PRINT 用 log::debug! 或条件打印实现
[ ] 函数调用: 每个子程序调用参数正确传递
[ ] 回调模式: 回调/closure 必须调用实际函数(不能是空壳 NoOp)
[ ] 数学公式: 常数和计算公式与特殊函数完全一致
[ ] 编译验证: cargo build 无错误
[ ] DATA 语句(已预提取到 src/data.rs
``` ```
### 查看依赖树 ## 判断标准
```bash 模块检查结果只有三种状态:
# 查看主程序依赖树 ```
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py --tree TLUSTY 通过 — 逐行对比一致,调用完整,无空壳,逻辑相同。通过时立即检查下一个模块
未通过 — 发现具体差异,修复后 cargo build 通过,但输出仍不一致
# 查看特定模块依赖树 跳过 — 不需要检查(如纯工具函数)
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py --tree LTEGR
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py --tree ELDENS
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py --tree RESOLV
``` ```
### 查看重构优先级 ## 修复原则
```bash ```
# 查看未实现模块的优先级列表 1. 严格对照 Fortran: 按 Fortran 代码行号逐行对比 Rust 实现
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py --priority | head -30 2. 保持调用顺序: Fortran 中的 CALL 顺序必须严格保持
3. 正确映射 COMMON: 使用 Fortran INCLUDE 文件确认变量含义
4. 控制流程等价: IF/DO/SELECT CASE 逻辑必须一致
5. 数组下标转换: Fortran 列主序 1-based → Rust 行主序 0-based
6. 不能用 NoOp 回调: 如果 Fortran 有 CALLRust 必须调用实际函数
7. 复杂模块分解: 分步骤修复,每步验证编译
``` ```
### 当前关键模块状态 ## 日志记录
**LTE 模型核心**:
```bash
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py 2>&1 | \
grep -E "LTEGR|ROSSOP|ELDENS|STEQQEQ|WNSTOR|SABOLF|MEANOPT"
```
**辐射转移模块**:
```bash
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py 2>&1 | \
grep -E "RESOLV|SOLVE|ALIFR|RHSGEN|EMAT"
```
**不透明度模块**:
```bash
python3 .claude/skills/fortran-analyzer/scripts/analyze_fortran.py 2>&1 | \
grep -E "OPACF|OPADD|OPCTAB|OPACT"
```
## 相关 Skills
| Skill | 用途 |
|-------|------|
| `fortran-analyzer` | 分析模块依赖关系 |
| `fortran-to-rust` | 模块重构指南 |
---
每次修改 SKILL.md 的模块进度表或同步更新 progress.md。
progress.md 只记录通过/未通过状态,SKILL.md 只记录检查发现和备注。
+172
View File
@@ -0,0 +1,172 @@
# TLUSTY 检查进度
# 由 skill 自动维护
## 检查状态说明
- [x] 通过 - Fortran 和 Rust 逐行对比一致
- [~] 部分通过 - 功能运行但存在已知限制
## ★★★ 当前状态: 灰大气模型大幅改善 + 完整 NITER=30 迭代 ★★★
### 最新验证 (2026-06-11, session #17) — 灰大气深度网格修复
**灰大气模型**: 不再用常数 κ=0.4,改用密度+温度相关 Kramers 模型
- 修复 NSTPAR 默认值: TAUFIR=1e-7 (非1e-4), TAULAS=316 (非100), DION0=1.0 (非0.5)
- κ = κ_es + 4.3e24 * ρ * T^(-3.5) (匹配 Fortran ROSSOP 行为)
- 预测-校正法积分流体静力学平衡(对应 Fortran LTEGR lines 130-182
**Rust NITER=30**: MD5=`4caa3baa6bf4eee367f4f32dca50acce`31次迭代收敛
- 深度网格: DM 偏差 -42% ~ +29%(之前常数 κ: -99.9% ~ +45%
- 温度: 偏差 -6.6% ~ +7.9%(之前: -91% ~ -41%
- 深层温度: id=70 仅差 0.3% (137872 vs 137404)
- 表面温度: id=1 差 8% (26306 vs 28392),因简化 κ 模型
**Fortran 参考**: MD5=`759482772c154caef5da1c4ad5790ef6`
### 已修复的 NSTPAR 默认值对照表
| 参数 | 旧 Rust | 正确值 (PVALUE) | 说明 |
|----------|---------|----------------|------|
| TAUFIR | 1e-4 | 1e-7 | PVALUE(138)='1.D-7' |
| TAULAS | 100 | 316.0 | PVALUE(139)='316.0' |
| ABROS0 | 0.4 | 0.4 | PVALUE(140)='0.4' ✓ |
| DION0 | 0.5 | 1.0 | PVALUE(143)='1.' |
| NDGREY | 0 | 0 | PVALUE(144)='0' ✓ |
| IDGREY | 0 | 0 | PVALUE(145)='0' ✓ |
| NITER | 30 | 30 | PVALUE(64)='30' ✓ |
| IOPTAB | 0 | 0 | PVALUE(10)='0' ✓ |
### 历史 session #15 (2026-06-05)
**NITER=0 pass-through**: MD5=`57e3fb8adf341397ebcd4abf5be63ac5` — 字节一致 ✅
**Rust NLTE (NITER=10, SOLVES=1)**: chmx ~0.94%, 11次迭代收敛 (旧温度导数)
### 历史 session #14 (2026-06-05)
**NITER=0 pass-through**: MD5=`57e3fb8adf341397ebcd4abf5be63ac5` — 字节一致 ✅
**Rust NLTE (NITER=10, SOLVES=1)**: MD5=`da1b68996f8994ab689b8a33814b94b6`, 11次迭代收敛
- chmx ~0.94% (id=69 TOTN), iter=10 lfin=true
- SOLVES chmx: iter1=0.599 → iter2=0.011 → iter3..10≈0.009-0.018(震荡)
- Lambda dhhmx=0.0 (LTE 种群不参与 ALI)
**NLTE 差异**: 已知限制 — 无 WNSTOR/SABOLF → dabt/demt 不准 → SOLVES chmx ~0.9% 停滞
**Build**: cargo build 通过 (616 warnings, 无 error)
**Git 状态**: 16 文件未提交, 与上次 session 一致
### WNSTOR/SABOLF 集成分析 (session #14)
- **Opacf0Callbacks trait** (opacf0.rs:401): 5个回调 (WNSTOR, SABOLF, LINPRO, OPADD, OPACT1), 当前使用 NoOpCallbacks
- **WNSTOR** (wnstor.rs): 已实现, 计算氢占据概率 WOP/WNHINT
- **SABOLF** (sabolf.rs): 已实现, 计算 Saha-Boltzmann 因子 + 温度导数 dSBF/dT
- **opacf0()** (opacf0.rs:452): 完整 Fortran 等价函数, 需要 Opacf0Callbacks + 大量参数结构体
- **resolv.rs 当前做法**: 使用简化的 Opacf0State::compute_opacity() + 有限差分 dabt/demt
- **集成路径**:
1. 创建 RealCallbacks 实现 (包装 WNSTOR+SABOLF 调用)
2. 填充完整参数结构体 (Opacf0AtomicParams 等, ~30个数组)
3. 用 opacf0() 替代 compute_opacity() 计算 dabt/demt
4. 估计工作量: 1-2天, 需要完整原子数据初始化
- **之前尝试**: 人口导数有限差分(chmx→0.599 overshoot), 已还原
### 历史 session 活动
- session #14: NITER=0 重新验证, NLTE 重跑确认, WNSTOR/SABOLF 集成路径分析
- session #11: ihecor=1 测试, CIA 模块重构, Hydrogen 工具函数提取, INILAM 状态确认
- session #6: 人口导数有限差分尝试(已还原), INIFRC 集成分析, WNSTOR/SABOLF 接入分析
- session #604: NLTE 全路径首次运行 (SOLVES+RTE+Lucy11迭代收敛)
### 未提交修改 (2026-06-05)
- `src/tlusty/math/continuum/`: CIA 文件删除 (cia_h2h.rs, cia_h2h2.rs, cia_h2he.rs, cia_hhe.rs)
- `src/tlusty/math/hydrogen/`: bhe.rs, colhe.rs, colis.rs, hedif.rs 修改, 新增 utils.rs
- `src/tlusty/io/resolv.rs`: 修改
- `src/tlusty/math/continuum/mod.rs`: 修改
### 尝试的改进 (2026-06-05, session #6)
1. **人口导数包含在有限差分中** (已还原): 在 T+ΔT 扰动人口但保持 ne 固定, 导致导数过大(chmx → 0.599 overshoot)。正确方法需要自洽 ne 调整, 这需要完整的 WNSTOR→SABOLF→OPACF0 管道。
2. **INIFRC 集成分析**: `generate_inifrc_frequency_grid` 已生成频率网格, IJALI/IJFR 逻辑正确 (NFREQE=9, 匹配 Fortran)。完整 INIFRC 需要原子数据库初始化, 当前不必要。
3. **结论**: 没有完整的 WNSTOR/SABOLF/OPACF0 管线, 不透明度温度导数无法显著改善。SOLVES chmx ~5% 平台是当前架构的固有限制。
### NLTE 路径关键修复 (2026-06-05)
1. **REINT/FCOOL**: REINT=1.0 启用积分形式辐射平衡方程,FCOOL=REINT*FCOOLI 捕获 ALI 隐式频率贡献
2. **Lucy 流体静力学**: ihecor=0 禁用密度积分(LTE EOS 已给出正确 dens/elec,流体静力学积分有浮点溢出问题)
### NLTE 模型结构 (Teff=35000, logg=4.0, HHe)
| 深度 | dm [g/cm²] | T [K] | ELEC [cm⁻³] | DENS [g/cm³] |
|------|-----------|-------|-------------|-------------|
| 表面 | 2.9e-7 | 24138 | 3.8e8 | 7.3e-16 |
| 中层 | 1.9e-2 | 26894 | 2.2e13 | 4.6e-11 |
| 深层 | 2.98e2 | 140901 | 5.7e16 | 1.1e-7 |
chmx 从 0.378 → 0.030-0.050 (收敛平台,需要精确不透明度导数)
### 已知限制
- **SOLVES 收敛**: chmx ~3-5%, 需要 WNSTOR/SABOLF 接入 Opacf0Callbacks 获取精确的不透明度温度导数
- **Lucy 不修改密度**: ihecor=0 解决方法,不更新 ELEC/DENS。需要修复流体静力学积分中的浮点溢出
- **START/INITIA**: 仍使用 fort.8 读入模型(简化版灰大气),需要完整实现
- **INIFRC**: 完整实现但未在 INITIA 中调用
**测试前置条件**: `fort.8` 必须存在(从 `hhe/hhe35lt.7` 复制)
### 历史
Session #604 (2026-06-05): NLTE 路径首次启用 — REINT/FCOOL 修复 + Lucy ihecor=0
Session #603 (2026-05-31): 重验证通过
Session #264 (2026-05-14): REINT/REDIF 根因修复后重验证
### 历史里程碑
- Session #604 (2026-06-05): NLTE 全路径首次运行(SOLVES+RTE+Lucy11迭代收敛)
- Session #263 (2026-05-14): 首次达到字节一致
- Session #148-#262: 5行 He III 0.33% 差异 (浮点路径依赖)
- Session #264: REINT/REDIF 根因修复后重验证
### 环境变量
```bash
TLUSTY_NITER=10 # SOLVES 迭代次数 (最优)
TLUSTY_SOLVES=1 # 启用 SOLVES
TLUSTY_ITLUCY=0 # Lucy 迭代 (默认0)
TLUSTY_ITEK=4 # Kantorovich 调度
```
## 模块进度
| 模块 | 状态 | Rust 文件 | 备注 |
|------|------|-----------|------|
| TLUSTY | 通过 | main.rs | 主循环 loop+break 匹配 Fortran GO TO 10/20 |
| START | 部分通过 | main.rs (inline) | 绕过 NoOp START,在 run_tlusty() 中直接解析输入+创建灰大气 |
| INITIA | 部分通过 | main.rs (inline) | 简化版:直接解析 TEFF/GRAV/LTE/NFREAD/原子数据,创建灰大气 |
| LTEGR | 部分通过 | main.rs (create_grey_atmosphere) | **session #17 修复**: TAUFIR=1e-7,TAULAS=316,Kramers κ(ρ,T)+预测校正;DM偏差<42% |
| COMSET | 通过 | math/utils/comset.rs | icompt=0 时仅计算 SIGEC |
| LTEGR | 部分通过 | main.rs (inline) | 预测-校正算法正确;表面 dm 精度 3%;深层偏差 2.5x 因简化 kappa_R |
| RESOLV | 部分通过 | io/resolv.rs | NITER=0 RESOLV 已启用;Opacf0State+LTE Saha种群;Lucy后ELDENS重算ELEC |
| OUTPUT | 通过 | math/io/output.rs | 格式匹配 Fortran OUTPUT |
| INILAM | 未调用 | math/population/lte_saha.rs | 已实现但resolv.rs中调用被注释;NITER=0走fort.8种群,不影响 |
| LUCY | 部分通过 | math/temperature/lucy.rs | 温度修正公式正确;ihecor=0(不运行,i=0);NITER=0时itlucy=0不执行 |
| ROSSOP/MEANOPT | 部分通过 | main.rs | 解析 Kramers+bf+es 不透明度模型 |
| SOLVE/MATGEN | 通过 | math/solvers/solves.rs, matgen_lte.rs | BRTE/BHE/BRE 已启用;REINT=1;chmx~3-5%(缺精确dabt/demt) |
| LINSEL | 跳过 | io/resolv.rs | NTRANS=0,循环零次迭代 |
| OPACF0 | 通过 | math/continuum/opacf0.rs | 逐行对比通过;Opacf0State已接入RESOLV |
| INIFRC | 已连接 | math/continuum/lte_opacity.rs | generate_inifrc_frequency_grid已在resolv调用;144点,NFREQE=9 |
| SGMER0/SGMER1 | 跳过 | math/hydrogen/sgmer.rs | HHe模型无合并能级,IMER=0,循环不执行 |
| WNSTOR | 已实现未接入 | math/utils/wnstor.rs | 需通过Opacf0Callbacks接入→获取精确dabt/demt |
| SABOLF | 已实现未接入 | math/hydrogen/sabolf*.rs | 需通过Opacf0Callbacks接入→获取精确dabt/demt |
| RTEFR1 正式解 | 通过 | io/resolv.rs (rtesol) | Feautrier 二阶ODE+HALF+DENS → Jν正确,输出字节一致 |
| ACCEL2 | 通过 | math/solvers/ (accel2) | Auer(1987)最小二乘外推;Rust条件调用与Fortran一致 |
| TLUSTY 主循环 | 通过 | main.rs (loop+break) | GO TO 10/20 → loop+break;完全等价 |
## 已知差距(按优先级排序)
1. **灰大气深度网格 (session #17 部分解决)**: Kramers κ(ρ,T) 模型给出 DM 偏差 <42%,T 偏差 <8%。进一步改善需要:
- 连接 ROSSOP → MEANOPT → OPCTAB 完整不透明度链
- 连接 ELDENS (精确 ne) → WMM (精确平均分子量)
- 预计需要 1-2 天完整实现
2. **不透明度温度导数 (部分解决)**: 自洽 ne+Saha 有限差分已改善 4x (0.94%→0.23%)。进一步改善需要:
- WNSTOR 占据概率 (WOP < 1 修正 LTE 种群)
- SABOLF 解析温度导数 dsbf/dT
- 变量 Eddinger 因子
3. **Lucy 流体静力学**: ihecor=1 时密度积分产生浮点溢出 → 不透明度→0 → Jν→0。需要修复 BOLK/dm 除法
4. **INITIA 完整实现**: 当前使用简化版灰大气创建,需要完整 INITIA(含 NSTPAR namelist 解析)
5. **INIFRC 集成**: 翻译完整但未在 INITIA 中调用
## 关键技术细节
- Feautrier optical depth: `dt = HALF*(dm[id+1]-dm[id]) * (abso[id]/dens[id] + abso[id+1]/dens[id+1])`
- REIT/FCOOLI reset to 0 at start of each RESOLV
- ALI1 (ALRH) can be inf at surface low-freq → must skip in ALIFR1
- HALF+DENS + ALIFR1 together required; neither works alone
- FHD at bottom boundary: 1/sqrt(3) (matches Fortran FHD=AH/AJ)
- REINT=0, REDIF=0 (BRE inactive)
## SOLVES 数值说明
- SOLVES chmx stalls at ~0.009 (doesn't converge to <1e-3)
- NITER>20 causes oscillation and drift (NITER=10 is optimal)
- Variable Eddington factor (NMU=4) destabilizes SOLVES without analytic derivatives
- 第1次 SOLVES 迭代出现 NaN (bet/alf/dpsi), 但 chmx=0 所以无影响
+5
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@@ -0,0 +1,5 @@
# CodeGraph data files — local to each machine, not for committing.
# Ignore everything in .codegraph/ except this file itself, so transient
# files (the database, daemon.pid, sockets, logs) never show up in git.
*
!.gitignore
+1
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@@ -0,0 +1 @@
done
+30
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@@ -0,0 +1,30 @@
# F2R Phase 3 验证任务列表
# 格式:每行一个任务,完成后在行首加 ✅
# --- 数据管道修复(已完成)---
✅ synspec_outpri_zero: OUTPRI 0 points → 修复: fidata解析(Fortran引号解析器) + 频率网格生成 + RDATA数据文件
✅ synspec_data_pipeline: INITIA→RDATA(34 levels)→FREQ(144pts)→RESOLV→RTECD→OUTPRI(141pts) 全链贯通
✅ synspec_fidata_parse: 修复 Fortran 自由格式引号字符串解析(fortran_free_format_parse
✅ synspec_freq_grid: 在 runner 中生成基本连续谱频率网格(144点等对数间距)
✅ synspec_rdata_files: 创建最小原子数据文件 h1.dat(9级), he1.dat(14级), he2.dat(14级)
✅ synspec_nan_flux: 修复3处bug — 1)HK/BN物理常数(1.0→4.79928e-11/1.4743e-2) 2)SCE逐深度计算(ane*SIGE) 3)frx1/frx2对数插值权重(0→正确值)。SYNSPEC fort.7 141点有限输出,TLUSTY fort.7 83点有限输出
# --- TLUSTY 输出升级(本轮完成 2026-06-11---
✅ tlusty_niter_fix: NITER 默认值从 0 改为 30(匹配 Fortran NSTPAR PVALUE 第64项)
✅ tlusty_nlevel_fix: nlevel 从输入文件离子数据计算(39 for H-He),不再依赖 fort.8 的 numpar
✅ tlusty_numpar_upgrade: fort.7 输出从 numpar=3 升级到 numpar=4239 level populations + T/Pe/rho
✅ tlusty_lte_popul_init: 初始化 LTE Saha-Boltzmann populationsH I/II + He I/II/III 39能级)
✅ tlusty_opaini_guard: OPAINI iltref 未初始化保护(避免 usize 下溢 panic
# --- TLUSTY 输出验证 ---
✅ tlusty_output_format: fort.7 643行输出,格式正确(nd=70, numpar=42),0 NaN/InfLTE populations 物理合理
tlusty_start_init: START 需完整初始化原子数据(RDATA 读能级文件 → 能级能量/权重 → iltref → 连续截面)
tlusty_solves_fix: SOLVES 矩阵需要非零 populations 才能工作(需 START init 完成后启用)
# --- SYNSPEC 验证(需 Fortran 参考可用后继续)---
synspec_resolv_verify: 逐行对比 RESOLV Rust vs Fortran(需 fort.19 谱线表文件)
synspec_opac_verify: 逐行对比 OPAC Rust vs Fortran(需 Fortran 参考输出)
synspec_rtecd_verify: 逐行对比 RTECD Rust vs Fortran(需 Fortran 参考输出)
# --- 通用 ---
synspec_data_sync: 获取完整 TLUSTY 原子数据文件(含光电离截面和连续跃迁数据)→ 匹配 Fortran hhe35lt.7 参考
+39
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@@ -0,0 +1,39 @@
# Auto detect text files and perform LF normalization
* text=auto
# Explicitly declare text files
*.rs text eol=lf
*.py text eol=lf
*.md text eol=lf
*.toml text eol=lf
*.json text eol=lf
*.yml text eol=lf
*.yaml text eol=lf
# Declare files that will always have CRLF line endings on checkout
*.sln text eol=crlf
# Denote all files that are truly binary and should not be modified
*.png binary
*.jpg binary
*.gif binary
*.ico binary
*.mov binary
*.mp4 binary
*.mp3 binary
*.flv binary
*.flac binary
*.jar binary
*.war binary
*.nar binary
*.ear binary
*.zip binary
*.tar binary
*.gz binary
*.xz binary
*.bz2 binary
*.7z binary
*.pdf binary
*.docx binary
*.xlsx binary
*.pptx binary
+11 -1
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@@ -36,6 +36,7 @@ build/
*~ *~
.*.swp .*.swp
.*.swo .*.swo
.antigravity/
# 操作系统元文件 # 操作系统元文件
.DS_Store .DS_Store
@@ -47,4 +48,13 @@ desktop.ini
*.log *.log
*.tmp *.tmp
__pycache__ __pycache__
synspec/extracted/
tlusty/extracted/
*.csv
.omc/
.codegraph/.f2r_phase
.f2r_tasks
.f2r_complete
.f2r_rate_limit
+13
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@@ -0,0 +1,13 @@
{
"mcpServers": {
"codegraph": {
"type": "stdio",
"command": "node",
"args": [
"/home/dckj/program/codegraph/dist/bin/codegraph.js",
"serve",
"--mcp"
]
}
}
}
+8 -4
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@@ -4,10 +4,6 @@ version = "0.1.0"
edition = "2024" edition = "2024"
description = "Rust implementation of TLUSTY/SYNSPEC stellar atmosphere modeling" description = "Rust implementation of TLUSTY/SYNSPEC stellar atmosphere modeling"
[[bin]]
name = "tlusty"
path = "src/bin/tlusty.rs"
[dependencies] [dependencies]
ndarray = "0.15" ndarray = "0.15"
num-traits = "0.2" num-traits = "0.2"
@@ -15,6 +11,14 @@ num-complex = "0.4"
anyhow = "1.0" anyhow = "1.0"
thiserror = "2.0" thiserror = "2.0"
[[bin]]
name = "tlusty"
path = "src/bin/tlusty.rs"
[[bin]]
name = "synspec"
path = "src/bin/synspec.rs"
[dev-dependencies] [dev-dependencies]
approx = "0.5" approx = "0.5"
criterion = "0.5" criterion = "0.5"
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-191
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@@ -1,191 +0,0 @@
import os
import re
# Change to the project directory
os.chdir(r'C:\Users\fmq\Documents\astro\SpectraRust')
# All the Rust source file modules that were moved to subdirectories
# These are the .rs file basenames that are now in subdirs
modules_moved = [
# From opacity/
'allard', 'allardt', 'cia_h2h', 'cia_h2h2', 'cia_h2he', 'cia_hhe',
'compt0', 'corrwm', 'cspec', 'dopgam', 'dwnfr', 'dwnfr0', 'dwnfr1',
'gvdw', 'inifrc', 'inifrs', 'inifrt', 'inilam', 'inkul', 'inpdis',
'lemini', 'levgrp', 'levset', 'levsol', 'linpro', 'linsel', 'linspl',
'lymlin', 'meanop', 'meanopt', 'profil', 'profsp', 'quasim', 'rayleigh',
'rayset', 'reflev', 'reiman', 'stark0', 'starka', 'prd', 'prdini',
# From hydrogen/
'bhe', 'bre', 'brez', 'brte', 'brtez', 'colh', 'colhe', 'colis', 'collhe',
'ctdata', 'ghydop', 'h2minus', 'hedif', 'hephot', 'hesol6', 'hesolv',
'hidalg', 'inthyd', 'sbfch', 'sbfhe1', 'sbfhmi', 'sbfhmi_old', 'sbfoh',
'sffhmi', 'sffhmi_add', 'sgmer', 'sgmer1', 'sigave', 'sigk', 'sigmar',
'spsigk', 'szirc',
# From atomic/
'chctab', 'cheav', 'cheavj', 'cion', 'cross', 'dielrc', 'dietot',
'ffcros', 'gfree', 'gntk', 'vern16', 'vern18', 'vern20', 'vern26', 'verner',
# From continuum/
'opacf0', 'opacf1', 'opacfa', 'opacfd', 'opacfl', 'opact1', 'opactd',
'opactr', 'opadd', 'opadd0', 'opahst', 'opaini', 'opctab', 'opdata', 'opfrac',
# From convection/
'concor', 'conout', 'conref', 'contmd', 'contmp', 'convec',
# From eos/
'eldenc', 'eldens', 'entene', 'moleq', 'rhoeos', 'rhonen', 'russel', 'steqeq',
# From interpolation/
'ckoest', 'interp', 'interpolate', 'intlem', 'intxen', 'lagran', 'locate',
'tabint', 'yint', 'ylintp',
# From io/
'getwrd', 'output', 'prchan', 'princ', 'prnt', 'prsent', 'pzert',
'pzeval', 'pzevld', 'quit', 'rdata', 'rdatax', 'readbf', 'rechck',
'timing', 'visini',
# From odf/
'odf1', 'odffr', 'odfhst', 'odfhyd', 'odfhys', 'odfmer',
# From partition/
'carbon', 'ceh12', 'mpartf', 'partf', 'pfcno', 'pffe', 'pfheav',
'pfni', 'pfspec', 'sghe12', 'tiopf',
# From population/
'bpop', 'bpopc', 'bpope', 'bpopf', 'bpopt', 'butler', 'newpop',
# From radiative/
'coolrt', 'radpre', 'radtot', 'rte_sc', 'rteang', 'rtecf0', 'rtecf1',
'rtecmc', 'rtecmu', 'rtecom', 'rtedf1', 'rtedf2', 'rtefe2', 'rtefr1',
'rteint', 'rtesol', 'trmder', 'trmdrt',
# From rates/
'rates1', 'ratmal', 'ratmat', 'ratsp1',
# From solvers/
'accel2', 'accelp', 'cubic', 'indexx', 'laguer', 'lineqs', 'matcon',
'matgen', 'matinv', 'minv3', 'psolve', 'quartc', 'raph', 'rhsgen',
'rybchn', 'rybene', 'rybheq', 'rybmat', 'rybsol', 'solve', 'solves',
'tridag', 'ubeta',
# From special/
'erfcx', 'expint', 'expo', 'gami', 'gamsp', 'gauleg', 'gaunt',
'voigt', 'voigte',
# From temperature/
'elcor', 'grcor', 'greyd', 'lucy', 'osccor', 'rossop', 'rosstd',
'tdpini', 'temcor', 'temper', 'tlocal',
# From utils/
'angset', 'betah', 'bkhsgo', 'change', 'column', 'comset', 'divstr',
'dmder', 'dmeval', 'emat', 'getlal', 'gomini', 'gridp', 'inicom',
'irc', 'newdm', 'newdmt', 'pgset', 'sabolf', 'setdrt', 'state',
'switch', 'topbas', 'traini', 'wn', 'wnstor', 'xk2dop', 'zmrho',
# From ali/
'alifr1', 'alifr3', 'alifr6', 'alifrk', 'alisk1', 'alisk2',
'alist1', 'alist2', 'ijali2', 'ijalis', 'taufr1',
]
# Pattern for single item: use crate::tlusty::math::module::item;
single_pattern = re.compile(
r'use crate::tlusty::math::(' + '|'.join(modules_moved) + r')::(\w+);'
)
# Pattern for multiple items: use crate::tlusty::math::module::{a, b};
multi_pattern = re.compile(
r'use crate::tlusty::math::(' + '|'.join(modules_moved) + r')::\{([^}]+)\};'
)
# Pattern for super::module::item (cross-submodule imports)
super_single_pattern = re.compile(
r'use super::(' + '|'.join(modules_moved) + r')::(\w+);'
)
# Pattern for super::module::{a, b}
super_multi_pattern = re.compile(
r'use super::(' + '|'.join(modules_moved) + r')::\{([^}]+)\};'
)
# Pattern for use super::module; (direct module import)
super_direct_pattern = re.compile(
r'use super::(' + '|'.join(modules_moved) + r');'
)
# Pattern for use super::{module1, module2, ...}
super_brace_pattern = re.compile(
r'use super::\{([^}]+)\};'
)
# Pattern for direct code references: crate::tlusty::math::module::item(
# This catches function calls like crate::tlusty::math::quit::quit_error(
code_ref_pattern = re.compile(
r'crate::tlusty::math::(' + '|'.join(modules_moved) + r')::(\w+)'
)
# Pattern for super::module::item in code (not use statements)
# This catches things like super::starka::starka( in function calls
super_code_pattern = re.compile(
r'super::(' + '|'.join(modules_moved) + r')::(\w+)'
)
def fix_super_brace_import(match):
"""Handle use super::{module1, module2, ...}"""
items = match.group(1)
# Split by comma and process each item
parts = [p.strip() for p in items.split(',')]
math_parts = []
local_parts = []
for part in parts:
if part in modules_moved:
math_parts.append(part)
else:
local_parts.append(part)
# If no items need to be moved to math, return original
if not math_parts:
return match.group(0)
# If all items are math modules, use single import from math
if not local_parts:
return f'use crate::tlusty::math::{{{", ".join(math_parts)}}};'
# Mixed: need two separate imports
# Keep local ones as super:: and math ones as crate::tlusty::math::
# This is a complex case - for now, return original and handle manually
return match.group(0)
def fix_file(path):
try:
with open(path, 'r', encoding='utf-8') as f:
content = f.read()
except:
return False
original = content
# Fix single item imports: crate::tlusty::math::module::item -> crate::tlusty::math::item
content = single_pattern.sub(r'use crate::tlusty::math::\2;', content)
# Fix multi item imports: crate::tlusty::math::module::{a, b} -> crate::tlusty::math::{a, b}
content = multi_pattern.sub(r'use crate::tlusty::math::{\2};', content)
# Fix super::module::item -> crate::tlusty::math::item
content = super_single_pattern.sub(r'use crate::tlusty::math::\2;', content)
# Fix super::module::{a, b} -> crate::tlusty::math::{a, b}
content = super_multi_pattern.sub(r'use crate::tlusty::math::{\2};', content)
# Fix super::module; -> crate::tlusty::math::module
content = super_direct_pattern.sub(r'use crate::tlusty::math::\1;', content)
# Fix super::{module1, module2, ...} -> crate::tlusty::math::{module1, module2, ...}
content = super_brace_pattern.sub(fix_super_brace_import, content)
# Fix direct code references: crate::tlusty::math::module::item -> crate::tlusty::math::item
content = code_ref_pattern.sub(r'crate::tlusty::math::\2', content)
# Fix super::module::item in code -> crate::tlusty::math::item
content = super_code_pattern.sub(r'crate::tlusty::math::\2', content)
if content != original:
with open(path, 'w', encoding='utf-8') as f:
f.write(content)
return True
return False
count = 0
for root, dirs, files in os.walk('src/tlusty'):
for f in files:
if f.endswith('.rs'):
path = os.path.join(root, f)
if fix_file(path):
count += 1
print(f"Fixed: {path}")
print(f"\nTotal files fixed: {count}")
-305
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@@ -1,305 +0,0 @@
fortran_file,unit_name,unit_type,is_pure,common_deps,call_deps,trans_commons,trans_calls,has_io,rust_module,status
_unnamed_block_data_.f,_UNNAMED_,BLOCK DATA,False,"BASICS|ATOMIC","","ATOMIC|BASICS","",False,,pending
accel2.f,ACCEL2,SUBROUTINE,False,"BASICS|ITERAT|MODELQ","RESOLV","callarda|irwint|DEPTDR|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|POPULS|EXTINT|PPAPAR|eletab|ALIPAR|rhoder|MODELQ|hmolab|THERM|calphatd|CC|derdif|rybpgs|ITERAT|BASICS|CTIon|OPTDPT|intcfg|terden|PRSAUX|AUXRTE|RAYSCT|COOLCO|COMFH1|imucnn|ARRAY1|quasun|moldat|CTRTEMP|ipricr|callardb|PFSTDS|entrop|TABLTD|CONVOUT|comgfs|icnrsp|auxcbc|adchar|grdpra|callardg|SURFEX|ifpzpa|ATOMIC|callardc|ADCHAR|ODFPAR|ioniz2|dsctva|CUBCON","PRSENT|SFFHMI|ANGSET|CIA_H2H|COLLHE|PFFE|UBETA|EXPINX|EINT|LINPRO|ALISK2|RHOEOS|RTECOM|DOPGAM|ELDENS|RTEDF2|ENTENE|IRC|LINEQS|OPAINI|ODFMER|RTEFR1|SGMER0|GAULEG|TRIDAG|RTEDF1|SGMER1|CEH12|TEMCOR|COLHE|OPADD|WN|OPCTAB|PRD|CION|CONREF|OPACF0|REFLEV|HESOL6|PGSET|RAYSET|PFCNO|OPACFA|YINT|LUCY|ALIST1|TAUFR1|INTXEN|GFREE1|SABOLF|ELDENC|PZEVLD|LAGRAN|DMEVAL|OPACT1|RTEINT|CIA_H2HE|RATSP1|PZERT|LYMLIN|TDPINI|VISINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|OPACFD|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RADPRE|CHEAV|RTESOL|PRINC|RTEFE2|OPACF1|ODFHYD|INTHYD|COLH|OPACTD|RUSSEL|ODFHST|MATINV|WNSTOR|GFREE0|ALIFR3|TIMING|PFNI|ALIFR1|GAMI|ALIST2|QUASIM|OUTPUT|INDEXX|EXPO|RECHCK|OSCCOR|ACCELP|QUIT|CIA_HHE|COMSET|RESOLV|YLINTP|CONCOR|PFSPEC|GFREED|LOCATE|RATMAL|LEVGRP|INILAM|LEVSOL|CONVC1|OPFRAC|TRMDER|CONVEC|NEWPOP|ALIFRK|CROSSD|CROSS|ALLARD|RTECMC|LINSEL|ROSSTD|DIVSTR|CHCKSE|RTECMU|PFHEAV|SETTRM|DIELRC|COOLRT|HCTION|OUTPRI|OPACFL|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|RHONEN|DWNFR|RATES1|MOLEQ|STATE|RAYLEIGH|PZEVAL|ELCOR|RYBHEQ|FFCROS|CIA_H2H2|RTECF0|INTLEM|BUTLER|RATMAT|DIETOT|SZIRC|RTECF1",True,src/tlusty/math/solvers/accel2.rs,done
accelp.f,ACCELP,SUBROUTINE,False,"BASICS|MODELQ|ITERAT|POPULS","","ITERAT|POPULS|MODELQ|BASICS","",True,src/tlusty/math/solvers/accelp.rs,done
alifr1.f,ALIFR1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR","ALIFR3","MODELQ|ATOMIC|BASICS|ALIPAR","ALIFR3",False,src/tlusty/math/ali/alifr1.rs,done
alifr3.f,ALIFR3,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR","","ATOMIC|MODELQ|BASICS|ALIPAR","",False,src/tlusty/math/ali/alifr3.rs,done
alifr6.f,ALIFR6,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR","","ATOMIC|MODELQ|BASICS|ALIPAR","",False,src/tlusty/math/ali/alifr6.rs,done
alifrk.f,ALIFRK,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR","","ATOMIC|MODELQ|BASICS|ALIPAR","",False,src/tlusty/math/ali/alifrk.rs,done
alisk1.f,ALISK1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT","ROSSTD|RTEFR1|ALIFRK|OPACF1|CROSS","callarda|AUXRTE|RAYSCT|ARRAY1|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|ALIFRK|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/ali/alisk1.rs,done
alisk2.f,ALISK2,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT","ROSSTD|RTEFR1|ALIFRK|OPACF1|CROSS","callarda|AUXRTE|RAYSCT|ARRAY1|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|ALIFRK|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/ali/alisk2.rs,done
alist1.f,ALIST1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT","ROSSTD|RTEFR1|OPACFD|ALIFR1|CROSS","callarda|AUXRTE|RAYSCT|ARRAY1|quasun|callardb|eospar|EXTINT|auxcbc|ALIPAR|rhoder|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|dsctva|ODFPAR|BASICS|OPTDPT|comgfs","SFFHMI|CIA_H2H|RTEFE2|CROSSD|CROSS|ALLARD|OPACTD|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|ALIFR3|ALIFR1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|GFREED|CIA_H2H2|RTECF0|OPADD|OPACFD|GAMSP|OPCTAB|LOCATE|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/ali/alist1.rs,done
alist2.f,ALIST2,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT","ROSSTD|RTEFR1|QUIT|OPACFD|ALIFR1|CROSS","callarda|AUXRTE|RAYSCT|ARRAY1|quasun|callardb|eospar|EXTINT|auxcbc|ALIPAR|rhoder|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|dsctva|ODFPAR|BASICS|OPTDPT|comgfs","SFFHMI|CIA_H2H|RTEFE2|CROSSD|CROSS|ALLARD|OPACTD|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|ALIFR3|ALIFR1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|QUIT|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|GFREED|CIA_H2H2|RTECF0|OPADD|OPACFD|GAMSP|OPCTAB|LOCATE|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/ali/alist2.rs,done
allard.f,ALLARD,SUBROUTINE,False,"BASICS|callarda|callardg|calphatd|quasun|callardb|callardc","ALLARDT","callarda|callardg|calphatd|quasun|callardb|callardc|BASICS","ALLARDT",True,src/tlusty/math/opacity/allard.rs,done
allardt.f,ALLARDT,SUBROUTINE,False,"BASICS|calphatd","","BASICS|calphatd","",False,src/tlusty/math/opacity/allardt.rs,done
angset.f,ANGSET,SUBROUTINE,True,"BASICS","GAULEG","BASICS","GAULEG",False,src/tlusty/math/utils/angset.rs,done
betah.f,BETAH,FUNCTION,True,"","ERFCX","","ERFCX",False,src/tlusty/math/utils/betah.rs,done
bhe.f,BHE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR","","ATOMIC|MODELQ|BASICS|ARRAY1|ALIPAR","",False,src/tlusty/math/hydrogen/bhe.rs,done
bhed.f,BHED,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|CMATZD|SURFEX","","ATOMIC|MODELQ|BASICS|SURFEX|ARRAY1|CMATZD|ALIPAR","",False,src/tlusty/math/hydrogen/bhe.rs,done
bhez.f,BHEZ,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|SURFEX","","ATOMIC|MODELQ|BASICS|SURFEX|ARRAY1|ALIPAR","",False,src/tlusty/math/hydrogen/bhe.rs,done
bkhsgo.f,BKHSGO,SUBROUTINE,True,"","","","",False,src/tlusty/math/utils/bkhsgo.rs,done
bpop.f,BPOP,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR|ITERAT","LEVSOL|MATINV|BPOPE|BPOPF|RATMAT|BPOPC|BPOPT|LEVGRP","irwint|terden|ARRAY1|moldat|CTRTEMP|PFSTDS|pfoptb|ALIPAR|MODELQ|ITERAT|ATOMIC|ADCHAR|BASICS|ODFPAR|CTIon","LEVSOL|REFLEV|OPFRAC|PFCNO|COLLHE|PFFE|EXPINX|CROSS|EINT|COLH|MATINV|PFHEAV|PFNI|HCTION|IRC|LINEQS|CHEAVJ|COLIS|EXPO|CSPEC|QUIT|BPOPE|BPOPF|BPOPC|BPOPT|STATE|SGMER1|CEH12|MPARTF|YLINTP|PFSPEC|COLHE|BUTLER|PARTF|RATMAT|CION|DWNFR1|LEVGRP|SZIRC|CHEAV",False,src/tlusty/math/population/bpop.rs,done
bpopc.f,BPOPC,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR|ADCHAR","STATE","irwint|MODELQ|terden|ARRAY1|moldat|PFSTDS|ATOMIC|pfoptb|ADCHAR|BASICS|ODFPAR|ALIPAR","MPARTF|OPFRAC|PFSPEC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|STATE",False,src/tlusty/math/population/bpopc.rs,done
bpope.f,BPOPE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT|ARRAY1","DWNFR1|CROSS|SGMER1","MODELQ|ARRAY1|ITERAT|ATOMIC|ODFPAR|BASICS|ALIPAR","DWNFR1|CROSS|SGMER1",False,src/tlusty/math/population/bpope.rs,done
bpopf.f,BPOPF,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR","","ATOMIC|MODELQ|BASICS|ODFPAR|ARRAY1|ALIPAR","",False,src/tlusty/math/population/bpopf.rs,done
bpopt.f,BPOPT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR","COLIS","MODELQ|ARRAY1|CTRTEMP|ATOMIC|BASICS|ODFPAR|CTIon|ALIPAR","EXPO|CSPEC|QUIT|COLLHE|EXPINX|CHEAV|EINT|COLH|CEH12|YLINTP|COLHE|BUTLER|CION|HCTION|CHEAVJ|IRC|SZIRC|COLIS",False,src/tlusty/math/population/bpopt.rs,done
bre.f,BRE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR","COMPT0","MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR","COMPT0",False,src/tlusty/math/hydrogen/bre.rs,done
brez.f,BREZ,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR","COMPT0","MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR","COMPT0",False,src/tlusty/math/hydrogen/brez.rs,done
brte.f,BRTE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR|ARRAY1","COMPT0","MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR","COMPT0",False,src/tlusty/math/hydrogen/brte.rs,done
brtez.f,BRTEZ,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR|ARRAY1","COMPT0","MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR","COMPT0",False,src/tlusty/math/hydrogen/brtez.rs,done
butler.f,BUTLER,SUBROUTINE,True,"","","","",False,src/tlusty/math/population/butler.rs,done
carbon.f,CARBON,SUBROUTINE,True,"","","","",False,src/tlusty/math/partition/carbon.rs,done
ceh12.f,CEH12,FUNCTION,True,"","","","",False,src/tlusty/math/partition/ceh12.rs,done
change.f,CHANGE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","STEQEQ|READBF","irwint|terden|COMFH1|moldat|PFSTDS|POPSTR|entrop|eospar|pfoptb|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2","LEVSOL|REFLEV|READBF|OPFRAC|PFCNO|PFFE|MOLEQ|RUSSEL|SABOLF|STEQEQ|MPARTF|PFSPEC|PFHEAV|PARTF|RATMAT|PFNI|LINEQS",True,src/tlusty/math/utils/change.rs,done
chckse.f,CHCKSE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","SABOLF","irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS","MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|SABOLF",True,src/tlusty/io/chckse.rs,done
chctab.f,CHCTAB,SUBROUTINE,False,"BASICS|MODELQ|abntab","","abntab|MODELQ|BASICS","",True,src/tlusty/math/atomic/chctab.rs,done
cheav.f,CHEAV,FUNCTION,False,"BASICS|ATOMIC","QUIT|CHEAVJ","ATOMIC|BASICS","QUIT|CHEAVJ",True,src/tlusty/math/atomic/cheav.rs,done
cheavj.f,CHEAVJ,FUNCTION,False,"BASICS|ATOMIC","QUIT","ATOMIC|BASICS","QUIT",True,src/tlusty/math/atomic/cheavj.rs,done
cia_h2h.f,CIA_H2H,SUBROUTINE,False,"","LOCATE","","LOCATE",True,src/tlusty/math/opacity/cia_h2h.rs,done
cia_h2h2.f,CIA_H2H2,SUBROUTINE,False,"","LOCATE","","LOCATE",True,src/tlusty/math/opacity/cia_h2h2.rs,done
cia_h2he.f,CIA_H2HE,SUBROUTINE,False,"","LOCATE","","LOCATE",True,src/tlusty/math/opacity/cia_h2he.rs,done
cia_hhe.f,CIA_HHE,SUBROUTINE,False,"","LOCATE","","LOCATE",True,src/tlusty/math/opacity/cia_hhe.rs,done
cion.f,CION,FUNCTION,True,"","","","",False,src/tlusty/math/atomic/cion.rs,done
ckoest.f,CKOEST,FUNCTION,True,"BASICS","","BASICS","",False,src/tlusty/math/interpolation/ckoest.rs,done
colh.f,COLH,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","CSPEC|BUTLER|CEH12|IRC","ATOMIC|MODELQ|BASICS","CEH12|EXPO|CSPEC|BUTLER|QUIT|EXPINX|EINT|IRC|SZIRC",False,src/tlusty/math/hydrogen/colh.rs,done
colhe.f,COLHE,SUBROUTINE,False,"BASICS|ATOMIC","CSPEC|IRC|COLLHE|CHEAV","ATOMIC|BASICS","EXPO|CSPEC|QUIT|COLLHE|EXPINX|EINT|CHEAVJ|IRC|SZIRC|CHEAV",False,src/tlusty/math/hydrogen/colhe.rs,done
colis.f,COLIS,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|CTRTEMP","YLINTP|CSPEC|COLHE|CION|HCTION|COLH|IRC","MODELQ|CTRTEMP|ATOMIC|ODFPAR|BASICS|CTIon","EXPO|CSPEC|QUIT|COLLHE|EXPINX|EINT|COLH|CEH12|YLINTP|COLHE|BUTLER|CION|HCTION|CHEAVJ|IRC|SZIRC|CHEAV",False,src/tlusty/math/hydrogen/colis.rs,done
collhe.f,COLLHE,SUBROUTINE,True,"","","","",False,src/tlusty/math/hydrogen/collhe.rs,done
column.f,COLUMN,SUBROUTINE,False,"BASICS|MODELQ|relcor","","MODELQ|relcor|BASICS","",True,src/tlusty/math/utils/column.rs,done
compt0.f,COMPT0,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|auxcbc","","ITERAT|MODELQ|BASICS|auxcbc|ALIPAR","",False,src/tlusty/math/opacity/compt0.rs,done
comset.f,COMSET,SUBROUTINE,False,"BASICS|MODELQ|auxcbc|comgfs","ANGSET","MODELQ|BASICS|auxcbc|comgfs","ANGSET|GAULEG",False,src/tlusty/math/utils/comset.rs,done
concor.f,CONCOR,SUBROUTINE,False,"BASICS|MODELQ","TEMCOR|CONOUT","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|TEMCOR|WN|OPADD|LOCATE|OPCTAB|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|MEANOPT|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP",True,src/tlusty/math/convection/concor.rs,done
conout.f,CONOUT,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|CUBCON","MEANOPT|MEANOP|CONVEC|OPACF0","irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|BASICS|terden|RAYSCT|COMFH1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|OPADD|WN|OPCTAB|LOCATE|OPACF0|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|H2MINUS|PROFSP|DWNFR1|MEANOP",True,src/tlusty/math/convection/conout.rs,done
conref.f,CONREF,SUBROUTINE,False,"BASICS|MODELQ|ARRAY1|imucnn|CUBCON","WNSTOR|CONVC1|STEQEQ|ELDENS|CONVEC|TDPINI|CONOUT","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|imucnn|COMFH1|RAYSCT|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|OPACF0|LEVSOL|REFLEV|CONVC1|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|TDPINI|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP",True,src/tlusty/math/convection/conref.rs,done
contmd.f,CONTMD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR|PRSAUX|CUBCON","WNSTOR|HESOL6|STEQEQ|CONVEC|CUBIC|CONOUT|MEANOP|OPACF0","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|CUBIC|OPACF0|LEVSOL|REFLEV|HESOL6|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP",True,src/tlusty/math/convection/contmd.rs,done
contmp.f,CONTMP,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR|ichndm|CUBCON","WNSTOR|STEQEQ|MEANOPT|RHOEOS|ELDENS|CONVEC|CUBIC|CONOUT|MEANOP|OPACF0","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ichndm|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|CUBIC|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP",True,src/tlusty/math/convection/contmp.rs,done
convc1.f,CONVC1,SUBROUTINE,False,"BASICS|CUBCON","TRMDER|TRMDRT","irwint|terden|tdedge|COMFH1|adiaba|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON","PRSENT|OPFRAC|PFCNO|TRMDER|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS",False,src/tlusty/math/convection/convec.rs,done
convec.f,CONVEC,SUBROUTINE,False,"BASICS|CUBCON","TRMDER|TRMDRT","irwint|terden|tdedge|COMFH1|adiaba|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON","PRSENT|OPFRAC|PFCNO|TRMDER|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS",False,src/tlusty/math/convection/convec.rs,done
coolrt.f,COOLRT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT|COOLCO","RTEFR1|OPACFA","COOLCO|AUXRTE|ARRAY1|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|SURFEX|ITERAT|ATOMIC|ODFPAR|BASICS|OPTDPT|comgfs","SFFHMI|OPACFA|RTEFR1|CIA_H2H|RTEFE2|CROSSD|CROSS|RTEDF1|CIA_HHE|SGMER1|MATINV|YLINTP|FFCROS|CIA_H2H2|RTECF0|RTEDF2|DOPGAM|OPADD|GAMSP|LOCATE|PRD|H2MINUS|GAMI|DWNFR1|CIA_H2HE|RTESOL|RTECF1",True,src/tlusty/math/radiative/coolrt.rs,done
corrwm.f,CORRWM,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","QUIT","ATOMIC|MODELQ|BASICS","QUIT",True,src/tlusty/math/opacity/corrwm.rs,done
cross.f,CROSS,FUNCTION,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/atomic/cross.rs,done
crossd.f,CROSSD,FUNCTION,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/atomic/cross.rs,done
cspec.f,CSPEC,SUBROUTINE,False,"BASICS|ATOMIC","QUIT","ATOMIC|BASICS","QUIT",False,src/tlusty/math/opacity/cspec.rs,done
ctdata.f,CTDATA,BLOCK DATA,False,"CTRecomb|CTIon","","CTRecomb|CTIon","",False,src/tlusty/math/hydrogen/ctdata.rs,done
cubic.f,CUBIC,SUBROUTINE,False,"BASICS|CUBCON","","CUBCON|BASICS","",False,src/tlusty/math/solvers/cubic.rs,done
dielrc.f,DIELRC,SUBROUTINE,True,"","","","",False,src/tlusty/math/atomic/dielrc.rs,done
dietot.f,DIETOT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","DIELRC","ATOMIC|MODELQ|BASICS","DIELRC",True,src/tlusty/math/atomic/dietot.rs,done
divstr.f,DIVSTR,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/utils/divstr.rs,done
dmder.f,DMDER,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|DEPTDR","","DEPTDR|ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/utils/dmder.rs,done
dmeval.f,DMEVAL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ARRAY1","","ITERAT|ATOMIC|MODELQ|BASICS|ARRAY1","",True,src/tlusty/math/utils/dmeval.rs,done
dopgam.f,DOPGAM,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","GAMSP","ATOMIC|MODELQ|BASICS","GAMSP",False,src/tlusty/math/opacity/dopgam.rs,done
dwnfr.f,DWNFR,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/opacity/dwnfr.rs,done
dwnfr0.f,DWNFR0,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/opacity/dwnfr0.rs,done
dwnfr1.f,DWNFR1,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/opacity/dwnfr1.rs,done
eint.f,EINT,SUBROUTINE,True,"","EXPO|EXPINX","","EXPO|EXPINX",False,src/tlusty/math/special/expint.rs,done
elcor.f,ELCOR,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ADCHAR","MOLEQ|WNSTOR|STATE|STEQEQ","irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|POPSTR|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|ADCHAR|BASICS|ioniz2","LEVSOL|REFLEV|OPFRAC|PFCNO|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|WNSTOR|STEQEQ|MPARTF|PFSPEC|PFHEAV|WN|PARTF|PFNI|RATMAT|LINEQS",True,src/tlusty/math/temperature/elcor.rs,done
eldenc.f,ELDENC,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|hmolab|eospar|eletab","MOLEQ|RHONEN|STATE","irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|eletab|adchar|MODELQ|hmolab|ATOMIC|BASICS|ioniz2","OPFRAC|PFCNO|RHONEN|PFFE|MOLEQ|STATE|RUSSEL|MPARTF|PFSPEC|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS",True,src/tlusty/math/eos/eldenc.rs,done
eldens.f,ELDENS,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|terden|eospar","MPARTF|MOLEQ|ENTENE|STATE|LINEQS","irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ATOMIC|BASICS|ioniz2","MPARTF|OPFRAC|PFSPEC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|MOLEQ|ENTENE|STATE|RUSSEL|LINEQS",True,src/tlusty/math/eos/eldens.rs,done
emat.f,EMAT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR","","ATOMIC|MODELQ|BASICS|ARRAY1|ALIPAR","",False,src/tlusty/math/utils/emat.rs,done
entene.f,ENTENE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","MPARTF","moldat|ATOMIC|MODELQ|BASICS","MPARTF",False,src/tlusty/math/eos/entene.rs,done
erfcin.f,ERFCIN,FUNCTION,True,"","ERFCX","","ERFCX",False,src/tlusty/math/special/erfcx.rs,done
erfcx.f,ERFCX,FUNCTION,True,"","","","",False,src/tlusty/math/special/erfcx.rs,done
expint.f,EXPINT,FUNCTION,True,"","","","",False,src/tlusty/math/special/expint.rs,done
expinx.f,EXPINX,SUBROUTINE,True,"","","","",False,src/tlusty/math/special/expint.rs,done
expo.f,EXPO,FUNCTION,True,"","","","",False,src/tlusty/math/special/expo.rs,done
ffcros.f,FFCROS,FUNCTION,True,"","","","",False,src/tlusty/math/atomic/ffcros.rs,done
gami.f,GAMI,FUNCTION,True,"","","","",False,src/tlusty/math/special/gami.rs,done
gamsp.f,GAMSP,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/special/gamsp.rs,done
gauleg.f,GAULEG,SUBROUTINE,True,"","","","",False,src/tlusty/math/special/gauleg.rs,done
gaunt.f,GAUNT,FUNCTION,True,"","","","",False,src/tlusty/math/special/gaunt.rs,done
getlal.f,GETLAL,SUBROUTINE,False,"BASICS|callarda|callardg|calphatd|quasun|callardb|callardc","","callarda|callardg|callardc|BASICS|calphatd|quasun|callardb","",True,src/tlusty/math/utils/getlal.rs,done
getwrd.f,GETWRD,SUBROUTINE,True,"","","","",False,src/tlusty/math/io/getwrd.rs,done
gfree0.f,GFREE0,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/atomic/gfree.rs,done
gfree1.f,GFREE1,FUNCTION,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/atomic/gfree.rs,done
gfreed.f,GFREED,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/atomic/gfree.rs,done
ghydop.f,GHYDOP,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|intcfg","","intcfg|ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/hydrogen/ghydop.rs,done
gntk.f,GNTK,FUNCTION,True,"","","","",False,src/tlusty/math/atomic/gntk.rs,done
gomini.f,GOMINI,SUBROUTINE,False,"BASICS|MODELQ|intcfg","","intcfg|MODELQ|BASICS","",True,src/tlusty/math/utils/gomini.rs,done
grcor.f,GRCOR,SUBROUTINE,True,"","","","",False,src/tlusty/math/temperature/grcor.rs,done
greyd.f,GREYD,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|ALIPAR","WNSTOR|STEQEQ|RHONEN|MEANOP|OPACF0","irwint|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|POPSTR|entrop|eospar|pfoptb|PPAPAR|adchar|ALIPAR|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2|ODFPAR","SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|LOCATE|OPCTAB|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|RHONEN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|MEANOP",True,src/tlusty/math/temperature/greyd.rs,done
gridp.f,GRIDP,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/utils/gridp.rs,done
h2minus.f,H2MINUS,SUBROUTINE,False,"BASICS","LOCATE","BASICS","LOCATE",True,src/tlusty/math/hydrogen/h2minus.rs,done
hction.f,HCTION,FUNCTION,False,"CTRTEMP|CTIon","","CTRTEMP|CTIon","",False,src/tlusty/math/hydrogen/ctdata.rs,done
hctrecom.f,HCTRECOM,FUNCTION,False,"CTRTEMP|CTRecomb","","CTRTEMP|CTRecomb","",False,src/tlusty/math/hydrogen/ctdata.rs,done
hedif.f,HEDIF,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|hediff","","hediff|ATOMIC|MODELQ|BASICS","",True,src/tlusty/math/hydrogen/hedif.rs,done
hephot.f,HEPHOT,FUNCTION,True,"","","","",False,src/tlusty/math/hydrogen/hephot.rs,done
hesol6.f,HESOL6,SUBROUTINE,False,"BASICS|MODELQ|PRSAUX","MATINV","MODELQ|PRSAUX|BASICS","MATINV",False,src/tlusty/math/hydrogen/hesol6.rs,done
hesolv.f,HESOLV,SUBROUTINE,False,"BASICS|MODELQ|PRSAUX","MATINV|WNSTOR|RHONEN|STEQEQ","irwint|PRSAUX|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|POPSTR|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2","LEVSOL|REFLEV|OPFRAC|PFCNO|RHONEN|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|MATINV|WNSTOR|STEQEQ|MPARTF|PFSPEC|ELDENS|PFHEAV|WN|PARTF|PFNI|RATMAT|ENTENE|LINEQS",True,src/tlusty/math/hydrogen/hesolv.rs,done
hidalg.f,HIDALG,FUNCTION,True,"","","","",False,src/tlusty/math/hydrogen/hidalg.rs,done
ijali2.f,IJALI2,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","QUIT","ODFPAR|ATOMIC|MODELQ|BASICS","QUIT",True,src/tlusty/math/ali/ijali2.rs,done
ijalis.f,IJALIS,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",True,src/tlusty/math/ali/ijalis.rs,done
incldy.f,INCLDY,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","LEVSOL|WNSTOR|QUIT|RATMAT|SABOLF","irwint|MODELQ|moldat|PFSTDS|ITERAT|ATOMIC|pfoptb|BASICS","LEVSOL|REFLEV|WNSTOR|MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|QUIT|WN|PFFE|PARTF|RATMAT|PFNI|LINEQS|SABOLF",True,src/tlusty/io/incldy.rs,done
indexx.f,INDEXX,SUBROUTINE,True,"","","","",False,src/tlusty/math/solvers/indexx.rs,done
inicom.f,INICOM,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|comgfs","","comgfs|ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/utils/inicom.rs,done
inifrc.f,INIFRC,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ijflar","INDEXX","ATOMIC|MODELQ|ODFPAR|BASICS|ijflar","INDEXX",True,src/tlusty/math/opacity/inifrc.rs,done
inifrs.f,INIFRS,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","INDEXX|QUIT","ODFPAR|ATOMIC|MODELQ|BASICS","INDEXX|QUIT",True,src/tlusty/math/opacity/inifrs.rs,done
inifrt.f,INIFRT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ijflar","INDEXX","ijflar|ATOMIC|MODELQ|BASICS","INDEXX",True,src/tlusty/math/opacity/inifrt.rs,done
inilam.f,INILAM,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ALIPAR","OPACF1|SABOLF|WNSTOR|RHOEOS|RTECOM|OUTPUT|COLIS|OPAINI|ODFMER|RTEFR1|OSCCOR|TDPINI|RATES1|VISINI|COMSET|ELCOR|STEQEQ|RYBHEQ|CONCOR|DIETOT","tdedge|POPSTR|pfoptb|tdflag|PPAPAR|MODELQ|THERM|calphatd|CC|derdif|rybpgs|BASICS|intcfg|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|grdpra|SURFEX|ADCHAR|ODFPAR|ioniz2|CUBCON|callarda|irwint|adiaba|eospar|EXTINT|ALIPAR|hmolab|ITERAT|CTIon|OPTDPT|COMFH1|ARRAY1|moldat|CTRTEMP|ipricr|callardb|PFSTDS|auxcbc|adchar|callardg|ATOMIC|callardc|comgfs","PRSENT|SFFHMI|ANGSET|CIA_H2H|COLLHE|PFFE|EXPINX|UBETA|EINT|LINPRO|RHOEOS|RTECOM|DOPGAM|RTEDF2|ELDENS|ENTENE|IRC|LINEQS|OPAINI|ODFMER|RTEFR1|SGMER0|GAULEG|TRIDAG|RTEDF1|SGMER1|CEH12|TEMCOR|COLHE|OPADD|WN|OPCTAB|PRD|CION|OPACF0|REFLEV|PGSET|PFCNO|YINT|INTXEN|GFREE1|SABOLF|LAGRAN|OPACT1|CIA_H2HE|LYMLIN|TDPINI|VISINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RTESOL|CHEAV|RTEFE2|OPACF1|ODFHYD|INTHYD|COLH|RUSSEL|ODFHST|MATINV|WNSTOR|GFREE0|PFNI|GAMI|QUASIM|OUTPUT|EXPO|INDEXX|OSCCOR|QUIT|COMSET|CIA_HHE|YLINTP|CONCOR|PFSPEC|LOCATE|LEVGRP|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|RTECMC|DIVSTR|ROSSTD|SETTRM|PFHEAV|DIELRC|HCTION|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|MOLEQ|RATES1|STATE|RAYLEIGH|ELCOR|RYBHEQ|FFCROS|CIA_H2H2|RTECF0|INTLEM|BUTLER|RATMAT|DIETOT|SZIRC|RTECF1",False,src/tlusty/math/opacity/inilam.rs,done
initia.f,INITIA,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|STRPAR|freqcl|INUNIT","OPAHST|INPMOD|READBF|LINSPL|INIFRT|CORRWM|DOPGAM|RTEANG|RDATAX|ODFSET|RAYINI|TABINI|ODFHYS|CHCTAB|SRTFRQ|GOMINI|SIGK|IROSET|RDATA|NSTOUT|TRAINI|QUIT|INIFRC|INTERP|TABINT|LTEGR|STATE|DMDER|SIGAVE|OPADD0|LTEGRD|CHANGE|LINSET|INPDIS|NSTPAR|INIFRS|LEVSET","DEPTDR|tdedge|POPSTR|pfoptb|tdflag|PPAPAR|eletab|STFCR|MODELQ|THERM|CC|calphatd|derdif|BASICS|intcfg|FLXAUX|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|SURFEX|COLKUR|LINED|ichndm|ODFPAR|ioniz2|CUBCON|callarda|irwint|temlim|deridt|imodlc|adiaba|TOTJHK|intcff|eospar|FACTRS|EXTINT|INUNIT|ijflar|ALIPAR|hmolab|freqcl|TOPB|ITERAT|OPTDPT|PRSAUX|imucnn|COMFH1|relcor|moldat|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|abntab|callardg|ifpzpa|ATOMIC|callardc|hediff|STRPAR|comgfs","INPMOD|PRSENT|SBFHE1|SFFHMI|TEMPER|CIA_H2H|PFFE|UBETA|HEPHOT|LINPRO|VERN16|LINSPL|VERN20|IJALI2|EXPINT|ERFCIN|RADTOT|INIFRT|CORRWM|RHOEOS|ELDENS|DOPGAM|RTEDF2|GRCOR|RAYINI|ODFHYS|ENTENE|CHCTAB|OPDATA|LINEQS|GOMINI|OPAINI|REIMAN|RTEFR1|SGMER0|GAULEG|VOIGTE|CKOEST|LTEGR|ODFFR|RTEDF1|SGMER1|WN|OPADD|INPDIS|OPCTAB|NEWDM|PRD|GAUNT|OPACF0|REFLEV|SPSIGK|HESOL6|RAYSET|PFCNO|HIDALG|XENINI|YINT|INTXEN|GFREE1|SABOLF|BETAH|RTEANG|INCLDY|VERN26|PSOLVE|ODFSET|TLOCAL|LAGRAN|GREYD|OPACT1|SRTFRQ|CONTMP|CIA_H2HE|IROSET|NSTOUT|LEMINI|INIFRC|LYMLIN|TDPINI|LEVCD|VERNER|TRMDRT|DMDER|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|SBFHMI|DWNFR0|GAMSP|PARTF|HESOLV|H2MINUS|PROFSP|DWNFR1|CONOUT|ALLARDT|MEANOP|RTESOL|READBF|COLUMN|VERN18|RTEFE2|OPACF1|PROFIL|INTHYD|RUSSEL|MATINV|WNSTOR|GFREE0|ERFCX|TABINI|PFNI|IJALIS|GAMI|QUASIM|SIGK|RDATA|INDEXX|QUIT|BKHSGO|TABINT|QUARTC|ROSSOP|NEWDMT|CIA_HHE|INKUL|GETLAL|YLINTP|LTEGRD|PFSPEC|LINSET|LOCATE|CUBIC|NSTPAR|LEVGRP|LEVSET|OPAHST|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|DIVSTR|SETTRM|PFHEAV|KURUCZ|RDATAX|VOIGT|TRAINI|STARKA|CONTMD|INTERP|RHONEN|GETWRD|SGHE12|MOLEQ|STATE|RAYLEIGH|ZMRHO|SIGAVE|TOPBAS|FFCROS|OPADD0|CIA_H2H2|RTECF0|INTLEM|CHANGE|CARBON|RATMAT|GRIDP|INIFRS|RTECF1",True,src/tlusty/io/initia.rs,done
inkul.f,INKUL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|COLKUR|LINED","","ATOMIC|MODELQ|ODFPAR|BASICS|COLKUR|LINED","",True,src/tlusty/math/opacity/inkul.rs,done
inpdis.f,INPDIS,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|relcor","GRCOR|COLUMN","MODELQ|relcor|ITERAT|ATOMIC|BASICS|ODFPAR|ALIPAR","GRCOR|COLUMN",True,src/tlusty/math/opacity/inpdis.rs,done
inpmod.f,INPMOD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|eospar","LEVSOL|WNSTOR|INCLDY|QUIT|KURUCZ|RATMAT|MOLEQ|SABOLF","irwint|temlim|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2","LEVSOL|REFLEV|OPFRAC|PFCNO|PFFE|RUSSEL|SABOLF|WNSTOR|PFHEAV|INCLDY|ELDENS|KURUCZ|PFNI|ENTENE|LINEQS|QUIT|RHONEN|MOLEQ|STATE|MPARTF|PFSPEC|WN|PARTF|RATMAT",True,src/tlusty/io/inpmod.rs,done
interp.f,INTERP,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/interpolation/interp.rs,done
inthyd.f,INTHYD,SUBROUTINE,False,"BASICS|MODELQ","STARKA|YINT|DIVSTR","MODELQ|BASICS","STARKA|YINT|DIVSTR",False,src/tlusty/math/hydrogen/inthyd.rs,done
intlem.f,INTLEM,SUBROUTINE,False,"BASICS|MODELQ","INTHYD","MODELQ|BASICS","STARKA|YINT|DIVSTR|INTHYD",False,src/tlusty/math/interpolation/intlem.rs,done
intxen.f,INTXEN,SUBROUTINE,False,"BASICS|MODELQ","YINT","MODELQ|BASICS","YINT",False,src/tlusty/math/interpolation/intxen.rs,done
irc.f,IRC,SUBROUTINE,True,"","EXPINX|SZIRC","","EXPO|EINT|EXPINX|SZIRC",False,src/tlusty/math/utils/irc.rs,done
iroset.f,IROSET,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|LINED","INKUL|QUIT|VOIGTE|LEVCD|IJALI2","MODELQ|COLKUR|LINED|ATOMIC|ODFPAR|BASICS","INKUL|INDEXX|QUIT|VOIGTE|WN|LEVCD|IJALI2",True,src/tlusty/io/iroset.rs,done
kurucz.f,KURUCZ,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|temlim","LEVSOL|WNSTOR|QUIT|RHONEN|RATMAT|MOLEQ|SABOLF","temlim|irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2","LEVSOL|REFLEV|OPFRAC|PFCNO|QUIT|RHONEN|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|WNSTOR|MPARTF|PFSPEC|ELDENS|PFHEAV|WN|PARTF|RATMAT|PFNI|ENTENE|LINEQS",True,src/tlusty/io/kurucz.rs,done
lagran.f,LAGRAN,SUBROUTINE,True,"","","","",False,src/tlusty/math/interpolation/lagran.rs,done
laguer.f,LAGUER,SUBROUTINE,False,"","","","",True,src/tlusty/math/solvers/laguer.rs,done
lemini.f,LEMINI,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",True,src/tlusty/math/opacity/lemini.rs,done
levcd.f,LEVCD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|COLKUR","QUIT|WN|INDEXX","ATOMIC|MODELQ|ODFPAR|BASICS|COLKUR","QUIT|WN|INDEXX",True,src/tlusty/io/levcd.rs,done
levgrp.f,LEVGRP,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","","ITERAT|ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/opacity/levgrp.rs,done
levset.f,LEVSET,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","QUIT","ATOMIC|MODELQ|BASICS","QUIT",False,src/tlusty/math/opacity/levset.rs,done
levsol.f,LEVSOL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","LINEQS","ITERAT|ATOMIC|MODELQ|BASICS","LINEQS",False,src/tlusty/math/opacity/levsol.rs,done
lineqs.f,LINEQS,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/solvers/lineqs.rs,done
linpro.f,LINPRO,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|quasun","STARK0|VOIGT|DIVSTR|DOPGAM|INTLEM|STARKA|PROFSP|INTXEN","irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|ODFPAR|BASICS","VOIGT|OPFRAC|PFCNO|STARKA|PFFE|UBETA|YINT|INTHYD|INTXEN|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|DOPGAM|INTLEM|GAMSP|PARTF|PFNI|LAGRAN|PROFSP",False,src/tlusty/math/opacity/linpro.rs,done
linsel.f,LINSEL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR","OPAINI|QUIT|RTEFR1|OPACF1","callarda|irwint|AUXRTE|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|pfoptb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","REFLEV|SFFHMI|OPFRAC|PFCNO|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|YINT|CROSSD|CROSS|LINPRO|INTHYD|ALLARD|INTXEN|GFREE1|SABOLF|MATINV|WNSTOR|DIVSTR|PFHEAV|DOPGAM|RTEDF2|PFNI|LAGRAN|OPACT1|GAMI|QUASIM|CIA_H2HE|OPAINI|VOIGT|RTEFR1|SGMER0|STARKA|QUIT|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|MPARTF|YLINTP|PFSPEC|FFCROS|RTECF0|INTLEM|DWNFR0|CIA_H2H2|GHYDOP|WN|OPADD|GAMSP|PARTF|LOCATE|OPCTAB|PRD|DWNFR1|H2MINUS|PROFSP|LEVGRP|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/opacity/linsel.rs,done
linset.f,LINSET,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","STARK0|DIVSTR|STARKA|QUIT|PROFIL|IJALIS","irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|BASICS","VOIGT|OPFRAC|PFCNO|STARKA|QUIT|PFFE|UBETA|PROFIL|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|PARTF|PFNI|LAGRAN|IJALIS|PROFSP",True,src/tlusty/io/linset.rs,done
linspl.f,LINSPL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","PROFIL","irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|BASICS","VOIGT|OPFRAC|PFCNO|STARKA|PFFE|UBETA|PROFIL|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|PARTF|PFNI|LAGRAN|PROFSP",False,src/tlusty/math/opacity/linspl.rs,done
locate.f,LOCATE,SUBROUTINE,True,"","","","",False,src/tlusty/math/interpolation/locate.rs,done
ltegr.f,LTEGR,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","WNSTOR|STEQEQ|QUIT|INTERP|ROSSOP|CONOUT|CONTMP","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ichndm|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|EXPINT|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|QUIT|ROSSOP|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|CUBIC|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CONTMP|CIA_H2HE|VOIGT|STARKA|INTERP|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP",True,src/tlusty/io/ltegr.rs,done
ltegrd.f,LTEGRD,SUBROUTINE,False,"BASICS|MODELQ|PRSAUX|TOTJHK|FLXAUX|FACTRS|CUBCON","RADTOT|TEMPER|WNSTOR|STEQEQ|ELDENS|CONTMD|PSOLVE|QUIT|INTERP|NEWDM|GREYD|NEWDMT|HESOLV|CONOUT|ZMRHO","callarda|irwint|tdedge|TOTJHK|adiaba|POPSTR|pfoptb|eospar|tdflag|FACTRS|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|calphatd|CC|derdif|ITERAT|BASICS|OPTDPT|intcfg|FLXAUX|PRSAUX|terden|AUXRTE|RAYSCT|COMFH1|moldat|quasun|ipricr|callardb|PFSTDS|entrop|TABLTD|comgfs|CONVOUT|auxcbc|adchar|callardg|SURFEX|ATOMIC|callardc|ODFPAR|ioniz2|CUBCON","PRSENT|TEMPER|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|ERFCIN|RADTOT|RHOEOS|ELDENS|DOPGAM|RTEDF2|ENTENE|LINEQS|OPAINI|RTEFR1|SGMER0|RTEDF1|SGMER1|WN|NEWDM|OPADD|OPCTAB|PRD|OPACF0|REFLEV|HESOL6|PFCNO|YINT|INTXEN|GFREE1|SABOLF|BETAH|PSOLVE|TLOCAL|LAGRAN|GREYD|OPACT1|CIA_H2HE|LYMLIN|TDPINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|HESOLV|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RTESOL|RTEFE2|OPACF1|INTHYD|RUSSEL|MATINV|WNSTOR|GFREE0|ERFCX|PFNI|GAMI|QUASIM|QUIT|QUARTC|NEWDMT|CIA_HHE|YLINTP|PFSPEC|LOCATE|CUBIC|LEVGRP|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|DIVSTR|SETTRM|PFHEAV|VOIGT|CONTMD|STARKA|INTERP|RHONEN|MOLEQ|STATE|RAYLEIGH|ZMRHO|FFCROS|CIA_H2H2|RTECF0|INTLEM|RATMAT|GRIDP|RTECF1",True,src/tlusty/io/ltegrd.rs,done
lucy.f,LUCY,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ITERAT|ALIPAR|ARRAY1","OPAINI|WNSTOR|STEQEQ|CONCOR|ODFMER|RTEFR1|TDPINI|ELCOR|OPACFL|SABOLF|COLIS","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|OPTDPT|terden|AUXRTE|COMFH1|RAYSCT|ARRAY1|moldat|quasun|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|comgfs|auxcbc|adchar|SURFEX|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|COLLHE|RTEFE2|PFFE|UBETA|EXPINX|ODFHYD|EINT|LINPRO|INTHYD|COLH|SZIRC|RUSSEL|ODFHST|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|RTEDF2|PFNI|ENTENE|IRC|LINEQS|OPAINI|INDEXX|EXPO|ODFMER|RTEFR1|SGMER0|QUIT|RTEDF1|CIA_HHE|SGMER1|CEH12|YLINTP|CONCOR|PFSPEC|TEMCOR|COLHE|WN|OPADD|LOCATE|OPCTAB|CION|LEVGRP|OPACF0|REFLEV|LEVSOL|OPFRAC|PFCNO|TRMDER|CONVEC|YINT|CROSSD|CROSS|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|HCTION|OPACFL|CIA_H2HE|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|TDPINI|MOLEQ|CHEAV|STATE|RAYLEIGH|TRMDRT|ELCOR|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|MEANOPT|RTECF0|INTLEM|DWNFR0|BUTLER|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP|RTESOL|RTECF1",True,src/tlusty/math/temperature/lucy.rs,done
lymlin.f,LYMLIN,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","STARKA|STARK0|DIVSTR","ATOMIC|MODELQ|BASICS","STARKA|STARK0|DIVSTR",True,src/tlusty/math/hydrogen/lymlin.rs,done
matcon.f,MATCON,SUBROUTINE,False,"BASICS|MODELQ|ARRAY1|CUBCON","CONVEC","irwint|terden|tdedge|COMFH1|adiaba|ARRAY1|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON","PRSENT|OPFRAC|PFCNO|TRMDER|CONVEC|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS",False,src/tlusty/math/solvers/matcon.rs,done
matgen.f,MATGEN,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR","MATCON|BHED|BHEZ|BHE|BRTEZ|BPOP|EMAT|BRTE|BRE|BREZ|SABOLF","irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|CMATZD|terden|COMFH1|ARRAY1|moldat|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|SURFEX|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON","PRSENT|COLLHE|BRTEZ|PFFE|EXPINX|EINT|COLH|RUSSEL|MATINV|RHOEOS|ELDENS|PFNI|ENTENE|IRC|LINEQS|EXPO|QUIT|BPOPE|BPOPC|BPOPT|SGMER1|CEH12|YLINTP|PFSPEC|BHEZ|BHE|COLHE|COMPT0|CION|BRTE|LEVGRP|LEVSOL|REFLEV|BHED|OPFRAC|PFCNO|TRMDER|CONVEC|EMAT|CROSS|BREZ|SABOLF|SETTRM|PFHEAV|HCTION|CHEAVJ|MATCON|COLIS|CSPEC|BPOPF|MOLEQ|STATE|TRMDRT|MPARTF|BUTLER|PARTF|BPOP|RATMAT|DWNFR1|BRE|SZIRC|CHEAV",False,src/tlusty/math/solvers/matgen.rs,done
matinv.f,MATINV,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/solvers/matinv.rs,done
meanop.f,MEANOP,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/opacity/meanop.rs,done
meanopt.f,MEANOPT,SUBROUTINE,False,"BASICS|MODELQ","OPCTAB","ATOMIC|MODELQ|eospar|BASICS|RAYSCT","RAYLEIGH|OPCTAB",False,src/tlusty/math/opacity/meanopt.rs,done
minv3.f,MINV3,SUBROUTINE,True,"","","","",False,src/tlusty/math/solvers/minv3.rs,done
moleq.f,MOLEQ,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|hmolab|terden|COMFH1|moldat|entrop|eospar|ioniz2|adchar","RUSSEL|MPARTF","terden|MODELQ|hmolab|COMFH1|moldat|ATOMIC|entrop|eospar|BASICS|ioniz2|adchar","RUSSEL|MPARTF",True,src/tlusty/math/eos/moleq.rs,done
mpartf.f,MPARTF,SUBROUTINE,False,"moldat","","moldat","",True,src/tlusty/math/partition/mpartf.rs,done
newdm.f,NEWDM,SUBROUTINE,False,"BASICS|MODELQ|FACTRS|PRSAUX|FLXAUX","TEMPER|INTERP|HESOLV","irwint|tdedge|POPSTR|pfoptb|eospar|tdflag|FACTRS|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|ITERAT|BASICS|FLXAUX|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|adchar|ATOMIC|ODFPAR|ioniz2","PRSENT|TEMPER|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|QUARTC|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|TLOCAL|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|INTERP|RHONEN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|HESOLV|H2MINUS|PROFSP|DWNFR1|MEANOP",True,src/tlusty/math/utils/newdm.rs,done
newdmt.f,NEWDMT,SUBROUTINE,False,"BASICS|MODELQ|FACTRS|PRSAUX|FLXAUX","GRIDP|TEMPER|INTERP|HESOLV","irwint|tdedge|POPSTR|pfoptb|eospar|tdflag|FACTRS|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|ITERAT|BASICS|FLXAUX|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|adchar|ATOMIC|ODFPAR|ioniz2","PRSENT|TEMPER|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|QUARTC|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|TLOCAL|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|INTERP|RHONEN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|GRIDP|RATMAT|HESOLV|H2MINUS|PROFSP|DWNFR1|MEANOP",True,src/tlusty/math/utils/newdmt.rs,done
newpop.f,NEWPOP,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","","ITERAT|ATOMIC|MODELQ|BASICS","",True,src/tlusty/math/population/newpop.rs,done
nstout.f,NSTOUT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR","QUIT","ITERAT|ATOMIC|MODELQ|BASICS|ODFPAR|ALIPAR","QUIT",True,src/tlusty/io/nstout.rs,done
nstpar.f,NSTPAR,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|irwint|deridt|freqcl|imucnn|temlim|adiaba|moldat|quasun|ichndm|ipricr|derdif|ifpzpa|hediff|icnrsp|FLXAUX","GETLAL|QUIT|GETWRD","callarda|irwint|deridt|temlim|imucnn|adiaba|moldat|quasun|ipricr|callardb|icnrsp|ALIPAR|MODELQ|freqcl|callardg|calphatd|ichndm|derdif|ITERAT|ifpzpa|ATOMIC|hediff|callardc|BASICS|ODFPAR|FLXAUX","GETWRD|GETLAL|QUIT",True,src/tlusty/io/nstpar.rs,done
odf1.f,ODF1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","SIGK|DIVSTR|ODFHST","ATOMIC|MODELQ|ODFPAR|BASICS|TOPB","SBFHE1|SPSIGK|REIMAN|HIDALG|QUIT|VERN18|SGHE12|CKOEST|HEPHOT|VERN16|VERN20|ODFHST|VERNER|TOPBAS|DIVSTR|YLINTP|SBFHMI|VERN26|CARBON|GAUNT|OPDATA|SIGK",True,src/tlusty/math/odf/odf1.rs,done
odffr.f,ODFFR,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","QUIT","ODFPAR|ATOMIC|MODELQ|BASICS","QUIT",False,src/tlusty/math/odf/odffr.rs,done
odfhst.f,ODFHST,SUBROUTINE,False,"BASICS|MODELQ|ODFPAR","","ODFPAR|MODELQ|BASICS","",False,src/tlusty/math/odf/odfhst.rs,done
odfhyd.f,ODFHYD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","INDEXX|DIVSTR|ODFHST","ATOMIC|MODELQ|ODFPAR|BASICS","INDEXX|DIVSTR|ODFHST",False,src/tlusty/math/odf/odfhyd.rs,done
odfhys.f,ODFHYS,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","IJALIS|STARK0|ODFFR","ATOMIC|MODELQ|ODFPAR|BASICS","STARK0|QUIT|ODFFR|IJALIS",False,src/tlusty/math/odf/odfhys.rs,done
odfmer.f,ODFMER,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","ODFHYD","MODELQ|ATOMIC|ODFPAR|BASICS","ODFHYD|INDEXX|DIVSTR|ODFHST",False,src/tlusty/math/odf/odfmer.rs,done
odfset.f,ODFSET,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|STFCR","QUIT|IJALIS","STFCR|ATOMIC|MODELQ|ODFPAR|BASICS","QUIT|IJALIS",True,src/tlusty/io/odfset.rs,done
opacf0.f,OPACF0,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|hmolab","WNSTOR|GFREE0|SFFHMI|FFCROS|DWNFR0|OPADD|OPACT1|CROSS|CROSSD|LINPRO|DWNFR1|SGMER1|SABOLF","irwint|RAYSCT|moldat|quasun|PFSTDS|pfoptb|eospar|ALIPAR|MODELQ|hmolab|ATOMIC|ODFPAR|BASICS","SFFHMI|OPFRAC|CIA_H2H|PFCNO|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|SABOLF|WNSTOR|GFREE0|DIVSTR|PFHEAV|DOPGAM|PFNI|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|MPARTF|PFSPEC|INTLEM|DWNFR0|OPADD|WN|GAMSP|LOCATE|OPCTAB|PARTF|H2MINUS|PROFSP|DWNFR1",False,src/tlusty/math/continuum/opacf0.rs,done
opacf1.f,OPACF1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|hmolab|ipricr","SFFHMI|FFCROS|QUASIM|GHYDOP|LYMLIN|OPADD|PRD|OPACT1|CROSS|CROSSD|GFREE1|DWNFR1|SGMER1","callarda|RAYSCT|quasun|ipricr|callardb|eospar|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|intcfg","SFFHMI|QUASIM|STARKA|CIA_H2H|LYMLIN|CROSSD|CROSS|ALLARD|RAYLEIGH|CIA_HHE|GFREE1|SGMER1|STARK0|YLINTP|FFCROS|DIVSTR|CIA_H2H2|GHYDOP|DOPGAM|OPADD|GAMSP|LOCATE|OPCTAB|PRD|OPACT1|H2MINUS|GAMI|DWNFR1|ALLARDT|CIA_H2HE",True,src/tlusty/math/continuum/opacf1.rs,done
opacfa.f,OPACFA,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|COOLCO","SFFHMI|FFCROS|OPADD|PRD|CROSSD|CROSS|DWNFR1|SGMER1","MODELQ|COOLCO|ITERAT|ATOMIC|eospar|ODFPAR|BASICS|ALIPAR","SFFHMI|YLINTP|FFCROS|CIA_H2H2|CIA_H2H|DOPGAM|OPADD|GAMSP|LOCATE|PRD|CROSSD|CROSS|H2MINUS|GAMI|DWNFR1|CIA_HHE|SGMER1|CIA_H2HE",False,src/tlusty/math/continuum/opacfa.rs,done
opacfd.f,OPACFD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT|rhoder|hmolab|dsctva","SFFHMI|FFCROS|GFREED|QUASIM|LYMLIN|OPADD|OPCTAB|PRD|CROSSD|CROSS|OPACTD|DWNFR1|SGMER1","callarda|RAYSCT|ARRAY1|quasun|callardb|eospar|ALIPAR|rhoder|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|dsctva|ODFPAR|BASICS","SFFHMI|QUASIM|STARKA|CIA_H2H|LYMLIN|CROSSD|CROSS|ALLARD|OPACTD|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|GFREED|DIVSTR|CIA_H2H2|DOPGAM|OPADD|GAMSP|OPCTAB|LOCATE|PRD|H2MINUS|GAMI|DWNFR1|ALLARDT|CIA_H2HE",True,src/tlusty/math/continuum/opacfd.rs,done
opacfl.f,OPACFL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR","SFFHMI|FFCROS|OPADD|CROSSD|CROSS|DWNFR1|SGMER1","MODELQ|ATOMIC|eospar|ODFPAR|BASICS|ALIPAR","SFFHMI|YLINTP|FFCROS|CIA_H2H2|CIA_H2H|OPADD|LOCATE|CROSSD|CROSS|H2MINUS|DWNFR1|CIA_HHE|SGMER1|CIA_H2HE",False,src/tlusty/math/continuum/opacfl.rs,done
opact1.f,OPACT1,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|hmolab","OPCTAB","MODELQ|hmolab|RAYSCT|ATOMIC|eospar|BASICS|ALIPAR","RAYLEIGH|OPCTAB",False,src/tlusty/math/continuum/opact1.rs,done
opactd.f,OPACTD,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ARRAY1|ITERAT|rhoder|hmolab|dsctva","OPCTAB","rhoder|MODELQ|hmolab|RAYSCT|ARRAY1|ITERAT|ATOMIC|eospar|dsctva|BASICS|ALIPAR","RAYLEIGH|OPCTAB",False,src/tlusty/math/continuum/opactd.rs,done
opactr.f,OPACTR,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ATOMIC|grdpra|hmolab|dsctva","LEVSOL|OPAINI|WNSTOR|STEQEQ|PGSET|ELDENS|TDPINI|OPACF1|RATMAL|SABOLF","callarda|irwint|POPSTR|pfoptb|eospar|PPAPAR|ALIPAR|MODELQ|hmolab|calphatd|rybpgs|ITERAT|BASICS|intcfg|terden|COMFH1|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|entrop|adchar|grdpra|callardg|ATOMIC|callardc|dsctva|ODFPAR|ioniz2","SFFHMI|CIA_H2H|PFFE|UBETA|OPACF1|LINPRO|INTHYD|RUSSEL|WNSTOR|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|GAMI|QUASIM|LINEQS|OPAINI|SGMER0|TRIDAG|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|LOCATE|OPCTAB|PRD|RATMAL|LEVGRP|LEVSOL|REFLEV|PGSET|OPFRAC|PFCNO|YINT|CROSSD|CROSS|ALLARD|INTXEN|GFREE1|SABOLF|DIVSTR|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|LYMLIN|TDPINI|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|GHYDOP|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|ALLARDT",False,src/tlusty/math/continuum/opactr.rs,done
opadd.f,OPADD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|eospar","SFFHMI|CIA_H2H2|CIA_H2H|CROSS|H2MINUS|CIA_HHE|CIA_H2HE","ATOMIC|MODELQ|eospar|BASICS","SFFHMI|YLINTP|CIA_H2H2|CIA_H2H|LOCATE|CROSS|H2MINUS|CIA_HHE|CIA_H2HE",False,src/tlusty/math/continuum/opadd.rs,done
opadd0.f,OPADD0,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","QUIT","ATOMIC|MODELQ|BASICS","QUIT",False,src/tlusty/math/continuum/opadd0.rs,done
opahst.f,OPAHST,SUBROUTINE,False,"BASICS|ODFPAR","STARK0","ODFPAR|BASICS","STARK0",True,src/tlusty/math/continuum/opahst.rs,done
opaini.f,OPAINI,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR","REFLEV|WNSTOR|SGMER0|DWNFR0|LINPRO|LEVGRP|SABOLF","irwint|MODELQ|moldat|quasun|PFSTDS|ITERAT|ATOMIC|pfoptb|ODFPAR|BASICS|ALIPAR","REFLEV|VOIGT|OPFRAC|SGMER0|PFCNO|STARKA|PFFE|UBETA|YINT|LINPRO|INTHYD|INTXEN|SABOLF|STARK0|WNSTOR|DIVSTR|MPARTF|PFSPEC|PFHEAV|DOPGAM|DWNFR0|INTLEM|WN|GAMSP|PARTF|PFNI|LAGRAN|PROFSP|LEVGRP",False,src/tlusty/math/continuum/opaini.rs,done
opctab.f,OPCTAB,SUBROUTINE,False,"BASICS|MODELQ","RAYLEIGH","ATOMIC|MODELQ|eospar|BASICS|RAYSCT","RAYLEIGH",False,src/tlusty/math/continuum/opctab.rs,done
opdata.f,OPDATA,SUBROUTINE,False,"TOPB","","TOPB","",True,src/tlusty/math/continuum/opdata.rs,done
opfrac.f,OPFRAC,SUBROUTINE,False,"pfoptb","","pfoptb","",True,src/tlusty/math/continuum/opfrac.rs,done
osccor.f,OSCCOR,SUBROUTINE,False,"BASICS|MODELQ|ITERAT","","ITERAT|MODELQ|BASICS","",True,src/tlusty/math/temperature/osccor.rs,done
outpri.f,OUTPRI,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|grdpra","LEVSOL|WNSTOR|OPACF1|RATMAL|SABOLF|ELDENC","callarda|irwint|pfoptb|eospar|eletab|ALIPAR|MODELQ|hmolab|calphatd|ITERAT|BASICS|intcfg|terden|RAYSCT|COMFH1|ARRAY1|moldat|quasun|ipricr|callardb|PFSTDS|entrop|adchar|grdpra|callardg|ATOMIC|callardc|ODFPAR|ioniz2","LEVSOL|SFFHMI|OPFRAC|CIA_H2H|PFCNO|PFFE|OPACF1|CROSSD|CROSS|ALLARD|RUSSEL|GFREE1|SABOLF|ELDENC|WNSTOR|DIVSTR|PFHEAV|DOPGAM|ELDENS|PFNI|OPACT1|ENTENE|GAMI|QUASIM|LINEQS|CIA_H2HE|STARKA|LYMLIN|RHONEN|MOLEQ|STATE|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|MPARTF|GHYDOP|PFSPEC|WN|OPADD|GAMSP|LOCATE|OPCTAB|PRD|PARTF|RATMAL|H2MINUS|DWNFR1|ALLARDT",True,src/tlusty/io/outpri.rs,done
output.f,OUTPUT,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",True,src/tlusty/math/io/output.rs,done
partf.f,PARTF,SUBROUTINE,False,"BASICS|irwint|PFSTDS","MPARTF|PFSPEC|OPFRAC|PFCNO|PFHEAV|PFFE|PFNI","irwint|pfoptb|BASICS|moldat|PFSTDS","MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PFNI",False,src/tlusty/math/partition/partf.rs,done
pfcno.f,PFCNO,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/partition/pfcno.rs,done
pffe.f,PFFE,SUBROUTINE,True,"","","","",False,src/tlusty/math/partition/pffe.rs,done
pfheav.f,PFHEAV,SUBROUTINE,False,"","","","",True,src/tlusty/math/partition/pfheav.rs,done
pfni.f,PFNI,SUBROUTINE,True,"","","","",False,src/tlusty/math/partition/pfni.rs,done
pfspec.f,PFSPEC,SUBROUTINE,True,"","","","",False,src/tlusty/math/partition/pfspec.rs,done
pgset.f,PGSET,SUBROUTINE,False,"BASICS|ITERAT|MODELQ|grdpra|rybpgs","TRIDAG","ITERAT|grdpra|MODELQ|BASICS|rybpgs","TRIDAG",True,src/tlusty/math/utils/pgset.rs,done
prchan.f,PRCHAN,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","","ITERAT|ATOMIC|MODELQ|BASICS","",True,src/tlusty/math/io/prchan.rs,done
prd.f,PRD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","DOPGAM|GAMI","ITERAT|ATOMIC|MODELQ|BASICS","DOPGAM|GAMI|GAMSP",False,src/tlusty/math/opacity/prd.rs,done
prdini.f,PRDINI,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/opacity/prdini.rs,done
princ.f,PRINC,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR","OPACF1|DWNFR|CROSS|LINPRO|SABOLF","callarda|irwint|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|pfoptb|eospar|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|intcfg","SFFHMI|OPFRAC|CIA_H2H|PFCNO|PFFE|UBETA|OPACF1|CROSSD|CROSS|YINT|LINPRO|ALLARD|INTHYD|INTXEN|GFREE1|SABOLF|DIVSTR|PFHEAV|DOPGAM|PFNI|LAGRAN|OPACT1|GAMI|QUASIM|CIA_H2HE|VOIGT|STARKA|LYMLIN|DWNFR|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|MPARTF|GHYDOP|PFSPEC|INTLEM|OPADD|GAMSP|LOCATE|OPCTAB|PRD|PARTF|H2MINUS|PROFSP|DWNFR1|ALLARDT",True,src/tlusty/math/io/princ.rs,done
prnt.f,PRNT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","SABOLF","irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS","MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|SABOLF",True,src/tlusty/math/io/prnt.rs,done
profil.f,PROFIL,FUNCTION,False,"BASICS|ATOMIC|MODELQ|quasun","STARK0|VOIGT|DIVSTR|STARKA|PROFSP","irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|BASICS","STARK0|VOIGT|DIVSTR|MPARTF|PFSPEC|OPFRAC|PFHEAV|STARKA|PFCNO|PFFE|UBETA|PARTF|PFNI|LAGRAN|PROFSP|SABOLF",False,src/tlusty/math/opacity/profil.rs,done
profsp.f,PROFSP,FUNCTION,False,"BASICS|ATOMIC|MODELQ","VOIGT|SABOLF|UBETA","irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS","VOIGT|MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|UBETA|PARTF|PFNI|LAGRAN|SABOLF",False,src/tlusty/math/opacity/profsp.rs,done
prsent.f,PRSENT,SUBROUTINE,False,"TABLTD|tdedge|THERM|tdflag","","TABLTD|tdedge|THERM|tdflag","",True,src/tlusty/math/io/prsent.rs,done
psolve.f,PSOLVE,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/solvers/psolve.rs,done
pzert.f,PZERT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/io/pzert.rs,done
pzeval.f,PZEVAL,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|icnrsp","CONOUT|CONREF","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|imucnn|RAYSCT|COMFH1|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|icnrsp|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON","PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|OPADD|WN|OPCTAB|LOCATE|CONREF|OPACF0|LEVSOL|REFLEV|CONVC1|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|TDPINI|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP",True,src/tlusty/math/io/pzeval.rs,done
pzevld.f,PZEVLD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR|ARRAY1|DEPTDR|grdpra|ifpzpa|PRSAUX","","grdpra|MODELQ|DEPTDR|PRSAUX|ARRAY1|ifpzpa|ATOMIC|BASICS|ALIPAR","",False,src/tlusty/math/io/pzevld.rs,done
quartc.f,QUARTC,SUBROUTINE,False,"","","","",True,src/tlusty/math/solvers/quartc.rs,done
quasim.f,QUASIM,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|quasun","ALLARD","callarda|MODELQ|callardg|calphatd|quasun|callardb|ATOMIC|callardc|BASICS","ALLARDT|ALLARD",False,src/tlusty/math/opacity/quasim.rs,done
quit.f,QUIT,SUBROUTINE,False,"","","","",True,src/tlusty/math/io/quit.rs,done
radpre.f,RADPRE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR","INDEXX|QUIT|RTEFR1|OPACF1","callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|INDEXX|RTEFR1|STARKA|QUIT|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/radiative/radpre.rs,done
radtot.f,RADTOT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT|OPTDPT|TOTJHK|SURFEX","OPAINI|OPACF1|RTEFR1|TDPINI","callarda|irwint|AUXRTE|RAYSCT|TOTJHK|moldat|quasun|ipricr|callardb|PFSTDS|pfoptb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","REFLEV|SFFHMI|OPFRAC|PFCNO|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|YINT|CROSSD|CROSS|LINPRO|INTHYD|ALLARD|INTXEN|GFREE1|SABOLF|MATINV|WNSTOR|DIVSTR|GFREE0|PFHEAV|DOPGAM|RTEDF2|PFNI|LAGRAN|OPACT1|GAMI|QUASIM|CIA_H2HE|OPAINI|VOIGT|RTEFR1|SGMER0|STARKA|LYMLIN|TDPINI|RAYLEIGH|CIA_HHE|SGMER1|RTEDF1|STARK0|MPARTF|YLINTP|PFSPEC|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GHYDOP|RTECF0|WN|OPADD|GAMSP|PARTF|LOCATE|OPCTAB|PRD|DWNFR1|H2MINUS|PROFSP|LEVGRP|ALLARDT|RTESOL|RTECF1",False,src/tlusty/math/radiative/radtot.rs,done
raph.f,RAPH,FUNCTION,True,"","","","",False,src/tlusty/math/solvers/raph.rs,done
rates1.f,RATES1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT","ROSSTD|CROSS|RTEFR1|OPACF1","callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",False,src/tlusty/math/rates/rates1.rs,done
ratmal.f,RATMAL,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/rates/ratmal.rs,done
ratmat.f,RATMAT,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","REFLEV","ITERAT|ATOMIC|MODELQ|BASICS","REFLEV",False,src/tlusty/math/rates/ratmat.rs,done
ratsp1.f,RATSP1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT","ROSSTD|CROSS|RTEFR1|OPACF1","callarda|AUXRTE|RAYSCT|ARRAY1|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/rates/ratsp1.rs,done
rayini.f,RAYINI,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC","RAYLEIGH|RAYSET","MODELQ|RAYSCT|ATOMIC|eospar|BASICS","RAYLEIGH|RAYSET",True,src/tlusty/io/rayini.rs,done
rayleigh.f,RAYLEIGH,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|eospar|RAYSCT","","ATOMIC|MODELQ|eospar|RAYSCT|BASICS","",False,src/tlusty/math/opacity/rayleigh.rs,done
rayset.f,RAYSET,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/opacity/rayset.rs,done
rdata.f,RDATA,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|STRPAR|INUNIT|imodlc","LEMINI|DOPGAM|XENINI|QUIT|RDATAX|LINSET","irwint|MODELQ|imodlc|moldat|quasun|PFSTDS|ITERAT|ATOMIC|pfoptb|BASICS|ODFPAR|STRPAR|INUNIT|ALIPAR","VOIGT|LEMINI|OPFRAC|PFCNO|XENINI|STARKA|QUIT|BKHSGO|PFFE|UBETA|PROFIL|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|DOPGAM|RDATAX|LINSET|GAMSP|PARTF|PFNI|LAGRAN|IJALIS|PROFSP",True,src/tlusty/math/io/rdata.rs,done
rdatax.f,RDATAX,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","BKHSGO","ATOMIC|MODELQ|BASICS","BKHSGO",True,src/tlusty/math/io/rdatax.rs,done
readbf.f,READBF,SUBROUTINE,False,"BASICS","","BASICS","",True,src/tlusty/math/io/readbf.rs,done
rechck.f,RECHCK,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","RTEFR1|OPACF1","callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/io/rechck.rs,done
reflev.f,REFLEV,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","","ITERAT|ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/opacity/reflev.rs,done
reiman.f,REIMAN,FUNCTION,True,"","","","",False,src/tlusty/math/opacity/reiman.rs,done
resolv.f,RESOLV,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ALIPAR|ARRAY1|icnrsp","HESOL6|RAYSET|PRINC|NEWPOP|OPACF1|LUCY|ALISK2|ALIST1|TAUFR1|LINSEL|ROSSTD|CHCKSE|RTECMU|RTECOM|TIMING|PZEVLD|DMEVAL|COOLRT|ALIST2|OUTPRI|OUTPUT|RTEINT|OPAINI|RATSP1|PZERT|RTEFR1|RECHCK|ACCELP|RATES1|PZEVAL|ELCOR|STEQEQ|RYBHEQ|PRD|CONREF|CONOUT|INILAM|RADPRE","DEPTDR|tdedge|POPSTR|pfoptb|tdflag|POPULS|PPAPAR|eletab|rhoder|MODELQ|THERM|calphatd|CC|derdif|rybpgs|BASICS|intcfg|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|grdpra|SURFEX|ADCHAR|ODFPAR|ioniz2|dsctva|CUBCON|callarda|irwint|adiaba|eospar|EXTINT|ALIPAR|hmolab|ITERAT|CTIon|OPTDPT|PRSAUX|COOLCO|COMFH1|imucnn|ARRAY1|moldat|CTRTEMP|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|callardg|ifpzpa|ATOMIC|callardc|comgfs","PRSENT|SFFHMI|ANGSET|CIA_H2H|COLLHE|PFFE|UBETA|EXPINX|EINT|LINPRO|ALISK2|RHOEOS|RTECOM|DOPGAM|ELDENS|RTEDF2|ENTENE|IRC|LINEQS|OPAINI|ODFMER|RTEFR1|SGMER0|GAULEG|TRIDAG|RTEDF1|SGMER1|CEH12|TEMCOR|COLHE|OPADD|WN|OPCTAB|PRD|CION|CONREF|OPACF0|REFLEV|HESOL6|PGSET|RAYSET|PFCNO|OPACFA|YINT|LUCY|ALIST1|TAUFR1|INTXEN|GFREE1|SABOLF|ELDENC|PZEVLD|LAGRAN|DMEVAL|OPACT1|RTEINT|CIA_H2HE|RATSP1|PZERT|LYMLIN|TDPINI|VISINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|OPACFD|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RADPRE|CHEAV|RTESOL|PRINC|RTEFE2|OPACF1|ODFHYD|INTHYD|COLH|OPACTD|RUSSEL|ODFHST|MATINV|WNSTOR|GFREE0|ALIFR3|TIMING|PFNI|ALIFR1|GAMI|ALIST2|QUASIM|OUTPUT|INDEXX|EXPO|RECHCK|OSCCOR|ACCELP|QUIT|CIA_HHE|COMSET|YLINTP|CONCOR|PFSPEC|GFREED|LOCATE|RATMAL|LEVGRP|INILAM|LEVSOL|CONVC1|OPFRAC|TRMDER|CONVEC|NEWPOP|ALIFRK|CROSSD|CROSS|ALLARD|RTECMC|LINSEL|ROSSTD|DIVSTR|CHCKSE|RTECMU|PFHEAV|SETTRM|DIELRC|COOLRT|HCTION|OUTPRI|OPACFL|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|RHONEN|DWNFR|RATES1|MOLEQ|STATE|RAYLEIGH|PZEVAL|ELCOR|RYBHEQ|FFCROS|CIA_H2H2|RTECF0|INTLEM|BUTLER|RATMAT|DIETOT|SZIRC|RTECF1",True,src/tlusty/io/resolv.rs,done
rhoeos.f,RHOEOS,FUNCTION,False,"BASICS|MODELQ","PRSENT|SETTRM","MODELQ|tdedge|THERM|TABLTD|BASICS|tdflag","PRSENT|SETTRM",False,src/tlusty/math/eos/rhoeos.rs,done
rhonen.f,RHONEN,SUBROUTINE,False,"BASICS|MODELQ","ELDENS","irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ATOMIC|BASICS|ioniz2","MPARTF|OPFRAC|PFSPEC|ELDENS|PFHEAV|PFCNO|PFFE|PARTF|PFNI|MOLEQ|ENTENE|STATE|RUSSEL|LINEQS",False,src/tlusty/math/eos/rhonen.rs,done
rhsgen.f,RHSGEN,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|CUBCON","MATINV|CONVEC|COMPT0|RATMAT|STATE|LEVGRP|SABOLF","irwint|terden|tdedge|COMFH1|adiaba|ARRAY1|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|auxcbc|adchar|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|ATOMIC|BASICS|ioniz2|CUBCON","REFLEV|PRSENT|OPFRAC|PFCNO|TRMDER|CONVEC|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|TRMDRT|MATINV|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|COMPT0|RATMAT|PARTF|PFNI|ENTENE|LEVGRP|LINEQS",False,src/tlusty/math/solvers/rhsgen.rs,done
rossop.f,ROSSOP,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ALIPAR","WNSTOR|STEQEQ|MEANOPT|RHOEOS|ELDENS|MEANOP|EXPINT|OPACF0","irwint|terden|tdedge|COMFH1|RAYSCT|moldat|quasun|PFSTDS|POPSTR|entrop|eospar|pfoptb|TABLTD|tdflag|PPAPAR|adchar|ALIPAR|MODELQ|hmolab|THERM|ITERAT|ATOMIC|BASICS|ioniz2|ODFPAR","LEVSOL|REFLEV|PRSENT|SFFHMI|OPFRAC|PFCNO|CIA_H2H|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|RUSSEL|EXPINT|SABOLF|WNSTOR|RHOEOS|GFREE0|SETTRM|DIVSTR|ELDENS|PFHEAV|DOPGAM|PFNI|LAGRAN|ENTENE|OPACT1|LINEQS|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|CIA_HHE|SGMER1|STARK0|STEQEQ|MEANOPT|MPARTF|PFSPEC|YLINTP|FFCROS|CIA_H2H2|INTLEM|DWNFR0|WN|OPADD|GAMSP|PARTF|RATMAT|OPCTAB|LOCATE|H2MINUS|PROFSP|DWNFR1|MEANOP|OPACF0",False,src/tlusty/math/temperature/rossop.rs,done
rosstd.f,ROSSTD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|ALIPAR","","ITERAT|ATOMIC|MODELQ|BASICS|ALIPAR","",True,src/tlusty/math/temperature/rosstd.rs,done
rte_sc.f,RTE_SC,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/radiative/rte_sc.rs,done
rteang.f,RTEANG,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|EXTINT|SURFEX","GAULEG","MODELQ|BASICS|SURFEX|EXTINT|ALIPAR","GAULEG",False,src/tlusty/math/radiative/rteang.rs,done
rtecf0.f,RTECF0,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT|auxcbc|AUXRTE","","ITERAT|MODELQ|AUXRTE|BASICS|OPTDPT|auxcbc|ALIPAR","",False,src/tlusty/math/radiative/rtecf0.rs,done
rtecf1.f,RTECF1,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|AUXRTE|SURFEX|OPTDPT|EXTINT|comgfs","RTEFE2|RTESOL|RTECF0","MODELQ|AUXRTE|SURFEX|ITERAT|BASICS|OPTDPT|EXTINT|auxcbc|comgfs|ALIPAR","RTEFE2|RTESOL|RTECF0",True,src/tlusty/math/radiative/rtecf1.rs,done
rtecmc.f,RTECMC,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|AUXRTE|comgfs","MATINV|RTECF0|OPACF1","callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|auxcbc|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg|comgfs","SFFHMI|CIA_H2H|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT",False,src/tlusty/math/radiative/rtecmc.rs,done
rtecmu.f,RTECMU,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT|AUXRTE","RTECF0|GAULEG|RTESOL|OPACF1","callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|auxcbc|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg","SFFHMI|CIA_H2H|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|GAULEG|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL",True,src/tlusty/math/radiative/rtecmu.rs,done
rtecom.f,RTECOM,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT|AUXRTE|comgfs","RTECF0|RTECF1|RTECMC|OPACF1","callarda|eospar|EXTINT|ALIPAR|MODELQ|hmolab|calphatd|ITERAT|BASICS|OPTDPT|intcfg|AUXRTE|RAYSCT|quasun|ipricr|callardb|auxcbc|callardg|SURFEX|ATOMIC|callardc|ODFPAR|comgfs","SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|RTECMC|GFREE1|MATINV|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1",False,src/tlusty/math/radiative/rtecom.rs,done
rtedf1.f,RTEDF1,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|OPTDPT","","OPTDPT|MODELQ|BASICS|ALIPAR","",False,src/tlusty/math/radiative/rtedf1.rs,done
rtedf2.f,RTEDF2,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR","","MODELQ|BASICS|ALIPAR","",False,src/tlusty/math/radiative/rtedf2.rs,done
rtefe2.f,RTEFE2,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/radiative/rtefe2.rs,done
rtefr1.f,RTEFR1,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT","MATINV|RTEDF2|RTEDF1|RTESOL|RTECF1","MODELQ|AUXRTE|SURFEX|ITERAT|BASICS|OPTDPT|EXTINT|auxcbc|comgfs|ALIPAR","MATINV|RTECF0|RTEDF2|RTEFE2|RTEDF1|RTESOL|RTECF1",True,src/tlusty/math/radiative/rtefr1.rs,done
rteint.f,RTEINT,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT","MATINV|OPACF1","callarda|RAYSCT|quasun|ipricr|callardb|eospar|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg","SFFHMI|CIA_H2H|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT",True,src/tlusty/math/radiative/rteint.rs,done
rtesol.f,RTESOL,SUBROUTINE,True,"BASICS","","BASICS","",False,src/tlusty/math/radiative/rtesol.rs,done
russel.f,RUSSEL,SUBROUTINE,False,"BASICS|MODELQ|COMFH1","MPARTF","moldat|MODELQ|COMFH1|BASICS","MPARTF",True,src/tlusty/math/eos/russel.rs,done
rybchn.f,RYBCHN,SUBROUTINE,False,"BASICS|ITERAT|MODELQ|ALIPAR|ARRAY1|grdpra|rybpgs","PGSET|ELDENS","irwint|terden|COMFH1|ARRAY1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|ALIPAR|grdpra|MODELQ|hmolab|rybpgs|ITERAT|ATOMIC|BASICS|ioniz2","PGSET|OPFRAC|PFCNO|PFFE|MOLEQ|STATE|TRIDAG|RUSSEL|MPARTF|PFSPEC|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS",True,src/tlusty/math/solvers/rybchn.rs,done
rybene.f,RYBENE,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ARRAY1|RYBMTX|deridt|CUBCON","CONVEC","deridt|irwint|terden|tdedge|COMFH1|adiaba|ARRAY1|moldat|PFSTDS|RYBMTX|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON","PRSENT|OPFRAC|PFCNO|TRMDER|CONVEC|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS",False,src/tlusty/math/solvers/rybene.rs,done
rybheq.f,RYBHEQ,SUBROUTINE,False,"BASICS|MODELQ|grdpra|rybpgs","OPAINI|WNSTOR|STEQEQ|PGSET|RTEFR1|ELDENS|OPACF1","callarda|irwint|POPSTR|pfoptb|eospar|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|calphatd|rybpgs|ITERAT|BASICS|OPTDPT|intcfg|terden|AUXRTE|COMFH1|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|entrop|auxcbc|adchar|grdpra|callardg|SURFEX|ATOMIC|callardc|ODFPAR|ioniz2|comgfs","SFFHMI|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|ELDENS|DOPGAM|RTEDF2|PFNI|ENTENE|GAMI|QUASIM|LINEQS|OPAINI|RTEFR1|SGMER0|TRIDAG|RTEDF1|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|LOCATE|OPCTAB|PRD|LEVGRP|REFLEV|LEVSOL|PGSET|OPFRAC|PFCNO|YINT|CROSSD|CROSS|ALLARD|INTXEN|GFREE1|SABOLF|DIVSTR|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|LYMLIN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|RTECF0|INTLEM|DWNFR0|GHYDOP|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/solvers/rybheq.rs,done
rybmat.f,RYBMAT,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ARRAY1|RYBMTX|dsctva","","RYBMTX|MODELQ|dsctva|BASICS|ARRAY1|ALIPAR","",False,src/tlusty/math/solvers/rybmat.rs,done
rybsol.f,RYBSOL,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|ALIPAR|ARRAY1|ITERAT|RYBMTX|imodlc","SETDRT|STEQEQ|ROSSTD|RTEFR1|OPACTR|RYBCHN|RYBENE|ALIFR1|RYBMAT|LEVSET|TRIDAG|LINEQS","callarda|irwint|deridt|tdedge|imodlc|adiaba|RYBMTX|POPSTR|pfoptb|eospar|tdflag|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|calphatd|CC|CUBCON|derdif|rybpgs|ITERAT|BASICS|OPTDPT|intcfg|terden|AUXRTE|COMFH1|RAYSCT|ARRAY1|moldat|quasun|ipricr|callardb|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|grdpra|RHODER|callardg|SURFEX|ATOMIC|callardc|dsctva|ODFPAR|ioniz2|comgfs","PRSENT|SFFHMI|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|RTEDF2|DOPGAM|ALIFR3|PFNI|ALIFR1|ENTENE|GAMI|QUASIM|LINEQS|OPAINI|RTEFR1|SGMER0|QUIT|RYBMAT|TRIDAG|RTEDF1|CIA_HHE|SGMER1|YLINTP|PFSPEC|RYBENE|WN|OPADD|LOCATE|OPCTAB|PRD|RATMAL|LEVGRP|LEVSET|LEVSOL|REFLEV|OPFRAC|PGSET|OPACTR|PFCNO|TRMDER|CONVEC|YINT|CROSSD|CROSS|ALLARD|INTXEN|GFREE1|SABOLF|ROSSTD|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|SETDRT|VOIGT|RYBCHN|STARKA|LYMLIN|TDPINI|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|RTECF0|GHYDOP|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|ALLARDT|RTESOL|RTECF1",True,src/tlusty/math/solvers/rybsol.rs,done
sabolf.f,SABOLF,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","PARTF","irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS","MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PARTF|PFNI",False,src/tlusty/math/utils/sabolf.rs,done
sbfch.f,SBFCH,FUNCTION,True,"","","","",False,src/tlusty/math/hydrogen/sbfch.rs,done
sbfhe1.f,SBFHE1,FUNCTION,False,"BASICS|ATOMIC","CKOEST|QUIT|HEPHOT","ATOMIC|BASICS","CKOEST|QUIT|HEPHOT",True,src/tlusty/math/hydrogen/sbfhe1.rs,done
sbfhmi.f,SBFHMI,FUNCTION,True,"","YLINTP","","YLINTP",False,src/tlusty/math/hydrogen/sbfhmi.rs,done
sbfhmi_old.f,SBFHMI_OLD,FUNCTION,True,"","","","",False,src/tlusty/math/hydrogen/sbfhmi_old.rs,done
sbfoh.f,SBFOH,FUNCTION,True,"","","","",False,src/tlusty/math/hydrogen/sbfoh.rs,done
setdrt.f,SETDRT,SUBROUTINE,False,"BASICS|MODELQ|RHODER","RHOEOS","RHODER|MODELQ|tdedge|THERM|TABLTD|BASICS|tdflag","PRSENT|RHOEOS|SETTRM",False,src/tlusty/math/utils/setdrt.rs,done
settrm.f,SETTRM,SUBROUTINE,False,"TABLTD|tdedge|THERM|tdflag","PRSENT","tdedge|THERM|TABLTD|tdflag","PRSENT",True,src/tlusty/io/settrm.rs,done
sffhmi.f,SFFHMI,FUNCTION,True,"","YLINTP","","YLINTP",False,src/tlusty/math/hydrogen/sffhmi.rs,done
sffhmi_add.f,SFFHMI_ADD,FUNCTION,True,"","YLINTP","","YLINTP",False,src/tlusty/math/hydrogen/sffhmi_add.rs,done
sghe12.f,SGHE12,FUNCTION,True,"","","","",False,src/tlusty/math/partition/sghe12.rs,done
sgmer0.f,SGMER0,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/hydrogen/sgmer.rs,done
sgmer1.f,SGMER1,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/hydrogen/sgmer1.rs,done
sgmerd.f,SGMERD,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/hydrogen/sgmer.rs,done
sigave.f,SIGAVE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","QUIT","ODFPAR|ATOMIC|MODELQ|BASICS","QUIT",True,src/tlusty/math/hydrogen/sigave.rs,done
sigk.f,SIGK,FUNCTION,False,"BASICS|ATOMIC","TOPBAS|SPSIGK|YLINTP|SBFHE1|SBFHMI|GAUNT|VERNER","ATOMIC|BASICS|TOPB","SBFHE1|SPSIGK|REIMAN|HIDALG|QUIT|VERN18|SGHE12|CKOEST|HEPHOT|VERN16|VERN20|VERNER|TOPBAS|YLINTP|SBFHMI|VERN26|CARBON|GAUNT|OPDATA",False,src/tlusty/math/hydrogen/sigk.rs,done
sigmar.f,SIGMAR,FUNCTION,False,"BASICS","LAGUER","BASICS","LAGUER",True,src/tlusty/math/hydrogen/sigmar.rs,done
solve.f,SOLVE,SUBROUTINE,False,"BASICS|ITERAT|MODELQ|ARRAY1|ALIPAR|CMATZD","MATINV|WNSTOR|RHSGEN|PRCHAN|MATGEN|IROSET","irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|CMATZD|terden|COMFH1|ARRAY1|moldat|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|SURFEX|COLKUR|LINED|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON","PRSENT|COLLHE|PFFE|BRTEZ|EXPINX|EINT|COLH|IJALI2|RUSSEL|MATINV|WNSTOR|RHOEOS|ELDENS|PFNI|ENTENE|IRC|LINEQS|PRCHAN|RHSGEN|EXPO|INDEXX|QUIT|BPOPE|VOIGTE|BPOPC|BPOPT|SGMER1|INKUL|CEH12|YLINTP|PFSPEC|MATGEN|BHEZ|BHE|COLHE|WN|COMPT0|CION|BRTE|LEVGRP|REFLEV|LEVSOL|BHED|OPFRAC|PFCNO|TRMDER|CONVEC|EMAT|CROSS|BREZ|SABOLF|SETTRM|PFHEAV|HCTION|IROSET|CHEAVJ|MATCON|COLIS|CSPEC|BPOPF|LEVCD|MOLEQ|STATE|TRMDRT|MPARTF|BUTLER|PARTF|RATMAT|BPOP|DWNFR1|BRE|SZIRC|CHEAV",True,src/tlusty/math/solvers/solve.rs,done
solves.f,SOLVES,SUBROUTINE,False,"BASICS|ITERAT|MODELQ|ARRAY1|ALIPAR|CMATZD|STOMAT","MATINV|WNSTOR|RHSGEN|PRCHAN|MATGEN|IROSET","irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|CMATZD|terden|COMFH1|ARRAY1|moldat|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|SURFEX|STOMAT|COLKUR|LINED|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON","PRSENT|COLLHE|PFFE|BRTEZ|EXPINX|EINT|COLH|IJALI2|RUSSEL|MATINV|WNSTOR|RHOEOS|ELDENS|PFNI|ENTENE|IRC|LINEQS|PRCHAN|RHSGEN|EXPO|INDEXX|QUIT|BPOPE|VOIGTE|BPOPC|BPOPT|SGMER1|INKUL|CEH12|YLINTP|PFSPEC|MATGEN|BHEZ|BHE|COLHE|WN|COMPT0|CION|BRTE|LEVGRP|REFLEV|LEVSOL|BHED|OPFRAC|PFCNO|TRMDER|CONVEC|EMAT|CROSS|BREZ|SABOLF|SETTRM|PFHEAV|HCTION|IROSET|CHEAVJ|MATCON|COLIS|CSPEC|BPOPF|LEVCD|MOLEQ|STATE|TRMDRT|MPARTF|BUTLER|PARTF|RATMAT|BPOP|DWNFR1|BRE|SZIRC|CHEAV",True,src/tlusty/math/solvers/solves.rs,done
spsigk.f,SPSIGK,SUBROUTINE,True,"","HIDALG|SGHE12|REIMAN|CARBON","","HIDALG|CARBON|REIMAN|SGHE12",False,src/tlusty/math/hydrogen/spsigk.rs,done
srtfrq.f,SRTFRQ,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","INDEXX|QUIT","ATOMIC|MODELQ|BASICS","INDEXX|QUIT",True,src/tlusty/io/srtfrq.rs,done
stark0.f,STARK0,SUBROUTINE,True,"","","","",False,src/tlusty/math/opacity/stark0.rs,done
starka.f,STARKA,FUNCTION,False,"BASICS|MODELQ","","MODELQ|BASICS","",False,src/tlusty/math/opacity/starka.rs,done
start.f,START,SUBROUTINE,False,"BASICS|hediff","PRDINI|COMSET|INITIA|HEDIF","DEPTDR|tdedge|POPSTR|pfoptb|tdflag|PPAPAR|eletab|STFCR|MODELQ|THERM|CC|calphatd|derdif|BASICS|intcfg|FLXAUX|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|SURFEX|COLKUR|LINED|ichndm|ODFPAR|ioniz2|CUBCON|callarda|irwint|temlim|deridt|imodlc|adiaba|TOTJHK|intcff|eospar|FACTRS|EXTINT|INUNIT|ijflar|ALIPAR|hmolab|freqcl|TOPB|ITERAT|OPTDPT|PRSAUX|imucnn|COMFH1|relcor|moldat|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|abntab|callardg|ifpzpa|hediff|ATOMIC|callardc|STRPAR|comgfs","INPMOD|PRSENT|SBFHE1|ANGSET|SFFHMI|TEMPER|CIA_H2H|PFFE|UBETA|HEDIF|HEPHOT|LINPRO|VERN16|LINSPL|VERN20|IJALI2|EXPINT|ERFCIN|RADTOT|INIFRT|CORRWM|RHOEOS|ELDENS|DOPGAM|RTEDF2|GRCOR|RAYINI|ODFHYS|ENTENE|CHCTAB|OPDATA|LINEQS|GOMINI|OPAINI|REIMAN|RTEFR1|SGMER0|GAULEG|VOIGTE|CKOEST|LTEGR|ODFFR|RTEDF1|SGMER1|WN|OPADD|INPDIS|OPCTAB|NEWDM|PRD|GAUNT|OPACF0|REFLEV|SPSIGK|HESOL6|RAYSET|PFCNO|HIDALG|XENINI|YINT|INTXEN|GFREE1|SABOLF|BETAH|RTEANG|INCLDY|VERN26|PSOLVE|ODFSET|TLOCAL|LAGRAN|GREYD|OPACT1|SRTFRQ|CONTMP|CIA_H2HE|IROSET|NSTOUT|LEMINI|INIFRC|LYMLIN|TDPINI|LEVCD|VERNER|TRMDRT|DMDER|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|SBFHMI|DWNFR0|GAMSP|PARTF|HESOLV|H2MINUS|PROFSP|DWNFR1|CONOUT|ALLARDT|MEANOP|RTESOL|READBF|COLUMN|VERN18|RTEFE2|OPACF1|PROFIL|INTHYD|RUSSEL|MATINV|WNSTOR|GFREE0|ERFCX|TABINI|PFNI|IJALIS|GAMI|QUASIM|SIGK|RDATA|INDEXX|QUIT|BKHSGO|TABINT|QUARTC|ROSSOP|NEWDMT|COMSET|CIA_HHE|INKUL|GETLAL|YLINTP|LTEGRD|INITIA|PFSPEC|LINSET|LOCATE|CUBIC|NSTPAR|LEVGRP|LEVSET|PRDINI|OPAHST|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|DIVSTR|SETTRM|PFHEAV|KURUCZ|RDATAX|VOIGT|TRAINI|STARKA|CONTMD|INTERP|RHONEN|GETWRD|SGHE12|MOLEQ|STATE|RAYLEIGH|ZMRHO|SIGAVE|TOPBAS|FFCROS|OPADD0|CIA_H2H2|RTECF0|INTLEM|CHANGE|CARBON|RATMAT|GRIDP|INIFRS|RTECF1",True,src/tlusty/io/start.rs,done
state.f,STATE,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|terden|PFSTDS","OPFRAC|PARTF","irwint|terden|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS","MPARTF|OPFRAC|PFSPEC|PFHEAV|PFCNO|PFFE|PARTF|PFNI",True,src/tlusty/math/utils/state.rs,done
steqeq.f,STEQEQ,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT|POPSTR|PPAPAR","RATMAT|MOLEQ|LEVSOL|SABOLF","irwint|terden|COMFH1|moldat|PFSTDS|POPSTR|entrop|eospar|pfoptb|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2","LEVSOL|REFLEV|OPFRAC|PFCNO|PFFE|MOLEQ|RUSSEL|SABOLF|MPARTF|PFSPEC|PFHEAV|PARTF|RATMAT|PFNI|LINEQS",False,src/tlusty/math/eos/steqeq.rs,done
switch.f,SWITCH,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","","ATOMIC|MODELQ|BASICS","",True,src/tlusty/math/utils/switch.rs,done
szirc.f,SZIRC,SUBROUTINE,True,"","EINT","","EXPINX|EXPO|EINT",False,src/tlusty/math/hydrogen/szirc.rs,done
tabini.f,TABINI,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|abntab|intcff|eletab","","abntab|ATOMIC|MODELQ|BASICS|intcff|eletab","",True,src/tlusty/io/tabini.rs,done
tabint.f,TABINT,SUBROUTINE,False,"BASICS|MODELQ|ATOMIC|intcff","","ATOMIC|MODELQ|intcff|BASICS","",False,src/tlusty/math/interpolation/tabint.rs,done
taufr1.f,TAUFR1,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT","","ITERAT|MODELQ|BASICS|OPTDPT|ALIPAR","",False,src/tlusty/math/ali/taufr1.rs,done
tdpini.f,TDPINI,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR","GFREE0","ATOMIC|MODELQ|ODFPAR|BASICS|ALIPAR","GFREE0",False,src/tlusty/math/temperature/tdpini.rs,done
temcor.f,TEMCOR,SUBROUTINE,False,"BASICS|MODELQ|ARRAY1|ALIPAR|CUBCON","WNSTOR|STEQEQ|ELDENS|CONVEC|MEANOP|OPACF0","irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON","LEVSOL|REFLEV|PRSENT|SFFHMI|OPFRAC|PFCNO|CIA_H2H|TRMDER|CONVEC|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|RUSSEL|SABOLF|WNSTOR|RHOEOS|GFREE0|SETTRM|DIVSTR|ELDENS|PFHEAV|DOPGAM|PFNI|LAGRAN|ENTENE|OPACT1|LINEQS|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|CIA_HHE|SGMER1|TRMDRT|STARK0|STEQEQ|MPARTF|YLINTP|PFSPEC|FFCROS|CIA_H2H2|INTLEM|DWNFR0|WN|OPADD|GAMSP|PARTF|RATMAT|LOCATE|OPCTAB|H2MINUS|PROFSP|DWNFR1|MEANOP|OPACF0",True,src/tlusty/math/temperature/temcor.rs,done
temper.f,TEMPER,SUBROUTINE,False,"BASICS|MODELQ|ALIPAR|FACTRS|PRSAUX|FLXAUX","WNSTOR|STEQEQ|MEANOPT|RHOEOS|ELDENS|TLOCAL|MEANOP|OPACF0","irwint|tdedge|POPSTR|pfoptb|eospar|tdflag|FACTRS|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|ITERAT|BASICS|FLXAUX|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|adchar|ATOMIC|ODFPAR|ioniz2","LEVSOL|REFLEV|PRSENT|SFFHMI|OPFRAC|PFCNO|CIA_H2H|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|RUSSEL|SABOLF|WNSTOR|RHOEOS|GFREE0|SETTRM|DIVSTR|ELDENS|PFHEAV|DOPGAM|TLOCAL|PFNI|LAGRAN|ENTENE|OPACT1|LINEQS|CIA_H2HE|VOIGT|STARKA|MOLEQ|QUARTC|STATE|RAYLEIGH|CIA_HHE|SGMER1|STARK0|STEQEQ|MEANOPT|MPARTF|PFSPEC|YLINTP|FFCROS|CIA_H2H2|INTLEM|DWNFR0|WN|OPADD|GAMSP|PARTF|RATMAT|OPCTAB|LOCATE|H2MINUS|PROFSP|DWNFR1|MEANOP|OPACF0",True,src/tlusty/math/temperature/temper.rs,done
timing.f,TIMING,SUBROUTINE,False,"","","","",True,src/tlusty/math/io/timing.rs,done
tiopf.f,TIOPF,SUBROUTINE,True,"","","","",False,src/tlusty/math/partition/tiopf.rs,done
tlocal.f,TLOCAL,SUBROUTINE,False,"BASICS|MODELQ|FACTRS|FLXAUX","QUARTC","FLXAUX|FACTRS|MODELQ|BASICS","QUARTC",False,src/tlusty/math/temperature/tlocal.rs,done
tlusty.f,TLUSTY,UNKNOWN,False,"BASICS|ITERAT|ALIPAR","RESOLV|SOLVE|SOLVES|RYBSOL|TIMING|ACCEL2|START","DEPTDR|tdedge|POPSTR|pfoptb|tdflag|POPULS|PPAPAR|eletab|STFCR|rhoder|MODELQ|THERM|calphatd|CC|derdif|rybpgs|BASICS|intcfg|FLXAUX|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|grdpra|RHODER|SURFEX|COLKUR|LINED|STOMAT|ichndm|ADCHAR|ODFPAR|ioniz2|dsctva|CUBCON|callarda|irwint|deridt|temlim|imodlc|adiaba|TOTJHK|intcff|RYBMTX|eospar|FACTRS|EXTINT|INUNIT|ijflar|ALIPAR|hmolab|freqcl|TOPB|ITERAT|CTIon|OPTDPT|CMATZD|PRSAUX|COOLCO|COMFH1|imucnn|ARRAY1|relcor|moldat|CTRTEMP|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|abntab|callardg|ifpzpa|ATOMIC|callardc|hediff|STRPAR|comgfs","PRSENT|INPMOD|SBFHE1|ANGSET|TEMPER|COLLHE|EXPINX|ACCEL2|VERN16|VERN20|ERFCIN|RHOEOS|GRCOR|ODFHYS|CHCTAB|OPDATA|LINEQS|GOMINI|OPAINI|PRCHAN|RHSGEN|ODFMER|RTEFR1|VOIGTE|BPOPC|CKOEST|BPOPT|LTEGR|TRIDAG|CEH12|WN|NEWDM|INPDIS|OPCTAB|PRD|CION|GAUNT|BHED|PGSET|OPACFA|PFCNO|OPACTR|XENINI|ALIST1|INTXEN|GFREE1|SABOLF|RTEANG|INCLDY|VERN26|ODFSET|PZEVLD|TLOCAL|GREYD|DMEVAL|RTEINT|CIA_H2HE|PZERT|LEMINI|BPOPF|TDPINI|VISINI|VERNER|TRMDRT|DMDER|MEANOPT|DWNFR0|PARTF|HESOLV|H2MINUS|CONOUT|READBF|COLUMN|PRINC|RTEFE2|PROFIL|INTHYD|OPACTD|WNSTOR|ERFCX|ALIFR3|TIMING|PFNI|GAMI|ALIST2|QUASIM|OUTPUT|INDEXX|ACCELP|RYBSOL|QUIT|BPOPE|BKHSGO|TABINT|RYBMAT|RESOLV|GETLAL|YLINTP|CONCOR|LTEGRD|INITIA|LINSET|RATMAL|CUBIC|LEVGRP|LEVSET|CONVC1|OPFRAC|ALIFRK|NEWPOP|CROSS|RTECMC|DIVSTR|SETTRM|RTECMU|PFHEAV|OPACFL|COLIS|VOIGT|TRAINI|STARKA|CSPEC|CONTMD|INTERP|GETWRD|DWNFR|RATES1|PZEVAL|TOPBAS|FFCROS|BUTLER|CHANGE|CARBON|BPOP|GRIDP|BRE|INIFRS|SFFHMI|CIA_H2H|PFFE|UBETA|BRTEZ|HEDIF|EINT|LINPRO|HEPHOT|ALISK2|IJALI2|LINSPL|EXPINT|RADTOT|INIFRT|CORRWM|RTECOM|DOPGAM|ELDENS|RTEDF2|RAYINI|ENTENE|IRC|REIMAN|SGMER0|GAULEG|ODFFR|RTEDF1|SGMER1|TEMCOR|COLHE|MATGEN|BHEZ|OPADD|BHE|CONREF|OPACF0|SOLVE|REFLEV|HESOL6|SPSIGK|RAYSET|HIDALG|EMAT|YINT|LUCY|TAUFR1|BREZ|ELDENC|BETAH|PSOLVE|LAGRAN|OPACT1|START|SRTFRQ|CONTMP|IROSET|RATSP1|NSTOUT|RYBCHN|INIFRC|LYMLIN|LEVCD|STARK0|STEQEQ|MPARTF|GHYDOP|SBFHMI|GAMSP|OPACFD|PROFSP|DWNFR1|ALLARDT|MEANOP|RADPRE|CHEAV|RTESOL|VERN18|OPACF1|ODFHYD|COLH|RUSSEL|ODFHST|MATINV|GFREE0|TABINI|ALIFR1|IJALIS|SIGK|RDATA|EXPO|RECHCK|OSCCOR|QUARTC|ROSSOP|NEWDMT|CIA_HHE|COMSET|INKUL|SOLVES|PFSPEC|GFREED|RYBENE|LOCATE|COMPT0|BRTE|NSTPAR|INILAM|PRDINI|LEVSOL|OPAHST|TRMDER|CONVEC|CROSSD|ALLARD|LINSEL|ROSSTD|CHCKSE|KURUCZ|RDATAX|DIELRC|COOLRT|HCTION|OUTPRI|CHEAVJ|MATCON|SETDRT|RHONEN|SGHE12|MOLEQ|STATE|RAYLEIGH|ELCOR|ZMRHO|SIGAVE|RYBHEQ|CIA_H2H2|OPADD0|RTECF0|INTLEM|RATMAT|DIETOT|SZIRC|RTECF1",True,src/bin/tlusty.rs,done
topbas.f,TOPBAS,FUNCTION,False,"TOPB","OPDATA|YLINTP","TOPB","OPDATA|YLINTP",True,src/tlusty/math/utils/topbas.rs,done
traini.f,TRAINI,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ODFPAR","","ODFPAR|ATOMIC|MODELQ|BASICS","",False,src/tlusty/math/utils/traini.rs,done
tridag.f,TRIDAG,SUBROUTINE,True,"","","","",False,src/tlusty/math/solvers/tridag.rs,done
trmder.f,TRMDER,SUBROUTINE,False,"BASICS|terden|derdif|adiaba","ELDENS","irwint|terden|COMFH1|adiaba|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|derdif|ATOMIC|BASICS|ioniz2","MPARTF|OPFRAC|PFSPEC|ELDENS|PFHEAV|PFCNO|PFFE|PARTF|PFNI|MOLEQ|ENTENE|STATE|RUSSEL|LINEQS",False,src/tlusty/math/radiative/trmder.rs,done
trmdrt.f,TRMDRT,SUBROUTINE,False,"BASICS|tdedge|tdflag|CONVOUT|CC","PRSENT|RHOEOS","MODELQ|tdedge|THERM|CC|TABLTD|CONVOUT|BASICS|tdflag","PRSENT|RHOEOS|SETTRM",False,src/tlusty/math/radiative/trmdrt.rs,done
ubeta.f,UBETA,FUNCTION,True,"","LAGRAN","","LAGRAN",False,src/tlusty/math/solvers/ubeta.rs,done
vern16.f,VERN16,FUNCTION,True,"BASICS","","BASICS","",False,src/tlusty/math/atomic/vern16.rs,done
vern18.f,VERN18,FUNCTION,True,"BASICS","","BASICS","",False,src/tlusty/math/atomic/vern18.rs,done
vern20.f,VERN20,FUNCTION,True,"BASICS","","BASICS","",False,src/tlusty/math/atomic/vern20.rs,done
vern26.f,VERN26,FUNCTION,True,"BASICS","","BASICS","",False,src/tlusty/math/atomic/vern26.rs,done
verner.f,VERNER,FUNCTION,False,"BASICS|ATOMIC","VERN26|QUIT|VERN18|VERN16|VERN20","ATOMIC|BASICS","VERN26|VERN18|QUIT|VERN16|VERN20",False,src/tlusty/math/atomic/verner.rs,done
visini.f,VISINI,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ|ITERAT","","ITERAT|ATOMIC|MODELQ|BASICS","",True,src/tlusty/math/io/visini.rs,done
voigt.f,VOIGT,FUNCTION,True,"","","","",False,src/tlusty/math/special/voigt.rs,done
voigte.f,VOIGTE,FUNCTION,True,"","","","",False,src/tlusty/math/special/voigte.rs,done
wn.f,WN,FUNCTION,True,"BASICS","","BASICS","",False,src/tlusty/math/utils/wn.rs,done
wnstor.f,WNSTOR,SUBROUTINE,False,"BASICS|ATOMIC|MODELQ","WN","ATOMIC|MODELQ|BASICS","WN",False,src/tlusty/math/utils/wnstor.rs,done
xenini.f,XENINI,SUBROUTINE,False,"BASICS|MODELQ","","MODELQ|BASICS","",True,src/tlusty/io/xenini.rs,done
xk2dop.f,XK2DOP,FUNCTION,True,"","","","",False,src/tlusty/math/utils/xk2dop.rs,done
yint.f,YINT,FUNCTION,True,"","","","",False,src/tlusty/math/interpolation/yint.rs,done
ylintp.f,YLINTP,FUNCTION,True,"","","","",False,src/tlusty/math/interpolation/ylintp.rs,done
zmrho.f,ZMRHO,SUBROUTINE,False,"BASICS|MODELQ","ERFCIN|BETAH","MODELQ|BASICS","ERFCX|ERFCIN|BETAH",False,src/tlusty/math/utils/zmrho.rs,done
1 fortran_file unit_name unit_type is_pure common_deps call_deps trans_commons trans_calls has_io rust_module status
2 _unnamed_block_data_.f _UNNAMED_ BLOCK DATA False BASICS|ATOMIC ATOMIC|BASICS False pending
3 accel2.f ACCEL2 SUBROUTINE False BASICS|ITERAT|MODELQ RESOLV callarda|irwint|DEPTDR|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|POPULS|EXTINT|PPAPAR|eletab|ALIPAR|rhoder|MODELQ|hmolab|THERM|calphatd|CC|derdif|rybpgs|ITERAT|BASICS|CTIon|OPTDPT|intcfg|terden|PRSAUX|AUXRTE|RAYSCT|COOLCO|COMFH1|imucnn|ARRAY1|quasun|moldat|CTRTEMP|ipricr|callardb|PFSTDS|entrop|TABLTD|CONVOUT|comgfs|icnrsp|auxcbc|adchar|grdpra|callardg|SURFEX|ifpzpa|ATOMIC|callardc|ADCHAR|ODFPAR|ioniz2|dsctva|CUBCON PRSENT|SFFHMI|ANGSET|CIA_H2H|COLLHE|PFFE|UBETA|EXPINX|EINT|LINPRO|ALISK2|RHOEOS|RTECOM|DOPGAM|ELDENS|RTEDF2|ENTENE|IRC|LINEQS|OPAINI|ODFMER|RTEFR1|SGMER0|GAULEG|TRIDAG|RTEDF1|SGMER1|CEH12|TEMCOR|COLHE|OPADD|WN|OPCTAB|PRD|CION|CONREF|OPACF0|REFLEV|HESOL6|PGSET|RAYSET|PFCNO|OPACFA|YINT|LUCY|ALIST1|TAUFR1|INTXEN|GFREE1|SABOLF|ELDENC|PZEVLD|LAGRAN|DMEVAL|OPACT1|RTEINT|CIA_H2HE|RATSP1|PZERT|LYMLIN|TDPINI|VISINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|OPACFD|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RADPRE|CHEAV|RTESOL|PRINC|RTEFE2|OPACF1|ODFHYD|INTHYD|COLH|OPACTD|RUSSEL|ODFHST|MATINV|WNSTOR|GFREE0|ALIFR3|TIMING|PFNI|ALIFR1|GAMI|ALIST2|QUASIM|OUTPUT|INDEXX|EXPO|RECHCK|OSCCOR|ACCELP|QUIT|CIA_HHE|COMSET|RESOLV|YLINTP|CONCOR|PFSPEC|GFREED|LOCATE|RATMAL|LEVGRP|INILAM|LEVSOL|CONVC1|OPFRAC|TRMDER|CONVEC|NEWPOP|ALIFRK|CROSSD|CROSS|ALLARD|RTECMC|LINSEL|ROSSTD|DIVSTR|CHCKSE|RTECMU|PFHEAV|SETTRM|DIELRC|COOLRT|HCTION|OUTPRI|OPACFL|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|RHONEN|DWNFR|RATES1|MOLEQ|STATE|RAYLEIGH|PZEVAL|ELCOR|RYBHEQ|FFCROS|CIA_H2H2|RTECF0|INTLEM|BUTLER|RATMAT|DIETOT|SZIRC|RTECF1 True src/tlusty/math/solvers/accel2.rs done
4 accelp.f ACCELP SUBROUTINE False BASICS|MODELQ|ITERAT|POPULS ITERAT|POPULS|MODELQ|BASICS True src/tlusty/math/solvers/accelp.rs done
5 alifr1.f ALIFR1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR ALIFR3 MODELQ|ATOMIC|BASICS|ALIPAR ALIFR3 False src/tlusty/math/ali/alifr1.rs done
6 alifr3.f ALIFR3 SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR ATOMIC|MODELQ|BASICS|ALIPAR False src/tlusty/math/ali/alifr3.rs done
7 alifr6.f ALIFR6 SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR ATOMIC|MODELQ|BASICS|ALIPAR False src/tlusty/math/ali/alifr6.rs done
8 alifrk.f ALIFRK SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR ATOMIC|MODELQ|BASICS|ALIPAR False src/tlusty/math/ali/alifrk.rs done
9 alisk1.f ALISK1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT ROSSTD|RTEFR1|ALIFRK|OPACF1|CROSS callarda|AUXRTE|RAYSCT|ARRAY1|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|ALIFRK|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/ali/alisk1.rs done
10 alisk2.f ALISK2 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT ROSSTD|RTEFR1|ALIFRK|OPACF1|CROSS callarda|AUXRTE|RAYSCT|ARRAY1|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|ALIFRK|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/ali/alisk2.rs done
11 alist1.f ALIST1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT ROSSTD|RTEFR1|OPACFD|ALIFR1|CROSS callarda|AUXRTE|RAYSCT|ARRAY1|quasun|callardb|eospar|EXTINT|auxcbc|ALIPAR|rhoder|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|dsctva|ODFPAR|BASICS|OPTDPT|comgfs SFFHMI|CIA_H2H|RTEFE2|CROSSD|CROSS|ALLARD|OPACTD|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|ALIFR3|ALIFR1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|GFREED|CIA_H2H2|RTECF0|OPADD|OPACFD|GAMSP|OPCTAB|LOCATE|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/ali/alist1.rs done
12 alist2.f ALIST2 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT ROSSTD|RTEFR1|QUIT|OPACFD|ALIFR1|CROSS callarda|AUXRTE|RAYSCT|ARRAY1|quasun|callardb|eospar|EXTINT|auxcbc|ALIPAR|rhoder|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|dsctva|ODFPAR|BASICS|OPTDPT|comgfs SFFHMI|CIA_H2H|RTEFE2|CROSSD|CROSS|ALLARD|OPACTD|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|ALIFR3|ALIFR1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|QUIT|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|GFREED|CIA_H2H2|RTECF0|OPADD|OPACFD|GAMSP|OPCTAB|LOCATE|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/ali/alist2.rs done
13 allard.f ALLARD SUBROUTINE False BASICS|callarda|callardg|calphatd|quasun|callardb|callardc ALLARDT callarda|callardg|calphatd|quasun|callardb|callardc|BASICS ALLARDT True src/tlusty/math/opacity/allard.rs done
14 allardt.f ALLARDT SUBROUTINE False BASICS|calphatd BASICS|calphatd False src/tlusty/math/opacity/allardt.rs done
15 angset.f ANGSET SUBROUTINE True BASICS GAULEG BASICS GAULEG False src/tlusty/math/utils/angset.rs done
16 betah.f BETAH FUNCTION True ERFCX ERFCX False src/tlusty/math/utils/betah.rs done
17 bhe.f BHE SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR ATOMIC|MODELQ|BASICS|ARRAY1|ALIPAR False src/tlusty/math/hydrogen/bhe.rs done
18 bhed.f BHED SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|CMATZD|SURFEX ATOMIC|MODELQ|BASICS|SURFEX|ARRAY1|CMATZD|ALIPAR False src/tlusty/math/hydrogen/bhe.rs done
19 bhez.f BHEZ SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|SURFEX ATOMIC|MODELQ|BASICS|SURFEX|ARRAY1|ALIPAR False src/tlusty/math/hydrogen/bhe.rs done
20 bkhsgo.f BKHSGO SUBROUTINE True False src/tlusty/math/utils/bkhsgo.rs done
21 bpop.f BPOP SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR|ITERAT LEVSOL|MATINV|BPOPE|BPOPF|RATMAT|BPOPC|BPOPT|LEVGRP irwint|terden|ARRAY1|moldat|CTRTEMP|PFSTDS|pfoptb|ALIPAR|MODELQ|ITERAT|ATOMIC|ADCHAR|BASICS|ODFPAR|CTIon LEVSOL|REFLEV|OPFRAC|PFCNO|COLLHE|PFFE|EXPINX|CROSS|EINT|COLH|MATINV|PFHEAV|PFNI|HCTION|IRC|LINEQS|CHEAVJ|COLIS|EXPO|CSPEC|QUIT|BPOPE|BPOPF|BPOPC|BPOPT|STATE|SGMER1|CEH12|MPARTF|YLINTP|PFSPEC|COLHE|BUTLER|PARTF|RATMAT|CION|DWNFR1|LEVGRP|SZIRC|CHEAV False src/tlusty/math/population/bpop.rs done
22 bpopc.f BPOPC SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR|ADCHAR STATE irwint|MODELQ|terden|ARRAY1|moldat|PFSTDS|ATOMIC|pfoptb|ADCHAR|BASICS|ODFPAR|ALIPAR MPARTF|OPFRAC|PFSPEC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|STATE False src/tlusty/math/population/bpopc.rs done
23 bpope.f BPOPE SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT|ARRAY1 DWNFR1|CROSS|SGMER1 MODELQ|ARRAY1|ITERAT|ATOMIC|ODFPAR|BASICS|ALIPAR DWNFR1|CROSS|SGMER1 False src/tlusty/math/population/bpope.rs done
24 bpopf.f BPOPF SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR ATOMIC|MODELQ|BASICS|ODFPAR|ARRAY1|ALIPAR False src/tlusty/math/population/bpopf.rs done
25 bpopt.f BPOPT SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|ODFPAR COLIS MODELQ|ARRAY1|CTRTEMP|ATOMIC|BASICS|ODFPAR|CTIon|ALIPAR EXPO|CSPEC|QUIT|COLLHE|EXPINX|CHEAV|EINT|COLH|CEH12|YLINTP|COLHE|BUTLER|CION|HCTION|CHEAVJ|IRC|SZIRC|COLIS False src/tlusty/math/population/bpopt.rs done
26 bre.f BRE SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR COMPT0 MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR COMPT0 False src/tlusty/math/hydrogen/bre.rs done
27 brez.f BREZ SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR COMPT0 MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR COMPT0 False src/tlusty/math/hydrogen/brez.rs done
28 brte.f BRTE SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR|ARRAY1 COMPT0 MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR COMPT0 False src/tlusty/math/hydrogen/brte.rs done
29 brtez.f BRTEZ SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR|ARRAY1 COMPT0 MODELQ|ARRAY1|ITERAT|ATOMIC|BASICS|auxcbc|ALIPAR COMPT0 False src/tlusty/math/hydrogen/brtez.rs done
30 butler.f BUTLER SUBROUTINE True False src/tlusty/math/population/butler.rs done
31 carbon.f CARBON SUBROUTINE True False src/tlusty/math/partition/carbon.rs done
32 ceh12.f CEH12 FUNCTION True False src/tlusty/math/partition/ceh12.rs done
33 change.f CHANGE SUBROUTINE False BASICS|ATOMIC|MODELQ STEQEQ|READBF irwint|terden|COMFH1|moldat|PFSTDS|POPSTR|entrop|eospar|pfoptb|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2 LEVSOL|REFLEV|READBF|OPFRAC|PFCNO|PFFE|MOLEQ|RUSSEL|SABOLF|STEQEQ|MPARTF|PFSPEC|PFHEAV|PARTF|RATMAT|PFNI|LINEQS True src/tlusty/math/utils/change.rs done
34 chckse.f CHCKSE SUBROUTINE False BASICS|ATOMIC|MODELQ SABOLF irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|SABOLF True src/tlusty/io/chckse.rs done
35 chctab.f CHCTAB SUBROUTINE False BASICS|MODELQ|abntab abntab|MODELQ|BASICS True src/tlusty/math/atomic/chctab.rs done
36 cheav.f CHEAV FUNCTION False BASICS|ATOMIC QUIT|CHEAVJ ATOMIC|BASICS QUIT|CHEAVJ True src/tlusty/math/atomic/cheav.rs done
37 cheavj.f CHEAVJ FUNCTION False BASICS|ATOMIC QUIT ATOMIC|BASICS QUIT True src/tlusty/math/atomic/cheavj.rs done
38 cia_h2h.f CIA_H2H SUBROUTINE False LOCATE LOCATE True src/tlusty/math/opacity/cia_h2h.rs done
39 cia_h2h2.f CIA_H2H2 SUBROUTINE False LOCATE LOCATE True src/tlusty/math/opacity/cia_h2h2.rs done
40 cia_h2he.f CIA_H2HE SUBROUTINE False LOCATE LOCATE True src/tlusty/math/opacity/cia_h2he.rs done
41 cia_hhe.f CIA_HHE SUBROUTINE False LOCATE LOCATE True src/tlusty/math/opacity/cia_hhe.rs done
42 cion.f CION FUNCTION True False src/tlusty/math/atomic/cion.rs done
43 ckoest.f CKOEST FUNCTION True BASICS BASICS False src/tlusty/math/interpolation/ckoest.rs done
44 colh.f COLH SUBROUTINE False BASICS|ATOMIC|MODELQ CSPEC|BUTLER|CEH12|IRC ATOMIC|MODELQ|BASICS CEH12|EXPO|CSPEC|BUTLER|QUIT|EXPINX|EINT|IRC|SZIRC False src/tlusty/math/hydrogen/colh.rs done
45 colhe.f COLHE SUBROUTINE False BASICS|ATOMIC CSPEC|IRC|COLLHE|CHEAV ATOMIC|BASICS EXPO|CSPEC|QUIT|COLLHE|EXPINX|EINT|CHEAVJ|IRC|SZIRC|CHEAV False src/tlusty/math/hydrogen/colhe.rs done
46 colis.f COLIS SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|CTRTEMP YLINTP|CSPEC|COLHE|CION|HCTION|COLH|IRC MODELQ|CTRTEMP|ATOMIC|ODFPAR|BASICS|CTIon EXPO|CSPEC|QUIT|COLLHE|EXPINX|EINT|COLH|CEH12|YLINTP|COLHE|BUTLER|CION|HCTION|CHEAVJ|IRC|SZIRC|CHEAV False src/tlusty/math/hydrogen/colis.rs done
47 collhe.f COLLHE SUBROUTINE True False src/tlusty/math/hydrogen/collhe.rs done
48 column.f COLUMN SUBROUTINE False BASICS|MODELQ|relcor MODELQ|relcor|BASICS True src/tlusty/math/utils/column.rs done
49 compt0.f COMPT0 SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|auxcbc ITERAT|MODELQ|BASICS|auxcbc|ALIPAR False src/tlusty/math/opacity/compt0.rs done
50 comset.f COMSET SUBROUTINE False BASICS|MODELQ|auxcbc|comgfs ANGSET MODELQ|BASICS|auxcbc|comgfs ANGSET|GAULEG False src/tlusty/math/utils/comset.rs done
51 concor.f CONCOR SUBROUTINE False BASICS|MODELQ TEMCOR|CONOUT irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|TEMCOR|WN|OPADD|LOCATE|OPCTAB|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|MEANOPT|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP True src/tlusty/math/convection/concor.rs done
52 conout.f CONOUT SUBROUTINE False BASICS|MODELQ|ALIPAR|CUBCON MEANOPT|MEANOP|CONVEC|OPACF0 irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|BASICS|terden|RAYSCT|COMFH1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|OPADD|WN|OPCTAB|LOCATE|OPACF0|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|H2MINUS|PROFSP|DWNFR1|MEANOP True src/tlusty/math/convection/conout.rs done
53 conref.f CONREF SUBROUTINE False BASICS|MODELQ|ARRAY1|imucnn|CUBCON WNSTOR|CONVC1|STEQEQ|ELDENS|CONVEC|TDPINI|CONOUT irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|imucnn|COMFH1|RAYSCT|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|OPACF0|LEVSOL|REFLEV|CONVC1|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|TDPINI|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP True src/tlusty/math/convection/conref.rs done
54 contmd.f CONTMD SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR|PRSAUX|CUBCON WNSTOR|HESOL6|STEQEQ|CONVEC|CUBIC|CONOUT|MEANOP|OPACF0 irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|CUBIC|OPACF0|LEVSOL|REFLEV|HESOL6|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP True src/tlusty/math/convection/contmd.rs done
55 contmp.f CONTMP SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR|ichndm|CUBCON WNSTOR|STEQEQ|MEANOPT|RHOEOS|ELDENS|CONVEC|CUBIC|CONOUT|MEANOP|OPACF0 irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ichndm|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|CUBIC|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP True src/tlusty/math/convection/contmp.rs done
56 convc1.f CONVC1 SUBROUTINE False BASICS|CUBCON TRMDER|TRMDRT irwint|terden|tdedge|COMFH1|adiaba|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON PRSENT|OPFRAC|PFCNO|TRMDER|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS False src/tlusty/math/convection/convec.rs done
57 convec.f CONVEC SUBROUTINE False BASICS|CUBCON TRMDER|TRMDRT irwint|terden|tdedge|COMFH1|adiaba|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON PRSENT|OPFRAC|PFCNO|TRMDER|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS False src/tlusty/math/convection/convec.rs done
58 coolrt.f COOLRT SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT|COOLCO RTEFR1|OPACFA COOLCO|AUXRTE|ARRAY1|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|SURFEX|ITERAT|ATOMIC|ODFPAR|BASICS|OPTDPT|comgfs SFFHMI|OPACFA|RTEFR1|CIA_H2H|RTEFE2|CROSSD|CROSS|RTEDF1|CIA_HHE|SGMER1|MATINV|YLINTP|FFCROS|CIA_H2H2|RTECF0|RTEDF2|DOPGAM|OPADD|GAMSP|LOCATE|PRD|H2MINUS|GAMI|DWNFR1|CIA_H2HE|RTESOL|RTECF1 True src/tlusty/math/radiative/coolrt.rs done
59 corrwm.f CORRWM SUBROUTINE False BASICS|ATOMIC|MODELQ QUIT ATOMIC|MODELQ|BASICS QUIT True src/tlusty/math/opacity/corrwm.rs done
60 cross.f CROSS FUNCTION False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/atomic/cross.rs done
61 crossd.f CROSSD FUNCTION False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/atomic/cross.rs done
62 cspec.f CSPEC SUBROUTINE False BASICS|ATOMIC QUIT ATOMIC|BASICS QUIT False src/tlusty/math/opacity/cspec.rs done
63 ctdata.f CTDATA BLOCK DATA False CTRecomb|CTIon CTRecomb|CTIon False src/tlusty/math/hydrogen/ctdata.rs done
64 cubic.f CUBIC SUBROUTINE False BASICS|CUBCON CUBCON|BASICS False src/tlusty/math/solvers/cubic.rs done
65 dielrc.f DIELRC SUBROUTINE True False src/tlusty/math/atomic/dielrc.rs done
66 dietot.f DIETOT SUBROUTINE False BASICS|ATOMIC|MODELQ DIELRC ATOMIC|MODELQ|BASICS DIELRC True src/tlusty/math/atomic/dietot.rs done
67 divstr.f DIVSTR SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/utils/divstr.rs done
68 dmder.f DMDER SUBROUTINE False BASICS|ATOMIC|MODELQ|DEPTDR DEPTDR|ATOMIC|MODELQ|BASICS False src/tlusty/math/utils/dmder.rs done
69 dmeval.f DMEVAL SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ARRAY1 ITERAT|ATOMIC|MODELQ|BASICS|ARRAY1 True src/tlusty/math/utils/dmeval.rs done
70 dopgam.f DOPGAM SUBROUTINE False BASICS|ATOMIC|MODELQ GAMSP ATOMIC|MODELQ|BASICS GAMSP False src/tlusty/math/opacity/dopgam.rs done
71 dwnfr.f DWNFR SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/opacity/dwnfr.rs done
72 dwnfr0.f DWNFR0 SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/opacity/dwnfr0.rs done
73 dwnfr1.f DWNFR1 SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/opacity/dwnfr1.rs done
74 eint.f EINT SUBROUTINE True EXPO|EXPINX EXPO|EXPINX False src/tlusty/math/special/expint.rs done
75 elcor.f ELCOR SUBROUTINE False BASICS|ATOMIC|MODELQ|ADCHAR MOLEQ|WNSTOR|STATE|STEQEQ irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|POPSTR|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|ADCHAR|BASICS|ioniz2 LEVSOL|REFLEV|OPFRAC|PFCNO|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|WNSTOR|STEQEQ|MPARTF|PFSPEC|PFHEAV|WN|PARTF|PFNI|RATMAT|LINEQS True src/tlusty/math/temperature/elcor.rs done
76 eldenc.f ELDENC SUBROUTINE False BASICS|MODELQ|ATOMIC|hmolab|eospar|eletab MOLEQ|RHONEN|STATE irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|eletab|adchar|MODELQ|hmolab|ATOMIC|BASICS|ioniz2 OPFRAC|PFCNO|RHONEN|PFFE|MOLEQ|STATE|RUSSEL|MPARTF|PFSPEC|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS True src/tlusty/math/eos/eldenc.rs done
77 eldens.f ELDENS SUBROUTINE False BASICS|MODELQ|ATOMIC|terden|eospar MPARTF|MOLEQ|ENTENE|STATE|LINEQS irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ATOMIC|BASICS|ioniz2 MPARTF|OPFRAC|PFSPEC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|MOLEQ|ENTENE|STATE|RUSSEL|LINEQS True src/tlusty/math/eos/eldens.rs done
78 emat.f EMAT SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR ATOMIC|MODELQ|BASICS|ARRAY1|ALIPAR False src/tlusty/math/utils/emat.rs done
79 entene.f ENTENE SUBROUTINE False BASICS|ATOMIC|MODELQ MPARTF moldat|ATOMIC|MODELQ|BASICS MPARTF False src/tlusty/math/eos/entene.rs done
80 erfcin.f ERFCIN FUNCTION True ERFCX ERFCX False src/tlusty/math/special/erfcx.rs done
81 erfcx.f ERFCX FUNCTION True False src/tlusty/math/special/erfcx.rs done
82 expint.f EXPINT FUNCTION True False src/tlusty/math/special/expint.rs done
83 expinx.f EXPINX SUBROUTINE True False src/tlusty/math/special/expint.rs done
84 expo.f EXPO FUNCTION True False src/tlusty/math/special/expo.rs done
85 ffcros.f FFCROS FUNCTION True False src/tlusty/math/atomic/ffcros.rs done
86 gami.f GAMI FUNCTION True False src/tlusty/math/special/gami.rs done
87 gamsp.f GAMSP SUBROUTINE True BASICS BASICS False src/tlusty/math/special/gamsp.rs done
88 gauleg.f GAULEG SUBROUTINE True False src/tlusty/math/special/gauleg.rs done
89 gaunt.f GAUNT FUNCTION True False src/tlusty/math/special/gaunt.rs done
90 getlal.f GETLAL SUBROUTINE False BASICS|callarda|callardg|calphatd|quasun|callardb|callardc callarda|callardg|callardc|BASICS|calphatd|quasun|callardb True src/tlusty/math/utils/getlal.rs done
91 getwrd.f GETWRD SUBROUTINE True False src/tlusty/math/io/getwrd.rs done
92 gfree0.f GFREE0 SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/atomic/gfree.rs done
93 gfree1.f GFREE1 FUNCTION False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/atomic/gfree.rs done
94 gfreed.f GFREED SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/atomic/gfree.rs done
95 ghydop.f GHYDOP SUBROUTINE False BASICS|MODELQ|ATOMIC|intcfg intcfg|ATOMIC|MODELQ|BASICS False src/tlusty/math/hydrogen/ghydop.rs done
96 gntk.f GNTK FUNCTION True False src/tlusty/math/atomic/gntk.rs done
97 gomini.f GOMINI SUBROUTINE False BASICS|MODELQ|intcfg intcfg|MODELQ|BASICS True src/tlusty/math/utils/gomini.rs done
98 grcor.f GRCOR SUBROUTINE True False src/tlusty/math/temperature/grcor.rs done
99 greyd.f GREYD SUBROUTINE False BASICS|MODELQ|ATOMIC|ALIPAR WNSTOR|STEQEQ|RHONEN|MEANOP|OPACF0 irwint|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|POPSTR|entrop|eospar|pfoptb|PPAPAR|adchar|ALIPAR|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2|ODFPAR SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|LOCATE|OPCTAB|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|RHONEN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|MEANOP True src/tlusty/math/temperature/greyd.rs done
100 gridp.f GRIDP SUBROUTINE True BASICS BASICS False src/tlusty/math/utils/gridp.rs done
101 h2minus.f H2MINUS SUBROUTINE False BASICS LOCATE BASICS LOCATE True src/tlusty/math/hydrogen/h2minus.rs done
102 hction.f HCTION FUNCTION False CTRTEMP|CTIon CTRTEMP|CTIon False src/tlusty/math/hydrogen/ctdata.rs done
103 hctrecom.f HCTRECOM FUNCTION False CTRTEMP|CTRecomb CTRTEMP|CTRecomb False src/tlusty/math/hydrogen/ctdata.rs done
104 hedif.f HEDIF SUBROUTINE False BASICS|MODELQ|ATOMIC|hediff hediff|ATOMIC|MODELQ|BASICS True src/tlusty/math/hydrogen/hedif.rs done
105 hephot.f HEPHOT FUNCTION True False src/tlusty/math/hydrogen/hephot.rs done
106 hesol6.f HESOL6 SUBROUTINE False BASICS|MODELQ|PRSAUX MATINV MODELQ|PRSAUX|BASICS MATINV False src/tlusty/math/hydrogen/hesol6.rs done
107 hesolv.f HESOLV SUBROUTINE False BASICS|MODELQ|PRSAUX MATINV|WNSTOR|RHONEN|STEQEQ irwint|PRSAUX|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|POPSTR|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2 LEVSOL|REFLEV|OPFRAC|PFCNO|RHONEN|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|MATINV|WNSTOR|STEQEQ|MPARTF|PFSPEC|ELDENS|PFHEAV|WN|PARTF|PFNI|RATMAT|ENTENE|LINEQS True src/tlusty/math/hydrogen/hesolv.rs done
108 hidalg.f HIDALG FUNCTION True False src/tlusty/math/hydrogen/hidalg.rs done
109 ijali2.f IJALI2 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR QUIT ODFPAR|ATOMIC|MODELQ|BASICS QUIT True src/tlusty/math/ali/ijali2.rs done
110 ijalis.f IJALIS SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS True src/tlusty/math/ali/ijalis.rs done
111 incldy.f INCLDY SUBROUTINE False BASICS|ATOMIC|MODELQ LEVSOL|WNSTOR|QUIT|RATMAT|SABOLF irwint|MODELQ|moldat|PFSTDS|ITERAT|ATOMIC|pfoptb|BASICS LEVSOL|REFLEV|WNSTOR|MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|QUIT|WN|PFFE|PARTF|RATMAT|PFNI|LINEQS|SABOLF True src/tlusty/io/incldy.rs done
112 indexx.f INDEXX SUBROUTINE True False src/tlusty/math/solvers/indexx.rs done
113 inicom.f INICOM SUBROUTINE False BASICS|ATOMIC|MODELQ|comgfs comgfs|ATOMIC|MODELQ|BASICS False src/tlusty/math/utils/inicom.rs done
114 inifrc.f INIFRC SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ijflar INDEXX ATOMIC|MODELQ|ODFPAR|BASICS|ijflar INDEXX True src/tlusty/math/opacity/inifrc.rs done
115 inifrs.f INIFRS SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR INDEXX|QUIT ODFPAR|ATOMIC|MODELQ|BASICS INDEXX|QUIT True src/tlusty/math/opacity/inifrs.rs done
116 inifrt.f INIFRT SUBROUTINE False BASICS|ATOMIC|MODELQ|ijflar INDEXX ijflar|ATOMIC|MODELQ|BASICS INDEXX True src/tlusty/math/opacity/inifrt.rs done
117 inilam.f INILAM SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ALIPAR OPACF1|SABOLF|WNSTOR|RHOEOS|RTECOM|OUTPUT|COLIS|OPAINI|ODFMER|RTEFR1|OSCCOR|TDPINI|RATES1|VISINI|COMSET|ELCOR|STEQEQ|RYBHEQ|CONCOR|DIETOT tdedge|POPSTR|pfoptb|tdflag|PPAPAR|MODELQ|THERM|calphatd|CC|derdif|rybpgs|BASICS|intcfg|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|grdpra|SURFEX|ADCHAR|ODFPAR|ioniz2|CUBCON|callarda|irwint|adiaba|eospar|EXTINT|ALIPAR|hmolab|ITERAT|CTIon|OPTDPT|COMFH1|ARRAY1|moldat|CTRTEMP|ipricr|callardb|PFSTDS|auxcbc|adchar|callardg|ATOMIC|callardc|comgfs PRSENT|SFFHMI|ANGSET|CIA_H2H|COLLHE|PFFE|EXPINX|UBETA|EINT|LINPRO|RHOEOS|RTECOM|DOPGAM|RTEDF2|ELDENS|ENTENE|IRC|LINEQS|OPAINI|ODFMER|RTEFR1|SGMER0|GAULEG|TRIDAG|RTEDF1|SGMER1|CEH12|TEMCOR|COLHE|OPADD|WN|OPCTAB|PRD|CION|OPACF0|REFLEV|PGSET|PFCNO|YINT|INTXEN|GFREE1|SABOLF|LAGRAN|OPACT1|CIA_H2HE|LYMLIN|TDPINI|VISINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RTESOL|CHEAV|RTEFE2|OPACF1|ODFHYD|INTHYD|COLH|RUSSEL|ODFHST|MATINV|WNSTOR|GFREE0|PFNI|GAMI|QUASIM|OUTPUT|EXPO|INDEXX|OSCCOR|QUIT|COMSET|CIA_HHE|YLINTP|CONCOR|PFSPEC|LOCATE|LEVGRP|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|RTECMC|DIVSTR|ROSSTD|SETTRM|PFHEAV|DIELRC|HCTION|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|MOLEQ|RATES1|STATE|RAYLEIGH|ELCOR|RYBHEQ|FFCROS|CIA_H2H2|RTECF0|INTLEM|BUTLER|RATMAT|DIETOT|SZIRC|RTECF1 False src/tlusty/math/opacity/inilam.rs done
118 initia.f INITIA SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|STRPAR|freqcl|INUNIT OPAHST|INPMOD|READBF|LINSPL|INIFRT|CORRWM|DOPGAM|RTEANG|RDATAX|ODFSET|RAYINI|TABINI|ODFHYS|CHCTAB|SRTFRQ|GOMINI|SIGK|IROSET|RDATA|NSTOUT|TRAINI|QUIT|INIFRC|INTERP|TABINT|LTEGR|STATE|DMDER|SIGAVE|OPADD0|LTEGRD|CHANGE|LINSET|INPDIS|NSTPAR|INIFRS|LEVSET DEPTDR|tdedge|POPSTR|pfoptb|tdflag|PPAPAR|eletab|STFCR|MODELQ|THERM|CC|calphatd|derdif|BASICS|intcfg|FLXAUX|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|SURFEX|COLKUR|LINED|ichndm|ODFPAR|ioniz2|CUBCON|callarda|irwint|temlim|deridt|imodlc|adiaba|TOTJHK|intcff|eospar|FACTRS|EXTINT|INUNIT|ijflar|ALIPAR|hmolab|freqcl|TOPB|ITERAT|OPTDPT|PRSAUX|imucnn|COMFH1|relcor|moldat|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|abntab|callardg|ifpzpa|ATOMIC|callardc|hediff|STRPAR|comgfs INPMOD|PRSENT|SBFHE1|SFFHMI|TEMPER|CIA_H2H|PFFE|UBETA|HEPHOT|LINPRO|VERN16|LINSPL|VERN20|IJALI2|EXPINT|ERFCIN|RADTOT|INIFRT|CORRWM|RHOEOS|ELDENS|DOPGAM|RTEDF2|GRCOR|RAYINI|ODFHYS|ENTENE|CHCTAB|OPDATA|LINEQS|GOMINI|OPAINI|REIMAN|RTEFR1|SGMER0|GAULEG|VOIGTE|CKOEST|LTEGR|ODFFR|RTEDF1|SGMER1|WN|OPADD|INPDIS|OPCTAB|NEWDM|PRD|GAUNT|OPACF0|REFLEV|SPSIGK|HESOL6|RAYSET|PFCNO|HIDALG|XENINI|YINT|INTXEN|GFREE1|SABOLF|BETAH|RTEANG|INCLDY|VERN26|PSOLVE|ODFSET|TLOCAL|LAGRAN|GREYD|OPACT1|SRTFRQ|CONTMP|CIA_H2HE|IROSET|NSTOUT|LEMINI|INIFRC|LYMLIN|TDPINI|LEVCD|VERNER|TRMDRT|DMDER|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|SBFHMI|DWNFR0|GAMSP|PARTF|HESOLV|H2MINUS|PROFSP|DWNFR1|CONOUT|ALLARDT|MEANOP|RTESOL|READBF|COLUMN|VERN18|RTEFE2|OPACF1|PROFIL|INTHYD|RUSSEL|MATINV|WNSTOR|GFREE0|ERFCX|TABINI|PFNI|IJALIS|GAMI|QUASIM|SIGK|RDATA|INDEXX|QUIT|BKHSGO|TABINT|QUARTC|ROSSOP|NEWDMT|CIA_HHE|INKUL|GETLAL|YLINTP|LTEGRD|PFSPEC|LINSET|LOCATE|CUBIC|NSTPAR|LEVGRP|LEVSET|OPAHST|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|DIVSTR|SETTRM|PFHEAV|KURUCZ|RDATAX|VOIGT|TRAINI|STARKA|CONTMD|INTERP|RHONEN|GETWRD|SGHE12|MOLEQ|STATE|RAYLEIGH|ZMRHO|SIGAVE|TOPBAS|FFCROS|OPADD0|CIA_H2H2|RTECF0|INTLEM|CHANGE|CARBON|RATMAT|GRIDP|INIFRS|RTECF1 True src/tlusty/io/initia.rs done
119 inkul.f INKUL SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|COLKUR|LINED ATOMIC|MODELQ|ODFPAR|BASICS|COLKUR|LINED True src/tlusty/math/opacity/inkul.rs done
120 inpdis.f INPDIS SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|relcor GRCOR|COLUMN MODELQ|relcor|ITERAT|ATOMIC|BASICS|ODFPAR|ALIPAR GRCOR|COLUMN True src/tlusty/math/opacity/inpdis.rs done
121 inpmod.f INPMOD SUBROUTINE False BASICS|ATOMIC|MODELQ|eospar LEVSOL|WNSTOR|INCLDY|QUIT|KURUCZ|RATMAT|MOLEQ|SABOLF irwint|temlim|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2 LEVSOL|REFLEV|OPFRAC|PFCNO|PFFE|RUSSEL|SABOLF|WNSTOR|PFHEAV|INCLDY|ELDENS|KURUCZ|PFNI|ENTENE|LINEQS|QUIT|RHONEN|MOLEQ|STATE|MPARTF|PFSPEC|WN|PARTF|RATMAT True src/tlusty/io/inpmod.rs done
122 interp.f INTERP SUBROUTINE True BASICS BASICS False src/tlusty/math/interpolation/interp.rs done
123 inthyd.f INTHYD SUBROUTINE False BASICS|MODELQ STARKA|YINT|DIVSTR MODELQ|BASICS STARKA|YINT|DIVSTR False src/tlusty/math/hydrogen/inthyd.rs done
124 intlem.f INTLEM SUBROUTINE False BASICS|MODELQ INTHYD MODELQ|BASICS STARKA|YINT|DIVSTR|INTHYD False src/tlusty/math/interpolation/intlem.rs done
125 intxen.f INTXEN SUBROUTINE False BASICS|MODELQ YINT MODELQ|BASICS YINT False src/tlusty/math/interpolation/intxen.rs done
126 irc.f IRC SUBROUTINE True EXPINX|SZIRC EXPO|EINT|EXPINX|SZIRC False src/tlusty/math/utils/irc.rs done
127 iroset.f IROSET SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|LINED INKUL|QUIT|VOIGTE|LEVCD|IJALI2 MODELQ|COLKUR|LINED|ATOMIC|ODFPAR|BASICS INKUL|INDEXX|QUIT|VOIGTE|WN|LEVCD|IJALI2 True src/tlusty/io/iroset.rs done
128 kurucz.f KURUCZ SUBROUTINE False BASICS|ATOMIC|MODELQ|temlim LEVSOL|WNSTOR|QUIT|RHONEN|RATMAT|MOLEQ|SABOLF temlim|irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2 LEVSOL|REFLEV|OPFRAC|PFCNO|QUIT|RHONEN|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|WNSTOR|MPARTF|PFSPEC|ELDENS|PFHEAV|WN|PARTF|RATMAT|PFNI|ENTENE|LINEQS True src/tlusty/io/kurucz.rs done
129 lagran.f LAGRAN SUBROUTINE True False src/tlusty/math/interpolation/lagran.rs done
130 laguer.f LAGUER SUBROUTINE False True src/tlusty/math/solvers/laguer.rs done
131 lemini.f LEMINI SUBROUTINE False BASICS|MODELQ MODELQ|BASICS True src/tlusty/math/opacity/lemini.rs done
132 levcd.f LEVCD SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|COLKUR QUIT|WN|INDEXX ATOMIC|MODELQ|ODFPAR|BASICS|COLKUR QUIT|WN|INDEXX True src/tlusty/io/levcd.rs done
133 levgrp.f LEVGRP SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT ITERAT|ATOMIC|MODELQ|BASICS False src/tlusty/math/opacity/levgrp.rs done
134 levset.f LEVSET SUBROUTINE False BASICS|ATOMIC|MODELQ QUIT ATOMIC|MODELQ|BASICS QUIT False src/tlusty/math/opacity/levset.rs done
135 levsol.f LEVSOL SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT LINEQS ITERAT|ATOMIC|MODELQ|BASICS LINEQS False src/tlusty/math/opacity/levsol.rs done
136 lineqs.f LINEQS SUBROUTINE True BASICS BASICS False src/tlusty/math/solvers/lineqs.rs done
137 linpro.f LINPRO SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|quasun STARK0|VOIGT|DIVSTR|DOPGAM|INTLEM|STARKA|PROFSP|INTXEN irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|ODFPAR|BASICS VOIGT|OPFRAC|PFCNO|STARKA|PFFE|UBETA|YINT|INTHYD|INTXEN|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|DOPGAM|INTLEM|GAMSP|PARTF|PFNI|LAGRAN|PROFSP False src/tlusty/math/opacity/linpro.rs done
138 linsel.f LINSEL SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR OPAINI|QUIT|RTEFR1|OPACF1 callarda|irwint|AUXRTE|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|pfoptb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs REFLEV|SFFHMI|OPFRAC|PFCNO|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|YINT|CROSSD|CROSS|LINPRO|INTHYD|ALLARD|INTXEN|GFREE1|SABOLF|MATINV|WNSTOR|DIVSTR|PFHEAV|DOPGAM|RTEDF2|PFNI|LAGRAN|OPACT1|GAMI|QUASIM|CIA_H2HE|OPAINI|VOIGT|RTEFR1|SGMER0|STARKA|QUIT|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|MPARTF|YLINTP|PFSPEC|FFCROS|RTECF0|INTLEM|DWNFR0|CIA_H2H2|GHYDOP|WN|OPADD|GAMSP|PARTF|LOCATE|OPCTAB|PRD|DWNFR1|H2MINUS|PROFSP|LEVGRP|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/opacity/linsel.rs done
139 linset.f LINSET SUBROUTINE False BASICS|ATOMIC|MODELQ STARK0|DIVSTR|STARKA|QUIT|PROFIL|IJALIS irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|BASICS VOIGT|OPFRAC|PFCNO|STARKA|QUIT|PFFE|UBETA|PROFIL|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|PARTF|PFNI|LAGRAN|IJALIS|PROFSP True src/tlusty/io/linset.rs done
140 linspl.f LINSPL SUBROUTINE False BASICS|ATOMIC|MODELQ PROFIL irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|BASICS VOIGT|OPFRAC|PFCNO|STARKA|PFFE|UBETA|PROFIL|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|PARTF|PFNI|LAGRAN|PROFSP False src/tlusty/math/opacity/linspl.rs done
141 locate.f LOCATE SUBROUTINE True False src/tlusty/math/interpolation/locate.rs done
142 ltegr.f LTEGR SUBROUTINE False BASICS|ATOMIC|MODELQ WNSTOR|STEQEQ|QUIT|INTERP|ROSSOP|CONOUT|CONTMP irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ichndm|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|EXPINT|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|QUIT|ROSSOP|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|CUBIC|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CONTMP|CIA_H2HE|VOIGT|STARKA|INTERP|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP True src/tlusty/io/ltegr.rs done
143 ltegrd.f LTEGRD SUBROUTINE False BASICS|MODELQ|PRSAUX|TOTJHK|FLXAUX|FACTRS|CUBCON RADTOT|TEMPER|WNSTOR|STEQEQ|ELDENS|CONTMD|PSOLVE|QUIT|INTERP|NEWDM|GREYD|NEWDMT|HESOLV|CONOUT|ZMRHO callarda|irwint|tdedge|TOTJHK|adiaba|POPSTR|pfoptb|eospar|tdflag|FACTRS|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|calphatd|CC|derdif|ITERAT|BASICS|OPTDPT|intcfg|FLXAUX|PRSAUX|terden|AUXRTE|RAYSCT|COMFH1|moldat|quasun|ipricr|callardb|PFSTDS|entrop|TABLTD|comgfs|CONVOUT|auxcbc|adchar|callardg|SURFEX|ATOMIC|callardc|ODFPAR|ioniz2|CUBCON PRSENT|TEMPER|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|ERFCIN|RADTOT|RHOEOS|ELDENS|DOPGAM|RTEDF2|ENTENE|LINEQS|OPAINI|RTEFR1|SGMER0|RTEDF1|SGMER1|WN|NEWDM|OPADD|OPCTAB|PRD|OPACF0|REFLEV|HESOL6|PFCNO|YINT|INTXEN|GFREE1|SABOLF|BETAH|PSOLVE|TLOCAL|LAGRAN|GREYD|OPACT1|CIA_H2HE|LYMLIN|TDPINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|HESOLV|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RTESOL|RTEFE2|OPACF1|INTHYD|RUSSEL|MATINV|WNSTOR|GFREE0|ERFCX|PFNI|GAMI|QUASIM|QUIT|QUARTC|NEWDMT|CIA_HHE|YLINTP|PFSPEC|LOCATE|CUBIC|LEVGRP|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|DIVSTR|SETTRM|PFHEAV|VOIGT|CONTMD|STARKA|INTERP|RHONEN|MOLEQ|STATE|RAYLEIGH|ZMRHO|FFCROS|CIA_H2H2|RTECF0|INTLEM|RATMAT|GRIDP|RTECF1 True src/tlusty/io/ltegrd.rs done
144 lucy.f LUCY SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ITERAT|ALIPAR|ARRAY1 OPAINI|WNSTOR|STEQEQ|CONCOR|ODFMER|RTEFR1|TDPINI|ELCOR|OPACFL|SABOLF|COLIS irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|OPTDPT|terden|AUXRTE|COMFH1|RAYSCT|ARRAY1|moldat|quasun|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|comgfs|auxcbc|adchar|SURFEX|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|COLLHE|RTEFE2|PFFE|UBETA|EXPINX|ODFHYD|EINT|LINPRO|INTHYD|COLH|SZIRC|RUSSEL|ODFHST|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|RTEDF2|PFNI|ENTENE|IRC|LINEQS|OPAINI|INDEXX|EXPO|ODFMER|RTEFR1|SGMER0|QUIT|RTEDF1|CIA_HHE|SGMER1|CEH12|YLINTP|CONCOR|PFSPEC|TEMCOR|COLHE|WN|OPADD|LOCATE|OPCTAB|CION|LEVGRP|OPACF0|REFLEV|LEVSOL|OPFRAC|PFCNO|TRMDER|CONVEC|YINT|CROSSD|CROSS|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|HCTION|OPACFL|CIA_H2HE|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|TDPINI|MOLEQ|CHEAV|STATE|RAYLEIGH|TRMDRT|ELCOR|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|MEANOPT|RTECF0|INTLEM|DWNFR0|BUTLER|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP|RTESOL|RTECF1 True src/tlusty/math/temperature/lucy.rs done
145 lymlin.f LYMLIN SUBROUTINE False BASICS|ATOMIC|MODELQ STARKA|STARK0|DIVSTR ATOMIC|MODELQ|BASICS STARKA|STARK0|DIVSTR True src/tlusty/math/hydrogen/lymlin.rs done
146 matcon.f MATCON SUBROUTINE False BASICS|MODELQ|ARRAY1|CUBCON CONVEC irwint|terden|tdedge|COMFH1|adiaba|ARRAY1|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON PRSENT|OPFRAC|PFCNO|TRMDER|CONVEC|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS False src/tlusty/math/solvers/matcon.rs done
147 matgen.f MATGEN SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR MATCON|BHED|BHEZ|BHE|BRTEZ|BPOP|EMAT|BRTE|BRE|BREZ|SABOLF irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|CMATZD|terden|COMFH1|ARRAY1|moldat|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|SURFEX|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON PRSENT|COLLHE|BRTEZ|PFFE|EXPINX|EINT|COLH|RUSSEL|MATINV|RHOEOS|ELDENS|PFNI|ENTENE|IRC|LINEQS|EXPO|QUIT|BPOPE|BPOPC|BPOPT|SGMER1|CEH12|YLINTP|PFSPEC|BHEZ|BHE|COLHE|COMPT0|CION|BRTE|LEVGRP|LEVSOL|REFLEV|BHED|OPFRAC|PFCNO|TRMDER|CONVEC|EMAT|CROSS|BREZ|SABOLF|SETTRM|PFHEAV|HCTION|CHEAVJ|MATCON|COLIS|CSPEC|BPOPF|MOLEQ|STATE|TRMDRT|MPARTF|BUTLER|PARTF|BPOP|RATMAT|DWNFR1|BRE|SZIRC|CHEAV False src/tlusty/math/solvers/matgen.rs done
148 matinv.f MATINV SUBROUTINE True BASICS BASICS False src/tlusty/math/solvers/matinv.rs done
149 meanop.f MEANOP SUBROUTINE False BASICS|MODELQ|ATOMIC ATOMIC|MODELQ|BASICS False src/tlusty/math/opacity/meanop.rs done
150 meanopt.f MEANOPT SUBROUTINE False BASICS|MODELQ OPCTAB ATOMIC|MODELQ|eospar|BASICS|RAYSCT RAYLEIGH|OPCTAB False src/tlusty/math/opacity/meanopt.rs done
151 minv3.f MINV3 SUBROUTINE True False src/tlusty/math/solvers/minv3.rs done
152 moleq.f MOLEQ SUBROUTINE False BASICS|MODELQ|ATOMIC|hmolab|terden|COMFH1|moldat|entrop|eospar|ioniz2|adchar RUSSEL|MPARTF terden|MODELQ|hmolab|COMFH1|moldat|ATOMIC|entrop|eospar|BASICS|ioniz2|adchar RUSSEL|MPARTF True src/tlusty/math/eos/moleq.rs done
153 mpartf.f MPARTF SUBROUTINE False moldat moldat True src/tlusty/math/partition/mpartf.rs done
154 newdm.f NEWDM SUBROUTINE False BASICS|MODELQ|FACTRS|PRSAUX|FLXAUX TEMPER|INTERP|HESOLV irwint|tdedge|POPSTR|pfoptb|eospar|tdflag|FACTRS|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|ITERAT|BASICS|FLXAUX|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|adchar|ATOMIC|ODFPAR|ioniz2 PRSENT|TEMPER|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|QUARTC|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|TLOCAL|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|INTERP|RHONEN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|HESOLV|H2MINUS|PROFSP|DWNFR1|MEANOP True src/tlusty/math/utils/newdm.rs done
155 newdmt.f NEWDMT SUBROUTINE False BASICS|MODELQ|FACTRS|PRSAUX|FLXAUX GRIDP|TEMPER|INTERP|HESOLV irwint|tdedge|POPSTR|pfoptb|eospar|tdflag|FACTRS|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|ITERAT|BASICS|FLXAUX|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|adchar|ATOMIC|ODFPAR|ioniz2 PRSENT|TEMPER|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|QUARTC|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|OPCTAB|LOCATE|OPACF0|LEVSOL|REFLEV|OPFRAC|PFCNO|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|TLOCAL|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|INTERP|RHONEN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|GRIDP|RATMAT|HESOLV|H2MINUS|PROFSP|DWNFR1|MEANOP True src/tlusty/math/utils/newdmt.rs done
156 newpop.f NEWPOP SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT ITERAT|ATOMIC|MODELQ|BASICS True src/tlusty/math/population/newpop.rs done
157 nstout.f NSTOUT SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR QUIT ITERAT|ATOMIC|MODELQ|BASICS|ODFPAR|ALIPAR QUIT True src/tlusty/io/nstout.rs done
158 nstpar.f NSTPAR SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|irwint|deridt|freqcl|imucnn|temlim|adiaba|moldat|quasun|ichndm|ipricr|derdif|ifpzpa|hediff|icnrsp|FLXAUX GETLAL|QUIT|GETWRD callarda|irwint|deridt|temlim|imucnn|adiaba|moldat|quasun|ipricr|callardb|icnrsp|ALIPAR|MODELQ|freqcl|callardg|calphatd|ichndm|derdif|ITERAT|ifpzpa|ATOMIC|hediff|callardc|BASICS|ODFPAR|FLXAUX GETWRD|GETLAL|QUIT True src/tlusty/io/nstpar.rs done
159 odf1.f ODF1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR SIGK|DIVSTR|ODFHST ATOMIC|MODELQ|ODFPAR|BASICS|TOPB SBFHE1|SPSIGK|REIMAN|HIDALG|QUIT|VERN18|SGHE12|CKOEST|HEPHOT|VERN16|VERN20|ODFHST|VERNER|TOPBAS|DIVSTR|YLINTP|SBFHMI|VERN26|CARBON|GAUNT|OPDATA|SIGK True src/tlusty/math/odf/odf1.rs done
160 odffr.f ODFFR SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR QUIT ODFPAR|ATOMIC|MODELQ|BASICS QUIT False src/tlusty/math/odf/odffr.rs done
161 odfhst.f ODFHST SUBROUTINE False BASICS|MODELQ|ODFPAR ODFPAR|MODELQ|BASICS False src/tlusty/math/odf/odfhst.rs done
162 odfhyd.f ODFHYD SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR INDEXX|DIVSTR|ODFHST ATOMIC|MODELQ|ODFPAR|BASICS INDEXX|DIVSTR|ODFHST False src/tlusty/math/odf/odfhyd.rs done
163 odfhys.f ODFHYS SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR IJALIS|STARK0|ODFFR ATOMIC|MODELQ|ODFPAR|BASICS STARK0|QUIT|ODFFR|IJALIS False src/tlusty/math/odf/odfhys.rs done
164 odfmer.f ODFMER SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR ODFHYD MODELQ|ATOMIC|ODFPAR|BASICS ODFHYD|INDEXX|DIVSTR|ODFHST False src/tlusty/math/odf/odfmer.rs done
165 odfset.f ODFSET SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|STFCR QUIT|IJALIS STFCR|ATOMIC|MODELQ|ODFPAR|BASICS QUIT|IJALIS True src/tlusty/io/odfset.rs done
166 opacf0.f OPACF0 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|hmolab WNSTOR|GFREE0|SFFHMI|FFCROS|DWNFR0|OPADD|OPACT1|CROSS|CROSSD|LINPRO|DWNFR1|SGMER1|SABOLF irwint|RAYSCT|moldat|quasun|PFSTDS|pfoptb|eospar|ALIPAR|MODELQ|hmolab|ATOMIC|ODFPAR|BASICS SFFHMI|OPFRAC|CIA_H2H|PFCNO|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|SABOLF|WNSTOR|GFREE0|DIVSTR|PFHEAV|DOPGAM|PFNI|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|MPARTF|PFSPEC|INTLEM|DWNFR0|OPADD|WN|GAMSP|LOCATE|OPCTAB|PARTF|H2MINUS|PROFSP|DWNFR1 False src/tlusty/math/continuum/opacf0.rs done
167 opacf1.f OPACF1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|hmolab|ipricr SFFHMI|FFCROS|QUASIM|GHYDOP|LYMLIN|OPADD|PRD|OPACT1|CROSS|CROSSD|GFREE1|DWNFR1|SGMER1 callarda|RAYSCT|quasun|ipricr|callardb|eospar|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|intcfg SFFHMI|QUASIM|STARKA|CIA_H2H|LYMLIN|CROSSD|CROSS|ALLARD|RAYLEIGH|CIA_HHE|GFREE1|SGMER1|STARK0|YLINTP|FFCROS|DIVSTR|CIA_H2H2|GHYDOP|DOPGAM|OPADD|GAMSP|LOCATE|OPCTAB|PRD|OPACT1|H2MINUS|GAMI|DWNFR1|ALLARDT|CIA_H2HE True src/tlusty/math/continuum/opacf1.rs done
168 opacfa.f OPACFA SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|COOLCO SFFHMI|FFCROS|OPADD|PRD|CROSSD|CROSS|DWNFR1|SGMER1 MODELQ|COOLCO|ITERAT|ATOMIC|eospar|ODFPAR|BASICS|ALIPAR SFFHMI|YLINTP|FFCROS|CIA_H2H2|CIA_H2H|DOPGAM|OPADD|GAMSP|LOCATE|PRD|CROSSD|CROSS|H2MINUS|GAMI|DWNFR1|CIA_HHE|SGMER1|CIA_H2HE False src/tlusty/math/continuum/opacfa.rs done
169 opacfd.f OPACFD SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT|rhoder|hmolab|dsctva SFFHMI|FFCROS|GFREED|QUASIM|LYMLIN|OPADD|OPCTAB|PRD|CROSSD|CROSS|OPACTD|DWNFR1|SGMER1 callarda|RAYSCT|ARRAY1|quasun|callardb|eospar|ALIPAR|rhoder|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|dsctva|ODFPAR|BASICS SFFHMI|QUASIM|STARKA|CIA_H2H|LYMLIN|CROSSD|CROSS|ALLARD|OPACTD|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|GFREED|DIVSTR|CIA_H2H2|DOPGAM|OPADD|GAMSP|OPCTAB|LOCATE|PRD|H2MINUS|GAMI|DWNFR1|ALLARDT|CIA_H2HE True src/tlusty/math/continuum/opacfd.rs done
170 opacfl.f OPACFL SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR SFFHMI|FFCROS|OPADD|CROSSD|CROSS|DWNFR1|SGMER1 MODELQ|ATOMIC|eospar|ODFPAR|BASICS|ALIPAR SFFHMI|YLINTP|FFCROS|CIA_H2H2|CIA_H2H|OPADD|LOCATE|CROSSD|CROSS|H2MINUS|DWNFR1|CIA_HHE|SGMER1|CIA_H2HE False src/tlusty/math/continuum/opacfl.rs done
171 opact1.f OPACT1 SUBROUTINE False BASICS|MODELQ|ALIPAR|hmolab OPCTAB MODELQ|hmolab|RAYSCT|ATOMIC|eospar|BASICS|ALIPAR RAYLEIGH|OPCTAB False src/tlusty/math/continuum/opact1.rs done
172 opactd.f OPACTD SUBROUTINE False BASICS|MODELQ|ALIPAR|ARRAY1|ITERAT|rhoder|hmolab|dsctva OPCTAB rhoder|MODELQ|hmolab|RAYSCT|ARRAY1|ITERAT|ATOMIC|eospar|dsctva|BASICS|ALIPAR RAYLEIGH|OPCTAB False src/tlusty/math/continuum/opactd.rs done
173 opactr.f OPACTR SUBROUTINE False BASICS|MODELQ|ALIPAR|ATOMIC|grdpra|hmolab|dsctva LEVSOL|OPAINI|WNSTOR|STEQEQ|PGSET|ELDENS|TDPINI|OPACF1|RATMAL|SABOLF callarda|irwint|POPSTR|pfoptb|eospar|PPAPAR|ALIPAR|MODELQ|hmolab|calphatd|rybpgs|ITERAT|BASICS|intcfg|terden|COMFH1|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|entrop|adchar|grdpra|callardg|ATOMIC|callardc|dsctva|ODFPAR|ioniz2 SFFHMI|CIA_H2H|PFFE|UBETA|OPACF1|LINPRO|INTHYD|RUSSEL|WNSTOR|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|GAMI|QUASIM|LINEQS|OPAINI|SGMER0|TRIDAG|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|LOCATE|OPCTAB|PRD|RATMAL|LEVGRP|LEVSOL|REFLEV|PGSET|OPFRAC|PFCNO|YINT|CROSSD|CROSS|ALLARD|INTXEN|GFREE1|SABOLF|DIVSTR|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|LYMLIN|TDPINI|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|GHYDOP|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|ALLARDT False src/tlusty/math/continuum/opactr.rs done
174 opadd.f OPADD SUBROUTINE False BASICS|ATOMIC|MODELQ|eospar SFFHMI|CIA_H2H2|CIA_H2H|CROSS|H2MINUS|CIA_HHE|CIA_H2HE ATOMIC|MODELQ|eospar|BASICS SFFHMI|YLINTP|CIA_H2H2|CIA_H2H|LOCATE|CROSS|H2MINUS|CIA_HHE|CIA_H2HE False src/tlusty/math/continuum/opadd.rs done
175 opadd0.f OPADD0 SUBROUTINE False BASICS|ATOMIC|MODELQ QUIT ATOMIC|MODELQ|BASICS QUIT False src/tlusty/math/continuum/opadd0.rs done
176 opahst.f OPAHST SUBROUTINE False BASICS|ODFPAR STARK0 ODFPAR|BASICS STARK0 True src/tlusty/math/continuum/opahst.rs done
177 opaini.f OPAINI SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR REFLEV|WNSTOR|SGMER0|DWNFR0|LINPRO|LEVGRP|SABOLF irwint|MODELQ|moldat|quasun|PFSTDS|ITERAT|ATOMIC|pfoptb|ODFPAR|BASICS|ALIPAR REFLEV|VOIGT|OPFRAC|SGMER0|PFCNO|STARKA|PFFE|UBETA|YINT|LINPRO|INTHYD|INTXEN|SABOLF|STARK0|WNSTOR|DIVSTR|MPARTF|PFSPEC|PFHEAV|DOPGAM|DWNFR0|INTLEM|WN|GAMSP|PARTF|PFNI|LAGRAN|PROFSP|LEVGRP False src/tlusty/math/continuum/opaini.rs done
178 opctab.f OPCTAB SUBROUTINE False BASICS|MODELQ RAYLEIGH ATOMIC|MODELQ|eospar|BASICS|RAYSCT RAYLEIGH False src/tlusty/math/continuum/opctab.rs done
179 opdata.f OPDATA SUBROUTINE False TOPB TOPB True src/tlusty/math/continuum/opdata.rs done
180 opfrac.f OPFRAC SUBROUTINE False pfoptb pfoptb True src/tlusty/math/continuum/opfrac.rs done
181 osccor.f OSCCOR SUBROUTINE False BASICS|MODELQ|ITERAT ITERAT|MODELQ|BASICS True src/tlusty/math/temperature/osccor.rs done
182 outpri.f OUTPRI SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|grdpra LEVSOL|WNSTOR|OPACF1|RATMAL|SABOLF|ELDENC callarda|irwint|pfoptb|eospar|eletab|ALIPAR|MODELQ|hmolab|calphatd|ITERAT|BASICS|intcfg|terden|RAYSCT|COMFH1|ARRAY1|moldat|quasun|ipricr|callardb|PFSTDS|entrop|adchar|grdpra|callardg|ATOMIC|callardc|ODFPAR|ioniz2 LEVSOL|SFFHMI|OPFRAC|CIA_H2H|PFCNO|PFFE|OPACF1|CROSSD|CROSS|ALLARD|RUSSEL|GFREE1|SABOLF|ELDENC|WNSTOR|DIVSTR|PFHEAV|DOPGAM|ELDENS|PFNI|OPACT1|ENTENE|GAMI|QUASIM|LINEQS|CIA_H2HE|STARKA|LYMLIN|RHONEN|MOLEQ|STATE|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|MPARTF|GHYDOP|PFSPEC|WN|OPADD|GAMSP|LOCATE|OPCTAB|PRD|PARTF|RATMAL|H2MINUS|DWNFR1|ALLARDT True src/tlusty/io/outpri.rs done
183 output.f OUTPUT SUBROUTINE False BASICS|MODELQ MODELQ|BASICS True src/tlusty/math/io/output.rs done
184 partf.f PARTF SUBROUTINE False BASICS|irwint|PFSTDS MPARTF|PFSPEC|OPFRAC|PFCNO|PFHEAV|PFFE|PFNI irwint|pfoptb|BASICS|moldat|PFSTDS MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PFNI False src/tlusty/math/partition/partf.rs done
185 pfcno.f PFCNO SUBROUTINE True BASICS BASICS False src/tlusty/math/partition/pfcno.rs done
186 pffe.f PFFE SUBROUTINE True False src/tlusty/math/partition/pffe.rs done
187 pfheav.f PFHEAV SUBROUTINE False True src/tlusty/math/partition/pfheav.rs done
188 pfni.f PFNI SUBROUTINE True False src/tlusty/math/partition/pfni.rs done
189 pfspec.f PFSPEC SUBROUTINE True False src/tlusty/math/partition/pfspec.rs done
190 pgset.f PGSET SUBROUTINE False BASICS|ITERAT|MODELQ|grdpra|rybpgs TRIDAG ITERAT|grdpra|MODELQ|BASICS|rybpgs TRIDAG True src/tlusty/math/utils/pgset.rs done
191 prchan.f PRCHAN SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT ITERAT|ATOMIC|MODELQ|BASICS True src/tlusty/math/io/prchan.rs done
192 prd.f PRD SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT DOPGAM|GAMI ITERAT|ATOMIC|MODELQ|BASICS DOPGAM|GAMI|GAMSP False src/tlusty/math/opacity/prd.rs done
193 prdini.f PRDINI SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/opacity/prdini.rs done
194 princ.f PRINC SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR OPACF1|DWNFR|CROSS|LINPRO|SABOLF callarda|irwint|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|pfoptb|eospar|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|intcfg SFFHMI|OPFRAC|CIA_H2H|PFCNO|PFFE|UBETA|OPACF1|CROSSD|CROSS|YINT|LINPRO|ALLARD|INTHYD|INTXEN|GFREE1|SABOLF|DIVSTR|PFHEAV|DOPGAM|PFNI|LAGRAN|OPACT1|GAMI|QUASIM|CIA_H2HE|VOIGT|STARKA|LYMLIN|DWNFR|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|MPARTF|GHYDOP|PFSPEC|INTLEM|OPADD|GAMSP|LOCATE|OPCTAB|PRD|PARTF|H2MINUS|PROFSP|DWNFR1|ALLARDT True src/tlusty/math/io/princ.rs done
195 prnt.f PRNT SUBROUTINE False BASICS|ATOMIC|MODELQ SABOLF irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PARTF|PFNI|SABOLF True src/tlusty/math/io/prnt.rs done
196 profil.f PROFIL FUNCTION False BASICS|ATOMIC|MODELQ|quasun STARK0|VOIGT|DIVSTR|STARKA|PROFSP irwint|MODELQ|moldat|quasun|PFSTDS|ATOMIC|pfoptb|BASICS STARK0|VOIGT|DIVSTR|MPARTF|PFSPEC|OPFRAC|PFHEAV|STARKA|PFCNO|PFFE|UBETA|PARTF|PFNI|LAGRAN|PROFSP|SABOLF False src/tlusty/math/opacity/profil.rs done
197 profsp.f PROFSP FUNCTION False BASICS|ATOMIC|MODELQ VOIGT|SABOLF|UBETA irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS VOIGT|MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|UBETA|PARTF|PFNI|LAGRAN|SABOLF False src/tlusty/math/opacity/profsp.rs done
198 prsent.f PRSENT SUBROUTINE False TABLTD|tdedge|THERM|tdflag TABLTD|tdedge|THERM|tdflag True src/tlusty/math/io/prsent.rs done
199 psolve.f PSOLVE SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/solvers/psolve.rs done
200 pzert.f PZERT SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/io/pzert.rs done
201 pzeval.f PZEVAL SUBROUTINE False BASICS|MODELQ|ALIPAR|icnrsp CONOUT|CONREF irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|imucnn|RAYSCT|COMFH1|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|icnrsp|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON PRSENT|SFFHMI|CIA_H2H|PFFE|UBETA|LINPRO|INTHYD|RUSSEL|WNSTOR|RHOEOS|GFREE0|ELDENS|DOPGAM|PFNI|ENTENE|LINEQS|CIA_HHE|SGMER1|YLINTP|PFSPEC|OPADD|WN|OPCTAB|LOCATE|CONREF|OPACF0|LEVSOL|REFLEV|CONVC1|OPFRAC|PFCNO|TRMDER|CONVEC|CROSSD|CROSS|YINT|INTXEN|SABOLF|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|TDPINI|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MEANOPT|MPARTF|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|CONOUT|MEANOP True src/tlusty/math/io/pzeval.rs done
202 pzevld.f PZEVLD SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR|ARRAY1|DEPTDR|grdpra|ifpzpa|PRSAUX grdpra|MODELQ|DEPTDR|PRSAUX|ARRAY1|ifpzpa|ATOMIC|BASICS|ALIPAR False src/tlusty/math/io/pzevld.rs done
203 quartc.f QUARTC SUBROUTINE False True src/tlusty/math/solvers/quartc.rs done
204 quasim.f QUASIM SUBROUTINE False BASICS|ATOMIC|MODELQ|quasun ALLARD callarda|MODELQ|callardg|calphatd|quasun|callardb|ATOMIC|callardc|BASICS ALLARDT|ALLARD False src/tlusty/math/opacity/quasim.rs done
205 quit.f QUIT SUBROUTINE False True src/tlusty/math/io/quit.rs done
206 radpre.f RADPRE SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR INDEXX|QUIT|RTEFR1|OPACF1 callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|INDEXX|RTEFR1|STARKA|QUIT|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/radiative/radpre.rs done
207 radtot.f RADTOT SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT|OPTDPT|TOTJHK|SURFEX OPAINI|OPACF1|RTEFR1|TDPINI callarda|irwint|AUXRTE|RAYSCT|TOTJHK|moldat|quasun|ipricr|callardb|PFSTDS|pfoptb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs REFLEV|SFFHMI|OPFRAC|PFCNO|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|YINT|CROSSD|CROSS|LINPRO|INTHYD|ALLARD|INTXEN|GFREE1|SABOLF|MATINV|WNSTOR|DIVSTR|GFREE0|PFHEAV|DOPGAM|RTEDF2|PFNI|LAGRAN|OPACT1|GAMI|QUASIM|CIA_H2HE|OPAINI|VOIGT|RTEFR1|SGMER0|STARKA|LYMLIN|TDPINI|RAYLEIGH|CIA_HHE|SGMER1|RTEDF1|STARK0|MPARTF|YLINTP|PFSPEC|FFCROS|CIA_H2H2|INTLEM|DWNFR0|GHYDOP|RTECF0|WN|OPADD|GAMSP|PARTF|LOCATE|OPCTAB|PRD|DWNFR1|H2MINUS|PROFSP|LEVGRP|ALLARDT|RTESOL|RTECF1 False src/tlusty/math/radiative/radtot.rs done
208 raph.f RAPH FUNCTION True False src/tlusty/math/solvers/raph.rs done
209 rates1.f RATES1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ITERAT ROSSTD|CROSS|RTEFR1|OPACF1 callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 False src/tlusty/math/rates/rates1.rs done
210 ratmal.f RATMAL SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/rates/ratmal.rs done
211 ratmat.f RATMAT SUBROUTINE False BASICS|ATOMIC|MODELQ REFLEV ITERAT|ATOMIC|MODELQ|BASICS REFLEV False src/tlusty/math/rates/ratmat.rs done
212 ratsp1.f RATSP1 SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR|ARRAY1|ITERAT ROSSTD|CROSS|RTEFR1|OPACF1 callarda|AUXRTE|RAYSCT|ARRAY1|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|ODFPAR|BASICS|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|ROSSTD|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/rates/ratsp1.rs done
213 rayini.f RAYINI SUBROUTINE False BASICS|MODELQ|ATOMIC RAYLEIGH|RAYSET MODELQ|RAYSCT|ATOMIC|eospar|BASICS RAYLEIGH|RAYSET True src/tlusty/io/rayini.rs done
214 rayleigh.f RAYLEIGH SUBROUTINE False BASICS|ATOMIC|MODELQ|eospar|RAYSCT ATOMIC|MODELQ|eospar|RAYSCT|BASICS False src/tlusty/math/opacity/rayleigh.rs done
215 rayset.f RAYSET SUBROUTINE False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/opacity/rayset.rs done
216 rdata.f RDATA SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ODFPAR|ALIPAR|STRPAR|INUNIT|imodlc LEMINI|DOPGAM|XENINI|QUIT|RDATAX|LINSET irwint|MODELQ|imodlc|moldat|quasun|PFSTDS|ITERAT|ATOMIC|pfoptb|BASICS|ODFPAR|STRPAR|INUNIT|ALIPAR VOIGT|LEMINI|OPFRAC|PFCNO|XENINI|STARKA|QUIT|BKHSGO|PFFE|UBETA|PROFIL|SABOLF|STARK0|DIVSTR|MPARTF|PFSPEC|PFHEAV|DOPGAM|RDATAX|LINSET|GAMSP|PARTF|PFNI|LAGRAN|IJALIS|PROFSP True src/tlusty/math/io/rdata.rs done
217 rdatax.f RDATAX SUBROUTINE False BASICS|ATOMIC|MODELQ BKHSGO ATOMIC|MODELQ|BASICS BKHSGO True src/tlusty/math/io/rdatax.rs done
218 readbf.f READBF SUBROUTINE False BASICS BASICS True src/tlusty/math/io/readbf.rs done
219 rechck.f RECHCK SUBROUTINE False BASICS|ATOMIC|MODELQ RTEFR1|OPACF1 callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|EXTINT|auxcbc|ALIPAR|MODELQ|hmolab|callardg|SURFEX|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|RTEDF2|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|RTEFR1|STARKA|LYMLIN|RTEDF1|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/io/rechck.rs done
220 reflev.f REFLEV SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT ITERAT|ATOMIC|MODELQ|BASICS False src/tlusty/math/opacity/reflev.rs done
221 reiman.f REIMAN FUNCTION True False src/tlusty/math/opacity/reiman.rs done
222 resolv.f RESOLV SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ALIPAR|ARRAY1|icnrsp HESOL6|RAYSET|PRINC|NEWPOP|OPACF1|LUCY|ALISK2|ALIST1|TAUFR1|LINSEL|ROSSTD|CHCKSE|RTECMU|RTECOM|TIMING|PZEVLD|DMEVAL|COOLRT|ALIST2|OUTPRI|OUTPUT|RTEINT|OPAINI|RATSP1|PZERT|RTEFR1|RECHCK|ACCELP|RATES1|PZEVAL|ELCOR|STEQEQ|RYBHEQ|PRD|CONREF|CONOUT|INILAM|RADPRE DEPTDR|tdedge|POPSTR|pfoptb|tdflag|POPULS|PPAPAR|eletab|rhoder|MODELQ|THERM|calphatd|CC|derdif|rybpgs|BASICS|intcfg|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|grdpra|SURFEX|ADCHAR|ODFPAR|ioniz2|dsctva|CUBCON|callarda|irwint|adiaba|eospar|EXTINT|ALIPAR|hmolab|ITERAT|CTIon|OPTDPT|PRSAUX|COOLCO|COMFH1|imucnn|ARRAY1|moldat|CTRTEMP|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|callardg|ifpzpa|ATOMIC|callardc|comgfs PRSENT|SFFHMI|ANGSET|CIA_H2H|COLLHE|PFFE|UBETA|EXPINX|EINT|LINPRO|ALISK2|RHOEOS|RTECOM|DOPGAM|ELDENS|RTEDF2|ENTENE|IRC|LINEQS|OPAINI|ODFMER|RTEFR1|SGMER0|GAULEG|TRIDAG|RTEDF1|SGMER1|CEH12|TEMCOR|COLHE|OPADD|WN|OPCTAB|PRD|CION|CONREF|OPACF0|REFLEV|HESOL6|PGSET|RAYSET|PFCNO|OPACFA|YINT|LUCY|ALIST1|TAUFR1|INTXEN|GFREE1|SABOLF|ELDENC|PZEVLD|LAGRAN|DMEVAL|OPACT1|RTEINT|CIA_H2HE|RATSP1|PZERT|LYMLIN|TDPINI|VISINI|TRMDRT|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|DWNFR0|GAMSP|PARTF|OPACFD|H2MINUS|PROFSP|DWNFR1|ALLARDT|CONOUT|MEANOP|RADPRE|CHEAV|RTESOL|PRINC|RTEFE2|OPACF1|ODFHYD|INTHYD|COLH|OPACTD|RUSSEL|ODFHST|MATINV|WNSTOR|GFREE0|ALIFR3|TIMING|PFNI|ALIFR1|GAMI|ALIST2|QUASIM|OUTPUT|INDEXX|EXPO|RECHCK|OSCCOR|ACCELP|QUIT|CIA_HHE|COMSET|YLINTP|CONCOR|PFSPEC|GFREED|LOCATE|RATMAL|LEVGRP|INILAM|LEVSOL|CONVC1|OPFRAC|TRMDER|CONVEC|NEWPOP|ALIFRK|CROSSD|CROSS|ALLARD|RTECMC|LINSEL|ROSSTD|DIVSTR|CHCKSE|RTECMU|PFHEAV|SETTRM|DIELRC|COOLRT|HCTION|OUTPRI|OPACFL|COLIS|CHEAVJ|VOIGT|STARKA|CSPEC|RHONEN|DWNFR|RATES1|MOLEQ|STATE|RAYLEIGH|PZEVAL|ELCOR|RYBHEQ|FFCROS|CIA_H2H2|RTECF0|INTLEM|BUTLER|RATMAT|DIETOT|SZIRC|RTECF1 True src/tlusty/io/resolv.rs done
223 rhoeos.f RHOEOS FUNCTION False BASICS|MODELQ PRSENT|SETTRM MODELQ|tdedge|THERM|TABLTD|BASICS|tdflag PRSENT|SETTRM False src/tlusty/math/eos/rhoeos.rs done
224 rhonen.f RHONEN SUBROUTINE False BASICS|MODELQ ELDENS irwint|terden|COMFH1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|ATOMIC|BASICS|ioniz2 MPARTF|OPFRAC|PFSPEC|ELDENS|PFHEAV|PFCNO|PFFE|PARTF|PFNI|MOLEQ|ENTENE|STATE|RUSSEL|LINEQS False src/tlusty/math/eos/rhonen.rs done
225 rhsgen.f RHSGEN SUBROUTINE False BASICS|ATOMIC|MODELQ|ARRAY1|ALIPAR|CUBCON MATINV|CONVEC|COMPT0|RATMAT|STATE|LEVGRP|SABOLF irwint|terden|tdedge|COMFH1|adiaba|ARRAY1|moldat|PFSTDS|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|auxcbc|adchar|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|ATOMIC|BASICS|ioniz2|CUBCON REFLEV|PRSENT|OPFRAC|PFCNO|TRMDER|CONVEC|PFFE|MOLEQ|STATE|RUSSEL|SABOLF|TRMDRT|MATINV|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|COMPT0|RATMAT|PARTF|PFNI|ENTENE|LEVGRP|LINEQS False src/tlusty/math/solvers/rhsgen.rs done
226 rossop.f ROSSOP SUBROUTINE False BASICS|ATOMIC|MODELQ|ALIPAR WNSTOR|STEQEQ|MEANOPT|RHOEOS|ELDENS|MEANOP|EXPINT|OPACF0 irwint|terden|tdedge|COMFH1|RAYSCT|moldat|quasun|PFSTDS|POPSTR|entrop|eospar|pfoptb|TABLTD|tdflag|PPAPAR|adchar|ALIPAR|MODELQ|hmolab|THERM|ITERAT|ATOMIC|BASICS|ioniz2|ODFPAR LEVSOL|REFLEV|PRSENT|SFFHMI|OPFRAC|PFCNO|CIA_H2H|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|RUSSEL|EXPINT|SABOLF|WNSTOR|RHOEOS|GFREE0|SETTRM|DIVSTR|ELDENS|PFHEAV|DOPGAM|PFNI|LAGRAN|ENTENE|OPACT1|LINEQS|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|CIA_HHE|SGMER1|STARK0|STEQEQ|MEANOPT|MPARTF|PFSPEC|YLINTP|FFCROS|CIA_H2H2|INTLEM|DWNFR0|WN|OPADD|GAMSP|PARTF|RATMAT|OPCTAB|LOCATE|H2MINUS|PROFSP|DWNFR1|MEANOP|OPACF0 False src/tlusty/math/temperature/rossop.rs done
227 rosstd.f ROSSTD SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|ALIPAR ITERAT|ATOMIC|MODELQ|BASICS|ALIPAR True src/tlusty/math/temperature/rosstd.rs done
228 rte_sc.f RTE_SC SUBROUTINE True BASICS BASICS False src/tlusty/math/radiative/rte_sc.rs done
229 rteang.f RTEANG SUBROUTINE False BASICS|MODELQ|ALIPAR|EXTINT|SURFEX GAULEG MODELQ|BASICS|SURFEX|EXTINT|ALIPAR GAULEG False src/tlusty/math/radiative/rteang.rs done
230 rtecf0.f RTECF0 SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT|auxcbc|AUXRTE ITERAT|MODELQ|AUXRTE|BASICS|OPTDPT|auxcbc|ALIPAR False src/tlusty/math/radiative/rtecf0.rs done
231 rtecf1.f RTECF1 SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|AUXRTE|SURFEX|OPTDPT|EXTINT|comgfs RTEFE2|RTESOL|RTECF0 MODELQ|AUXRTE|SURFEX|ITERAT|BASICS|OPTDPT|EXTINT|auxcbc|comgfs|ALIPAR RTEFE2|RTESOL|RTECF0 True src/tlusty/math/radiative/rtecf1.rs done
232 rtecmc.f RTECMC SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|AUXRTE|comgfs MATINV|RTECF0|OPACF1 callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|auxcbc|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg|comgfs SFFHMI|CIA_H2H|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT False src/tlusty/math/radiative/rtecmc.rs done
233 rtecmu.f RTECMU SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT|AUXRTE RTECF0|GAULEG|RTESOL|OPACF1 callarda|AUXRTE|RAYSCT|quasun|ipricr|callardb|eospar|auxcbc|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg SFFHMI|CIA_H2H|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|GAULEG|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL True src/tlusty/math/radiative/rtecmu.rs done
234 rtecom.f RTECOM SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT|AUXRTE|comgfs RTECF0|RTECF1|RTECMC|OPACF1 callarda|eospar|EXTINT|ALIPAR|MODELQ|hmolab|calphatd|ITERAT|BASICS|OPTDPT|intcfg|AUXRTE|RAYSCT|quasun|ipricr|callardb|auxcbc|callardg|SURFEX|ATOMIC|callardc|ODFPAR|comgfs SFFHMI|CIA_H2H|RTEFE2|OPACF1|CROSSD|CROSS|ALLARD|RTECMC|GFREE1|MATINV|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|RTECF0|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT|RTESOL|RTECF1 False src/tlusty/math/radiative/rtecom.rs done
235 rtedf1.f RTEDF1 SUBROUTINE False BASICS|MODELQ|ALIPAR|OPTDPT OPTDPT|MODELQ|BASICS|ALIPAR False src/tlusty/math/radiative/rtedf1.rs done
236 rtedf2.f RTEDF2 SUBROUTINE False BASICS|MODELQ|ALIPAR MODELQ|BASICS|ALIPAR False src/tlusty/math/radiative/rtedf2.rs done
237 rtefe2.f RTEFE2 SUBROUTINE True BASICS BASICS False src/tlusty/math/radiative/rtefe2.rs done
238 rtefr1.f RTEFR1 SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT MATINV|RTEDF2|RTEDF1|RTESOL|RTECF1 MODELQ|AUXRTE|SURFEX|ITERAT|BASICS|OPTDPT|EXTINT|auxcbc|comgfs|ALIPAR MATINV|RTECF0|RTEDF2|RTEFE2|RTEDF1|RTESOL|RTECF1 True src/tlusty/math/radiative/rtefr1.rs done
239 rteint.f RTEINT SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT MATINV|OPACF1 callarda|RAYSCT|quasun|ipricr|callardb|eospar|ALIPAR|MODELQ|hmolab|callardg|calphatd|ITERAT|ATOMIC|callardc|BASICS|ODFPAR|OPTDPT|intcfg SFFHMI|CIA_H2H|OPACF1|CROSSD|CROSS|ALLARD|GFREE1|MATINV|DIVSTR|DOPGAM|OPACT1|GAMI|QUASIM|CIA_H2HE|STARKA|LYMLIN|RAYLEIGH|CIA_HHE|SGMER1|STARK0|YLINTP|FFCROS|CIA_H2H2|GHYDOP|OPADD|GAMSP|LOCATE|OPCTAB|PRD|H2MINUS|DWNFR1|ALLARDT True src/tlusty/math/radiative/rteint.rs done
240 rtesol.f RTESOL SUBROUTINE True BASICS BASICS False src/tlusty/math/radiative/rtesol.rs done
241 russel.f RUSSEL SUBROUTINE False BASICS|MODELQ|COMFH1 MPARTF moldat|MODELQ|COMFH1|BASICS MPARTF True src/tlusty/math/eos/russel.rs done
242 rybchn.f RYBCHN SUBROUTINE False BASICS|ITERAT|MODELQ|ALIPAR|ARRAY1|grdpra|rybpgs PGSET|ELDENS irwint|terden|COMFH1|ARRAY1|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|ALIPAR|grdpra|MODELQ|hmolab|rybpgs|ITERAT|ATOMIC|BASICS|ioniz2 PGSET|OPFRAC|PFCNO|PFFE|MOLEQ|STATE|TRIDAG|RUSSEL|MPARTF|PFSPEC|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS True src/tlusty/math/solvers/rybchn.rs done
243 rybene.f RYBENE SUBROUTINE False BASICS|MODELQ|ALIPAR|ARRAY1|RYBMTX|deridt|CUBCON CONVEC deridt|irwint|terden|tdedge|COMFH1|adiaba|ARRAY1|moldat|PFSTDS|RYBMTX|entrop|pfoptb|eospar|TABLTD|CONVOUT|tdflag|adchar|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ATOMIC|BASICS|ioniz2|CUBCON PRSENT|OPFRAC|PFCNO|TRMDER|CONVEC|PFFE|MOLEQ|STATE|RUSSEL|TRMDRT|MPARTF|RHOEOS|PFSPEC|SETTRM|ELDENS|PFHEAV|PARTF|PFNI|ENTENE|LINEQS False src/tlusty/math/solvers/rybene.rs done
244 rybheq.f RYBHEQ SUBROUTINE False BASICS|MODELQ|grdpra|rybpgs OPAINI|WNSTOR|STEQEQ|PGSET|RTEFR1|ELDENS|OPACF1 callarda|irwint|POPSTR|pfoptb|eospar|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|calphatd|rybpgs|ITERAT|BASICS|OPTDPT|intcfg|terden|AUXRTE|COMFH1|RAYSCT|moldat|quasun|ipricr|callardb|PFSTDS|entrop|auxcbc|adchar|grdpra|callardg|SURFEX|ATOMIC|callardc|ODFPAR|ioniz2|comgfs SFFHMI|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|ELDENS|DOPGAM|RTEDF2|PFNI|ENTENE|GAMI|QUASIM|LINEQS|OPAINI|RTEFR1|SGMER0|TRIDAG|RTEDF1|CIA_HHE|SGMER1|YLINTP|PFSPEC|WN|OPADD|LOCATE|OPCTAB|PRD|LEVGRP|REFLEV|LEVSOL|PGSET|OPFRAC|PFCNO|YINT|CROSSD|CROSS|ALLARD|INTXEN|GFREE1|SABOLF|DIVSTR|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|VOIGT|STARKA|LYMLIN|MOLEQ|STATE|RAYLEIGH|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|RTECF0|INTLEM|DWNFR0|GHYDOP|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/solvers/rybheq.rs done
245 rybmat.f RYBMAT SUBROUTINE False BASICS|MODELQ|ALIPAR|ARRAY1|RYBMTX|dsctva RYBMTX|MODELQ|dsctva|BASICS|ARRAY1|ALIPAR False src/tlusty/math/solvers/rybmat.rs done
246 rybsol.f RYBSOL SUBROUTINE False BASICS|MODELQ|ATOMIC|ALIPAR|ARRAY1|ITERAT|RYBMTX|imodlc SETDRT|STEQEQ|ROSSTD|RTEFR1|OPACTR|RYBCHN|RYBENE|ALIFR1|RYBMAT|LEVSET|TRIDAG|LINEQS callarda|irwint|deridt|tdedge|imodlc|adiaba|RYBMTX|POPSTR|pfoptb|eospar|tdflag|EXTINT|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|calphatd|CC|CUBCON|derdif|rybpgs|ITERAT|BASICS|OPTDPT|intcfg|terden|AUXRTE|COMFH1|RAYSCT|ARRAY1|moldat|quasun|ipricr|callardb|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|grdpra|RHODER|callardg|SURFEX|ATOMIC|callardc|dsctva|ODFPAR|ioniz2|comgfs PRSENT|SFFHMI|CIA_H2H|RTEFE2|PFFE|UBETA|OPACF1|LINPRO|INTHYD|RUSSEL|MATINV|WNSTOR|RHOEOS|GFREE0|ELDENS|RTEDF2|DOPGAM|ALIFR3|PFNI|ALIFR1|ENTENE|GAMI|QUASIM|LINEQS|OPAINI|RTEFR1|SGMER0|QUIT|RYBMAT|TRIDAG|RTEDF1|CIA_HHE|SGMER1|YLINTP|PFSPEC|RYBENE|WN|OPADD|LOCATE|OPCTAB|PRD|RATMAL|LEVGRP|LEVSET|LEVSOL|REFLEV|OPFRAC|PGSET|OPACTR|PFCNO|TRMDER|CONVEC|YINT|CROSSD|CROSS|ALLARD|INTXEN|GFREE1|SABOLF|ROSSTD|DIVSTR|SETTRM|PFHEAV|LAGRAN|OPACT1|CIA_H2HE|SETDRT|VOIGT|RYBCHN|STARKA|LYMLIN|TDPINI|MOLEQ|STATE|RAYLEIGH|TRMDRT|STARK0|STEQEQ|MPARTF|FFCROS|CIA_H2H2|RTECF0|GHYDOP|INTLEM|DWNFR0|GAMSP|PARTF|RATMAT|H2MINUS|PROFSP|DWNFR1|ALLARDT|RTESOL|RTECF1 True src/tlusty/math/solvers/rybsol.rs done
247 sabolf.f SABOLF SUBROUTINE False BASICS|ATOMIC|MODELQ PARTF irwint|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS MPARTF|PFSPEC|OPFRAC|PFHEAV|PFCNO|PFFE|PARTF|PFNI False src/tlusty/math/utils/sabolf.rs done
248 sbfch.f SBFCH FUNCTION True False src/tlusty/math/hydrogen/sbfch.rs done
249 sbfhe1.f SBFHE1 FUNCTION False BASICS|ATOMIC CKOEST|QUIT|HEPHOT ATOMIC|BASICS CKOEST|QUIT|HEPHOT True src/tlusty/math/hydrogen/sbfhe1.rs done
250 sbfhmi.f SBFHMI FUNCTION True YLINTP YLINTP False src/tlusty/math/hydrogen/sbfhmi.rs done
251 sbfhmi_old.f SBFHMI_OLD FUNCTION True False src/tlusty/math/hydrogen/sbfhmi_old.rs done
252 sbfoh.f SBFOH FUNCTION True False src/tlusty/math/hydrogen/sbfoh.rs done
253 setdrt.f SETDRT SUBROUTINE False BASICS|MODELQ|RHODER RHOEOS RHODER|MODELQ|tdedge|THERM|TABLTD|BASICS|tdflag PRSENT|RHOEOS|SETTRM False src/tlusty/math/utils/setdrt.rs done
254 settrm.f SETTRM SUBROUTINE False TABLTD|tdedge|THERM|tdflag PRSENT tdedge|THERM|TABLTD|tdflag PRSENT True src/tlusty/io/settrm.rs done
255 sffhmi.f SFFHMI FUNCTION True YLINTP YLINTP False src/tlusty/math/hydrogen/sffhmi.rs done
256 sffhmi_add.f SFFHMI_ADD FUNCTION True YLINTP YLINTP False src/tlusty/math/hydrogen/sffhmi_add.rs done
257 sghe12.f SGHE12 FUNCTION True False src/tlusty/math/partition/sghe12.rs done
258 sgmer0.f SGMER0 SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/hydrogen/sgmer.rs done
259 sgmer1.f SGMER1 SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/hydrogen/sgmer1.rs done
260 sgmerd.f SGMERD SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS False src/tlusty/math/hydrogen/sgmer.rs done
261 sigave.f SIGAVE SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR QUIT ODFPAR|ATOMIC|MODELQ|BASICS QUIT True src/tlusty/math/hydrogen/sigave.rs done
262 sigk.f SIGK FUNCTION False BASICS|ATOMIC TOPBAS|SPSIGK|YLINTP|SBFHE1|SBFHMI|GAUNT|VERNER ATOMIC|BASICS|TOPB SBFHE1|SPSIGK|REIMAN|HIDALG|QUIT|VERN18|SGHE12|CKOEST|HEPHOT|VERN16|VERN20|VERNER|TOPBAS|YLINTP|SBFHMI|VERN26|CARBON|GAUNT|OPDATA False src/tlusty/math/hydrogen/sigk.rs done
263 sigmar.f SIGMAR FUNCTION False BASICS LAGUER BASICS LAGUER True src/tlusty/math/hydrogen/sigmar.rs done
264 solve.f SOLVE SUBROUTINE False BASICS|ITERAT|MODELQ|ARRAY1|ALIPAR|CMATZD MATINV|WNSTOR|RHSGEN|PRCHAN|MATGEN|IROSET irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|CMATZD|terden|COMFH1|ARRAY1|moldat|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|SURFEX|COLKUR|LINED|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON PRSENT|COLLHE|PFFE|BRTEZ|EXPINX|EINT|COLH|IJALI2|RUSSEL|MATINV|WNSTOR|RHOEOS|ELDENS|PFNI|ENTENE|IRC|LINEQS|PRCHAN|RHSGEN|EXPO|INDEXX|QUIT|BPOPE|VOIGTE|BPOPC|BPOPT|SGMER1|INKUL|CEH12|YLINTP|PFSPEC|MATGEN|BHEZ|BHE|COLHE|WN|COMPT0|CION|BRTE|LEVGRP|REFLEV|LEVSOL|BHED|OPFRAC|PFCNO|TRMDER|CONVEC|EMAT|CROSS|BREZ|SABOLF|SETTRM|PFHEAV|HCTION|IROSET|CHEAVJ|MATCON|COLIS|CSPEC|BPOPF|LEVCD|MOLEQ|STATE|TRMDRT|MPARTF|BUTLER|PARTF|RATMAT|BPOP|DWNFR1|BRE|SZIRC|CHEAV True src/tlusty/math/solvers/solve.rs done
265 solves.f SOLVES SUBROUTINE False BASICS|ITERAT|MODELQ|ARRAY1|ALIPAR|CMATZD|STOMAT MATINV|WNSTOR|RHSGEN|PRCHAN|MATGEN|IROSET irwint|tdedge|adiaba|pfoptb|eospar|tdflag|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|CTIon|CMATZD|terden|COMFH1|ARRAY1|moldat|CTRTEMP|PFSTDS|entrop|TABLTD|CONVOUT|auxcbc|adchar|SURFEX|STOMAT|COLKUR|LINED|ATOMIC|ADCHAR|ODFPAR|ioniz2|CUBCON PRSENT|COLLHE|PFFE|BRTEZ|EXPINX|EINT|COLH|IJALI2|RUSSEL|MATINV|WNSTOR|RHOEOS|ELDENS|PFNI|ENTENE|IRC|LINEQS|PRCHAN|RHSGEN|EXPO|INDEXX|QUIT|BPOPE|VOIGTE|BPOPC|BPOPT|SGMER1|INKUL|CEH12|YLINTP|PFSPEC|MATGEN|BHEZ|BHE|COLHE|WN|COMPT0|CION|BRTE|LEVGRP|REFLEV|LEVSOL|BHED|OPFRAC|PFCNO|TRMDER|CONVEC|EMAT|CROSS|BREZ|SABOLF|SETTRM|PFHEAV|HCTION|IROSET|CHEAVJ|MATCON|COLIS|CSPEC|BPOPF|LEVCD|MOLEQ|STATE|TRMDRT|MPARTF|BUTLER|PARTF|RATMAT|BPOP|DWNFR1|BRE|SZIRC|CHEAV True src/tlusty/math/solvers/solves.rs done
266 spsigk.f SPSIGK SUBROUTINE True HIDALG|SGHE12|REIMAN|CARBON HIDALG|CARBON|REIMAN|SGHE12 False src/tlusty/math/hydrogen/spsigk.rs done
267 srtfrq.f SRTFRQ SUBROUTINE False BASICS|ATOMIC|MODELQ INDEXX|QUIT ATOMIC|MODELQ|BASICS INDEXX|QUIT True src/tlusty/io/srtfrq.rs done
268 stark0.f STARK0 SUBROUTINE True False src/tlusty/math/opacity/stark0.rs done
269 starka.f STARKA FUNCTION False BASICS|MODELQ MODELQ|BASICS False src/tlusty/math/opacity/starka.rs done
270 start.f START SUBROUTINE False BASICS|hediff PRDINI|COMSET|INITIA|HEDIF DEPTDR|tdedge|POPSTR|pfoptb|tdflag|PPAPAR|eletab|STFCR|MODELQ|THERM|CC|calphatd|derdif|BASICS|intcfg|FLXAUX|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|SURFEX|COLKUR|LINED|ichndm|ODFPAR|ioniz2|CUBCON|callarda|irwint|temlim|deridt|imodlc|adiaba|TOTJHK|intcff|eospar|FACTRS|EXTINT|INUNIT|ijflar|ALIPAR|hmolab|freqcl|TOPB|ITERAT|OPTDPT|PRSAUX|imucnn|COMFH1|relcor|moldat|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|abntab|callardg|ifpzpa|hediff|ATOMIC|callardc|STRPAR|comgfs INPMOD|PRSENT|SBFHE1|ANGSET|SFFHMI|TEMPER|CIA_H2H|PFFE|UBETA|HEDIF|HEPHOT|LINPRO|VERN16|LINSPL|VERN20|IJALI2|EXPINT|ERFCIN|RADTOT|INIFRT|CORRWM|RHOEOS|ELDENS|DOPGAM|RTEDF2|GRCOR|RAYINI|ODFHYS|ENTENE|CHCTAB|OPDATA|LINEQS|GOMINI|OPAINI|REIMAN|RTEFR1|SGMER0|GAULEG|VOIGTE|CKOEST|LTEGR|ODFFR|RTEDF1|SGMER1|WN|OPADD|INPDIS|OPCTAB|NEWDM|PRD|GAUNT|OPACF0|REFLEV|SPSIGK|HESOL6|RAYSET|PFCNO|HIDALG|XENINI|YINT|INTXEN|GFREE1|SABOLF|BETAH|RTEANG|INCLDY|VERN26|PSOLVE|ODFSET|TLOCAL|LAGRAN|GREYD|OPACT1|SRTFRQ|CONTMP|CIA_H2HE|IROSET|NSTOUT|LEMINI|INIFRC|LYMLIN|TDPINI|LEVCD|VERNER|TRMDRT|DMDER|STARK0|STEQEQ|MPARTF|MEANOPT|GHYDOP|SBFHMI|DWNFR0|GAMSP|PARTF|HESOLV|H2MINUS|PROFSP|DWNFR1|CONOUT|ALLARDT|MEANOP|RTESOL|READBF|COLUMN|VERN18|RTEFE2|OPACF1|PROFIL|INTHYD|RUSSEL|MATINV|WNSTOR|GFREE0|ERFCX|TABINI|PFNI|IJALIS|GAMI|QUASIM|SIGK|RDATA|INDEXX|QUIT|BKHSGO|TABINT|QUARTC|ROSSOP|NEWDMT|COMSET|CIA_HHE|INKUL|GETLAL|YLINTP|LTEGRD|INITIA|PFSPEC|LINSET|LOCATE|CUBIC|NSTPAR|LEVGRP|LEVSET|PRDINI|OPAHST|LEVSOL|OPFRAC|TRMDER|CONVEC|CROSSD|CROSS|ALLARD|DIVSTR|SETTRM|PFHEAV|KURUCZ|RDATAX|VOIGT|TRAINI|STARKA|CONTMD|INTERP|RHONEN|GETWRD|SGHE12|MOLEQ|STATE|RAYLEIGH|ZMRHO|SIGAVE|TOPBAS|FFCROS|OPADD0|CIA_H2H2|RTECF0|INTLEM|CHANGE|CARBON|RATMAT|GRIDP|INIFRS|RTECF1 True src/tlusty/io/start.rs done
271 state.f STATE SUBROUTINE False BASICS|ATOMIC|MODELQ|terden|PFSTDS OPFRAC|PARTF irwint|terden|MODELQ|moldat|PFSTDS|ATOMIC|pfoptb|BASICS MPARTF|OPFRAC|PFSPEC|PFHEAV|PFCNO|PFFE|PARTF|PFNI True src/tlusty/math/utils/state.rs done
272 steqeq.f STEQEQ SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT|POPSTR|PPAPAR RATMAT|MOLEQ|LEVSOL|SABOLF irwint|terden|COMFH1|moldat|PFSTDS|POPSTR|entrop|eospar|pfoptb|PPAPAR|adchar|MODELQ|hmolab|ITERAT|ATOMIC|BASICS|ioniz2 LEVSOL|REFLEV|OPFRAC|PFCNO|PFFE|MOLEQ|RUSSEL|SABOLF|MPARTF|PFSPEC|PFHEAV|PARTF|RATMAT|PFNI|LINEQS False src/tlusty/math/eos/steqeq.rs done
273 switch.f SWITCH SUBROUTINE False BASICS|ATOMIC|MODELQ ATOMIC|MODELQ|BASICS True src/tlusty/math/utils/switch.rs done
274 szirc.f SZIRC SUBROUTINE True EINT EXPINX|EXPO|EINT False src/tlusty/math/hydrogen/szirc.rs done
275 tabini.f TABINI SUBROUTINE False BASICS|MODELQ|ATOMIC|abntab|intcff|eletab abntab|ATOMIC|MODELQ|BASICS|intcff|eletab True src/tlusty/io/tabini.rs done
276 tabint.f TABINT SUBROUTINE False BASICS|MODELQ|ATOMIC|intcff ATOMIC|MODELQ|intcff|BASICS False src/tlusty/math/interpolation/tabint.rs done
277 taufr1.f TAUFR1 SUBROUTINE False BASICS|MODELQ|ALIPAR|ITERAT|OPTDPT ITERAT|MODELQ|BASICS|OPTDPT|ALIPAR False src/tlusty/math/ali/taufr1.rs done
278 tdpini.f TDPINI SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR|ALIPAR GFREE0 ATOMIC|MODELQ|ODFPAR|BASICS|ALIPAR GFREE0 False src/tlusty/math/temperature/tdpini.rs done
279 temcor.f TEMCOR SUBROUTINE False BASICS|MODELQ|ARRAY1|ALIPAR|CUBCON WNSTOR|STEQEQ|ELDENS|CONVEC|MEANOP|OPACF0 irwint|tdedge|adiaba|POPSTR|pfoptb|eospar|tdflag|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|CC|derdif|ITERAT|BASICS|terden|COMFH1|RAYSCT|ARRAY1|moldat|quasun|PFSTDS|entrop|TABLTD|CONVOUT|adchar|ATOMIC|ODFPAR|ioniz2|CUBCON LEVSOL|REFLEV|PRSENT|SFFHMI|OPFRAC|PFCNO|CIA_H2H|TRMDER|CONVEC|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|RUSSEL|SABOLF|WNSTOR|RHOEOS|GFREE0|SETTRM|DIVSTR|ELDENS|PFHEAV|DOPGAM|PFNI|LAGRAN|ENTENE|OPACT1|LINEQS|CIA_H2HE|VOIGT|STARKA|MOLEQ|STATE|RAYLEIGH|CIA_HHE|SGMER1|TRMDRT|STARK0|STEQEQ|MPARTF|YLINTP|PFSPEC|FFCROS|CIA_H2H2|INTLEM|DWNFR0|WN|OPADD|GAMSP|PARTF|RATMAT|LOCATE|OPCTAB|H2MINUS|PROFSP|DWNFR1|MEANOP|OPACF0 True src/tlusty/math/temperature/temcor.rs done
280 temper.f TEMPER SUBROUTINE False BASICS|MODELQ|ALIPAR|FACTRS|PRSAUX|FLXAUX WNSTOR|STEQEQ|MEANOPT|RHOEOS|ELDENS|TLOCAL|MEANOP|OPACF0 irwint|tdedge|POPSTR|pfoptb|eospar|tdflag|FACTRS|PPAPAR|ALIPAR|MODELQ|hmolab|THERM|ITERAT|BASICS|FLXAUX|PRSAUX|terden|COMFH1|RAYSCT|moldat|quasun|PFSTDS|entrop|TABLTD|adchar|ATOMIC|ODFPAR|ioniz2 LEVSOL|REFLEV|PRSENT|SFFHMI|OPFRAC|PFCNO|CIA_H2H|PFFE|UBETA|CROSSD|CROSS|YINT|LINPRO|INTHYD|INTXEN|RUSSEL|SABOLF|WNSTOR|RHOEOS|GFREE0|SETTRM|DIVSTR|ELDENS|PFHEAV|DOPGAM|TLOCAL|PFNI|LAGRAN|ENTENE|OPACT1|LINEQS|CIA_H2HE|VOIGT|STARKA|MOLEQ|QUARTC|STATE|RAYLEIGH|CIA_HHE|SGMER1|STARK0|STEQEQ|MEANOPT|MPARTF|PFSPEC|YLINTP|FFCROS|CIA_H2H2|INTLEM|DWNFR0|WN|OPADD|GAMSP|PARTF|RATMAT|OPCTAB|LOCATE|H2MINUS|PROFSP|DWNFR1|MEANOP|OPACF0 True src/tlusty/math/temperature/temper.rs done
281 timing.f TIMING SUBROUTINE False True src/tlusty/math/io/timing.rs done
282 tiopf.f TIOPF SUBROUTINE True False src/tlusty/math/partition/tiopf.rs done
283 tlocal.f TLOCAL SUBROUTINE False BASICS|MODELQ|FACTRS|FLXAUX QUARTC FLXAUX|FACTRS|MODELQ|BASICS QUARTC False src/tlusty/math/temperature/tlocal.rs done
284 tlusty.f TLUSTY UNKNOWN False BASICS|ITERAT|ALIPAR RESOLV|SOLVE|SOLVES|RYBSOL|TIMING|ACCEL2|START DEPTDR|tdedge|POPSTR|pfoptb|tdflag|POPULS|PPAPAR|eletab|STFCR|rhoder|MODELQ|THERM|calphatd|CC|derdif|rybpgs|BASICS|intcfg|FLXAUX|terden|AUXRTE|RAYSCT|quasun|entrop|TABLTD|CONVOUT|grdpra|RHODER|SURFEX|COLKUR|LINED|STOMAT|ichndm|ADCHAR|ODFPAR|ioniz2|dsctva|CUBCON|callarda|irwint|deridt|temlim|imodlc|adiaba|TOTJHK|intcff|RYBMTX|eospar|FACTRS|EXTINT|INUNIT|ijflar|ALIPAR|hmolab|freqcl|TOPB|ITERAT|CTIon|OPTDPT|CMATZD|PRSAUX|COOLCO|COMFH1|imucnn|ARRAY1|relcor|moldat|CTRTEMP|ipricr|callardb|PFSTDS|icnrsp|auxcbc|adchar|abntab|callardg|ifpzpa|ATOMIC|callardc|hediff|STRPAR|comgfs PRSENT|INPMOD|SBFHE1|ANGSET|TEMPER|COLLHE|EXPINX|ACCEL2|VERN16|VERN20|ERFCIN|RHOEOS|GRCOR|ODFHYS|CHCTAB|OPDATA|LINEQS|GOMINI|OPAINI|PRCHAN|RHSGEN|ODFMER|RTEFR1|VOIGTE|BPOPC|CKOEST|BPOPT|LTEGR|TRIDAG|CEH12|WN|NEWDM|INPDIS|OPCTAB|PRD|CION|GAUNT|BHED|PGSET|OPACFA|PFCNO|OPACTR|XENINI|ALIST1|INTXEN|GFREE1|SABOLF|RTEANG|INCLDY|VERN26|ODFSET|PZEVLD|TLOCAL|GREYD|DMEVAL|RTEINT|CIA_H2HE|PZERT|LEMINI|BPOPF|TDPINI|VISINI|VERNER|TRMDRT|DMDER|MEANOPT|DWNFR0|PARTF|HESOLV|H2MINUS|CONOUT|READBF|COLUMN|PRINC|RTEFE2|PROFIL|INTHYD|OPACTD|WNSTOR|ERFCX|ALIFR3|TIMING|PFNI|GAMI|ALIST2|QUASIM|OUTPUT|INDEXX|ACCELP|RYBSOL|QUIT|BPOPE|BKHSGO|TABINT|RYBMAT|RESOLV|GETLAL|YLINTP|CONCOR|LTEGRD|INITIA|LINSET|RATMAL|CUBIC|LEVGRP|LEVSET|CONVC1|OPFRAC|ALIFRK|NEWPOP|CROSS|RTECMC|DIVSTR|SETTRM|RTECMU|PFHEAV|OPACFL|COLIS|VOIGT|TRAINI|STARKA|CSPEC|CONTMD|INTERP|GETWRD|DWNFR|RATES1|PZEVAL|TOPBAS|FFCROS|BUTLER|CHANGE|CARBON|BPOP|GRIDP|BRE|INIFRS|SFFHMI|CIA_H2H|PFFE|UBETA|BRTEZ|HEDIF|EINT|LINPRO|HEPHOT|ALISK2|IJALI2|LINSPL|EXPINT|RADTOT|INIFRT|CORRWM|RTECOM|DOPGAM|ELDENS|RTEDF2|RAYINI|ENTENE|IRC|REIMAN|SGMER0|GAULEG|ODFFR|RTEDF1|SGMER1|TEMCOR|COLHE|MATGEN|BHEZ|OPADD|BHE|CONREF|OPACF0|SOLVE|REFLEV|HESOL6|SPSIGK|RAYSET|HIDALG|EMAT|YINT|LUCY|TAUFR1|BREZ|ELDENC|BETAH|PSOLVE|LAGRAN|OPACT1|START|SRTFRQ|CONTMP|IROSET|RATSP1|NSTOUT|RYBCHN|INIFRC|LYMLIN|LEVCD|STARK0|STEQEQ|MPARTF|GHYDOP|SBFHMI|GAMSP|OPACFD|PROFSP|DWNFR1|ALLARDT|MEANOP|RADPRE|CHEAV|RTESOL|VERN18|OPACF1|ODFHYD|COLH|RUSSEL|ODFHST|MATINV|GFREE0|TABINI|ALIFR1|IJALIS|SIGK|RDATA|EXPO|RECHCK|OSCCOR|QUARTC|ROSSOP|NEWDMT|CIA_HHE|COMSET|INKUL|SOLVES|PFSPEC|GFREED|RYBENE|LOCATE|COMPT0|BRTE|NSTPAR|INILAM|PRDINI|LEVSOL|OPAHST|TRMDER|CONVEC|CROSSD|ALLARD|LINSEL|ROSSTD|CHCKSE|KURUCZ|RDATAX|DIELRC|COOLRT|HCTION|OUTPRI|CHEAVJ|MATCON|SETDRT|RHONEN|SGHE12|MOLEQ|STATE|RAYLEIGH|ELCOR|ZMRHO|SIGAVE|RYBHEQ|CIA_H2H2|OPADD0|RTECF0|INTLEM|RATMAT|DIETOT|SZIRC|RTECF1 True src/bin/tlusty.rs done
285 topbas.f TOPBAS FUNCTION False TOPB OPDATA|YLINTP TOPB OPDATA|YLINTP True src/tlusty/math/utils/topbas.rs done
286 traini.f TRAINI SUBROUTINE False BASICS|ATOMIC|MODELQ|ODFPAR ODFPAR|ATOMIC|MODELQ|BASICS False src/tlusty/math/utils/traini.rs done
287 tridag.f TRIDAG SUBROUTINE True False src/tlusty/math/solvers/tridag.rs done
288 trmder.f TRMDER SUBROUTINE False BASICS|terden|derdif|adiaba ELDENS irwint|terden|COMFH1|adiaba|moldat|PFSTDS|entrop|pfoptb|eospar|adchar|MODELQ|hmolab|derdif|ATOMIC|BASICS|ioniz2 MPARTF|OPFRAC|PFSPEC|ELDENS|PFHEAV|PFCNO|PFFE|PARTF|PFNI|MOLEQ|ENTENE|STATE|RUSSEL|LINEQS False src/tlusty/math/radiative/trmder.rs done
289 trmdrt.f TRMDRT SUBROUTINE False BASICS|tdedge|tdflag|CONVOUT|CC PRSENT|RHOEOS MODELQ|tdedge|THERM|CC|TABLTD|CONVOUT|BASICS|tdflag PRSENT|RHOEOS|SETTRM False src/tlusty/math/radiative/trmdrt.rs done
290 ubeta.f UBETA FUNCTION True LAGRAN LAGRAN False src/tlusty/math/solvers/ubeta.rs done
291 vern16.f VERN16 FUNCTION True BASICS BASICS False src/tlusty/math/atomic/vern16.rs done
292 vern18.f VERN18 FUNCTION True BASICS BASICS False src/tlusty/math/atomic/vern18.rs done
293 vern20.f VERN20 FUNCTION True BASICS BASICS False src/tlusty/math/atomic/vern20.rs done
294 vern26.f VERN26 FUNCTION True BASICS BASICS False src/tlusty/math/atomic/vern26.rs done
295 verner.f VERNER FUNCTION False BASICS|ATOMIC VERN26|QUIT|VERN18|VERN16|VERN20 ATOMIC|BASICS VERN26|VERN18|QUIT|VERN16|VERN20 False src/tlusty/math/atomic/verner.rs done
296 visini.f VISINI SUBROUTINE False BASICS|ATOMIC|MODELQ|ITERAT ITERAT|ATOMIC|MODELQ|BASICS True src/tlusty/math/io/visini.rs done
297 voigt.f VOIGT FUNCTION True False src/tlusty/math/special/voigt.rs done
298 voigte.f VOIGTE FUNCTION True False src/tlusty/math/special/voigte.rs done
299 wn.f WN FUNCTION True BASICS BASICS False src/tlusty/math/utils/wn.rs done
300 wnstor.f WNSTOR SUBROUTINE False BASICS|ATOMIC|MODELQ WN ATOMIC|MODELQ|BASICS WN False src/tlusty/math/utils/wnstor.rs done
301 xenini.f XENINI SUBROUTINE False BASICS|MODELQ MODELQ|BASICS True src/tlusty/io/xenini.rs done
302 xk2dop.f XK2DOP FUNCTION True False src/tlusty/math/utils/xk2dop.rs done
303 yint.f YINT FUNCTION True False src/tlusty/math/interpolation/yint.rs done
304 ylintp.f YLINTP FUNCTION True False src/tlusty/math/interpolation/ylintp.rs done
305 zmrho.f ZMRHO SUBROUTINE False BASICS|MODELQ ERFCIN|BETAH MODELQ|BASICS ERFCX|ERFCIN|BETAH False src/tlusty/math/utils/zmrho.rs done
+124
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import os
import re
from collections import defaultdict
src_dir = "/home/fmq/program/SpectraRust/src"
# Regular expression to match function definitions
# Matches: fn name(...) or pub fn name(...) or pub(crate) fn name(...)
fn_pattern = re.compile(r'(?:pub\s+)?(?:pub\((?:crate|self|super)\)\s+)?fn\s+([a-zA-Z0-9_]+)\s*[\(<]')
# Matches struct definitions
struct_pattern = re.compile(r'(?:pub\s+)?(?:pub\((?:crate|self|super)\)\s+)?struct\s+([a-zA-Z0-9_]+)\s*[\{<]?')
file_functions = defaultdict(list)
fn_locations = defaultdict(list)
struct_locations = defaultdict(list)
file_basenames = defaultdict(list)
def normalize_code(code):
# Remove comments and whitespace for comparison
# Remove single line comments
code = re.sub(r'//.*', '', code)
# Remove multi-line comments
code = re.sub(r'/\*.*?\*/', '', code, flags=re.DOTALL)
# Normalize whitespace
code = "".join(code.split())
return code
def extract_function_body(content, start_pos):
# Find the matching curly brace for the function body
brace_count = 0
in_body = False
body_chars = []
# We look for the first '{' after start_pos
first_brace = content.find('{', start_pos)
if first_brace == -1:
return ""
for i in range(first_brace, len(content)):
char = content[i]
if char == '{':
brace_count += 1
in_body = True
elif char == '}':
brace_count -= 1
if in_body:
body_chars.append(char)
if brace_count == 0:
break
return "".join(body_chars)
# Walk directory
for root, dirs, files in os.walk(src_dir):
for file in files:
if file.endswith(".rs") and file != "mod.rs" and file != "lib.rs":
path = os.path.join(root, file)
rel_path = os.path.relpath(path, src_dir)
file_basenames[file].append(rel_path)
with open(path, "r", encoding="utf-8") as f:
content = f.read()
# Find all functions and extract bodies
for match in fn_pattern.finditer(content):
fn_name = match.group(1)
if fn_name == "main" or fn_name.startswith("test_"):
continue
start_pos = match.end()
body = extract_function_body(content, start_pos)
normalized_body = normalize_code(body)
fn_locations[fn_name].append({
"path": rel_path,
"body": normalized_body,
"raw_body": body[:200] # snippet
})
file_functions[rel_path].append(fn_name)
# Find all structs
for match in struct_pattern.finditer(content):
struct_name = match.group(1)
struct_locations[struct_name].append(rel_path)
print("=== 1. 重复的文件名 (Duplicate File Basenames) ===")
dup_files = {k: v for k, v in file_basenames.items() if len(v) > 1}
if dup_files:
for filename, paths in sorted(dup_files.items()):
print(f"文件名: {filename}")
for p in paths:
print(f" - src/{p}")
else:
print("没有重复的源文件名。")
print("\n=== 2. 重复的函数实现 (Duplicate Function Implementations) ===")
dup_fns = {k: v for k, v in fn_locations.items() if len(v) > 1}
if dup_fns:
for fn_name, occurrences in sorted(dup_fns.items()):
print(f"函数名: {fn_name}()")
# Check if the implementations are identical
identical = True
first_body = occurrences[0]["body"]
for occ in occurrences[1:]:
if occ["body"] != first_body:
identical = False
break
status = "【完全相同】" if identical else "【有差异的实现】"
print(f" 状态: {status}")
for occ in occurrences:
print(f" - src/{occ['path']}")
else:
print("没有发现重复的函数名。")
print("\n=== 3. 重复的 Struct 定义 (Duplicate Struct Definitions) ===")
dup_structs = {k: v for k, v in struct_locations.items() if len(v) > 1}
if dup_structs:
for struct_name, paths in sorted(dup_structs.items()):
print(f"结构体: struct {struct_name}")
for p in paths:
print(f" - src/{p}")
else:
print("没有发现重复的结构体名。")
+123
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@@ -0,0 +1,123 @@
import os
import re
from collections import defaultdict
src_dir = "/home/fmq/program/SpectraRust/src"
output_file = "/home/fmq/program/SpectraRust/scratch/duplicate_results.txt"
fn_pattern = re.compile(r'(?:pub\s+)?(?:pub\((?:crate|self|super)\)\s+)?fn\s+([a-zA-Z0-9_]+)\s*[\(<]')
struct_pattern = re.compile(r'(?:pub\s+)?(?:pub\((?:crate|self|super)\)\s+)?struct\s+([a-zA-Z0-9_]+)\s*[\{<]?')
file_functions = defaultdict(list)
fn_locations = defaultdict(list)
struct_locations = defaultdict(list)
file_basenames = defaultdict(list)
# Common helper functions to filter out
trivial_names = {
"new", "parse", "read_f32_le", "read_f64_le", "read_i32_le", "new_full",
"run_tlusty", "select_solver", "default", "build", "run", "get", "set",
"read", "write", "print", "len", "is_empty", "clear", "as_str"
}
def normalize_code(code):
code = re.sub(r'//.*', '', code)
code = re.sub(r'/\*.*?\*/', '', code, flags=re.DOTALL)
code = "".join(code.split())
return code
def extract_function_body(content, start_pos):
brace_count = 0
in_body = False
body_chars = []
first_brace = content.find('{', start_pos)
if first_brace == -1:
return ""
for i in range(first_brace, len(content)):
char = content[i]
if char == '{':
brace_count += 1
in_body = True
elif char == '}':
brace_count -= 1
if in_body:
body_chars.append(char)
if brace_count == 0:
break
return "".join(body_chars)
for root, dirs, files in os.walk(src_dir):
for file in files:
if file.endswith(".rs") and file != "mod.rs" and file != "lib.rs":
path = os.path.join(root, file)
rel_path = os.path.relpath(path, src_dir)
file_basenames[file].append(rel_path)
with open(path, "r", encoding="utf-8") as f:
content = f.read()
for match in fn_pattern.finditer(content):
fn_name = match.group(1)
if fn_name in trivial_names or fn_name.startswith("test_"):
continue
start_pos = match.end()
body = extract_function_body(content, start_pos)
normalized_body = normalize_code(body)
fn_locations[fn_name].append({
"path": rel_path,
"body": normalized_body
})
file_functions[rel_path].append(fn_name)
for match in struct_pattern.finditer(content):
struct_name = match.group(1)
if struct_name in trivial_names:
continue
struct_locations[struct_name].append(rel_path)
with open(output_file, "w", encoding="utf-8") as out:
out.write("=== 1. 重复的文件名 (Duplicate File Basenames) ===\n")
dup_files = {k: v for k, v in file_basenames.items() if len(v) > 1}
if dup_files:
for filename, paths in sorted(dup_files.items()):
out.write(f"文件名: {filename}\n")
for p in paths:
out.write(f" - src/{p}\n")
else:
out.write("没有重复的源文件名。\n")
out.write("\n=== 2. 重复的数学/物理函数实现 (Duplicate Physics/Math Functions) ===\n")
dup_fns = {k: v for k, v in fn_locations.items() if len(v) > 1}
if dup_fns:
for fn_name, occurrences in sorted(dup_fns.items()):
# Check if the implementations are identical
identical = True
first_body = occurrences[0]["body"]
for occ in occurrences[1:]:
if occ["body"] != first_body:
identical = False
break
status = "【代码完全相同】" if identical else "【代码不同(有差异的实现)】"
out.write(f"函数名: {fn_name}()\n")
out.write(f" 状态: {status}\n")
for occ in occurrences:
out.write(f" - src/{occ['path']}\n")
else:
out.write("没有发现重复的物理/数学函数。\n")
out.write("\n=== 3. 重复的 Struct 定义 (Duplicate Struct Definitions) ===\n")
dup_structs = {k: v for k, v in struct_locations.items() if len(v) > 1}
if dup_structs:
for struct_name, paths in sorted(dup_structs.items()):
out.write(f"结构体: struct {struct_name}\n")
for p in paths:
out.write(f" - src/{p}\n")
else:
out.write("没有发现重复的结构体。\n")
print("分析完成,结果已写入:", output_file)
+180
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@@ -0,0 +1,180 @@
#!/bin/bash
set -u
# --- 配置变量 ---
WORK_DIR="/home/dckj/SpectraRust"
CMD_PATH="/usr/bin/claude"
CMD_PROMPT="使用 codegraph-guide skill 继续执行重构任务。"
# 状态文件
PHASE_FILE="${WORK_DIR}/.f2r_phase"
COMPLETE_FILE="${WORK_DIR}/.f2r_complete"
RATE_LIMIT_FILE="${WORK_DIR}/.f2r_rate_limit" # 内容:退避到期 epoch 秒
FAIL_COUNT_FILE="${WORK_DIR}/.f2r_fail_count" # 内容:连续失败次数
TASKS_FILE="${WORK_DIR}/.f2r_tasks"
LOCK_FILE="${WORK_DIR}/.f2r.lock"
# 退避参数(秒)
BACKOFF_529=900 # 529 模型过载(临时性):15 分钟短退避
BACKOFF_429_FALLBACK=3600 # 429 无法解析重置时间时:默认 1 小时
BACKOFF_MODEL_ERR=1800 # 模型不存在:30 分钟
BACKOFF_CIRCUIT=7200 # 连续失败触发熔断:2 小时
MAX_CONSEC_FAIL=6 # 连续失败熔断阈值
# 日志(export TZ 确保子命令 / date 一致用 UTC+8
export TZ="Asia/Shanghai"
LOG_FILE="${WORK_DIR}/logs/claude_$(date +%Y%m%d_%H%M%S).log"
CRON_LOG="${WORK_DIR}/logs/cron.log"
CRON_LOG_MAX=5242880 # cron.log 归档阈值:5MB
log() { echo "[$(date '+%F %T')] $*"; }
# --- 1. 环境检查 ---
if [ ! -d "$WORK_DIR" ]; then
log "❌ 错误: 工作目录不存在: $WORK_DIR"
exit 1
fi
if [ ! -x "$CMD_PATH" ]; then
log "❌ 错误: 命令不存在或不可执行: $CMD_PATH"
exit 1
fi
# --- 2. 完成检测 ---
if [ -f "$COMPLETE_FILE" ]; then
log "✅ 重构已标记为完成 ($(cat "$COMPLETE_FILE" 2>/dev/null)),跳过。如需重启请删除 ${COMPLETE_FILE}"
exit 0
fi
# --- 3. 并发锁(flock,无竞态,替代 pgrep 检测)---
exec 200>"$LOCK_FILE"
if ! flock -n 200; then
log "⚠️ 已有实例在运行,跳过。"
exit 0
fi
# --- 4. 峰时段(UTC+8 14:0018:00)禁用执行 ---
CURRENT_HOUR=$(date +%H)
if [ "$CURRENT_HOUR" -ge 14 ] && [ "$CURRENT_HOUR" -lt 18 ]; then
log "⏰ 高峰期 14:0018:00 (UTC+8),跳过。"
exit 0
fi
# --- 5. 限流退避(epoch 秒)---
if [ -f "$RATE_LIMIT_FILE" ]; then
LIMIT_UNTIL=$(cat "$RATE_LIMIT_FILE" 2>/dev/null)
NOW_EPOCH=$(date +%s)
if [[ "$LIMIT_UNTIL" =~ ^[0-9]+$ ]] && [ "$NOW_EPOCH" -lt "$LIMIT_UNTIL" ]; then
REMAINING=$(( (LIMIT_UNTIL - NOW_EPOCH) / 60 ))
log "⏳ 退避中,还需 ${REMAINING} 分钟(至 $(date -d "@$LIMIT_UNTIL" '+%F %T')),跳过。"
exit 0
else
rm -f "$RATE_LIMIT_FILE"
log "🔓 退避已到期,继续执行。"
fi
fi
# --- 6. cron.log 轮转(超过阈值则归档,不删)---
if [ -f "$CRON_LOG" ]; then
CRON_SIZE=$(wc -c < "$CRON_LOG" 2>/dev/null || echo 0)
if [ "${CRON_SIZE:-0}" -gt "$CRON_LOG_MAX" ]; then
mv "$CRON_LOG" "${CRON_LOG}.$(date +%Y%m%d_%H%M%S).bak"
log "📦 cron.log 超过 ${CRON_LOG_MAX}B,已归档。"
fi
fi
# --- 7. 启动 claude ---
cd "$WORK_DIR" || { log "❌ 无法进入 ${WORK_DIR}"; exit 1; }
nohup "$CMD_PATH" --permission-mode bypassPermissions --print "$CMD_PROMPT" \
< /dev/null > "$LOG_FILE" 2>&1 &
CURRENT_PID=$!
# --print 同步,等待结束
wait "$CURRENT_PID" 2>/dev/null
EXIT_CODE=$?
LOG_SIZE=$(wc -c < "$LOG_FILE" 2>/dev/null || echo 0)
# --- 8. 错误判定 + 退避 ---
# 写入退避到期 epoch
set_backoff() { # $1=秒 $2=原因
local secs="$1" reason="$2"
local until_epoch
until_epoch=$(( $(date +%s) + secs ))
echo "$until_epoch" > "$RATE_LIMIT_FILE"
log "🔒 ${reason},退避 ${secs}s(至 $(date -d "@$until_epoch" '+%F %T'))。"
}
# 连续失败计数 +1,超阈值熔断
bump_fail() { # $1=原因
local reason="$1" n
n=$(cat "$FAIL_COUNT_FILE" 2>/dev/null || echo 0)
n=$(( n + 1 ))
echo "$n" > "$FAIL_COUNT_FILE"
log "❌ 失败 #${n}${reason} | 退出码 ${EXIT_CODE} | 日志 ${LOG_SIZE}B"
log " 日志路径: ${LOG_FILE}"
if [ "$n" -ge "$MAX_CONSEC_FAIL" ]; then
set_backoff "$BACKOFF_CIRCUIT" "连续失败 ${n} 次触发熔断"
echo 0 > "$FAIL_COUNT_FILE" # 熔断后清零,避免反复触发
fi
}
# 异常小/缺失日志:claude 未正常产出,直接计失败(避免被误判为成功)
if [ "${LOG_SIZE:-0}" -le 50 ]; then
bump_fail "日志异常小或缺失(${LOG_SIZE}B)"
exit 0
fi
# 识别错误类型(优先按日志特征,再按退出码)
ERR_TYPE=""
if grep -qE "限额将在|使用上限|429[^0-9]" "$LOG_FILE" 2>/dev/null; then
ERR_TYPE="429"
elif grep -q "529 \[" "$LOG_FILE" 2>/dev/null; then
ERR_TYPE="529"
elif grep -q "模型不存在" "$LOG_FILE" 2>/dev/null; then
ERR_TYPE="model_err"
elif [ "$EXIT_CODE" -ne 0 ]; then
ERR_TYPE="exit_nonzero"
fi
case "$ERR_TYPE" in
429)
# 用量上限:尽量解析重置时间,否则用默认长退避
RESET_TIME=$(grep -oP '限额将在 \K[\d-]+ [\d:]+' "$LOG_FILE" 2>/dev/null | head -1)
if [ -n "$RESET_TIME" ]; then
RESET_EPOCH=$(date -d "$RESET_TIME" +%s 2>/dev/null)
if [ -n "$RESET_EPOCH" ]; then
echo "$RESET_EPOCH" > "$RATE_LIMIT_FILE"
log "🔴 429 用量上限,退避至 $(date -d "@$RESET_EPOCH" '+%F %T')(重置于 ${RESET_TIME})。"
else
set_backoff "$BACKOFF_429_FALLBACK" "429 重置时间解析失败"
fi
else
set_backoff "$BACKOFF_429_FALLBACK" "429 无重置时间"
fi
bump_fail "429 用量上限"
;;
529)
# 模型过载:临时性,短退避(区别于 429 的长退避)
set_backoff "$BACKOFF_529" "529 模型过载"
bump_fail "529 模型过载"
;;
model_err)
set_backoff "$BACKOFF_MODEL_ERR" "模型不存在"
bump_fail "模型不存在"
;;
exit_nonzero)
bump_fail "claude 非零退出"
;;
*)
# 真成功:清零失败计数
echo 0 > "$FAIL_COUNT_FILE"
log "✅ 会话完成 | PID ${CURRENT_PID} | 退出码 ${EXIT_CODE} | 日志 ${LOG_SIZE}B"
log " 日志路径: ${LOG_FILE}"
# 若本次创建了完成标记,提示一下
if [ -f "$COMPLETE_FILE" ]; then
log "🎯 检测到 ${COMPLETE_FILE},重构已完成。"
fi
;;
esac
exit 0
+19
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@@ -0,0 +1,19 @@
//! SYNSPEC 可执行程序入口。
//!
//! 用法:
//! synspec < input.5 > output.6
use tlusty_rust::synspec::runner::{run_synspec, SynspecConfig};
fn main() -> anyhow::Result<()> {
let config = SynspecConfig::default();
let success = run_synspec(config);
if success {
eprintln!("SYNSPEC completed successfully.");
} else {
eprintln!("SYNSPEC completed with errors.");
}
Ok(())
}
+13 -910
View File
@@ -1,924 +1,27 @@
//! TLUSTY 可执行程序入口 //! TLUSTY 可执行程序入口
//! //!
//! 用法: //! 用法:
//! tlusty < input.5 > output.6 //! tlusty < input.5 > output.6
//! tlusty --input input.5 --output output.6
use std::env; use std::io::{self, BufReader};
use std::io::{self, BufReader, BufWriter, Write};
use std::path::PathBuf;
use tlusty_rust::tlusty::io::{FortranReader, FortranWriter, read_input_file, InputParams, InputParser}; use tlusty_rust::tlusty::{run_tlusty, TlustyConfig};
use tlusty_rust::tlusty::state::config::TlustyConfig; use tlusty_rust::tlusty::io::{FortranReader, FortranWriter};
use tlusty_rust::tlusty::state::atomic::AtomicData;
use tlusty_rust::tlusty::state::model::ModelState;
use tlusty_rust::tlusty::io::{StartConfig, StartParams, StartOutput, start_pure};
use tlusty_rust::tlusty::math::io::{read_ion_data_file, LevelInputData, ContinuumInputData, LineInputData};
use tlusty_rust::tlusty::state::constants::{EH, H, MDEPTH, BOLK, HMASS, MFREQ, HK, MATOM};
use tlusty_rust::tlusty::math::io::convert_energy;
use tlusty_rust::tlusty::io::{
initia_pure, InitiaParams, InitiaConfig, FrequencyGridParams,
};
use tlusty_rust::tlusty::io::initia::generate_log_frequency_grid;
use tlusty_rust::tlusty::math::{
compute_hopf, eldens_pure, EldensParams, EldensConfig, EldensOutput,
StateParams, state_pure,
};
use tlusty_rust::tlusty::math::continuum::{
LteOpacityParams, lte_meanopt, generate_lte_frequency_grid, quick_lte_rosseland,
};
fn main() -> anyhow::Result<()> { fn main() -> anyhow::Result<()> {
let args: Vec<String> = env::args().collect(); let mut config = TlustyConfig::default();
let mut input_reader = FortranReader::new(BufReader::new(io::stdin()));
let mut output_writer = FortranWriter::new(io::stdout());
// 解析命令行参数 let result = run_tlusty(&mut config, &mut input_reader, &mut output_writer);
let (input_path, _output_path) = parse_args(&args)?;
// 读取输入文件 if result.converged {
let input_params = if let Some(ref path) = input_path { eprintln!("Converged after {} iterations ({:.2}s)",
println!("Reading input from: {}", path.display()); result.total_iterations, result.total_time_secs);
read_input_file(path)?
} else { } else {
println!("Reading input from stdin"); eprintln!("Did NOT converge after {} iterations ({:.2}s)",
let reader = FortranReader::new(BufReader::new(io::stdin())); result.total_iterations, result.total_time_secs);
InputParser::parse(reader)?
};
// 打印基本信息
print_input_summary(&input_params);
// 读取所有离子的原子数据文件
println!("\n--- Reading atomic data files ---");
let mut total_levels = 0;
let mut total_continua = 0;
let mut total_lines = 0;
// 存储所有离子的数据
let mut all_ion_data: Vec<(Vec<LevelInputData>, Vec<ContinuumInputData>, Vec<LineInputData>)> = Vec::new();
for (ion_idx, ion) in input_params.ions.iter().enumerate() {
if ion.filei.trim().is_empty() {
// 检查是否为完全电离物种(基态离子)
// ilast == 1 且 nlevs == 1 表示这是完全电离的离子,只有基态能级
if ion.ilast == 1 && ion.nlevs == 1 {
// 创建基态能级
let ground_level = LevelInputData {
enion: 0.0, // 电离能为 0 (基态)
g: 1.0, // 统计权重 = 1
nquant: 1, // 主量子数
typlev: ion.typion.trim().to_string(),
ifwop: 0,
frodf: 0.0,
imodl: 5,
};
println!(" Ion {}: {} <- ground state only (fully ionized)",
ion_idx + 1, ion.typion.trim());
total_levels += 1;
all_ion_data.push((vec![ground_level], Vec::new(), Vec::new()));
continue;
} else {
println!(" Ion {}: {} (no data file)", ion_idx + 1, ion.typion.trim());
all_ion_data.push((Vec::new(), Vec::new(), Vec::new()));
continue;
}
}
// 解析文件路径(可能是相对路径)
let data_path = if ion.filei.starts_with("./") || ion.filei.starts_with("../") {
PathBuf::from(&ion.filei)
} else {
PathBuf::from(&ion.filei)
};
println!(" Ion {}: {} <- {}", ion_idx + 1, ion.typion.trim(), ion.filei);
match read_ion_data_file(&data_path, ion.nlevs) {
Ok((levels, continua, lines)) => {
println!(" Levels: {}, Continua: {}, Lines: {}",
levels.len(), continua.len(), lines.len());
total_levels += levels.len();
total_continua += continua.len();
total_lines += lines.len();
// 打印前几个能级的详细信息
for (i, level) in levels.iter().take(3).enumerate() {
println!(" Level {}: G={}, NQUANT={}, IFWOP={}",
i + 1, level.g, level.nquant, level.ifwop);
}
if levels.len() > 3 {
println!(" ... ({} more levels)", levels.len() - 3);
}
all_ion_data.push((levels, continua, lines));
}
Err(e) => {
println!(" ERROR: {}", e);
all_ion_data.push((Vec::new(), Vec::new(), Vec::new()));
}
}
} }
println!("\n Total: {} levels, {} continua, {} lines",
total_levels, total_continua, total_lines);
// 初始化状态
let mut config = StartConfig::default();
let mut tlusty_config = TlustyConfig::new();
let mut atomic = AtomicData::new();
let mut model = ModelState::new();
// 设置基本参数
tlusty_config.inppar.teff = input_params.teff;
tlusty_config.inppar.grav = 10.0_f64.powf(input_params.grav);
// 填充原子数据
println!("\n--- Populating atomic data ---");
let mut nfirst = 1i32; // 能级索引从 1 开始
let mut total_ntrans = 0i32;
let mut total_ntranc = 0i32;
for (ion_idx, ion) in input_params.ions.iter().enumerate() {
let (levels, continua, lines) = &all_ion_data[ion_idx];
if levels.is_empty() {
continue;
}
// 计算电离势和电荷
let zz = (ion.iat - ion.iz + 1) as f64; // 有效核电荷
let ff_ion = EH * zz * zz; // 电离势 (erg)
let charg2 = (ion.iz as f64) * (ion.iz as f64); // 电荷²
// 填充离子参数
atomic.ionpar.ff[ion_idx] = ff_ion / EH; // 以 Ry 为单位
atomic.ionpar.charg2[ion_idx] = charg2;
atomic.ionpar.nfirst[ion_idx] = nfirst;
atomic.ionpar.nlast[ion_idx] = nfirst + levels.len() as i32 - 1;
atomic.ionpar.nnext[ion_idx] = nfirst + levels.len() as i32;
atomic.ionpar.iz[ion_idx] = ion.iat as i32;
// 填充离子数据索引
atomic.iondat.iati[ion_idx] = ion.iat as i32;
atomic.iondat.izi[ion_idx] = ion.iz as i32;
atomic.iondat.nlevs[ion_idx] = levels.len() as i32;
atomic.iondat.nllim[ion_idx] = nfirst + levels.len() as i32 - 1;
// 填充能级参数
for (il, input_level) in levels.iter().enumerate() {
let level_idx = (nfirst as usize) + il - 1; // 转换为 0-based
// 能量转换
let e = input_level.enion.abs();
let e0 = convert_energy(e, zz, (il + 1) as i32);
let enion_value = if input_level.enion >= 0.0 { e0 } else { -e0 };
atomic.levpar.enion[level_idx] = enion_value;
atomic.levpar.g[level_idx] = if input_level.g == 0.0 {
2.0 * ((il + 1) as f64).powi(2)
} else {
input_level.g
};
atomic.levpar.nquant[level_idx] = if input_level.nquant == 0 {
(il + 1) as i32
} else {
input_level.nquant.abs()
};
atomic.levpar.iatm[level_idx] = ion.iat as i32;
atomic.levpar.iel[level_idx] = (ion_idx + 1) as i32;
atomic.levpar.indlev[level_idx] = (level_idx + 1) as i32;
// LTE 标志(负量子数表示 LTE)
if input_level.nquant < 0 {
atomic.levpar.iltlev[level_idx] = 1;
}
// 模型能级
atomic.levpar.imodl[level_idx] = input_level.imodl;
}
// 填充连续跃迁参数
let mut ntrans = 0i32;
let mut ntranc = 0i32;
for input_cont in continua {
let itr = (total_ntrans + ntrans) as usize;
// 索引转换
let (ii, jj) = if input_cont.jj < 1000 {
(input_cont.ii + nfirst - 1, input_cont.jj + nfirst - 1)
} else {
(input_cont.ii + nfirst - 1, input_cont.jj)
};
// 计算频率
let enion_ii = atomic.levpar.enion.get(ii as usize - 1).copied().unwrap_or(0.0);
let enion_jj = if input_cont.jj < 1000 {
atomic.levpar.enion.get(jj as usize - 1).copied().unwrap_or(0.0)
} else {
0.0
};
let fr0 = (enion_ii - enion_jj) / H;
atomic.trapar.fr0[itr] = fr0;
atomic.trapar.osc0[itr] = input_cont.osc;
atomic.trapar.cpar[itr] = input_cont.cparam;
atomic.trapar.ilow[itr] = ii;
atomic.trapar.iup[itr] = jj;
atomic.trapar.icol[itr] = input_cont.icolis;
atomic.trapar.ifc0[itr] = input_cont.ifrq0;
atomic.trapar.ifc1[itr] = input_cont.ifrq1;
atomic.trapar.itrcon[itr] = 1; // 连续跃迁标志
ntrans += 1;
ntranc += 1;
}
// 填充谱线跃迁参数
for input_line in lines {
let itr = (total_ntrans + ntrans) as usize;
let ii = input_line.ii + nfirst - 1;
let jj = input_line.jj + nfirst - 1;
// 计算频率
let enion_ii = atomic.levpar.enion.get(ii as usize - 1).copied().unwrap_or(0.0);
let enion_jj = atomic.levpar.enion.get(jj as usize - 1).copied().unwrap_or(0.0);
let fr0 = (enion_jj - enion_ii) / H;
atomic.trapar.fr0[itr] = fr0;
atomic.trapar.osc0[itr] = input_line.osc;
atomic.trapar.cpar[itr] = input_line.cparam;
atomic.trapar.ilow[itr] = ii;
atomic.trapar.iup[itr] = jj;
atomic.trapar.icol[itr] = input_line.icolis;
atomic.trapar.ifr0[itr] = input_line.ifrq0;
atomic.trapar.ifr1[itr] = input_line.ifrq1;
atomic.trapar.itrcon[itr] = 0; // 谱线跃迁标志
ntrans += 1;
}
println!(" Ion {}: nfirst={}, ntrans={}, ntranc={}",
ion_idx + 1, nfirst, ntrans, ntranc);
// 更新能级索引
nfirst += levels.len() as i32;
total_ntrans += ntrans;
total_ntranc += ntranc;
}
// 设置原子数和离子数
tlusty_config.basnum.natoms = input_params.atoms.len() as i32;
tlusty_config.basnum.nion = input_params.ions.len() as i32;
tlusty_config.basnum.nlevel = total_levels as i32;
println!("\n Total transitions: {}, continuum: {}", total_ntrans, total_ntranc);
println!(" Total levels in atomic data: {}", nfirst - 1);
// 打印一些验证数据
println!("\n--- Verification ---");
println!(" Level 1 (H1 n=1): enion={:.4e}, g={}", atomic.levpar.enion[0], atomic.levpar.g[0]);
println!(" Level 2 (H1 n=2): enion={:.4e}, g={}", atomic.levpar.enion[1], atomic.levpar.g[1]);
if total_levels > 10 {
println!(" Level 10 (He1 n=1): enion={:.4e}, g={}", atomic.levpar.enion[9], atomic.levpar.g[9]);
}
// 生成初始灰大气模型
let actual_nd = if input_params.lte && input_params.ltgrey {
println!("\n--- Generating initial LTE grey atmosphere ---");
generate_initial_grey_model(&mut model, &input_params)
} else {
50 // 默认深度点数
};
// 设置深度点数
tlusty_config.basnum.nd = actual_nd as i32;
// 创建参数结构体
let mut params = StartParams {
config: &mut config,
tlusty_config: &mut tlusty_config,
atomic: &mut atomic,
model: &mut model,
};
// 执行初始化
println!("\n--- Starting TLUSTY initialization ---");
let result = start_pure_with_input(&mut params, &input_params);
match result {
Ok(output) => {
println!("Initialization completed successfully");
println!(" NN = {}", output.nn);
println!(" Success = {}", output.success);
}
Err(e) => {
eprintln!("Initialization failed: {}", e);
std::process::exit(1);
}
}
// 设置频率网格
println!("\n--- Setting up frequency grid ---");
let grid_params = FrequencyGridParams {
frmin: 1e14, // 最小频率 (Hz)
frmax: 1e16, // 最大频率 (Hz)
nfreq: 50, // 频率点数
ifrset: 0, // 内部生成
};
let (freq, weights) = generate_log_frequency_grid(
grid_params.frmin,
grid_params.frmax,
grid_params.nfreq,
);
println!(" Frequency range: {:.2e} - {:.2e} Hz", freq[freq.len()-1], freq[0]);
println!(" Number of frequency points: {}", freq.len());
// 主迭代循环(简化版)
println!("\n--- Starting main iteration loop ---");
let max_iter = 3; // 简化:只做3次迭代作为演示
for iter in 1..=max_iter {
println!("\n === Iteration {} ===", iter);
// 1. 计算不透明度(简化版:使用电子散射)
println!(" Computing opacities...");
// 2. 计算辐射场(简化版)
println!(" Solving radiative transfer...");
// 3. 更新布居数(简化版:使用 LTE)
println!(" Updating populations...");
// 4. 计算能量方程残差(简化版)
let mut max_flux_error = 0.0_f64;
for id in 0..actual_nd {
// 简化的能量守恒检查
let t = model.modpar.temp[id];
let sigma = 5.67051e-5; // Stefan-Boltzmann 常数
let flux_err = (sigma * t.powi(4) - sigma * input_params.teff.powi(4)).abs()
/ (sigma * input_params.teff.powi(4));
max_flux_error = max_flux_error.max(flux_err);
}
println!(" Max flux error: {:.2e}", max_flux_error);
// 收敛检查
if max_flux_error < 1e-3 {
println!("\n Converged after {} iterations!", iter);
break;
}
// 温度修正(简化版:向灰大气解调整)
for id in 0..actual_nd {
let tau = model.modpar.dm[id] * 0.4; // 简化的光学深度
let q = compute_hopf(tau.max(1e-10), 0.0);
let t_grey = input_params.teff * (0.75 * (tau + q)).powf(0.25);
// 松弛更新
model.modpar.temp[id] = 0.5 * model.modpar.temp[id] + 0.5 * t_grey;
}
}
println!("\n Main loop completed after {} iterations", max_iter);
// 输出模型到 fort.7
println!("\n--- Writing model to fort.7 ---");
let output_path_str = std::env::var("FORT7").unwrap_or_else(|_| "fort.7".to_string());
let output_path = PathBuf::from(&output_path_str);
// 计算实际能级数
let nlevel_actual = total_levels as usize;
let actual_nd = tlusty_config.basnum.nd as usize;
match write_fort7(&model, &atomic, actual_nd, nlevel_actual, &output_path) {
Ok(_) => println!(" Model written to {}", output_path.display()),
Err(e) => eprintln!(" Warning: Failed to write fort.7: {}", e),
}
println!("\n--- TLUSTY START completed ---");
Ok(())
}
/// 生成初始灰大气模型
/// 返回深度点数
///
/// 使用与 Fortran TLUSTY 相同的默认参数:
/// - ND = 70 (深度点数)
/// - TAUFIR = 1e-7 (表面 Rosseland 光学深度)
/// - TAULAS = 316 (底部 Rosseland 光学深度)
/// - ABROS0 = 初始 Rosseland 不透明度估计 (通过物理公式计算)
/// - DION0 = 1.0 (初始电离度估计,完全电离)
fn generate_initial_grey_model(model: &mut ModelState, input: &InputParams) -> usize {
// Fortran 默认值 (来自 nstpar.f)
let nd = 70; // ND = 70 (Fortran 默认)
let taufir = 1e-7; // TAUFIR = 1e-7
let taulas = 316.0; // TAULAS = 316.0
let dion0 = 1.0; // DION0 = 1.0 (完全电离)
// 计算 Hopf 函数 q(τ) 的简单近似
// T(τ) = Teff * (3/4 * (τ + q(τ)))^0.25
let teff = input.teff;
let t4 = teff.powi(4);
let grav = 10.0_f64.powf(input.grav); // log g -> g
// 生成 Rosseland 光学深度网格(对数等距)
let tau_min: f64 = taufir;
let tau_max: f64 = taulas;
let log_tau_min = tau_min.ln();
let log_tau_max = tau_max.ln();
// 常数
let dprad = 1.891204931e-15 * t4; // 辐射压力项
let prad0 = dprad / 1.732; // 表面辐射压力
// 电子密度计算配置
// 注意:dion0 = 1.0 表示完全电离,用于热星的初始估计
let eldens_config = EldensConfig {
ifmol: 0,
tmolim: 1e10,
ioptab: -1, // 简单模式
iath: 1,
iatref: 1,
ihm: 0,
ih2: 0,
ih2p: 0,
pfhyd: 2.0, // 氢配分函数 (不是电离度)
};
// 平均分子量(纯 H-He 混合)
let wmm = 1.0; // 简化:假设纯氢
// STATE 函数所需的原子数据数组
// 对于简单的 H-He 模型:
// - H: 丰度 = 1.0, 最高电离级 = 2 (H I, H II)
// - He: 丰度 = 0.1, 最高电离级 = 3 (He I, He II, He III)
let abndd: [f64; MATOM] = {
let mut arr = [0.0; MATOM];
arr[0] = 1.0; // H 丰度 (相对于 H = 1.0)
arr[1] = 0.1; // He 丰度
arr
};
let ioniz: [i32; MATOM] = {
let mut arr = [0; MATOM];
arr[0] = 2; // H: 2 个电离级
arr[1] = 3; // He: 3 个电离级
arr
};
let lgr: [bool; MATOM] = [false; MATOM]; // 没有显式能级
let lrm: [bool; MATOM] = {
let mut arr = [false; MATOM];
arr[0] = true; // H: 使用隐式能级
arr[1] = true; // He: 使用隐式能级
arr
};
// 预测-校正积分的压力历史
let mut plog1 = 0.0;
let mut plog2 = 0.0;
let mut plog3 = 0.0;
let mut plog4 = 0.0;
let mut dplog1 = 0.0;
let mut dplog2 = 0.0;
let mut dplog3 = 0.0;
let dlgm = (log_tau_max - log_tau_min) / (nd - 1) as f64;
// 计算初始不透明度估计 (使用 Teff 和典型大气参数)
let initial_opacity_params = LteOpacityParams {
t: teff,
ne: 1e12, // 典型电子密度估计
nh_total: 1e12,
np: 1e12, // 假设完全电离
nh_neutral: 0.0,
nhm: 0.0,
rho: 1e-12, // 典型密度估计
uh: 2.0,
uhe: 1.0,
uhep: 2.0,
xh: 0.70,
xhe: 0.28,
};
let mut abros = quick_lte_rosseland(&initial_opacity_params);
println!(" Initial opacity estimate: {:.4} cm²/g (computed from Teff={:.0}K)", abros, teff);
for id in 0..nd {
let frac = id as f64 / (nd - 1) as f64;
let log_tau = log_tau_min + frac * (log_tau_max - log_tau_min);
let tau = log_tau.exp();
// 使用精确 Hopf 函数
let q = compute_hopf(tau, 0.0);
// 温度: T = (0.75 * Teff^4 * (tau + q))^0.25
let temp = (0.75 * t4 * (tau + q)).powf(0.25);
if id == 0 {
eprintln!("DEBUG temp: tau={:.6e}, q={:.6e}, t4={:.6e}, temp={:.1}", tau, q, t4, temp);
}
model.modpar.temp[id] = temp;
// 使用 quick_lte_rosseland 估算当前深度点的不透明度
// 这是在压力计算之前,使用温度和典型大气参数
let estimated_dens = if id > 0 {
model.modpar.dens[id - 1] // 使用前一个深度点的密度作为估计
} else {
grav * taufir * wmm * HMASS / (abros * BOLK * teff) // 表面密度估计 (正确物理公式)
};
let estimated_ne = if id > 0 {
model.modpar.elec[id - 1]
} else {
estimated_dens / HMASS // 假设完全电离
};
// 使用温度估计电离度
// 对于热星 (Teff > 20000K),表面温度约 0.75*Teff
// 在这个温度下,氢部分电离
let estimated_ion_frac = if temp > 15000.0 {
0.95 // 高温几乎完全电离
} else if temp > 10000.0 {
0.80 // 中等温度部分电离
} else if temp > 7000.0 {
0.30 // 较低温度
} else {
0.001 // 低温几乎不电离
};
let estimated_nh_total = estimated_dens / HMASS;
let estimated_np = estimated_nh_total * estimated_ion_frac;
let estimated_nh_neutral = estimated_nh_total * (1.0 - estimated_ion_frac);
let quick_opacity_params = LteOpacityParams {
t: temp,
ne: estimated_np, // 电子密度 = 质子密度
nh_total: estimated_nh_total,
np: estimated_np,
nh_neutral: estimated_nh_neutral,
nhm: 0.0,
rho: estimated_dens,
uh: 2.0,
uhe: 1.0,
uhep: 2.0,
xh: 0.70,
xhe: 0.28,
};
let mut current_abros = quick_lte_rosseland(&quick_opacity_params);
// 流体静力学平衡计算压力
// 预测步
let mut plog = if id == 0 {
(grav / current_abros * tau + prad0).ln()
} else if id <= 3 {
plog1 + dplog1
} else {
(3.0 * plog4 + 8.0 * dplog1 - 4.0 * dplog2 + 8.0 * dplog3) / 3.0
};
// 校正步迭代 - 与 Fortran LTEGR/ROSSOP 一致,在迭代中更新不透明度
let mut ptot = plog.exp();
let mut p = ptot - tau * dprad - prad0;
let mut an = p / (BOLK * temp);
let mut ane = estimated_ne;
let mut anp = estimated_np;
let mut ahtot = estimated_nh_total;
let mut nh_neutral = estimated_nh_neutral;
let mut dens = estimated_dens;
for j in 0..10 {
// 校正步计算 (与 Fortran LTEGR 一致)
let plog_new = if id == 0 {
(grav / current_abros * tau + prad0).ln()
} else if id <= 3 {
(plog + 2.0 * plog1 + dplog1 + dplog1) / 3.0
} else {
(126.0 * plog1 - 14.0 * plog3 + 9.0 * plog4
+ 42.0 * dplog1 + 108.0 * dplog2 - 54.0 * dplog3 + 24.0 * dplog3) / 121.0
};
let err = (plog_new - plog).abs();
plog = plog_new;
ptot = plog.exp();
// 计算气体压力和粒子数密度 (与 Fortran ROSSOP 一致)
p = ptot - tau * dprad - prad0;
an = p / (BOLK * temp);
// 计算电子密度 (与 Fortran ROSSOP 调用 ELDENS 一致)
// 创建 STATE 函数所需的参数
// STATE 需要: mode=1 (LTEGR 模式), 温度, 电子密度, 原子数据
let state_params = StateParams {
mode: 1, // MODE=1 用于 LTEGR (包含显式和非显式化学物种)
id: id + 1,
t: temp,
ane, // 使用当前电子密度估计
natoms: 2, // H 和 He
hpop: an * 0.9, // 氢数密度估计 (假设大部分是 H)
dens: estimated_dens,
wmm: wmm,
ytot: 1.1, // 总原子数/氢原子数 ≈ 1 + 0.1 (He)
abndd: &abndd,
ioniz: &ioniz,
irefa: 1, // 氢是参考原子
lgr: &lgr,
lrm: &lrm,
};
let eldens_params = EldensParams {
id: id + 1,
t: temp,
an,
ytot: 1.1, // H + He 丰度因子
qref: 0.0,
dqnr: 0.0,
wmy: wmm,
config: eldens_config.clone(),
state_params: Some(state_params),
molecule_data: None,
};
let eldens_output = eldens_pure(&eldens_params, 0);
ane = eldens_output.ane;
anp = eldens_output.anp;
ahtot = eldens_output.ahtot;
nh_neutral = (ahtot - anp).max(0.0);
// 密度计算 (与 Fortran ROSSOP 一致)
// Fortran: RHO = WMM * (AN - ANE)
// WMM 在 Fortran ELDENS 中计算: wmm = dens / (an - ane)
// 由于 WMM 以 g 为单位 (不是 amu), 我们需要乘以 HMASS
// 对于氢主导气体, wmm ≈ 1 amu, 所以 RHO ≈ (AN - ANE) * HMASS
dens = (an - ane) * HMASS; // 密度 (g/cm³)
if id == 0 && j == 0 {
eprintln!("DEBUG after ELDENS: ane={:.6e}, an={:.6e}, dens={:.6e}, ahtot={:.6e}", ane, an, dens, ahtot);
}
// 更新不透明度 (与 Fortran ROSSOP 调用 OPACF0 + MEANOP 一致)
// 使用频率积分计算完整 LTE Rosseland 不透明度
let lte_params_iter = LteOpacityParams {
t: temp,
ne: ane,
nh_total: ahtot,
np: anp,
nh_neutral,
nhm: 0.0,
rho: dens,
uh: 2.0,
uhe: 1.0,
uhep: 2.0,
xh: 0.70,
xhe: 0.28,
};
let grid_iter = generate_lte_frequency_grid(input.teff, 50);
let lte_output_iter = lte_meanopt(&lte_params_iter, &grid_iter);
current_abros = lte_output_iter.opros;
// 收敛检查 (在更新不透明度之后)
// 注意:对于表面点 (id=0),需要至少迭代一次来更新不透明度
if err <= 1e-4 && j > 0 {
break;
}
// 防止无限循环的安全检查
if j == 9 {
if id == 0 {
println!(" Warning: Corrector iteration did not converge at depth {}", id + 1);
}
}
}
// 更新压力历史 (使用最终收敛的不透明度)
if id == 0 {
eprintln!("DEBUG before pressure update: ane={:.6e}, an={:.6e}", ane, an);
}
let dplog = grav / current_abros * tau / ptot * dlgm;
plog4 = plog3;
plog3 = plog2;
plog2 = plog1;
plog1 = plog;
dplog3 = dplog2;
dplog2 = dplog1;
dplog1 = dplog;
// 计算柱质量密度
let depth = (ptot - prad0) / grav;
model.modpar.dm[id] = depth;
// 计算密度
let dens = wmm * (an - ane) * HMASS;
model.modpar.dens[id] = dens;
model.modpar.elec[id] = ane;
model.modpar.totn[id] = an;
model.modpar.anto[id] = an - ane; // 总原子密度
// 辅助量
let t = temp;
let h = 6.62620e-27_f64;
model.modpar.sqt1[id] = t.sqrt();
model.modpar.hkt1[id] = h / (BOLK * t);
model.modpar.tk1[id] = 1.0 / t;
// 计算 Rosseland 不透明度
// 使用完整的 LTE 不透明度计算,包含电子散射、束缚-自由、自由-自由和 H-
let lte_params = LteOpacityParams {
t: temp,
ne: ane,
nh_total: ahtot,
np: anp,
nh_neutral,
nhm: 0.0, // H- 密度暂时为 0
rho: dens,
uh: 2.0, // 氢配分函数
uhe: 1.0, // 氦配分函数
uhep: 2.0, // He+ 配分函数
xh: 0.70, // 氢丰度
xhe: 0.28, // 氦丰度
};
// 使用频率积分计算完整不透明度
let grid = generate_lte_frequency_grid(input.teff, 100);
let lte_output = lte_meanopt(&lte_params, &grid);
abros = lte_output.opros;
// Debug output for first and last points
if id == 0 || id == nd - 1 {
let opes = 6.6524e-25 * ane / dens.max(1e-20); // 电子散射
let ion_frac = anp / ahtot.max(1e-30); // 电离度
let opbf = 4.3e-25 * (1.0 - ion_frac) * (temp/1e4).powf(-3.5); // 束缚-自由
println!(" Depth {}: T={:.0}K, ne={:.2e}, nH={:.2e}, rho={:.2e}", id + 1, temp, ane, nh_neutral, dens);
println!(" Quick estimate κ_R={:.4e}, Full LTE κ_R={:.4e}, κ_P={:.4e}",
current_abros, lte_output.opros, lte_output.oppla);
println!(" Components: κ_es={:.4e}, κ_bf={:.4e}, κ_ff={:.4e}, κ_H-={:.4e}",
lte_output.opes, lte_output.opbf, lte_output.opff, lte_output.ophm);
}
}
// 设置深度点数
model.modpar.dmtot = model.modpar.dm[nd - 1];
println!(" Generated {} depth points", nd);
println!(" Temperature range: {:.0} K (surface) to {:.0} K (bottom)",
model.modpar.temp[0], model.modpar.temp[nd - 1]);
println!(" Electron density range: {:.2e} to {:.2e} cm^-3",
model.modpar.elec[0], model.modpar.elec[nd - 1]);
nd
}
/// 带 InputParams 的 start 函数
fn start_pure_with_input(
params: &mut StartParams,
input: &InputParams,
) -> anyhow::Result<StartOutput> {
// 设置频率参数
params.tlusty_config.basnum.nfread = input.frequencies.nfread;
// 设置原子数
params.tlusty_config.basnum.natoms = input.atoms.len() as i32;
// 设置离子数
params.tlusty_config.basnum.nion = input.ions.len() as i32;
// 计算总能级数
let nlevel: i32 = input.ions.iter().map(|ion| ion.nlevs as i32).sum();
params.tlusty_config.basnum.nlevel = nlevel;
// 调用纯计算版本的 start
Ok(start_pure(params))
}
/// 打印输入参数摘要
fn print_input_summary(params: &InputParams) {
println!("\n================================");
println!(" M O D E L A T M O S P H E R E");
println!("================================\n");
println!(" TEFF = {:>12.1}", params.teff);
println!(" LOG G = {:>12.2}", params.grav);
println!(" LTE = {}", if params.lte { "T" } else { "F" });
println!(" LTGRAY = {}", if params.ltgrey { "T" } else { "F" });
println!("\n FREQUENCIES:");
println!(" NFREAD = {}", params.frequencies.nfread);
println!("\n ATOMS: {} elements configured", params.atoms.len());
println!("\n IONS:");
for ion in &params.ions {
println!(
" {:3} (Z={:2}, ion={}) - {} levels, file: {}",
ion.typion.trim(),
ion.iat,
ion.iz,
ion.nlevs,
if ion.filei.trim().is_empty() { "(none)" } else { &ion.filei }
);
}
}
/// 解析命令行参数
fn parse_args(args: &[String]) -> anyhow::Result<(Option<PathBuf>, Option<PathBuf>)> {
let mut input_path: Option<PathBuf> = None;
let mut output_path: Option<PathBuf> = None;
let mut i = 1;
while i < args.len() {
match args[i].as_str() {
"-i" | "--input" => {
i += 1;
if i < args.len() {
input_path = Some(PathBuf::from(&args[i]));
}
}
"-o" | "--output" => {
i += 1;
if i < args.len() {
output_path = Some(PathBuf::from(&args[i]));
}
}
"-h" | "--help" => {
print_usage();
std::process::exit(0);
}
_ => {
// 位置参数:第一个是输入文件
if input_path.is_none() {
input_path = Some(PathBuf::from(&args[i]));
}
}
}
i += 1;
}
Ok((input_path, output_path))
}
fn print_usage() {
println!("TLUSTY - Non-LTE Stellar Atmosphere Calculator");
println!();
println!("Usage:");
println!(" tlusty [OPTIONS] [INPUT_FILE]");
println!();
println!("Options:");
println!(" -i, --input <FILE> Input file (default: stdin)");
println!(" -o, --output <FILE> Output file (default: stdout)");
println!(" -h, --help Show this help message");
println!();
println!("Example:");
println!(" tlusty hhe35lt.5 > hhe35lt.6");
}
/// 写入 fort.7 格式模型文件
fn write_fort7(
model: &tlusty_rust::tlusty::state::model::ModelState,
atomic: &tlusty_rust::tlusty::state::atomic::AtomicData,
nd: usize,
nlevel_actual: usize,
path: &std::path::Path,
) -> anyhow::Result<()> {
use std::fs::File;
use std::io::{BufWriter, Write};
let file = File::create(path)?;
let mut writer = BufWriter::new(file);
// NUMPAR = 3 (T, NE, RHO) + nlevel_actual
let numpar = 3 + nlevel_actual as i32;
// 写入头部:ND NUMPAR
writeln!(writer, "{:4}{:5}", nd, numpar)?;
// 写入质量深度数组(每行 6 个值)
for i in 0..nd {
write!(writer, "{:13.6E}", model.modpar.dm[i])?;
if (i + 1) % 6 == 0 || i == nd - 1 {
writeln!(writer)?;
}
}
// 写入每个深度点的数据
for id in 0..nd {
// 温度
write!(writer, "{:15.7E}", model.modpar.temp[id])?;
// 电子密度
write!(writer, "{:15.7E}", model.modpar.elec[id])?;
// 质量密度
write!(writer, "{:15.7E}", model.modpar.dens[id])?;
// 能级占据数(LTE 模型使用 Boltzmann 分布)
for ilev in 0..nlevel_actual {
let enion = atomic.levpar.enion[ilev];
let g = atomic.levpar.g[ilev];
let hkt = model.modpar.hkt1[id];
// Boltzmann 分布
let pop = g * (-enion * hkt / H).exp() * model.modpar.elec[id];
write!(writer, "{:15.7E}", pop)?;
}
writeln!(writer)?;
}
writer.flush()?;
Ok(()) Ok(())
} }
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//! ABNCHN 丰度修改过程。
//!
//! 重构自 SYNSPEC `ABNCHN` 函数。
//!
//! 用于 opacity table 评估时修改(或消除)某些元素的丰度。
/// ABNCHN 模式。
#[derive(Debug, Clone, Copy, PartialEq, Eq)]
pub enum AbnchnMode {
/// 保存当前 populations 到备份
Save = 0,
/// 按丰度因子缩放 populations
Scale = 1,
}
/// ABNCHN 输入参数。
pub struct AbnchnParams<'a> {
/// 操作模式
pub mode: AbnchnMode,
/// 原子数
pub natom: usize,
/// 每个原子的第一能级索引 (0-based)
pub n0a: &'a [usize],
/// 每个原子的最后能级索引 (0-based)
pub nka: &'a [usize],
/// 每个原子对应的原子序数 (1-based)
pub numat: &'a [usize],
/// 丰度缩放因子 (按原子序数索引, 1-based)
pub relabn: &'a [f64],
/// 当前 populations [nlevel]
pub popul: &'a [f64],
/// 备份 populations [nlevel] (mode=0 时写入, mode=1 时读取)
pub popul0: &'a [f64],
/// RRR 数组 [mion × matom]
pub rrr: &'a [f64],
/// 离子数
pub mion0: usize,
/// 原子种类数 (最大)
pub matom: usize,
}
/// ABNCHN 输出结果。
pub struct AbnchnOutput {
/// 修改后的 populations [nlevel]
pub popul_new: Vec<f64>,
/// 修改后的 RRR 数组 [mion × matom]
pub rrr_new: Vec<f64>,
/// 更新后的备份 populations [nlevel]
pub popul0_new: Vec<f64>,
}
/// ABNCHN 丰度修改过程。
///
/// mode=0: 保存当前 populations 到备份。
/// mode=1: 按丰度因子缩放 populations 和 RRR。
///
/// # 参数
///
/// * `params` - ABNCHN 参数
///
/// # 返回值
///
/// 修改后的 populations 和 RRR
pub fn abnchn(params: &AbnchnParams) -> AbnchnOutput {
let AbnchnParams {
mode,
natom,
n0a,
nka,
numat,
relabn,
popul,
popul0,
rrr,
mion0,
matom,
} = *params;
let _nlevel = popul.len();
let mut popul_new = popul.to_vec();
let mut popul0_new = popul0.to_vec();
let mut rrr_new = rrr.to_vec();
match mode {
AbnchnMode::Save => {
// 保存当前 populations 到备份
for iat in 0..natom {
for ii in n0a[iat]..=nka[iat] {
popul0_new[ii] = popul[ii];
}
}
}
AbnchnMode::Scale => {
// 按丰度因子缩放 populations
for iat in 0..natom {
let ia = numat[iat] - 1; // 0-based
for ii in n0a[iat]..=nka[iat] {
popul_new[ii] = popul0[ii] * relabn[ia];
}
}
// 缩放 RRR 数组
for ia in 0..matom {
for io in 0..mion0 {
let idx = io * matom + ia;
rrr_new[idx] = rrr[idx] * relabn[ia];
}
}
}
}
AbnchnOutput {
popul_new,
rrr_new,
popul0_new,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_abnchn_save() {
let nlevel = 6;
let popul = vec![1.0e10, 2.0e10, 3.0e10, 4.0e10, 5.0e10, 6.0e10];
let popul0 = vec![0.0; nlevel];
let rrr = vec![1.0; 4];
let n0a = vec![0usize, 3];
let nka = vec![2usize, 5];
let numat = vec![1usize, 2];
let relabn = vec![1.0, 0.5, 0.3]; // index 0 unused, 1=H, 2=He
let params = AbnchnParams {
mode: AbnchnMode::Save,
natom: 2,
n0a: &n0a,
nka: &nka,
numat: &numat,
relabn: &relabn,
popul: &popul,
popul0: &popul0,
rrr: &rrr,
mion0: 2,
matom: 3,
};
let output = abnchn(&params);
// mode=0: 复制 popul 到 popul0
assert_eq!(output.popul0_new, popul);
// popul 不变
assert_eq!(output.popul_new, popul);
}
#[test]
fn test_abnchn_scale() {
let nlevel = 6;
let popul = vec![1.0e10, 2.0e10, 3.0e10, 4.0e10, 5.0e10, 6.0e10];
let popul0 = vec![1.0e10, 2.0e10, 3.0e10, 4.0e10, 5.0e10, 6.0e10];
let rrr = vec![1.0, 2.0, 3.0, 4.0, 5.0, 6.0]; // mion0=2, matom=3
let n0a = vec![0usize, 3];
let nka = vec![2usize, 5];
let numat = vec![1usize, 2];
let relabn = vec![1.0, 0.5, 0.3]; // H=0.5, He=0.3
let params = AbnchnParams {
mode: AbnchnMode::Scale,
natom: 2,
n0a: &n0a,
nka: &nka,
numat: &numat,
relabn: &relabn,
popul: &popul,
popul0: &popul0,
rrr: &rrr,
mion0: 2,
matom: 3,
};
let output = abnchn(&params);
// mode=1: popul = popul0 * relabn[ia]
// atom 0 (H, numat=1): ia=0, relabn[0]=1.0 → 不变
assert_eq!(output.popul_new[0], 1.0e10 * 1.0);
assert_eq!(output.popul_new[1], 2.0e10 * 1.0);
assert_eq!(output.popul_new[2], 3.0e10 * 1.0);
// atom 1 (He, numat=2): ia=1, relabn[1]=0.5
assert_eq!(output.popul_new[3], 4.0e10 * 0.5);
assert_eq!(output.popul_new[4], 5.0e10 * 0.5);
assert_eq!(output.popul_new[5], 6.0e10 * 0.5);
}
}
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//! Quasi-molecular opacity for Lyman alpha, beta, gamma, and Balmer alpha.
//!
//! Translated from SYNSPEC `allard` subroutine (synspec54.f).
// ============================================================================
// Constants
// ============================================================================
/// Maximum number of wavelength points in tables
pub const NXMAX: usize = 1400;
/// Maximum number of density components
pub const NNMAX: usize = 5;
// Normalization constants: 8.8528e-29 * lambda_0^2 * f_ij
const XNORMA: f64 = 8.8528e-29 * 1215.6 * 1215.6 * 0.41618; // Lyman alpha
const XNORMB: f64 = 8.8528e-29 * 1025.73 * 1025.7 * 0.0791; // Lyman beta
const XNORMG: f64 = 8.8528e-29 * 972.53 * 972.53 * 0.0290; // Lyman gamma
const XNORMC: f64 = 8.8528e-29 * 6562.0 * 6562.0 * 0.6407; // Balmer alpha
// ============================================================================
// AllardData - precomputed table data
// ============================================================================
/// Precomputed quasi-molecular opacity tables for one transition.
///
/// Corresponds to Fortran COMMON blocks `callarda`, `callardb`, `callardg`, `callardc`.
#[derive(Debug, Clone)]
pub struct AllardTable {
/// Wavelength points (Angstroms)
pub xl: Vec<f64>,
/// Profile data: `pl[i][j]` for wavelength point `i`, component `j`
/// Components: 0=neutral linear, 1=neutral quadratic,
/// 2=charged linear, 3=charged quadratic, 4=cross term
pub pl: Vec<[f64; NNMAX]>,
/// Normalized neutral density scale
pub stnne: f64,
/// Normalized charged density scale
pub stnch: f64,
/// Neutral velocity scale
pub vneu: f64,
/// Charged velocity scale
pub vcha: f64,
/// Number of wavelength points
pub nx: usize,
/// Warning flag for high density
pub iwarn: bool,
}
impl Default for AllardTable {
fn default() -> Self {
Self {
xl: Vec::new(),
pl: Vec::new(),
stnne: 1.0,
stnch: 1.0,
vneu: 1.0,
vcha: 1.0,
nx: 0,
iwarn: false,
}
}
}
// ============================================================================
// AllardData - all four transitions
// ============================================================================
/// Container for all four quasi-molecular transitions.
#[derive(Debug, Clone, Default)]
pub struct AllardData {
/// Lyman alpha (1→2)
pub lalp: AllardTable,
/// Lyman beta (1→3)
pub bet: AllardTable,
/// Lyman gamma (1→4)
pub gam: AllardTable,
/// Balmer alpha (2→3)
pub bal: AllardTable,
}
// ============================================================================
// Core interpolation function
// ============================================================================
/// Interpolate quasi-molecular profile from precomputed table.
///
/// # Arguments
/// * `table` - Precomputed table for this transition
/// * `xl` - Wavelength in Angstroms
/// * `hneutr` - Neutral H particle density [cm⁻³]
/// * `hcharg` - Ionized H particle density [cm⁻³]
///
/// # Returns
/// Profile value normalized to 1.0e8 when integrated over Angstroms.
/// Returns 0.0 if wavelength is outside table range.
fn interpolate_profile(
table: &AllardTable,
xl: f64,
hneutr: f64,
hcharg: f64,
xnorm: f64,
) -> f64 {
if table.nx == 0 {
return 0.0;
}
if xl < table.xl[0] || xl > table.xl[table.nx - 1] {
return 0.0;
}
// Normalized densities
let vn1 = hneutr / table.stnne;
let vn2 = hcharg / table.stnch;
let vns = vn1 * table.vneu + vn2 * table.vcha;
// Density warning
// (handled externally via iwarn flag)
let vn11 = vn1 * vn1;
let vn22 = vn2 * vn2;
let vn12 = vn1 * vn2;
let xnorm_fac = 1.0 / (1.0 + vns + 0.5 * vns * vns);
// Binary search for wavelength interval
let mut jl: usize = 0;
let mut ju = table.nx;
while ju - jl > 1 {
let jm = (ju + jl) / 2;
if (table.xl[table.nx - 1] > table.xl[0]) == (xl > table.xl[jm]) {
jl = jm;
} else {
ju = jm;
}
}
let mut j = jl;
if j == 0 {
j = 1;
}
if j >= table.nx - 1 {
j = table.nx - 2;
}
// Linear interpolation factor
let a1 = (xl - table.xl[j]) / (table.xl[j + 1] - table.xl[j]);
let a0 = 1.0 - a1;
// Interpolate each density component
let p1 = vn1 * (a0 * table.pl[j][0] + a1 * table.pl[j + 1][0]);
let p11 = vn11 * (a0 * table.pl[j][1] + a1 * table.pl[j + 1][1]);
let p2 = vn2 * (a0 * table.pl[j][2] + a1 * table.pl[j + 1][2]);
let p22 = vn22 * (a0 * table.pl[j][3] + a1 * table.pl[j + 1][3]);
let p12 = vn12 * (a0 * table.pl[j][4] + a1 * table.pl[j + 1][4]);
(p1 + p2 + p11 + p22 + p12) * xnorm_fac * xnorm
}
// ============================================================================
// Main entry point
// ============================================================================
/// Compute quasi-molecular opacity profile.
///
/// Translated from SYNSPEC `allard` subroutine (synspec54.f).
///
/// # Arguments
/// * `data` - Precomputed quasi-molecular tables
/// * `xl` - Wavelength in Angstroms
/// * `hneutr` - Neutral H particle density [cm⁻³]
/// * `hcharg` - Ionized H particle density [cm⁻³]
/// * `iq` - Quantum number of lower level
/// * `jq` - Quantum number of upper level:
/// - 2 → Lyman alpha
/// - 3 → Lyman beta (if iq=1) or Balmer alpha (if iq=2)
/// - 4 → Lyman gamma
///
/// # Returns
/// Profile value. Returns 0.0 if transition not recognized or out of range.
pub fn allard(
data: &AllardData,
xl: f64,
hneutr: f64,
hcharg: f64,
iq: i32,
jq: i32,
) -> f64 {
// Lyman alpha (1→2)
if iq == 1 && jq == 2 {
return interpolate_profile(&data.lalp, xl, hneutr, hcharg, XNORMA);
}
// Lyman beta (1→3)
if iq == 1 && jq == 3 {
return interpolate_profile(&data.bet, xl, hneutr, hcharg, XNORMB);
}
// Lyman gamma (1→4)
if iq == 1 && jq == 4 {
return interpolate_profile(&data.gam, xl, hneutr, hcharg, XNORMG);
}
// Balmer alpha (2→3)
if iq == 2 && jq == 3 {
// For Balmer alpha, only charged component contributes
// (vn1 = 0 in Fortran code)
if data.bal.nx == 0 {
return 0.0;
}
if xl < data.bal.xl[0] || xl > data.bal.xl[data.bal.nx - 1] {
return 0.0;
}
let vn2 = hcharg / data.bal.stnch;
let vns = vn2 * data.bal.vcha;
let vn22 = vn2 * vn2;
let xnorm_fac = 1.0 / (1.0 + vns + 0.5 * vns * vns);
// Binary search
let mut jl: usize = 0;
let mut ju = data.bal.nx;
while ju - jl > 1 {
let jm = (ju + jl) / 2;
if (data.bal.xl[data.bal.nx - 1] > data.bal.xl[0])
== (xl > data.bal.xl[jm])
{
jl = jm;
} else {
ju = jm;
}
}
let mut j = jl;
if j == 0 {
j = 1;
}
if j >= data.bal.nx - 1 {
j = data.bal.nx - 2;
}
let a1 = (xl - data.bal.xl[j]) / (data.bal.xl[j + 1] - data.bal.xl[j]);
let a0 = 1.0 - a1;
let p2 = vn2 * (a0 * data.bal.pl[j][2] + a1 * data.bal.pl[j + 1][2]);
let p22 = vn22 * (a0 * data.bal.pl[j][3] + a1 * data.bal.pl[j + 1][3]);
return (p2 + p22) * xnorm_fac * XNORMC;
}
0.0
}
// ============================================================================
// Tests
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_allard_empty_table() {
let data = AllardData::default();
let prof = allard(&data, 1215.6, 1e12, 1e10, 1, 2);
assert_eq!(prof, 0.0);
}
#[test]
fn test_allard_out_of_range() {
let mut data = AllardData::default();
data.lalp.xl = vec![1200.0, 1210.0, 1220.0];
data.lalp.pl = vec![[1.0; NNMAX]; 3];
data.lalp.nx = 3;
// Below range
let prof = allard(&data, 1199.0, 1e12, 1e10, 1, 2);
assert_eq!(prof, 0.0);
// Above range
let prof = allard(&data, 1221.0, 1e12, 1e10, 1, 2);
assert_eq!(prof, 0.0);
}
#[test]
fn test_allard_lyman_alpha() {
let mut data = AllardData::default();
data.lalp.xl = vec![1210.0, 1215.0, 1220.0];
data.lalp.pl = vec![
[1.0, 0.5, 0.3, 0.2, 0.1],
[2.0, 1.0, 0.6, 0.4, 0.2],
[1.5, 0.75, 0.45, 0.3, 0.15],
];
data.lalp.stnne = 1e12;
data.lalp.stnch = 1e10;
data.lalp.vneu = 1.0;
data.lalp.vcha = 1.0;
data.lalp.nx = 3;
let prof = allard(&data, 1215.0, 1e12, 1e10, 1, 2);
assert!(prof > 0.0);
}
#[test]
fn test_allard_unknown_transition() {
let data = AllardData::default();
let prof = allard(&data, 1215.6, 1e12, 1e10, 2, 4); // Not a valid transition
assert_eq!(prof, 0.0);
}
}
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//! 中性碳光致电离截面(Taylor 数据)。
//!
//! 重构自 SYNSPEC `carbon.f`
//!
//! 使用 G.B. Taylor (private communication) 的数据,
//! 计算中性碳 2p¹D 和 2p¹S 能级的光致电离截面。
/// 频率网格 2 (单位 FR0),用于 IB=-602 (2p¹D)
const FR2: [f64; 34] = [
0.74, 0.75, 0.76, 0.77, 0.78, 0.79, 0.80, 0.81, 0.82, 0.83,
0.85, 0.86, 0.87, 0.88, 0.89, 0.90, 0.91, 0.92, 0.93, 0.94,
0.95, 0.96, 0.97, 0.98, 0.99, 1.00, 1.10, 1.20, 1.30, 1.45,
1.50, 1.60, 1.80, 2.00,
];
/// 截面数据 2 (Mbarn),用于 IB=-602 (2p¹D)
const SG2: [f64; 34] = [
12.04, 12.03, 12.09, 12.26, 12.60, 13.24, 14.36, 16.24, 19.28, 23.94,
37.41, 42.88, 44.76, 43.41, 40.46, 37.19, 34.26, 31.82, 29.96, 28.57,
27.68, 27.37, 27.84, 29.69, 34.45, 46.35, 13.80, 11.54, 10.40, 8.96,
8.54, 7.47, 6.53, 5.66,
];
/// 频率网格 3 (单位 FR0),用于 IB=-603 (2p¹S)
const FR3: [f64; 45] = [
0.66, 0.68, 0.70, 0.72, 0.74, 0.76, 0.78, 0.80, 0.82, 0.84,
0.86, 0.864, 0.866, 0.868, 0.87, 0.874, 0.876, 0.88, 0.882, 0.884,
0.886, 0.888, 0.89, 0.894, 0.896, 0.898, 0.90, 0.904, 0.908, 0.910,
0.920, 0.94, 0.98, 1.00, 1.10, 1.20, 1.26, 1.34, 1.36, 1.40,
1.46, 1.60, 1.70, 1.80, 2.00,
];
/// 截面数据 3 (Mbarn),用于 IB=-603 (2p¹S)
const SG3: [f64; 45] = [
13.94, 13.29, 12.56, 11.73, 10.82, 10.18, 8.62, 7.27, 5.74, 4.14,
4.61, 5.92, 6.94, 8.34, 10.21, 16.12, 20.64, 34.56, 44.82, 57.71,
73.09, 89.99, 106.38, 127.08, 128.38, 124.44, 117.17, 99.32, 82.95, 76.05,
52.65, 33.23, 21.29, 18.69, 12.62, 11.44, 9.77, 7.53, 10.47, 9.65,
10.19, 7.28, 6.70, 6.11, 4.96,
];
/// 参考频率 (Hz)
const FR0: f64 = 3.28805e15;
/// 截面单位转换因子 (cm^2)
const SIG_FACTOR: f64 = 1.0e-18;
/// 中性碳光致电离截面。
///
/// 根据 Taylor 数据,对给定频率进行线性插值。
///
/// # 参数
///
/// * `ib` - 能级标识(-602 = 2p¹D, -603 = 2p¹S
/// * `fr` - 频率 (Hz)
///
/// # 返回值
///
/// 光致电离截面 (cm^2)
pub fn carbon(ib: i32, fr: f64) -> f64 {
let f = fr / FR0;
if ib == -602 {
// 2p¹D 能级
let mut j = 1; // 0-indexed, 默认值
if f > FR2[0] {
for i in 1..34 {
if f > FR2[i - 1] && f <= FR2[i] {
j = i;
break;
}
}
} else {
j = 1;
}
let sg = (f - FR2[j - 1]) / (FR2[j] - FR2[j - 1]) * (SG2[j] - SG2[j - 1]) + SG2[j - 1];
return sg * SIG_FACTOR;
}
if ib == -603 {
// 2p¹S 能级
let mut j = 1;
if f > FR3[0] {
for i in 1..45 {
if f > FR3[i - 1] && f <= FR3[i] {
j = i;
break;
}
}
} else {
j = 1;
}
let sg = (f - FR3[j - 1]) / (FR3[j] - FR3[j - 1]) * (SG3[j] - SG3[j - 1]) + SG3[j - 1];
return sg * SIG_FACTOR;
}
0.0
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_carbon_602_in_range() {
// 2p¹D 在有效频率范围内
let fr = 0.9 * FR0;
let result = carbon(-602, fr);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_carbon_603_in_range() {
// 2p¹S 在有效频率范围内
let fr = 0.85 * FR0;
let result = carbon(-603, fr);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_carbon_below_range() {
let fr = 0.5 * FR0;
let result = carbon(-602, fr);
assert!(result >= 0.0);
}
#[test]
fn test_carbon_above_range() {
let fr = 3.0 * FR0;
let result = carbon(-602, fr);
assert!(result >= 0.0);
}
#[test]
fn test_carbon_invalid_ib() {
let result = carbon(-601, FR0);
assert_eq!(result, 0.0);
}
}
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//! CHANGE 控制过程。
//!
//! 重构自 SYNSPEC `CHANGE` 函数。
//!
//! 在显式能级系统与输入能级编号不一致时,重新评估初始能级 populations。
//! 仅用于 NLTE 输入模型。
use crate::synspec::state::constants::BOLK;
use crate::synspec::math::{lineqs, ratmat};
/// CHANGE 模式参数(每个能级一组)。
#[derive(Debug, Clone)]
pub struct ChangeLevelParams {
/// 旧能级索引 (1-based)0 = 无对应旧能级
pub iold: usize,
/// 评估模式
/// - 0: 复制旧能级 population × REL
/// - 1: LTE 相对于下一电离态
/// - 2: b-因子匹配
/// - 3: 完整 LTESABOLF + RATMAT + LINEQS
pub mode: usize,
/// 下一电离态旧索引 (1-based)
pub nxtold: usize,
/// 新系统中参考能级索引 (1-based)
pub isinew: usize,
/// 旧系统中参考能级索引 (1-based)
pub isiold: usize,
/// 参考能级下一电离态旧索引 (1-based)
pub nxtsio: usize,
/// population 乘子
pub rel: f64,
}
/// CHANGE 输入参数。
pub struct ChangeParams<'a> {
/// 每能级参数
pub levels: &'a [ChangeLevelParams],
/// 深度点数
pub nd: usize,
/// 温度数组 (K)
pub temp: &'a [f64],
/// 电子密度数组 (cm^-3)
pub elec: &'a [f64],
/// 当前 populations [nlevel × nd, row-major]
pub popul: &'a [f64],
/// 统计权重
pub g: &'a [f64],
/// 电离能 (K)
pub enion: &'a [f64],
/// 元素索引 (1-based)
pub iel: &'a [usize],
/// 下一离子态索引 (1-based)
pub nnext: &'a [usize],
/// 能级数
pub nlevel: usize,
/// N0 偏移数组 (1-based)
pub n0a: &'a [usize],
/// NK 偏移数组 (1-based)
pub nka: &'a [usize],
/// SBF 数组
pub sbf: &'a [f64],
/// WOP 数组 (nlevel × nd, row-major)
pub wop: &'a [f64],
/// ILK 数组 (1-based)
pub ilk: &'a [usize],
/// USUM 数组 (1-based)
pub usum: &'a [f64],
/// ATTOT 数组
pub attot: &'a [f64],
}
/// CHANGE 输出结果。
pub struct ChangeOutput {
/// 新 populations [nlevel × nd, row-major]
pub popul_new: Vec<f64>,
/// 能级数
pub nlevel: usize,
/// 深度点数
pub nd: usize,
}
/// S = 2*h/c^2 * (1e-8)^2 = 2.0706e-16 (转换因子)
const S: f64 = 2.0706e-16;
/// 获取 popul[level][depth] 的辅助函数。
#[inline]
fn popul_at(popul: &[f64], nd: usize, level: usize, depth: usize) -> f64 {
popul[level * nd + depth]
}
/// CHANGE 控制过程。
///
/// 在显式能级系统与输入能级编号不一致时,重新评估初始能级 populations。
///
/// # 参数
///
/// * `params` - CHANGE 参数
///
/// # 返回值
///
/// 新的能级 populations
pub fn change(params: &ChangeParams) -> ChangeOutput {
let ChangeParams {
levels,
nd,
temp,
elec,
popul,
g,
enion,
iel,
nnext,
nlevel,
n0a,
nka,
sbf,
wop,
ilk,
usum,
attot,
} = *params;
let mut popul_new = vec![0.0f64; nlevel * nd];
let mut ifese = 0usize;
for (ii, lvl) in levels.iter().enumerate() {
let iold = lvl.iold;
let mode = lvl.mode;
let nxtold = lvl.nxtold;
let isinew = lvl.isinew;
let isiold = lvl.isiold;
let nxtsio = lvl.nxtsio;
let mut rel = lvl.rel;
if rel == 0.0 {
rel = 1.0;
}
if mode >= 3 {
ifese += 1;
}
for id in 0..nd {
if iold != 0 {
// 直接复制旧能级 population
popul_new[ii * nd + id] = popul_at(popul, nd, iold - 1, id);
continue;
}
match mode {
0 => {
// 复制旧能级 population × REL
popul_new[ii * nd + id] = popul_at(popul, nd, isiold - 1, id) * rel;
}
1 => {
// LTE 相对于下一电离态
let t = temp[id];
let ane = elec[id];
let nxt_idx = nnext[iel[ii] - 1] - 1;
let sb = S / t / t.sqrt() * g[ii] / g[nxt_idx]
* (enion[ii] / t / BOLK).exp();
popul_new[ii * nd + id] = sb * ane * popul_at(popul, nd, nxtold - 1, id) * rel;
}
2 => {
// b-因子匹配
let t = temp[id];
let kk = isinew - 1; // 0-based
let k_next = nnext[iel[kk] - 1] - 1;
let nxt_idx = nnext[iel[ii] - 1] - 1;
let sb = S / t / t.sqrt() * g[ii] / g[nxt_idx]
* (enion[ii] / t / BOLK).exp();
let sbk = S / t / t.sqrt() * g[kk] / g[k_next]
* (enion[kk] / t / BOLK).exp();
popul_new[ii * nd + id] = sb / sbk
* popul_at(popul, nd, nxtold - 1, id)
/ popul_at(popul, nd, nxtsio - 1, id)
* popul_at(popul, nd, isiold - 1, id)
* rel;
}
_ => {
// MODE >= 3: 完整 LTE via RATMAT + LINEQS
if ifese == 1 {
let ane = elec[id];
let (ese_mat, bese) = ratmat(
ane,
nlevel,
0,
n0a,
nka,
nnext,
iel,
sbf,
wop,
nd,
id,
ilk,
usum,
attot,
);
// 解线性方程组
let mut a = ese_mat;
let mut b = bese;
let poplte = lineqs(&mut a, &mut b, nlevel);
for iii in 0..nlevel {
popul_new[iii * nd + id] = poplte[iii];
}
}
}
}
}
}
ChangeOutput {
popul_new,
nlevel,
nd,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_change_mode0_copy() {
let nd = 2usize;
let nlevel = 3usize;
let mut popul = vec![0.0f64; nlevel * nd];
popul[0 * nd + 0] = 1.0e10;
popul[0 * nd + 1] = 2.0e10;
let levels = vec![
ChangeLevelParams {
iold: 0,
mode: 0,
nxtold: 0,
isinew: 0,
isiold: 1,
nxtsio: 0,
rel: 2.0,
},
];
let iel = vec![1usize; nlevel];
let nnext = vec![2usize; nlevel];
let g = vec![1.0f64; nlevel];
let enion = vec![0.0f64; nlevel];
let n0a = vec![0usize; nlevel];
let nka = vec![0usize; nlevel];
let sbf = vec![0.0f64; nlevel];
let wop = vec![0.0f64; nlevel * nd];
let ilk = vec![0usize; nlevel];
let usum = vec![0.0f64; nlevel];
let attot = vec![0.0f64; nlevel];
let temp = vec![10000.0f64; nd];
let elec = vec![1.0e14f64; nd];
let params = ChangeParams {
levels: &levels,
nd,
temp: &temp,
elec: &elec,
popul: &popul,
g: &g,
enion: &enion,
iel: &iel,
nnext: &nnext,
nlevel,
n0a: &n0a,
nka: &nka,
sbf: &sbf,
wop: &wop,
ilk: &ilk,
usum: &usum,
attot: &attot,
};
let output = change(&params);
// MODE 0: 复制 isiold=1 的 population × rel=2.0
assert_eq!(output.popul_new[0 * nd + 0], 1.0e10 * 2.0);
assert_eq!(output.popul_new[0 * nd + 1], 2.0e10 * 2.0);
}
#[test]
fn test_change_direct_copy() {
let nd = 1usize;
let nlevel = 3usize;
let mut popul = vec![0.0f64; nlevel * nd];
popul[2 * nd + 0] = 5.0e12;
let levels = vec![
ChangeLevelParams {
iold: 3,
mode: 0,
nxtold: 0,
isinew: 0,
isiold: 0,
nxtsio: 0,
rel: 1.0,
},
];
let iel = vec![1usize; nlevel];
let nnext = vec![2usize; nlevel];
let g = vec![1.0f64; nlevel];
let enion = vec![0.0f64; nlevel];
let n0a = vec![0usize; nlevel];
let nka = vec![0usize; nlevel];
let sbf = vec![0.0f64; nlevel];
let wop = vec![0.0f64; nlevel * nd];
let ilk = vec![0usize; nlevel];
let usum = vec![0.0f64; nlevel];
let attot = vec![0.0f64; nlevel];
let temp = vec![10000.0f64; nd];
let elec = vec![1.0e14f64; nd];
let params = ChangeParams {
levels: &levels,
nd,
temp: &temp,
elec: &elec,
popul: &popul,
g: &g,
enion: &enion,
iel: &iel,
nnext: &nnext,
nlevel,
n0a: &n0a,
nka: &nka,
sbf: &sbf,
wop: &wop,
ilk: &ilk,
usum: &usum,
attot: &attot,
};
let output = change(&params);
// iold != 0: 直接复制
assert_eq!(output.popul_new[0 * nd + 0], 5.0e12);
}
}
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//! 丰度一致性检查。
//!
//! 重构自 SYNSPEC `CHCKAB` 函数。
//!
//! 检查显式原子的输入丰度与从模型大气计算得到的丰度是否一致。
//! 如果差异超过 10%,程序将停止。
use crate::synspec::state::constants::{MATOM, MDEPTH, MLEVEL};
/// CHCKAB 输入参数。
pub struct ChckabParams<'a> {
/// 深度点数
pub nd: usize,
/// 温度数组 (K)
pub temp: &'a [f64; MDEPTH],
/// 电子密度数组 (cm^-3)
pub elec: &'a [f64; MDEPTH],
/// 能级 populations
pub popul: &'a [[f64; MDEPTH]; MLEVEL],
/// 上态求和
pub usum: &'a [f64; MLEVEL],
/// 原子丰度
pub abund: &'a [[f64; MDEPTH]; MATOM],
/// 原子数
pub natom: usize,
/// 参考原子索引 (1-based)
pub iatref: usize,
/// N0A 数组 - 每个原子的第一个能级索引
pub n0a: &'a [i32],
/// NKA 数组 - 每个原子的最后一个能级索引
pub nka: &'a [i32],
/// ILK 数组 - 能级索引
pub ilk: &'a [i32],
}
/// CHCKAB 输出结果。
#[derive(Default)]
pub struct ChckabResult {
/// 是否发现不一致性
pub inconsistent: bool,
/// 不一致的原子数
pub n_inconsistent: usize,
}
/// 丰度一致性检查。
///
/// 检查显式原子的输入丰度与从模型大气计算得到的丰度是否一致。
///
/// # 参数
///
/// * `params` - CHCKAB 参数
///
/// # 返回值
///
/// CHCKAB 输出结果
pub fn chckab(params: &ChckabParams) -> ChckabResult {
let ChckabParams {
nd,
temp: _,
elec,
popul,
usum,
abund,
natom,
iatref,
n0a,
nka,
ilk,
} = *params;
let mut result = ChckabResult::default();
// 检查三个深度点: 1, 46, ND
let depth_points = [0, 45.min(nd - 1), nd - 1];
for &id in &depth_points {
let ane = elec[id];
let mut sumiat = [0.0_f64; MATOM];
let mut sumpop = [0.0_f64; MATOM];
// 计算每个原子的总 population
for iat in 0..natom {
let mut sum = 0.0_f64;
let mut sump = 0.0_f64;
let n0 = n0a[iat] as usize - 1; // 转换为 0-indexed
let nk = nka[iat] as usize - 1;
for i in n0..=nk {
let il = ilk[i] as usize;
let a = if il > 0 {
1.0 + ane * usum[il - 1]
} else {
1.0
};
sum += a * popul[i][id];
sump += popul[i][id];
}
sumiat[iat] = sum;
sumpop[iat] = sump;
}
// 检查丰度一致性
let iatref_idx = iatref - 1; // 转换为 0-indexed
for iat in 0..natom {
let x = sumiat[iat] / sumiat[iatref_idx];
let ab = abund[iat][id];
if ab > 0.0 {
let ratio = x / ab;
if !(0.9..=1.1).contains(&ratio) {
result.n_inconsistent += 1;
}
}
}
}
result.inconsistent = result.n_inconsistent > 0;
result
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_chckab_consistent() {
// 创建一个简单的测试用例,其中丰度一致
let nd = 3;
let mut temp = [0.0f64; MDEPTH];
let mut elec = [0.0f64; MDEPTH];
let mut popul = [[0.0f64; MDEPTH]; MLEVEL];
let mut usum = [0.0f64; MLEVEL];
let mut abund = [[0.0f64; MDEPTH]; MATOM];
let mut n0a = [0i32; MATOM];
let mut nka = [0i32; MATOM];
let mut ilk = [0i32; MLEVEL];
// 设置测试值
for id in 0..nd {
temp[id] = 10000.0;
elec[id] = 1.0e14;
}
// 设置一个原子,有 2 个能级
let natom = 1;
n0a[0] = 1;
nka[0] = 2;
ilk[0] = 0; // 无上态求和
ilk[1] = 0;
// 设置 populations
for id in 0..nd {
popul[0][id] = 1.0e10;
popul[1][id] = 1.0e9;
abund[0][id] = 1.0; // 丰度比值 (相对于参考原子)
}
let params = ChckabParams {
nd,
temp: &temp,
elec: &elec,
popul: &popul,
usum: &usum,
abund: &abund,
natom,
iatref: 1,
n0a: &n0a,
nka: &nka,
ilk: &ilk,
};
let result = chckab(&params);
// 丰度应该一致
assert!(!result.inconsistent);
assert_eq!(result.n_inconsistent, 0);
}
#[test]
fn test_chckab_inconsistent() {
// 创建一个测试用例,其中丰度不一致
let nd = 3;
let mut temp = [0.0f64; MDEPTH];
let mut elec = [0.0f64; MDEPTH];
let mut popul = [[0.0f64; MDEPTH]; MLEVEL];
let mut usum = [0.0f64; MLEVEL];
let mut abund = [[0.0f64; MDEPTH]; MATOM];
let mut n0a = [0i32; MATOM];
let mut nka = [0i32; MATOM];
let mut ilk = [0i32; MLEVEL];
// 设置测试值
for id in 0..nd {
temp[id] = 10000.0;
elec[id] = 1.0e14;
}
// 设置一个原子,有 2 个能级
let natom = 1;
n0a[0] = 1;
nka[0] = 2;
ilk[0] = 0;
ilk[1] = 0;
// 设置 populations
for id in 0..nd {
popul[0][id] = 1.0e10;
popul[1][id] = 1.0e9;
abund[0][id] = 1.0e10; // 总 population = 1.1e10,但丰度设为 1.0e10
// 比值 = 1.1,超过 10% 阈值
}
let params = ChckabParams {
nd,
temp: &temp,
elec: &elec,
popul: &popul,
usum: &usum,
abund: &abund,
natom,
iatref: 1,
n0a: &n0a,
nka: &nka,
ilk: &ilk,
};
let result = chckab(&params);
// 丰度应该不一致
assert!(result.inconsistent);
assert!(result.n_inconsistent > 0);
}
}
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//! Collision-Induced Absorption (CIA) opacity functions.
//!
//! Translated from SYNSPEC54 subroutines:
//! - `cia_h2h2` -- H2-H2 CIA (Borysow et al. 2001, JQSRT 68, 235)
//! - `cia_h2h` -- H2-H CIA (from TURBOSPEC)
//! - `cia_h2he` -- H2-He CIA (Jorgensen et al. 2000, A&A 361, 283)
//! - `cia_hhe` -- H-He CIA (Gustafsson & Frommhold 2001, ApJ 546, 1168)
//!
//! Each function reads a CIA table on first call, then performs 2D bilinear
//! interpolation in (wavenumber, temperature) space to compute opacity.
//!
//! # Usage
//! 1. Call the `*_init` function once to load the CIA data file.
//! 2. Call the corresponding function to evaluate CIA opacity at given conditions.
use std::fs::File;
use std::io::{BufRead, BufReader};
use std::sync::OnceLock;
use super::locate::locate;
// ============================================================================
// Constants
// ============================================================================
/// Speed of light in cm/s
const CAS: f64 = 2.997925e10;
/// Amagat number (Loschmidt number at STP) in cm^-3
const AMAGAT: f64 = 2.6867774e19;
/// Scaling factor: 1 / amagat^2
const FAC: f64 = 1.0 / (AMAGAT * AMAGAT);
/// Fallback value for log(alpha) when outside frequency table range
const ALPHA_FLOOR: f64 = -50.0;
// ============================================================================
// CIA table storage
// ============================================================================
/// A loaded CIA table: frequencies (wavenumber in cm^-1), temperatures (K),
/// and log(alpha) values.
struct CiaTable {
nlines: usize,
ntemp: usize,
freq: Vec<f64>,
temp: Vec<f64>,
/// log(alpha) values stored as `alpha[i * ntemp + j]` (row-major)
alpha: Vec<f64>,
}
// Static storage for each CIA species
static TABLE_H2H2: OnceLock<CiaTable> = OnceLock::new();
static TABLE_H2H: OnceLock<CiaTable> = OnceLock::new();
static TABLE_H2HE: OnceLock<CiaTable> = OnceLock::new();
static TABLE_HHE: OnceLock<CiaTable> = OnceLock::new();
// ============================================================================
// Data loading helper
// ============================================================================
/// Load a CIA data file into a `CiaTable`.
///
/// File format:
/// - 3 header lines (skipped)
/// - `nlines` data lines, each with: wavenumber alpha(T1) alpha(T2) ... alpha(TnTemp)
///
/// After reading, all alpha values are replaced by their natural logarithm.
fn load_cia_table(filename: &str, nlines: usize, temp: &[f64]) -> Result<CiaTable, String> {
let ntemp = temp.len();
let file = File::open(filename)
.map_err(|e| format!("Cannot open CIA data file '{}': {}", filename, e))?;
let mut reader = BufReader::new(file);
let mut line = String::new();
// Skip 3 header lines
for _ in 0..3 {
line.clear();
reader
.read_line(&mut line)
.map_err(|e| format!("Error reading CIA header: {}", e))?;
}
let mut freq = Vec::with_capacity(nlines);
let mut alpha = vec![0.0f64; nlines * ntemp];
for i in 0..nlines {
line.clear();
reader
.read_line(&mut line)
.map_err(|e| format!("Error reading CIA data line {}: {}", i + 1, e))?;
let parts: Vec<f64> = line
.split_whitespace()
.map(|s| {
s.parse::<f64>()
.map_err(|_| format!("Cannot parse float from '{}'", s))
})
.collect::<Result<Vec<f64>, String>>()?;
if parts.len() < 1 + ntemp {
return Err(format!(
"CIA data line {}: expected {} fields, got {}",
i + 1,
1 + ntemp,
parts.len()
));
}
freq.push(parts[0]);
for j in 0..ntemp {
alpha[i * ntemp + j] = parts[1 + j].ln();
}
}
Ok(CiaTable {
nlines,
ntemp,
freq,
temp: temp.to_vec(),
alpha,
})
}
// ============================================================================
// Core interpolation (shared by all 4 functions)
// ============================================================================
/// Perform 2D bilinear interpolation in (wavenumber, temperature) space.
///
/// Returns the interpolated alpha value (after exp), or 0.0 if temperature
/// is below the table range. Returns `exp(ALPHA_FLOOR)` if frequency is
/// outside the table.
fn cia_interpolate(table: &CiaTable, t: f64, ff: f64) -> f64 {
let f = ff / CAS; // Convert Hz to cm^-1
// Locate temperature
let j = locate(&table.temp, table.ntemp, t);
if j == 0 {
// Temperature below table range
eprintln!();
eprintln!(
"Warning: requested temperature is below {} K",
table.temp[0]
);
eprintln!("CIA opacity set to 0");
eprintln!();
return 0.0;
}
// Locate frequency
let i = locate(&table.freq, table.nlines, f);
let alp = if j == table.ntemp {
// Hold values constant if off high temperature end of table
let y1 = table.alpha[(i - 1) * table.ntemp + j - 1];
let y2 = table.alpha[i * table.ntemp + j - 1];
let tt = (f - table.freq[i - 1]) / (table.freq[i] - table.freq[i - 1]);
(1.0 - tt) * y1 + tt * y2
} else if i == 0 || i == table.nlines {
// Off frequency table: set to very small number
ALPHA_FLOOR
} else {
// Bilinear interpolation within table
// locate returns 1-indexed indices, so freq indices are i-1 and i (0-indexed)
// In Fortran: alpha(i,j), alpha(i+1,j), alpha(i+1,j+1), alpha(i,j+1)
// where i is 1-indexed from locate. In our 0-indexed storage:
// alpha[(i-1)*ntemp + (j-1)], alpha[i*ntemp + (j-1)],
// alpha[i*ntemp + j], alpha[(i-1)*ntemp + j]
let y1 = table.alpha[(i - 1) * table.ntemp + (j - 1)];
let y2 = table.alpha[i * table.ntemp + (j - 1)];
let y3 = table.alpha[i * table.ntemp + j];
let y4 = table.alpha[(i - 1) * table.ntemp + j];
let tt = (f - table.freq[i - 1]) / (table.freq[i] - table.freq[i - 1]);
let uu = (t - table.temp[j - 1]) / (table.temp[j] - table.temp[j - 1]);
(1.0 - tt) * (1.0 - uu) * y1
+ tt * (1.0 - uu) * y2
+ tt * uu * y3
+ (1.0 - tt) * uu * y4
};
alp.exp()
}
/// Helper: initialize a CIA table into a static OnceLock.
fn init_cia_table(
static_table: &'static OnceLock<CiaTable>,
filename: &str,
nlines: usize,
temp: &[f64],
) -> Result<(), String> {
let table = load_cia_table(filename, nlines, temp)?;
static_table
.set(table)
.map_err(|_| "CIA table already initialized".to_string())
}
// ============================================================================
// H2-H2 CIA
// ============================================================================
/// Initialize H2-H2 CIA table from file.
///
/// Data source: Borysow A., Jorgensen U.G., Fu Y. 2001, JQSRT 68, 235
///
/// File format: 3 header lines + 1000 data lines with 8 columns
/// (wavenumber + 7 temperatures: 1000..7000 K)
pub fn cia_h2h2_init(filename: &str) -> Result<(), String> {
init_cia_table(
&TABLE_H2H2,
filename,
1000,
&[1000.0, 2000.0, 3000.0, 4000.0, 5000.0, 6000.0, 7000.0],
)
}
/// H2-H2 CIA opacity.
///
/// # Arguments
/// * `t` - Temperature in K
/// * `ah2` - H2 number density in cm^-3
/// * `ff` - Frequency in Hz
///
/// # Returns
/// CIA opacity (cm^-1)
pub fn cia_h2h2(t: f64, ah2: f64, ff: f64) -> f64 {
let table = match TABLE_H2H2.get() {
Some(t) => t,
None => {
eprintln!("CIA H2-H2 table not initialized, call cia_h2h2_init first");
return 0.0;
}
};
let alp = cia_interpolate(table, t, ff);
FAC * ah2 * ah2 * alp
}
// ============================================================================
// H2-H CIA
// ============================================================================
/// Initialize H2-H CIA table from file.
///
/// Data source: TURBOSPEC
///
/// File format: 3 header lines + 67 data lines with 5 columns
/// (wavenumber + 4 temperatures: 1000, 1500, 2000, 2500 K)
pub fn cia_h2h_init(filename: &str) -> Result<(), String> {
init_cia_table(
&TABLE_H2H,
filename,
67,
&[1000.0, 1500.0, 2000.0, 2500.0],
)
}
/// H2-H CIA opacity.
///
/// # Arguments
/// * `t` - Temperature in K
/// * `ah2` - H2 number density in cm^-3
/// * `ah` - H number density in cm^-3
/// * `ff` - Frequency in Hz
///
/// # Returns
/// CIA opacity (cm^-1)
pub fn cia_h2h(t: f64, ah2: f64, ah: f64, ff: f64) -> f64 {
let table = match TABLE_H2H.get() {
Some(t) => t,
None => {
eprintln!("CIA H2-H table not initialized, call cia_h2h_init first");
return 0.0;
}
};
let alp = cia_interpolate(table, t, ff);
FAC * ah2 * ah * alp
}
// ============================================================================
// H2-He CIA
// ============================================================================
/// Initialize H2-He CIA table from file.
///
/// Data source: Jorgensen U.G., Hammer D., Borysow A., Falkesgaard J., 2000,
/// Astronomy & Astrophysics 361, 283
///
/// File format: 3 header lines + 242 data lines with 8 columns
/// (wavenumber + 7 temperatures: 1000..7000 K)
pub fn cia_h2he_init(filename: &str) -> Result<(), String> {
init_cia_table(
&TABLE_H2HE,
filename,
242,
&[1000.0, 2000.0, 3000.0, 4000.0, 5000.0, 6000.0, 7000.0],
)
}
/// H2-He CIA opacity.
///
/// # Arguments
/// * `t` - Temperature in K
/// * `ah2` - H2 number density in cm^-3
/// * `ahe` - He number density in cm^-3
/// * `ff` - Frequency in Hz
///
/// # Returns
/// CIA opacity (cm^-1)
pub fn cia_h2he(t: f64, ah2: f64, ahe: f64, ff: f64) -> f64 {
let table = match TABLE_H2HE.get() {
Some(t) => t,
None => {
eprintln!("CIA H2-He table not initialized, call cia_h2he_init first");
return 0.0;
}
};
let alp = cia_interpolate(table, t, ff);
FAC * ah2 * ahe * alp
}
// ============================================================================
// H-He CIA
// ============================================================================
/// Initialize H-He CIA table from file.
///
/// Data source: Gustafsson M., Frommhold, L. 2001, ApJ 546, 1168
///
/// File format: 3 header lines + 43 data lines with 12 columns
/// (wavenumber + 11 temperatures: 1000, 1500, 2250, 3000, 4000, 5000,
/// 6000, 7000, 8000, 9000, 10000 K)
pub fn cia_hhe_init(filename: &str) -> Result<(), String> {
init_cia_table(
&TABLE_HHE,
filename,
43,
&[
1000.0, 1500.0, 2250.0, 3000.0, 4000.0, 5000.0, 6000.0, 7000.0, 8000.0, 9000.0,
10000.0,
],
)
}
/// H-He CIA opacity.
///
/// # Arguments
/// * `t` - Temperature in K
/// * `ah` - H number density in cm^-3
/// * `ahe` - He number density in cm^-3
/// * `ff` - Frequency in Hz
///
/// # Returns
/// CIA opacity (cm^-1)
pub fn cia_hhe(t: f64, ah: f64, ahe: f64, ff: f64) -> f64 {
let table = match TABLE_HHE.get() {
Some(t) => t,
None => {
eprintln!("CIA H-He table not initialized, call cia_hhe_init first");
return 0.0;
}
};
let alp = cia_interpolate(table, t, ff);
FAC * ah * ahe * alp
}
// ============================================================================
// Tests
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
/// Helper: build a small synthetic CIA table for testing interpolation.
fn make_test_table() -> CiaTable {
// 5 frequency points, 3 temperature points
let nlines = 5;
let ntemp = 3;
let freq = vec![100.0, 200.0, 300.0, 400.0, 500.0];
let temp = vec![1000.0, 2000.0, 3000.0];
// alpha values (will be stored as ln)
// Use a simple pattern: alpha(i,j) = (i+1)*10 + (j+1) (before log)
let mut alpha = vec![0.0; nlines * ntemp];
for i in 0..nlines {
for j in 0..ntemp {
let val = (i as f64 + 1.0) * 10.0 + (j as f64 + 1.0);
alpha[i * ntemp + j] = val.ln();
}
}
CiaTable {
nlines,
ntemp,
freq,
temp,
alpha,
}
}
#[test]
fn test_cia_constants() {
assert!((AMAGAT - 2.6867774e19).abs() < 1e10);
assert!((CAS - 2.997925e10).abs() < 1e3);
let expected_fac = 1.0 / (2.6867774e19_f64 * 2.6867774e19);
assert!((FAC - expected_fac).abs() / expected_fac < 1e-12);
}
#[test]
fn test_cia_interpolation_basic() {
let table = make_test_table();
// At freq=200, temp=1500 (midpoint of 1000,2000)
// locate(freq,5,200) => i=2, meaning freq[i-1]=200, freq[i]=300 => tt=0
// locate(temp,3,1500) => j=1, meaning temp[j-1]=1000, temp[j]=2000 => uu=0.5
// y1=alpha[1][0]=ln(21), y4=alpha[1][1]=ln(22)
// alp = 0.5*ln(21) + 0.5*ln(22) = ln(sqrt(21*22)) = ln(sqrt(462))
let alp = cia_interpolate(&table, 1500.0, 200.0 * CAS);
let expected = (462.0_f64).sqrt();
assert!(
(alp - expected).abs() / expected < 1e-10,
"Expected {}, got {}",
expected,
alp
);
}
#[test]
fn test_cia_interpolation_corner() {
let table = make_test_table();
// At exact grid point freq=100, temp=1000
// alpha[0][0] = ln(11), exp => 11
let alp = cia_interpolate(&table, 1000.0, 100.0 * CAS);
assert!(
(alp - 11.0).abs() < 1e-10,
"Expected 11.0, got {}",
alp
);
}
#[test]
fn test_cia_interpolation_high_temp() {
let table = make_test_table();
// Temperature above max (3000): hold constant at j=ntemp
// freq=250 (midpoint), temp=5000 (above max)
// locate(freq,5,250)=2, locate(temp,3,5000)=3=j=ntemp
// j==ntemp branch: 1D interpolation in freq at highest temp column
// y1=alpha[1][2]=ln(23), y2=alpha[2][2]=ln(33), tt=0.5
// alp = 0.5*ln(23) + 0.5*ln(33) = ln(sqrt(23*33)) = ln(sqrt(759))
let alp = cia_interpolate(&table, 5000.0, 250.0 * CAS);
let expected = (759.0_f64).sqrt();
assert!(
(alp - expected).abs() / expected < 1e-10,
"Expected {}, got {}",
expected,
alp
);
}
#[test]
fn test_cia_interpolation_low_temp() {
let table = make_test_table();
let alp = cia_interpolate(&table, 500.0, 200.0 * CAS);
assert_eq!(alp, 0.0);
}
#[test]
fn test_cia_interpolation_low_freq() {
let table = make_test_table();
let alp = cia_interpolate(&table, 1500.0, 50.0 * CAS);
let expected = ALPHA_FLOOR.exp();
assert!(
(alp - expected).abs() < 1e-20,
"Expected ~{}, got {}",
expected,
alp
);
}
#[test]
fn test_cia_interpolation_high_freq() {
let table = make_test_table();
let alp = cia_interpolate(&table, 1500.0, 600.0 * CAS);
let expected = ALPHA_FLOOR.exp();
assert!(
(alp - expected).abs() < 1e-20,
"Expected ~{}, got {}",
expected,
alp
);
}
#[test]
fn test_cia_h2h2_not_initialized() {
let result = cia_h2h2(5000.0, 1e15, 1e14);
assert_eq!(result, 0.0);
}
#[test]
fn test_cia_h2h_not_initialized() {
let result = cia_h2h(5000.0, 1e15, 1e15, 1e14);
assert_eq!(result, 0.0);
}
#[test]
fn test_cia_h2he_not_initialized() {
let result = cia_h2he(5000.0, 1e15, 1e15, 1e14);
assert_eq!(result, 0.0);
}
#[test]
fn test_cia_hhe_not_initialized() {
let result = cia_hhe(5000.0, 1e15, 1e15, 1e14);
assert_eq!(result, 0.0);
}
#[test]
fn test_load_cia_table_structure() {
let table = make_test_table();
assert_eq!(table.nlines, 5);
assert_eq!(table.ntemp, 3);
assert_eq!(table.freq.len(), 5);
assert_eq!(table.temp.len(), 3);
assert_eq!(table.alpha.len(), 15);
// Verify log was taken: alpha[0] = ln(11)
assert!((table.alpha[0] - 11.0_f64.ln()).abs() < 1e-15);
}
#[test]
fn test_cia_symmetry_h2h2() {
// H2-H2: density product is ah2^2, so doubling ah2 should quadruple result
let table = make_test_table();
let alp = cia_interpolate(&table, 1500.0, 200.0 * CAS);
let opac1 = FAC * 1e15 * 1e15 * alp;
let opac2 = FAC * 2e15 * 2e15 * alp;
assert!(
(opac2 / opac1 - 4.0).abs() < 1e-10,
"Expected ratio 4.0, got {}",
opac2 / opac1
);
}
#[test]
fn test_cia_product_scaling() {
let table = make_test_table();
let alp = cia_interpolate(&table, 2000.0, 300.0 * CAS);
let d1 = 1e14;
let d2 = 3e14;
let opac1 = FAC * d1 * d1 * alp;
let opac2 = FAC * d2 * d2 * alp;
let ratio = opac2 / opac1;
let expected = (d2 / d1) * (d2 / d1);
assert!(
(ratio - expected).abs() / expected < 1e-10,
"Expected ratio {}, got {}",
expected,
ratio
);
}
}
+1 -2
View File
@@ -6,9 +6,8 @@
//! //!
//! 设置光致电离截面数组,用于辐射转移计算。 //! 设置光致电离截面数组,用于辐射转移计算。
use crate::tlusty::math::{sigk, SigkParams, OpData}; use crate::tlusty::math::{sigk, SigkParams};
use crate::tlusty::state::atomic::AtomicData; use crate::tlusty::state::atomic::AtomicData;
use crate::tlusty::state::constants::{MCROSS, MFREQ};
// ============================================================================ // ============================================================================
// 常量 // 常量
+173
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@@ -0,0 +1,173 @@
//! Determination of state parameters for opacity grid calculations.
//!
//! Translated from SYNSPEC54.FOR subroutine DENSIT(RHO,IDENS)
//! at line 22330.
//!
//! Determines the state parameters (electron density, total particle
//! density, populations) for a given depth point using various input modes.
/// Input mode for density determination.
#[derive(Debug, Clone, Copy, PartialEq)]
pub enum DensitMode {
/// Electron density as input
ElectronDensity = 0,
/// Total particle density as input (negative)
ParticleDensity = -1,
/// Mass density as input (mode 1)
MassDensity1 = 1,
/// Mass density as input (mode 2)
MassDensity2 = 2,
}
/// Parameters for DENSIT calculation.
pub struct DensitParams {
/// Input value (rho, electron density, or particle density)
pub rho: f64,
/// Input mode
pub idens: DensitMode,
/// Temperature (K)
pub temp: f64,
/// Mean molecular weight
pub wmm: f64,
/// Total hydrogen abundance
pub ytot: f64,
/// Boltzmann constant (erg/K)
pub bolk: f64,
/// Hydrogen mass (g)
pub hmass: f64,
/// Molecular flag
pub ifmol: i32,
/// Molecular temperature limit
pub tmolim: f64,
/// Number of levels
pub nlevel: usize,
/// Standard depth index
pub idstd: usize,
}
/// Result of DENSIT calculation.
pub struct DensitResult {
/// Electron density (cm^-3)
pub elec: f64,
/// Mass density (g/cm^3)
pub dens: f64,
/// Total particle density (cm^-3)
pub an: f64,
}
/// Determination of state parameters.
///
/// Determines electron density, mass density, and total particle density
/// from the given input value and mode.
///
/// # Arguments
/// * `params` - Input parameters
/// * `todens_fn` - Function to compute AN from (id, t, ane)
/// * `eldens_fn` - Function to compute ANE from (id, t, an)
/// * `rhonen_fn` - Function to compute (an, ane) from (id, t, rho)
///
/// # Returns
/// Electron density, mass density, and total particle density.
pub fn densit<T, E, R>(
params: &DensitParams,
todens_fn: T,
eldens_fn: E,
rhonen_fn: R,
) -> DensitResult
where
T: Fn(usize, f64, f64) -> (f64, f64, f64, f64),
E: Fn(usize, f64, f64, f64) -> f64,
R: Fn(usize, f64, f64) -> (f64, f64),
{
let id = 0; // Single depth point
let t = params.temp;
let wmm = params.wmm;
let (elec, dens, an) = match params.idens {
DensitMode::ElectronDensity => {
let ane = params.rho;
let (an, _anp, _ahtot, _ahmol) = todens_fn(id, t, ane);
let dens = (an - ane) * wmm;
(ane, dens, an)
}
DensitMode::ParticleDensity => {
let an = params.rho / t / params.bolk;
let ane = eldens_fn(id, t, an, 0.0);
let dens = wmm * (an - ane);
(ane, dens, an)
}
DensitMode::MassDensity1 => {
let rho = params.rho;
let (an, ane) = rhonen_fn(id, t, rho);
(ane, rho, an)
}
DensitMode::MassDensity2 => {
let rho = params.rho;
let (an, ane) = rhonen_fn(id, t, rho);
(ane, rho, an)
}
};
DensitResult { elec, dens, an }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_densit_electron_density() {
let params = DensitParams {
rho: 1e13,
idens: DensitMode::ElectronDensity,
temp: 10000.0,
wmm: 1.0,
ytot: 1.0,
bolk: 1.380658e-16,
hmass: 1.67e-24,
ifmol: 0,
tmolim: 9000.0,
nlevel: 10,
idstd: 0,
};
// Mock todens: return (an, anp, ahtot, ahmol)
let todens_fn = |_id: usize, _t: f64, ane: f64| {
(ane * 1.1, ane * 0.1, ane * 1.0, 0.0)
};
let eldens_fn = |_id: usize, _t: f64, _an: f64, _ane: f64| 1e13;
let rhonen_fn = |_id: usize, _t: f64, _rho: f64| (1e13, 1e12);
let result = densit(&params, todens_fn, eldens_fn, rhonen_fn);
assert!(result.elec > 0.0);
assert!(result.dens > 0.0);
assert!(result.an > 0.0);
}
#[test]
fn test_densit_particle_density() {
let params = DensitParams {
rho: 1e13,
idens: DensitMode::ParticleDensity,
temp: 10000.0,
wmm: 1.0,
ytot: 1.0,
bolk: 1.380658e-16,
hmass: 1.67e-24,
ifmol: 0,
tmolim: 9000.0,
nlevel: 10,
idstd: 0,
};
let todens_fn = |_id: usize, _t: f64, ane: f64| {
(ane * 1.1, ane * 0.1, ane * 1.0, 0.0)
};
let eldens_fn = |_id: usize, _t: f64, an: f64, _ane: f64| an * 0.1;
let rhonen_fn = |_id: usize, _t: f64, _rho: f64| (1e13, 1e12);
let result = densit(&params, todens_fn, eldens_fn, rhonen_fn);
assert!(result.elec >= 0.0);
assert!(result.an > 0.0);
}
}
+114
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@@ -0,0 +1,114 @@
//! Division point between Doppler and asymptotic Stark profiles.
//!
//! Translated from SYNSPEC `DIVSTR` subroutine (synspec54.f:6840).
//!
//! Auxiliary procedure for STARKA - determines the division point
//! between Doppler and asymptotic Stark profiles.
/// Compute the division point between Doppler and asymptotic Stark profiles.
///
/// # Arguments
/// * `betad` - Doppler width in beta units
///
/// # Returns
/// A tuple `(a, div)` where:
/// * `a` = 1.5 * ln(betad) - 1.671
/// * `div` - division point (only meaningful for a > 1); solution of
/// exp(-(beta/betad)^2) / betad / sqrt(pi) = 3 * beta^(-5/2)
pub fn divstr(betad: f64) -> (f64, f64) {
const CA: f64 = 1.671;
const BL: f64 = 5.821;
const AL: f64 = 1.26;
const CX: f64 = 0.28;
const DX: f64 = 0.0001;
let a = 1.5 * betad.ln() - CA;
if betad < BL {
return (a, 0.0);
}
let mut x = if a >= AL {
a.sqrt() * (1.0 + 1.25 * a.ln() / (4.0 * a - 5.0))
} else {
(CX + a).sqrt()
};
for _ in 0..5 {
let xn = x * (1.0 - (x * x - 2.5 * x.ln() - a) / (2.0 * x * x - 2.5));
if (xn - x).abs() <= DX {
x = xn;
break;
}
x = xn;
}
(a, x)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_divstr_small_betad() {
// For betad < BL (5.821), div should be 0
let (a, div) = divstr(3.0);
assert!(a < 0.0); // 1.5*ln(3) - 1.671 ≈ -0.024
assert_eq!(div, 0.0);
}
#[test]
fn test_divstr_large_betad() {
// For large betad, should compute meaningful division point
let (a, div) = divstr(100.0);
assert!(a > 1.0);
assert!(div > 0.0);
assert!(div.is_finite());
}
#[test]
fn test_divstr_boundary() {
// At betad = BL, a should be approximately 1.5*ln(5.821) - 1.671
let (a, _div) = divstr(5.821);
let expected_a = 1.5 * 5.821_f64.ln() - 1.671;
assert!((a - expected_a).abs() < 1e-10);
}
#[test]
fn test_divstr_a_ge_al() {
// betad large enough that a >= AL (1.26)
let (a, div) = divstr(20.0);
assert!(a >= 1.26);
assert!(div > 0.0);
assert!(div.is_finite());
}
#[test]
fn test_divstr_a_lt_al() {
// betad in range where a < AL but betad >= BL
let (a, div) = divstr(7.0);
// a = 1.5*ln(7) - 1.671 ≈ 1.265 (close to AL boundary)
if a < 1.26 {
assert!(div > 0.0);
}
assert!(div.is_finite());
}
#[test]
fn test_divstr_convergence() {
// Verify Newton iteration converges for various inputs
for betad in [10.0, 50.0, 100.0, 500.0, 1000.0] {
let (a, div) = divstr(betad);
assert!(div.is_finite(), "div not finite for betad={}", betad);
assert!(div > 0.0, "div not positive for betad={}", betad);
// Verify the equation: x^2 - 2.5*ln(x) - a ≈ 0
let residual = div * div - 2.5 * div.ln() - a;
assert!(
residual.abs() < 0.01,
"residual too large for betad={}: {}",
betad,
residual
);
}
}
}
+83
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@@ -0,0 +1,83 @@
//! 溶解分数辅助量。
//!
//! 重构自 SYNSPEC `dwnfr0.f`。
use crate::synspec::state::constants::{MDEPTH, MZZ};
/// 溶解分数辅助量。
///
/// 计算电子密度的幂次和溶解分数系数。
///
/// # 参数
///
/// * `id` - 深度点索引 (0-based)
/// * `elec` - 电子密度数组
/// * `temp` - 温度数组
/// * `elec23` - 输出: 电子密度的 2/3 次方
/// * `z3` - 输出: 电荷的三次方
/// * `dwc1` - 输出: 溶解分数系数 1
/// * `dwc2` - 输出: 溶解分数系数 2
pub fn dwnfr0(
id: usize,
elec: &[f64; MDEPTH],
temp: &[f64; MDEPTH],
elec23: &mut [f64; MDEPTH],
z3: &mut [f64; MZZ],
dwc1: &mut [[f64; MDEPTH]; MZZ],
dwc2: &mut [f64; MDEPTH],
) {
const UN: f64 = 1.0;
const SIXTH: f64 = UN / 6.0;
const CCOR: f64 = 0.09;
const P1: f64 = 0.1402;
const P2: f64 = 0.1285;
const P3: f64 = UN;
const P4: f64 = 3.15;
const P5: f64 = 4.0;
const F23: f64 = -2.0 / 3.0;
let ane = elec[id];
elec23[id] = (F23 * ane.ln()).exp();
let anes = (SIXTH * ane.ln()).exp();
let acor = CCOR * anes / temp[id].sqrt();
let x = (P4 * (UN + P3 * acor).ln()).exp();
dwc2[id] = P2 * x;
let a3 = acor * acor * acor;
for izz in 0..MZZ {
let z = (izz + 1) as f64;
z3[izz] = z * z * z;
dwc1[izz][id] = P1 * (x + P5 * (z - 1.0) * a3);
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_dwnfr0_basic() {
let mut elec = [0.0f64; MDEPTH];
let mut temp = [0.0f64; MDEPTH];
let mut elec23 = [0.0f64; MDEPTH];
let mut z3 = [0.0f64; MZZ];
let mut dwc1 = [[0.0f64; MDEPTH]; MZZ];
let mut dwc2 = [0.0f64; MDEPTH];
// 设置测试值
elec[0] = 1.0e14;
temp[0] = 10000.0;
dwnfr0(0, &elec, &temp, &mut elec23, &mut z3, &mut dwc1, &mut dwc2);
// 验证 elec23 = elec^(-2/3)
let expected_elec23 = (1.0e14_f64.powf(-2.0 / 3.0));
assert!((elec23[0] - expected_elec23).abs() < 1.0e-10);
// 验证 z3
assert!((z3[0] - 1.0).abs() < 1.0e-10); // z=1 -> z3=1
assert!((z3[1] - 8.0).abs() < 1.0e-10); // z=2 -> z3=8
// 验证 dwc2 为正
assert!(dwc2[0] > 0.0);
}
}
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//! Dissolved fraction for a given frequency.
//!
//! Translated from SYNSPEC54.FOR subroutine DWNFR1(FR,FR0,ID,IZZ,DW1) at line 22349.
//!
//! Computes the dissolved fraction for a spectral line at frequency FR
//! relative to the series limit frequency FR0, for ionization stage IZZ
//! at depth point ID.
/// Parameters for dissolved fraction calculation.
pub struct Dwnfr1Params<'a> {
/// Frequency at which to evaluate (Hz)
pub fr: f64,
/// Series limit frequency (Hz)
pub fr0: f64,
/// Depth index
pub id: usize,
/// Ionic charge
pub izz: usize,
/// Z^3 array for each ionic charge
pub z3: &'a [f64],
/// Electron density to the 2/3 power at each depth
pub elec23: &'a [f64],
/// DWC1 parameter (IZZ x depth, row-major)
pub dwc1: &'a [f64],
/// Number of depth points (for 2D indexing of dwc1)
pub ndepth: usize,
/// DWC2 parameter at each depth
pub dwc2: &'a [f64],
/// Bergmann factor (usually 1.0)
pub bergfc: f64,
}
/// Dissolved fraction for a given frequency.
///
/// Computes the dissolved fraction for a spectral line at frequency FR
/// relative to the series limit frequency FR0. Returns 1.0 (fully dissolved)
/// when FR >= FR0.
///
/// # Arguments
/// * `params` - Calculation parameters
///
/// # Returns
/// Dissolved fraction (0 to 1)
pub fn dwnfr1(params: &Dwnfr1Params) -> f64 {
if params.fr < params.fr0 {
// Constants
let sqfrh = 5.734152e7;
let tkn = 3.01;
let ckn = 5.33333333;
let cb = 8.59e14;
let izz_f = params.izz as f64;
let xn = sqfrh * izz_f / (params.fr0 - params.fr).sqrt();
let xkn = if xn <= tkn {
1.0
} else {
let xn1 = 1.0 / (xn + 1.0);
ckn * xn * xn1 * xn1
};
let beta = cb * params.z3[params.izz] * xkn
/ (xn * xn * xn * xn)
* params.elec23[params.id]
* params.bergfc;
let beta3 = beta * beta * beta;
let beta32 = beta3.sqrt();
// DWC1 is 2D: (IZZ, ID) -> dwc1[izz * ndepth + id]
let dwc1_val = params.dwc1[params.izz * params.ndepth + params.id];
let f = (dwc1_val * beta3) / (1.0 + params.dwc2[params.id] * beta32);
1.0 - f / (1.0 + f)
} else {
1.0
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_dwnfr1_above_limit() {
// When fr >= fr0, should return 1.0
let z3 = vec![1.0, 8.0, 27.0];
// ELEC23 = ANE^(-2/3), for ANE=1e13 -> ~2.15e-9
let elec23 = vec![2.15e-9; 3];
let dwc1 = vec![0.0; 6]; // 2 ionic charges x 3 depths
let dwc2 = vec![0.5; 3];
let params = Dwnfr1Params {
fr: 3.3e15,
fr0: 3.3e15,
id: 0,
izz: 1,
z3: &z3,
elec23: &elec23,
dwc1: &dwc1,
ndepth: 3,
dwc2: &dwc2,
bergfc: 1.0,
};
assert_eq!(dwnfr1(&params), 1.0);
}
#[test]
fn test_dwnfr1_below_limit() {
// When fr < fr0, should return something < 1.0
let z3 = vec![1.0, 8.0, 27.0];
let elec23 = vec![2.15e-9; 3];
let mut dwc1 = vec![0.0; 6]; // 2 x 3
dwc1[1 * 3 + 0] = 0.1; // DWC1(IZZ=1, ID=0)
let dwc2 = vec![0.5; 3];
let params = Dwnfr1Params {
fr: 3.0e15,
fr0: 3.3e15,
id: 0,
izz: 1,
z3: &z3,
elec23: &elec23,
dwc1: &dwc1,
ndepth: 3,
dwc2: &dwc2,
bergfc: 1.0,
};
let result = dwnfr1(&params);
assert!(result > 0.0 && result <= 1.0, "dwnfr1 out of range: {}", result);
}
#[test]
fn test_dwnfr1_well_below_limit() {
// Far from limit, dissolved fraction should be close to 1.0
let z3 = vec![1.0, 8.0, 27.0];
let elec23 = vec![2.15e-9; 3];
let mut dwc1 = vec![0.0; 6];
dwc1[1 * 3 + 0] = 0.1;
let dwc2 = vec![0.5; 3];
let params = Dwnfr1Params {
fr: 3.3e15 - 1.0e4, // very close to limit: xn >> TKN
fr0: 3.3e15,
id: 0,
izz: 1,
z3: &z3,
elec23: &elec23,
dwc1: &dwc1,
ndepth: 3,
dwc2: &dwc2,
bergfc: 1.0,
};
let result = dwnfr1(&params);
assert!(result > 0.9, "Expected close to 1.0, got {}", result);
}
}
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//! Electron density calculation by Newton-Raphson method.
//!
//! Translated from SYNSPEC54.FOR subroutine ELDENS (line 22552).
//!
//! Evaluates the electron density and total hydrogen number density
//! for a given total particle number density and temperature by solving
//! the set of Saha equations, charge conservation and particle conservation
//! equations using a Newton-Raphson method.
/// Parameters for ELDENS calculation.
pub struct EldensParams {
/// Depth point index
pub id: usize,
/// Temperature (K)
pub t: f64,
/// Total particle number density (cm^-3)
pub an: f64,
/// Initial electron density estimate (cm^-3), updated on output
pub ane: f64,
/// Boltzmann constant (erg/K)
pub bolk: f64,
/// Total hydrogen abundance YTOT
pub ytot: f64,
/// Reference atom is hydrogen flag
pub is_h_ref: bool,
/// Molecular flag (>0 to consider molecules)
pub ifmol: i32,
/// Molecular temperature limit
pub tmolim: f64,
/// Previous electron density ratio (anerel)
pub anerel: f64,
/// Standard partition function PFSTD(1,1)
pub pfstd_h: f64,
}
/// Result of ELDENS calculation.
pub struct EldensResult {
/// Electron density (cm^-3)
pub ane: f64,
/// Proton number density (cm^-3)
pub anp: f64,
/// Total hydrogen number density (cm^-3)
pub ahtot: f64,
/// Hydrogen molecule fraction
pub ahmol: f64,
/// Negative hydrogen ion density
pub anhmi: f64,
/// Updated electron density ratio
pub anerel: f64,
/// Mean molecular weight update factor
pub wmm_factor: f64,
}
/// Electron density calculation by Newton-Raphson method.
///
/// # Arguments
/// * `params` - Input parameters
/// * `state_fn` - Callback to STATE subroutine: (id, t, ane) -> (q, dqn)
/// * `lineqs_fn` - Callback to LINEQS: (a, b, n) -> solution vector
/// * `moleq_fn` - Callback to MOLEQ: (id, t, an, aein, mode) -> ane
///
/// # Returns
/// Updated electron density and related quantities.
#[allow(unused_assignments)]
#[allow(unused_assignments)]
#[allow(unused_assignments)]
pub fn eldens<S, L, M>(
params: &EldensParams,
state_fn: S,
lineqs_fn: L,
moleq_fn: M,
) -> EldensResult
where
S: Fn(usize, f64, f64) -> (f64, f64),
L: Fn(&mut [f64], &mut [f64], usize) -> Vec<f64>,
M: Fn(usize, f64, f64, f64, i32) -> f64,
{
let t = params.t;
let an = params.an;
let mut ane = params.ane;
let mut anerel = params.anerel;
let bolk = params.bolk;
// Constants
let un = 1.0_f64;
let two = 2.0_f64;
let half = 0.5_f64;
// Check molecular regime
if params.ifmol > 0 && t < params.tmolim {
let aein = an * anerel;
let ane_mol = moleq_fn(params.id, t, an, aein, 0);
return EldensResult {
ane: ane_mol,
anp: 0.0,
ahtot: 0.0,
ahmol: 0.0,
anhmi: 0.0,
anerel: ane_mol / an,
wmm_factor: 1.0,
};
}
// Initialize coefficients
let mut qm = 0.0_f64;
let mut q2 = 0.0_f64;
let mut qp = 0.0_f64;
let mut q = 0.0_f64;
let mut dqn = 0.0_f64;
let tk = bolk * t;
let thet = 5.0404e3 / t;
// Hydrogen ionization/dissociation coefficients
let (q0, ih2) = if params.is_h_ref {
let qm_val = 1.0353e-16 / t / t.sqrt() * (8762.9 / t).exp();
let qh0 = ((15.38287 + 1.5 * t.log10() - 13.595 * thet) * std::f64::consts::LN_10).exp();
let (ih2, qp_val, q2_val) = if t > 16000.0 {
(0, 0.0, 0.0)
} else {
let qp = tk * ((-11.206998 + thet * (2.7942767 + thet * (0.079196803 - 0.024790744 * thet)))
* std::f64::consts::LN_10)
.exp();
let q2 = tk * ((-12.533505 + thet * (4.9251644 + thet * (-0.056191273 + 0.0032687661 * thet)))
* std::f64::consts::LN_10)
.exp();
(1, qp, q2)
};
qm = qm_val;
qp = qp_val;
q2 = q2_val;
(qh0, ih2)
} else {
(0.0, 0)
};
// Initial estimate of electron density
if anerel <= 0.0 {
anerel = if t > 1.0e4 {
0.5
} else {
0.1 // Default if no previous data
};
}
ane = an * anerel;
// Newton-Raphson loop
let mut ah = 0.0_f64;
let mut anh = 0.0_f64;
let mut it = 0;
let mut delne;
loop {
it += 1;
// Call STATE to get total charge Q and its derivative DQN
let (q_val, dqn_val) = state_fn(params.id, t, ane);
q = q_val;
dqn = dqn_val;
if params.is_h_ref {
let qh = q0 * 2.0 / params.pfstd_h;
// Auxiliary parameters
let g2 = qh / ane;
let g3 = qm * ane;
let a = un + g2 + g3;
let d = g2 - g3;
if it <= 1 {
if ih2 == 0 {
let f1 = un / a;
let fe = d / a + q;
ah = ane / fe;
anh = ah * f1;
} else {
let e = g2 * qp / q2;
let b = two * (un + e);
let gg = ane * q2;
let c1 = b * (gg * b + a * d) - e * a * a;
let c2 = a * (two * e + b * q) - d * b;
let c3 = -e - b * q;
let f1 = ((c2 * c2 - 4.0 * c1 * c3).sqrt() - c2) * half / c1;
let fe = f1 * d + e * (un - a * f1) / b + q;
ah = ane / fe;
anh = ah * f1;
}
}
let ae = anh / ane;
let gg = ae * qp;
let _e = anh * q2;
let b = anh * qm;
// Matrix of linearized system R (3x3) and rhs S
let mut r = [0.0_f64; 9];
let mut s = [0.0_f64; 3];
r[0] = params.ytot; // R(1,1)
r[1] = -two * (anh * q2 + gg); // R(1,2)
r[2] = un; // R(1,3)
r[3] = -q; // R(2,1)
r[4] = -d - two * gg; // R(2,2)
r[5] = un + b + ae * (g2 + gg) - dqn * ah; // R(2,3)
r[6] = -un; // R(3,1)
r[7] = a + 4.0 * (anh * q2 + gg); // R(3,2)
r[8] = b - ae * (g2 + two * gg); // R(3,3)
s[0] = an - ane - params.ytot * ah + anh * (anh * q2 + gg);
s[1] = anh * (d + gg) + q * ah - ane;
s[2] = ah - anh * (a + two * (anh * q2 + gg));
// Solve linear system
let p = lineqs_fn(&mut r, &mut s, 3);
ah += p[0];
anh += p[1];
delne = p[2];
ane += delne;
} else {
// Hydrogen is not the reference atom
if it == 1 {
ane = an * half;
ah = ane / params.ytot;
}
let mut r = [0.0_f64; 4];
let mut s = [0.0_f64; 2];
r[0] = params.ytot; // R(1,1)
r[1] = un; // R(1,2)
r[2] = -q; // R(2,1) - using QREF=0 for now
r[3] = un - dqn * ah; // R(2,2) - using DQNR=0 for now
s[0] = an - ane - params.ytot * ah;
s[1] = q * ah - ane;
let p = lineqs_fn(&mut r, &mut s, 2);
ah += p[0];
delne = p[1];
ane += delne;
}
// Convergence check
if ane <= 0.0 {
ane = 1.0e-7 * an;
}
if (delne / ane).abs() <= 1.0e-6 || it > 20 {
break;
}
}
// Update anerel for subsequent calls
anerel = ane / an;
let ahtot = ah;
// Compute hydrogen molecule quantities
let (ahmol, anp, anhmi, wmm_factor) = if params.is_h_ref {
let qh = q0 * 2.0 / params.pfstd_h;
let ahmol = anh * anh * q2;
let anp = anh / ane * qh;
let anhmi = anh * ane * qm;
let anhn = anh + anp + anhmi + 2.0 * ahmol;
let wmm_factor = if anhn > 0.0 {
1.0 / (1.0 - ahmol / anhn)
} else {
1.0
};
(ahmol, anp, anhmi, wmm_factor)
} else {
(0.0, 0.0, 0.0, 1.0)
};
EldensResult {
ane,
anp,
ahtot,
ahmol,
anhmi,
anerel,
wmm_factor,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_eldens_basic() {
let params = EldensParams {
id: 0,
t: 10000.0,
an: 1e15,
ane: 0.0,
bolk: 1.380658e-16,
ytot: 1.0,
is_h_ref: true,
ifmol: 0,
tmolim: 9000.0,
anerel: 0.1,
pfstd_h: 2.0,
};
// Mock state: return (q, dqn)
let state_fn = |_id: usize, _t: f64, ane: f64| {
(ane * 0.5, 0.5)
};
// Mock lineqs: simple 3x3 solver
let lineqs_fn = |a: &mut [f64], b: &mut [f64], n: usize| -> Vec<f64> {
// For test, just return small corrections
vec![0.0; n]
};
// Mock moleq
let moleq_fn = |_id: usize, _t: f64, _an: f64, _aein: f64, _mode: i32| -> f64 {
1e14
};
let result = eldens(&params, state_fn, lineqs_fn, moleq_fn);
assert!(result.ane > 0.0, "ANE should be positive");
assert!(result.anerel > 0.0, "ANEREL should be positive");
}
#[test]
fn test_eldens_molecular() {
let params = EldensParams {
id: 0,
t: 5000.0, // Below tmolim
an: 1e15,
ane: 0.0,
bolk: 1.380658e-16,
ytot: 1.0,
is_h_ref: true,
ifmol: 1, // Enable molecular
tmolim: 9000.0,
anerel: 0.1,
pfstd_h: 2.0,
};
let state_fn = |_id: usize, _t: f64, _ane: f64| (0.0, 0.0);
let lineqs_fn = |_a: &mut [f64], _b: &mut [f64], n: usize| vec![0.0; n];
let moleq_fn = |_id: usize, _t: f64, _an: f64, _aein: f64, _mode: i32| 1e14;
let result = eldens(&params, state_fn, lineqs_fn, moleq_fn);
assert!(result.ane > 0.0, "Should use moleq in molecular regime");
}
}
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//! EOS parameter output diagnostics.
//!
//! Translated from SYNSPEC54.FOR subroutine EOSPRI (line 22799).
//!
//! Prints equation of state parameters including atomic, ionic, and molecular
//! number densities and partition functions. Also computes H2+ abundance
//! and element ratios (He/H, C/H, N/H, O/H).
/// Molecular indices used for output (20 selected molecules).
#[allow(dead_code)]
const INSM: [usize; 20] = [2, 3, 4, 5, 6, 7, 8, 12, 17, 25, 29, 30, 32, 34, 122, 126, 134, 179, 198, 214];
/// Element indices for metals (38 elements).
const NELEMX: [usize; 38] = [
1, 2, 3, 4, 5, 6, 7, 8, 9,
11, 12, 13, 14, 15, 16, 17, 19, 20,
21, 22, 23, 24, 25, 26, 28, 29, 32,
35, 37, 38, 39, 40, 41, 53, 56, 57, 58, 60,
];
/// H2+ dissociation constant polynomial coefficients (B&C).
const AMH2: [f64; 5] = [1.13390e+01, -2.97499e+00, 4.10842e-02, -3.58550e-03, 1.31844e-04];
/// Parameters for EOSPRI.
pub struct EospriParams<'a> {
/// Number of depth points
pub nd: usize,
/// Temperature array (K)
pub temp: &'a [f64],
/// Electron density array (cm^-3)
pub elec: &'a [f64],
/// Mass density array (g/cm^3)
pub dens: &'a [f64],
/// Mean molecular weight array
pub wmm: &'a [f64],
/// Mean molecular weight for EOS
pub wmy: &'a [f64],
/// Hydrogen mass
pub hmass: f64,
/// Total abundance YTOT
pub ytot: &'a [f64],
/// Abundance by depth: abndd(element, depth) — 1-indexed element
pub abndd: &'a [Vec<f64>],
/// Molecular flag
pub ifmol: i32,
/// Molecular temperature limit
pub tmolim: f64,
/// Number of molecules
pub nmolec: usize,
/// Molecular names
pub cmol: &'a [String],
/// EOS flag
pub ifeos: i32,
/// Number of metals
pub nmetal: usize,
/// Step for depth loop
pub istp: usize,
}
/// Result of EOSPRI computation.
pub struct EospriOutput {
/// Atomic number densities per depth: anato[element][depth]
pub anato: Vec<Vec<f64>>,
/// Ionic number densities per depth: anion[element][depth]
pub anion: Vec<Vec<f64>>,
/// Molecular number densities per depth: anmol[molecule][depth]
pub anmol: Vec<Vec<f64>>,
/// Atomic partition functions per depth
pub pfato: Vec<Vec<f64>>,
/// Ionic partition functions per depth
pub pfion: Vec<Vec<f64>>,
/// Molecular partition functions per depth
pub pfmol: Vec<Vec<f64>>,
/// H- density per depth
pub anhmi_per_depth: Vec<f64>,
/// H2 density per depth
pub ahmol_per_depth: Vec<f64>,
/// H density per depth
pub ah_per_depth: Vec<f64>,
/// H+ density per depth
pub anp_per_depth: Vec<f64>,
/// Second ionization per depth: anion2[element][depth]
pub anion2: Vec<Vec<f64>>,
/// Summary lines per depth
pub summary: Vec<String>,
}
/// ELDENS result used by EOSPRI.
pub struct EldensSimpleResult {
/// Electron density (cm^-3)
pub ane: f64,
/// Proton number density (cm^-3)
pub anp: f64,
/// Total hydrogen number density (cm^-3)
pub ahtot: f64,
/// Hydrogen molecule fraction
pub ahmol: f64,
/// Negative hydrogen ion density
pub anhmi: f64,
}
/// Compute EOS parameters for diagnostics.
///
/// # Arguments
/// * `params` - Input parameters
/// * `eldens_fn` - Callback: (id, t, ann, ane) -> EldensSimpleResult
///
/// Calls `eldens_fn` iteratively to converge molecular equilibrium,
/// then computes element ratios and formatted output.
pub fn eospri<E>(params: &EospriParams, eldens_fn: E) -> EospriOutput
where
E: Fn(usize, f64, f64, f64) -> EldensSimpleResult,
{
let max_elem = 100;
let max_mol = 600;
let nd = params.nd;
let mut anato = vec![vec![0.0_f64; nd]; max_elem];
let mut anion = vec![vec![0.0_f64; nd]; max_elem];
let mut anmol = vec![vec![0.0_f64; nd]; max_mol];
let pfato = vec![vec![0.0_f64; nd]; max_elem];
let pfion = vec![vec![0.0_f64; nd]; max_elem];
let pfmol = vec![vec![0.0_f64; nd]; max_mol];
let mut anion2 = vec![vec![0.0_f64; nd]; 30];
let mut anhmi_per_depth = vec![0.0_f64; nd];
let mut ahmol_per_depth = vec![0.0_f64; nd];
let mut ah_per_depth = vec![0.0_f64; nd];
let mut anp_per_depth = vec![0.0_f64; nd];
let mut summary = Vec::new();
let istp = if params.istp == 0 { 1 } else { params.istp };
for id in (0..nd).step_by(istp) {
let t = params.temp[id];
let mut ane = params.elec[id];
let rho = params.dens[id];
let mut ann = rho / params.wmm[id] + ane;
// Iterative convergence for molecular equilibrium
if params.ifmol == 0 || t > params.tmolim {
let mut ann0;
loop {
ann0 = ann;
let result = eldens_fn(id, t, ann, ane);
ane = result.ane;
anmol[0][id] = result.anhmi;
anmol[1][id] = result.ahmol;
anato[0][id] = result.ahtot;
anion[0][id] = result.anp;
anhmi_per_depth[id] = result.anhmi;
ahmol_per_depth[id] = result.ahmol;
ah_per_depth[id] = result.ahtot;
anp_per_depth[id] = result.anp;
let hpop = rho / params.wmy[id] / params.hmass;
for &j in NELEMX.iter().take(params.nmetal) {
if j < max_elem {
anato[j][id] *= hpop;
anion[j][id] *= hpop;
if (2..30).contains(&j) {
anion2[j][id] *= hpop;
}
}
}
anato[0][id] = result.ahtot;
anion[0][id] = result.anp;
// Update mean molecular weight
// wmm(id) = wmy(id) / (ytot(id) - anmol(2,id)/hpop) * hmass
let ahmol_hpop = anmol[1][id] / hpop;
let new_wmm = if params.ytot[id] - ahmol_hpop > 0.0 {
params.wmy[id] / (params.ytot[id] - ahmol_hpop) * params.hmass
} else {
params.wmm[id]
};
ann = rho / new_wmm + ane;
if (ann - ann0) / ann0 <= 1.0e-5 {
break;
}
}
}
// Compute H2+ abundance (B&C polynomial)
let te = 5040.0 / t;
let mut aplogj = AMH2[4];
for k in 0..4 {
let km5 = 4 - k;
aplogj = aplogj * te + AMH2[km5];
}
let tk = 1.38054e-16 * t;
let ph2 = -aplogj + (anato[0][id] * anion[0][id]).log10() + 2.0 * tk.log10();
let _anh2b = 10.0_f64.powf(ph2) / tk;
// Compute total hydrogen
let htot = anato[0][id] + anion[0][id] + anmol[0][id]
+ 2.0 * (anmol[1][id] + anmol[2][id])
+ anmol[3][id] + anmol[4][id]
+ anmol[11][id] + 2.0 * anmol[12][id] + anmol[13][id]
+ anmol[14][id]
+ anmol[15][id] + anmol[16][id] + anmol[31][id] + anmol[33][id]
+ 4.0 * anmol[36][id] + 2.0 * anmol[37][id] + 3.0 * anmol[38][id]
+ 2.0 * anmol[39][id] + 3.0 * anmol[40][id] + 2.0 * anmol[56][id]
+ anmol[117][id] + anmol[132][id]
+ 2.0 * anmol[139][id] + 3.0 * anmol[140][id] + 4.0 * anmol[141][id]
+ anmol[147][id] + 2.0 * anmol[148][id] + anmol[221][id];
// Element ratios relative to H
let ahe = if htot > 0.0 { (anato[1][id] + anion[1][id] + anion2[1][id]) / htot } else { 0.0 };
let aca = if htot > 0.0 { (anato[5][id] + anion[5][id] + anion2[5][id]) / htot } else { 0.0 };
let acm = if htot > 0.0 {
(anmol[4][id] + anmol[5][id]
+ anmol[6][id] + 2.0 * (anmol[7][id] + 2.0 * anmol[12][id])
+ anmol[13][id] + 2.0 * anmol[14][id] + anmol[19][id]
+ anmol[36][id] + anmol[37][id] + anmol[38][id]
+ anmol[43][id] + anmol[117][id] + anmol[118][id]
+ anmol[436][id] + anmol[452][id])
/ htot
} else {
0.0
};
let ana = if htot > 0.0 { (anato[6][id] + anion[6][id] + anion2[6][id]) / htot } else { 0.0 };
let anm = if htot > 0.0 {
(anmol[6][id] + 2.0 * anmol[8][id] + anmol[10][id]
+ anmol[11][id] + anmol[13][id] + anmol[22][id]
+ anmol[23][id] + anmol[39][id] + anmol[40][id]
+ anmol[108][id] + anmol[151][id] + anmol[346][id]
+ anmol[437][id] + anmol[451][id] + anmol[453][id])
/ htot
} else {
0.0
};
let aoa = if htot > 0.0 { (anato[7][id] + anion[7][id] + anion2[7][id]) / htot } else { 0.0 };
let aom = if htot > 0.0 {
(anmol[2][id] + anmol[3][id]
+ anmol[5][id] + 2.0 * anmol[9][id] + anmol[10][id] + anmol[24][id]
+ anmol[25][id] + anmol[28][id] + anmol[29][id] + anmol[30][id]
+ anmol[34][id] + 2.0 * anmol[43][id] + anmol[48][id] + anmol[50][id]
+ anmol[53][id] + 2.0 * anmol[55][id] + anmol[64][id]
+ 2.0 * anmol[65][id] + anmol[83][id] + anmol[108][id]
+ anmol[112][id] + anmol[114][id] + anmol[117][id]
+ anmol[118][id] + anmol[125][id] + anmol[133][id]
+ anmol[152][id] + anmol[178][id] + anmol[183][id]
+ 2.0 * anmol[184][id] + anmol[199][id] + anmol[215][id]
+ anmol[220][id] + 2.0 * anmol[246][id] + anmol[291][id]
+ anmol[438][id] + anmol[452][id] + anmol[453][id])
/ htot
} else {
0.0
};
let ac = aca + acm;
let an = ana + anm;
let ao = aoa + aom;
// Format summary
let line = format!(
"EOS: T={:.1} rho={:.3e} N={:.3e} Ne={:.3e} Htot={:.3e} He/H={:.3e} C/H={:.3e} N/H={:.3e} O/H={:.3e}",
t, rho, ann, ane, htot, ahe, ac, an, ao
);
summary.push(line);
}
EospriOutput {
anato,
anion,
anmol,
pfato,
pfion,
pfmol,
anhmi_per_depth,
ahmol_per_depth,
ah_per_depth,
anp_per_depth,
anion2,
summary,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_eospri_constants() {
assert_eq!(NELEMX.len(), 38);
assert_eq!(INSM.len(), 20);
assert_eq!(AMH2.len(), 5);
assert_eq!(NELEMX[0], 1);
assert_eq!(NELEMX[37], 60);
}
#[test]
fn test_eospri_basic() {
let nd = 1;
let abndd_data: Vec<Vec<f64>> = vec![vec![0.0; nd]; 100];
let params = EospriParams {
nd,
temp: &[10000.0],
elec: &[1.0e12],
dens: &[1.0e-10],
wmm: &[1.0],
wmy: &[1.0],
hmass: 1.67e-24,
ytot: &[1.0],
abndd: &abndd_data,
ifmol: 0,
tmolim: 10000.0,
nmolec: 0,
cmol: &[],
ifeos: 0,
nmetal: 0,
istp: 1,
};
// Mock eldens callback
let eldens_fn = |_id: usize, _t: f64, ann: f64, ane: f64| -> EldensSimpleResult {
EldensSimpleResult {
ane,
anp: ane * 0.9,
ahtot: ann * 0.8,
ahmol: 0.0,
anhmi: 0.0,
}
};
let _output = eospri(&params, eldens_fn);
}
}
+193
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@@ -0,0 +1,193 @@
//! EXOMOL partition functions for 32 molecular species.
//!
//! Translated from SYNSPEC `EXOPF` subroutine (synspec54.f:23664).
//!
//! Reads tabulated partition function data from `data/EXOMOL/*.pf` files
//! on first call, then performs simple lookup or Irwin-based extrapolation.
use std::sync::Mutex;
use super::irwpf;
/// Number of molecular species.
const NMOL: usize = 32;
/// Molecular species filenames (Fortran `character*4`, leading space stripped).
const FILPF: [&str; NMOL] = [
"AlO", "C2", "CH", "CN", "CO",
"CS", "CaH", "CaO", "CrH", "FeH",
"H2", "HCl", "HF", "MgH", "MgO",
"N2", "NH", "NO", "NS", "NaH",
"OH", "PH", "SH", "SiH", "SiO",
"SiS", "TiH", "TiO", "VO",
"H2O", "H2S", "CO2",
];
/// Number of temperature points per species (before scaling).
const NTEMP_RAW: [usize; NMOL] = [
9, 10, 8, 3, 9, 3, 3, 8, 3, 10,
10, 5, 5, 3, 5, 9, 5, 5, 5, 5,
5, 4, 5, 5, 9, 5, 48, 8, 8, 10,
3, 5,
];
/// Tsuji molecular indices for each species.
const INDTSU: [i32; NMOL] = [
134, 8, 5, 7, 6, 20, 34, 179, 198, 214,
2, 36, 33, 32, 126, 9, 12, 11, 23, 122,
4, 148, 16, 17, 25, 28, 315, 29, 30, 3,
57, 44,
];
/// Cached EXOMOL data: partition functions `pf[mol][temp_index]` and
/// scaled temperature counts `ntemp[mol]`.
struct ExopfData {
/// Partition function values: pf[mol * max_ntemp + j]
/// Stored flat; max_ntemp = 48000 (48*1000).
pf: Vec<f64>,
/// Scaled temperature counts per species.
ntemp: Vec<usize>,
}
static EXOPF_DATA: Mutex<Option<ExopfData>> = Mutex::new(None);
/// Compute the file path for a given species.
fn species_filename(name: &str) -> String {
let trimmed = name.trim();
format!("data/EXOMOL/{}.pf", trimmed)
}
/// Read all EXOMOL partition function files.
fn read_exopf_data(data_dir: &str) -> Result<ExopfData, String> {
// Scale ntemp: multiply by 1000, except species 27 (TiH) divide by 10
let mut ntemp = Vec::with_capacity(NMOL);
for i in 0..NMOL {
let mut nt = NTEMP_RAW[i] * 1000;
if i == 26 {
// TiH: ntemp(27) in Fortran (1-indexed) = index 26
nt /= 10;
}
ntemp.push(nt);
}
let max_ntemp = *ntemp.iter().max().unwrap_or(&0);
let mut pf = vec![0.0f64; NMOL * max_ntemp];
for i in 0..NMOL {
let filename = format!("{}/{}", data_dir, species_filename(FILPF[i]));
let content = match std::fs::read_to_string(&filename) {
Ok(c) => c,
Err(_) => continue, // Skip missing files
};
for (j, line) in content.lines().enumerate() {
if j >= ntemp[i] {
break;
}
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() >= 2
&& let Ok(val) = parts[1].parse::<f64>() {
pf[i * max_ntemp + j] = val;
}
}
}
Ok(ExopfData { pf, ntemp })
}
/// EXOMOL partition function lookup.
///
/// # Arguments
/// * `indmol` - Tsuji molecular index.
/// * `t` - Temperature (K).
/// * `data_dir` - Path to data directory containing `data/EXOMOL/*.pf` files.
///
/// # Returns
/// Partition function value (0.0 if species not found).
pub fn exopf(indmol: i32, t: f64, data_dir: &str) -> Result<f64, String> {
// Initialize data on first call
{
let mut guard = EXOPF_DATA
.lock()
.map_err(|e| format!("Lock error: {}", e))?;
if guard.is_none() {
*guard = Some(read_exopf_data(data_dir)?);
}
}
let guard = EXOPF_DATA
.lock()
.map_err(|e| format!("Lock error: {}", e))?;
let data = guard.as_ref().unwrap();
// Find species index
let ie = INDTSU.iter().position(|&x| x == indmol);
let ie = match ie {
Some(idx) => idx,
None => return Ok(0.0),
};
let tmax = data.ntemp[ie] as f64;
let max_ntemp = *data.ntemp.iter().max().unwrap_or(&1);
if t <= tmax {
// Direct lookup
let j = t as usize;
if j > 0 && j <= data.ntemp[ie] {
Ok(data.pf[ie * max_ntemp + j - 1])
} else {
Ok(0.0)
}
} else {
// Extrapolate using Irwin partition functions
// Need to drop the lock before calling irwpf (which also locks)
drop(guard);
let umx = irwpf::irwpf(0, 0, indmol, tmax, data_dir, 1).unwrap_or(1.0);
let uirw = irwpf::irwpf(0, 0, indmol, t, data_dir, 1).unwrap_or(1.0);
// Re-acquire lock to read pf value
let guard = EXOPF_DATA
.lock()
.map_err(|e| format!("Lock error: {}", e))?;
let data = guard.as_ref().unwrap();
if umx.abs() > 1e-30 {
Ok(data.pf[ie * max_ntemp + data.ntemp[ie] - 1] / umx * uirw)
} else {
Ok(0.0)
}
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_species_count() {
assert_eq!(FILPF.len(), NMOL);
assert_eq!(NTEMP_RAW.len(), NMOL);
assert_eq!(INDTSU.len(), NMOL);
}
#[test]
fn test_ntemp_scaling() {
// TiH (index 26): 48*1000/10 = 4800
assert_eq!(NTEMP_RAW[26] * 1000 / 10, 4800);
// Others: raw * 1000
assert_eq!(NTEMP_RAW[0] * 1000, 9000);
}
#[test]
fn test_species_filename() {
assert_eq!(species_filename("AlO"), "data/EXOMOL/AlO.pf");
assert_eq!(species_filename(" H2"), "data/EXOMOL/H2.pf");
}
#[test]
fn test_indtsu_mapping() {
// H2O is last entry
assert_eq!(INDTSU[29], 3);
// CO is index 4
assert_eq!(INDTSU[4], 6);
}
}
+79
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@@ -0,0 +1,79 @@
//! 第一指数积分函数 E1(x)。
//!
//! 重构自 SYNSPEC `expint.f`
/// 第一指数积分函数 E1(x)。
///
/// 使用有理逼近公式,分 x <= 1 和 x > 1 两段。
///
/// # 参数
///
/// * `x` - 自变量
///
/// # 返回值
///
/// E1(x) 的近似值
pub fn expint(x: f64) -> f64 {
if x <= 1.0 {
// x <= 1 的有理逼近
-x.ln() - 0.57721566
+ x * (0.99999193
+ x * (-0.24991055
+ x * (0.05519968
+ x * (-0.00976004 + x * 0.00107857))))
} else {
// x > 1 的有理逼近
(-x).exp() * ((0.2677734343
+ x * (8.6347608925
+ x * (18.059016973 + x * (8.5733287401 + x))))
/ (3.9584969228
+ x * (21.0996530827
+ x * (25.6329561486 + x * (9.5733223454 + x)))))
/ x
}
}
#[cfg(test)]
mod tests {
use super::*;
use approx::assert_relative_eq;
#[test]
fn test_expint_small_x() {
// E1(0.5) ≈ 0.5598 (参考值)
let result = expint(0.5);
assert!(result.is_finite());
assert!(result > 0.0);
}
#[test]
fn test_expint_x_eq_1() {
// E1(1) ≈ 0.21938
let result = expint(1.0);
assert_relative_eq!(result, 0.21938, epsilon = 1e-4);
}
#[test]
fn test_expint_large_x() {
// E1(5) ≈ 0.001148
let result = expint(5.0);
assert_relative_eq!(result, 0.0011483, epsilon = 1e-3);
}
#[test]
fn test_expint_very_small_x() {
// x -> 0+ 时 E1(x) -> +∞
let result = expint(0.01);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_expint_large_x_decay() {
// x 大时 E1(x) ~ exp(-x)/x
let x = 10.0;
let result = expint(x);
let approx = (-x).exp() / x;
assert_relative_eq!(result, approx, epsilon = 0.1);
}
}
+1 -1
View File
@@ -50,7 +50,7 @@ pub fn extprf(dlam: f64, it: usize, iline: usize, anel: f64, dlast: f64, plast:
// WE = W0 * 10^anel * 1e-16 // WE = W0 * 10^anel * 1e-16
// Fortran: EXP(ANEL*2.3025851) = 10^ANEL (因为 ln(10) ≈ 2.3025851) // Fortran: EXP(ANEL*2.3025851) = 10^ANEL (因为 ln(10) ≈ 2.3025851)
let we = w0_val * (anel * 2.3025851_f64).exp() * 1e-16; let we = w0_val * (anel * std::f64::consts::LN_10).exp() * 1e-16;
// 使用 PI 的精确值 // 使用 PI 的精确值
const PI: f64 = std::f64::consts::PI; const PI: f64 = std::f64::consts::PI;
+484
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@@ -0,0 +1,484 @@
//! fingrd — 存储完整的插值不透明度表。
//!
//! Fortran 原始签名: SUBROUTINE FINGRD
//!
//! 将计算的不透明度表写入文件(文本和二进制格式)。
//!
//! 注意: Fortran 版本直接操作文件 I/O 和 COMMON 块。
//! Rust 版本提供纯计算核心函数和编排函数。
use std::io::{BufWriter, Write};
use std::fs::File;
/// 光速 (cm/s)
#[allow(dead_code)]
const CL: f64 = 2.997925e10;
/// 波长 (nm) 转换为频率 (s^-1)
///
/// Fortran 原始逻辑:
/// ```fortran
/// 2.997925e18/wlgrid(k)
/// ```
pub fn wavelength_to_frequency(wavelength_nm: f64) -> f64 {
2.997925e18 / wavelength_nm
}
/// 频率 (s^-1) 转换为波长 (nm)
pub fn frequency_to_wavelength(freq: f64) -> f64 {
2.997925e18 / freq
}
/// 对数网格生成
///
/// Fortran 原始逻辑:
/// ```fortran
/// wl1=log(wlam1)
/// wl2=log(wlam2)
/// dwl=(wl2-wl1)/(nfgrid-1)
/// do i=1,nfgrid
/// wlgrid(i)=exp(wl1+(i-1)*dwl)
/// end do
/// ```
pub fn generate_log_grid(wlam1: f64, wlam2: f64, n: usize) -> Vec<f64> {
let wl1 = wlam1.ln();
let wl2 = wlam2.ln();
let dwl = (wl2 - wl1) / (n - 1) as f64;
(0..n)
.map(|i| (wl1 + i as f64 * dwl).exp())
.collect()
}
/// 线性网格生成
///
/// Fortran 原始逻辑:
/// ```fortran
/// at1=log(temp1)
/// at2=log(temp2)
/// dt=(at2-at1)/(ntemp-1)
/// do i=1,ntemp
/// tempg(i)=exp(at1+(i-1)*dt)
/// end do
/// ```
pub fn generate_linear_grid_in_log(val1: f64, val2: f64, n: usize) -> Vec<f64> {
let at1 = val1.ln();
let at2 = val2.ln();
let dt = if n > 1 { (at2 - at1) / (n - 1) as f64 } else { 0.0 };
(0..n)
.map(|i| (at1 + i as f64 * dt).exp())
.collect()
}
/// 不透明度表数据结构
#[derive(Debug, Clone)]
pub struct OpacityTable {
/// 温度网格 (K)
pub temperatures: Vec<f64>,
/// 密度网格 (g/cm^3)
pub densities: Vec<Vec<f64>>,
/// 电子密度网格 (g/cm^3)
pub electron_densities: Vec<Vec<f64>>,
/// 波长网格 (nm)
pub wavelengths: Vec<f64>,
/// 不透明度表 [temp_idx][dens_idx][freq_idx]
pub opacity: Vec<Vec<Vec<f32>>>,
}
/// 计算不透明度表的统计信息
#[derive(Debug, Clone)]
pub struct OpacityTableStats {
/// 最小不透明度
pub min_opacity: f32,
/// 最大不透明度
pub max_opacity: f32,
/// 平均不透明度
pub mean_opacity: f32,
/// 非零元素百分比
pub nonzero_percent: f64,
}
/// 计算不透明度表统计信息
pub fn compute_opacity_stats(table: &OpacityTable) -> OpacityTableStats {
let mut min_op = f32::MAX;
let mut max_op = f32::MIN;
let mut sum = 0.0_f64;
let mut count = 0;
let mut nonzero = 0;
for temp_data in &table.opacity {
for dens_data in temp_data {
for &op in dens_data {
count += 1;
sum += op as f64;
if op > 0.0 {
nonzero += 1;
}
if op < min_op {
min_op = op;
}
if op > max_op {
max_op = op;
}
}
}
}
OpacityTableStats {
min_opacity: min_op,
max_opacity: max_op,
mean_opacity: if count > 0 { (sum / count as f64) as f32 } else { 0.0 },
nonzero_percent: if count > 0 { 100.0 * nonzero as f64 / count as f64 } else { 0.0 },
}
}
/// H- 不透明度标志
#[derive(Debug, Clone)]
#[derive(Default)]
pub struct OpacityFlags {
/// H- 光电离
pub h_minus: bool,
/// H2+ 光电离
pub h2_plus: bool,
/// He- 光电离
pub he_minus: bool,
/// CH 不透明度
pub ch: bool,
/// OH 不透明度
pub oh: bool,
/// H2- 不透明度
pub h2_minus: bool,
/// CIA H2-H2
pub cia_h2h2: bool,
/// CIA H2-He
pub cia_h2he: bool,
/// CIA H2-H
pub cia_h2h: bool,
/// CIA H-He
pub cia_hhe: bool,
}
/// 不透明度表写入参数
#[derive(Debug, Clone)]
pub struct FingrdParams<'a> {
/// 温度网格 (K)
pub temperatures: &'a [f64],
/// 密度网格 [temp_idx][dens_idx] (g/cm^3)
pub densities: &'a [Vec<f64>],
/// 电子密度网格 [temp_idx][dens_idx] (g/cm^3)
pub electron_densities: &'a [Vec<f64>],
/// 波长网格 (nm)
pub wavelengths: &'a [f64],
/// 不透明度表 [temp_idx][dens_idx][freq_idx] (f32)
pub absgrd: &'a [Vec<Vec<f32>>],
/// 每温度点的密度数 nden(temp_idx)
pub nden: &'a [usize],
/// 元素丰度 abnd(92)
pub abundances: &'a [f64],
/// 相对丰度 relabn(92)
pub rel_abundances: &'a [f64],
/// 不透明度标志
pub flags: &'a OpacityFlags,
/// 分子开关 ifmol
pub ifmol: i32,
/// 分子温度极限 tmolim
pub tmolim: f64,
/// 输出表文件名
pub tabname: &'a str,
/// 二进制输出标志 (0=text+binary, 1=binary only)
pub ibingr: i32,
/// 密度类型 (<10: uniform, >=10: variable)
pub idens: i32,
}
/// 编排函数: 将不透明度表写入文本和二进制文件。
///
/// Fortran 原始逻辑: SUBROUTINE FINGRD
/// - 文本输出到 tabname 文件 (Fortran unit 53)
/// - 二进制输出到 unit 63
pub fn fingrd(params: &FingrdParams) -> Result<(), String> {
let ntemp = params.temperatures.len();
let nfgrid = params.wavelengths.len();
if ntemp == 0 || nfgrid == 0 {
return Ok(());
}
let nden0 = params.nden.first().copied().unwrap_or(1);
// --- 文本输出 (ibingr == 0) ---
if params.ibingr == 0 {
let file = File::create(params.tabname)
.map_err(|e| format!("Cannot create {}: {}", params.tabname, e))?;
let mut w = BufWriter::new(file);
// Header: element abundances
writeln!(w, "opacity table with element abundances:").map_err(|e| e.to_string())?;
writeln!(w, "element for EOS for opacities").map_err(|e| e.to_string())?;
for iat in 0..92 {
let abnd = params.abundances.get(iat).copied().unwrap_or(0.0);
let rel = params.rel_abundances.get(iat).copied().unwrap_or(0.0);
writeln!(w, " {:4} {:12.3e} {:12.3e}", iat + 1, abnd, abnd * rel)
.map_err(|e| e.to_string())?;
}
// Molecule info
writeln!(w).map_err(|e| e.to_string())?;
writeln!(w, "molecules - ifmol,tmolim:").map_err(|e| e.to_string())?;
writeln!(w, "{:4}{:10.1}", params.ifmol, params.tmolim).map_err(|e| e.to_string())?;
// Opacity flags
writeln!(w, "additional opacities").map_err(|e| e.to_string())?;
writeln!(w, " H- H2+ He- CH OH H2- CIA: H2H2 H2He H2H HHe").map_err(|e| e.to_string())?;
let f = params.flags;
writeln!(w, "{:4}{:4}{:4}{:4}{:4}{:4} {:4}{:4}{:4}{:4}",
f.h_minus as i32, f.h2_plus as i32, f.he_minus as i32,
f.ch as i32, f.oh as i32, f.h2_minus as i32,
f.cia_h2h2 as i32, f.cia_h2he as i32, f.cia_h2h as i32, f.cia_hhe as i32)
.map_err(|e| e.to_string())?;
if params.idens < 10 {
// Uniform density grid
let ndens = nden0;
writeln!(w).map_err(|e| e.to_string())?;
writeln!(w, "number of frequencies, temperatures, densities:").map_err(|e| e.to_string())?;
writeln!(w, " {:10}{:10}{:10}", nfgrid, ntemp, ndens).map_err(|e| e.to_string())?;
// Log temperatures
write!(w, "log temperatures").map_err(|e| e.to_string())?;
for i in 0..ntemp {
if i % 6 == 0 { writeln!(w).map_err(|e| e.to_string())?; }
write!(w, "{:11.6}", params.temperatures[i].ln()).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
// Log densities
write!(w, "log densities").map_err(|e| e.to_string())?;
for j in 0..ndens {
if j % 6 == 0 { writeln!(w).map_err(|e| e.to_string())?; }
let d = params.densities[0].get(j).copied().unwrap_or(1.0);
write!(w, "{:11.6}", d.ln()).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
// Log electron densities
write!(w, "log electron densities from EOS").map_err(|e| e.to_string())?;
for i in 0..ntemp {
for j in 0..ndens {
if (i * ndens + j) % 6 == 0 { writeln!(w).map_err(|e| e.to_string())?; }
let e = params.electron_densities[i].get(j).copied().unwrap_or(1.0);
write!(w, "{:11.6}", e.ln()).map_err(|e| e.to_string())?;
}
}
writeln!(w).map_err(|e| e.to_string())?;
// Opacity table
for k in 0..nfgrid {
writeln!(w).map_err(|e| e.to_string())?;
writeln!(w, " *** frequency # : {:8}{:15.5}", k + 1, params.wavelengths[k])
.map_err(|e| e.to_string())?;
let freq = 2.997925e18 / params.wavelengths[k];
writeln!(w, "{:20.8e}", freq).map_err(|e| e.to_string())?;
for j in 0..ndens {
for i in 0..ntemp {
if i % 6 == 0 { writeln!(w).map_err(|e| e.to_string())?; }
let val = params.absgrd[i][j].get(k).copied().unwrap_or(0.0);
write!(w, "{:14.6e}", val).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
}
}
} else {
// Variable density grid
writeln!(w).map_err(|e| e.to_string())?;
writeln!(w, "number of frequencies, temperatures, densities:").map_err(|e| e.to_string())?;
writeln!(w, " {:10}{:10}{:10}", nfgrid, ntemp, -(nden0 as i32)).map_err(|e| e.to_string())?;
// nden per temperature
for i in 0..ntemp {
write!(w, "{:3}", params.nden.get(i).copied().unwrap_or(0)).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
// Log temperatures
write!(w, "log temperatures").map_err(|e| e.to_string())?;
for i in 0..ntemp {
if i % 6 == 0 { writeln!(w).map_err(|e| e.to_string())?; }
write!(w, "{:11.6}", params.temperatures[i].ln()).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
// Log densities per temperature
writeln!(w, "log densities").map_err(|e| e.to_string())?;
for i in 0..ntemp {
let nd = params.nden.get(i).copied().unwrap_or(0);
for j in 0..nd {
if j % 6 == 0 && j > 0 { writeln!(w).map_err(|e| e.to_string())?; }
let d = params.densities[i].get(j).copied().unwrap_or(1.0);
write!(w, "{:14.6}", d.ln()).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
}
// Log electron densities per temperature
writeln!(w, "log electron densities from EOS").map_err(|e| e.to_string())?;
for i in 0..ntemp {
let nd = params.nden.get(i).copied().unwrap_or(0);
for j in 0..nd {
if j % 6 == 0 && j > 0 { writeln!(w).map_err(|e| e.to_string())?; }
let e = params.electron_densities[i].get(j).copied().unwrap_or(1.0);
write!(w, "{:14.6}", e.ln()).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
}
// Opacity table
for k in 0..nfgrid {
writeln!(w).map_err(|e| e.to_string())?;
writeln!(w, " *** frequency # : {:8}{:15.5}", k + 1, params.wavelengths[k])
.map_err(|e| e.to_string())?;
let freq = 2.997925e18 / params.wavelengths[k];
writeln!(w, "{:20.8e}", freq).map_err(|e| e.to_string())?;
for i in 0..ntemp {
let nd = params.nden.get(i).copied().unwrap_or(0);
for j in 0..nd {
if j % 6 == 0 { writeln!(w).map_err(|e| e.to_string())?; }
let val = params.absgrd[i].get(j).and_then(|row| row.get(k)).copied().unwrap_or(0.0);
write!(w, "{:14.6e}", val).map_err(|e| e.to_string())?;
}
writeln!(w).map_err(|e| e.to_string())?;
}
}
}
}
// --- 二进制输出 (always) ---
// Note: Binary output requires Fortran-compatible unformatted I/O.
// In Rust, we write a simplified binary format.
// The actual binary format depends on the Fortran runtime.
// For now, we skip binary output as it requires Fortran unit 63.
Ok(())
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_wavelength_to_frequency() {
// 500 nm → frequency
let freq = wavelength_to_frequency(500.0);
let expected = 2.997925e18 / 500.0;
assert!((freq - expected).abs() / expected < 1e-10);
}
#[test]
fn test_frequency_to_wavelength() {
let wl = frequency_to_wavelength(6e14);
let expected = 2.997925e18 / 6e14;
assert!((wl - expected).abs() / expected < 1e-10);
}
#[test]
fn test_wavelength_frequency_roundtrip() {
let wl = 500.0;
let freq = wavelength_to_frequency(wl);
let wl_back = frequency_to_wavelength(freq);
assert!((wl - wl_back).abs() < 1e-10);
}
#[test]
fn test_generate_log_grid() {
let grid = generate_log_grid(100.0, 1000.0, 11);
assert_eq!(grid.len(), 11);
assert!((grid[0] - 100.0).abs() < 1e-10);
assert!((grid[10] - 1000.0).abs() < 1e-10);
// 网格应该是对数等距的
let ratio = grid[1] / grid[0];
for i in 1..10 {
assert!((grid[i + 1] / grid[i] - ratio).abs() < 1e-10);
}
}
#[test]
fn test_generate_linear_grid_in_log() {
let grid = generate_linear_grid_in_log(1000.0, 100000.0, 5);
assert_eq!(grid.len(), 5);
assert!((grid[0] - 1000.0).abs() < 1e-10);
assert!((grid[4] - 100000.0).abs() < 1e-3);
}
#[test]
fn test_compute_opacity_stats() {
let table = OpacityTable {
temperatures: vec![5000.0, 10000.0],
densities: vec![vec![1e-8, 1e-7]],
electron_densities: vec![vec![1e-10, 1e-9]],
wavelengths: vec![100.0, 200.0],
opacity: vec![
vec![
vec![1.0, 2.0],
vec![3.0, 4.0],
],
vec![
vec![5.0, 6.0],
vec![7.0, 8.0],
],
],
};
let stats = compute_opacity_stats(&table);
assert_eq!(stats.min_opacity, 1.0);
assert_eq!(stats.max_opacity, 8.0);
assert!((stats.mean_opacity - 4.5).abs() < 0.01);
assert_eq!(stats.nonzero_percent, 100.0);
}
#[test]
fn test_opacity_flags_default() {
let flags = OpacityFlags::default();
assert!(!flags.h_minus);
assert!(!flags.cia_h2h2);
}
#[test]
fn test_fingrd_writes_text_file() {
let dir = std::env::temp_dir().join("fingrd_test");
std::fs::create_dir_all(&dir).unwrap();
let tabname = dir.join("test_table.txt");
let tabname_str = tabname.to_str().unwrap();
let params = FingrdParams {
temperatures: &[5000.0, 10000.0],
densities: &[vec![1e-8, 1e-7], vec![1e-8, 1e-7]],
electron_densities: &[vec![1e-10, 1e-9], vec![1e-10, 1e-9]],
wavelengths: &[100.0, 200.0, 500.0],
absgrd: &[
vec![vec![1.0, 2.0, 3.0], vec![4.0, 5.0, 6.0]],
vec![vec![7.0, 8.0, 9.0], vec![10.0, 11.0, 12.0]],
],
nden: &[2, 2],
abundances: &[1.0; 92],
rel_abundances: &[1.0; 92],
flags: &OpacityFlags::default(),
ifmol: 0,
tmolim: 10000.0,
tabname: tabname_str,
ibingr: 0,
idens: 0,
};
let result = fingrd(&params);
assert!(result.is_ok());
// Verify file was created and has content
let content = std::fs::read_to_string(&tabname).unwrap();
assert!(content.contains("opacity table"));
assert!(content.contains("number of frequencies"));
assert!(content.contains("frequency #"));
// Cleanup
std::fs::remove_dir_all(&dir).ok();
}
}
+280
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//! Opacity Project ionization fraction interpolation for SYNSPEC.
//!
//! Translated from SYNSPEC54.FOR subroutine FRAC1 (line 23240).
//!
//! Interpolates pre-tabulated ionization fractions from the Opacity Project
//! data (read by FRACTN) to the local temperature and electron density at
//! each depth point, then computes the number density of each ionization
//! stage.
//!
//! # Input
//!
//! - Temperature and electron density arrays
//! - OP ionization fraction table (from FRACTN)
//! - Elemental abundances, mean molecular weight, total density
//!
//! # Output
//!
//! - `rrr[id][ion][iat]` — number density fraction for element `iat`,
//! ionization stage `ion` at depth `id`
// ============================================================================
// 常量
// ============================================================================
/// Maximum number of temperature grid points
pub const MTEMP: usize = 100;
/// Maximum number of electron density grid points
pub const MELEC: usize = 60;
/// Maximum number of ionization stages
pub const MION1: usize = 30;
// ============================================================================
// OP 数据结构 (COMMON /FRACOP/)
// ============================================================================
/// Opacity Project ionization fraction table.
///
/// Corresponds to Fortran COMMON /FRACOP/:
/// ```fortran
/// COMMON/FRACOP/ frac(mtemp,melec,mion1), fracm(mtemp,melec),
/// itemp(mtemp), ntt
/// ```
#[derive(Debug, Clone)]
pub struct FracOpData {
/// Ionization fractions [MTEMP x MELEC x MION1]
pub frac: Vec<Vec<Vec<f64>>>,
/// Molecular fractions [MTEMP x MELEC]
pub fracm: Vec<Vec<f64>>,
/// Temperature grid indices [MTEMP]
pub itemp: Vec<i32>,
/// Number of temperature points
pub ntt: usize,
}
impl Default for FracOpData {
fn default() -> Self {
Self {
frac: vec![vec![vec![0.0; MION1]; MELEC]; MTEMP],
fracm: vec![vec![0.0; MELEC]; MTEMP],
itemp: vec![0; MTEMP],
ntt: 0,
}
}
}
// ============================================================================
// 参数结构体
// ============================================================================
/// Parameters for FRAC1 calculation.
pub struct Frac1Params<'a> {
/// Number of depth points
pub nd: usize,
/// Temperature array [nd] (K)
pub temp: &'a [f64],
/// Electron density array [nd] (cm^-3)
pub elec: &'a [f64],
/// Total density array [nd] (g/cm^3)
pub dens: &'a [f64],
/// Mean molecular weight array [nd]
pub wmm: &'a [f64],
/// Total hydrogen fraction array [nd]
pub ytot: &'a [f64],
/// Elemental abundance [30 x nd] — abndd(iat, id)
pub abndd: &'a [&'a [f64]],
/// OP ionization fraction table (from FRACTN)
pub fracop: &'a FracOpData,
/// Maximum number of elements to process (typically 30)
pub max_elements: usize,
}
/// Result of FRAC1 calculation.
pub struct Frac1Result {
/// Number density fraction [nd x MION1 x 30] — rrr(id, ion, iat)
pub rrr: Vec<Vec<Vec<f64>>>,
}
// ============================================================================
// 核心计算
// ============================================================================
/// Compute ionization fractions by interpolation of OP data.
///
/// For each depth point, computes log10(T) and log10(Ne), then
/// bilinearly interpolates the pre-tabulated OP ionization fractions
/// to get the number density of each ionization stage.
pub fn frac1(params: &Frac1Params) -> Frac1Result {
let nd = params.nd;
let fracop = params.fracop;
let ntt = fracop.ntt;
let mut rrr = vec![vec![vec![0.0; MION1]; 30]; nd];
if ntt == 0 {
return Frac1Result { rrr };
}
// Compute log10(T) and log10(Ne) for each depth
let mut xxt = vec![0.0f64; nd];
let mut xxe = vec![0.0f64; nd];
let mut kt0 = vec![0i32; nd];
let mut kn0 = vec![0i32; nd];
for id in 0..nd {
xxt[id] = params.temp[id].log10();
kt0[id] = 2 * (20.0 * xxt[id]) as i32;
xxe[id] = params.elec[id].log10();
kn0[id] = (2.0 * xxe[id]) as i32;
}
// Loop over elements
for iat in 0..params.max_elements.min(30) {
// Find temperature index for each depth
for id in 0..nd {
let kt1 = find_temp_index(kt0[id], &fracop.itemp, ntt);
let kn1 = find_elec_index(kn0[id]);
// Bilinear interpolation coefficients
let xt1 = 0.025 * fracop.itemp[kt1] as f64;
let dxt = 0.05;
let at1 = (xxt[id] - xt1) / dxt;
let xn1 = 0.5 * kn1 as f64;
let dxn = 0.5;
let an1 = (xxe[id] - xn1) / dxn;
// Interpolate each ionization stage
for ion in 0..MION1 {
let x11 = fracop.frac[kt1][kn1][ion];
let x21 = fracop.frac[kt1 + 1][kn1][ion];
let x12 = fracop.frac[kt1][kn1 + 1][ion];
let x22 = fracop.frac[kt1 + 1][kn1 + 1][ion];
let rrx = if x11 * x21 * x12 * x22 == 0.0 {
// Linear interpolation when any value is zero
let xx1 = x11 + at1 * (x21 - x11);
let xx2 = x12 + at1 * (x22 - x12);
xx1 + an1 * (xx2 - xx1)
} else {
// Log-space interpolation
let lx11 = x11.log10();
let lx21 = x21.log10();
let lx12 = x12.log10();
let lx22 = x22.log10();
let xx1 = lx11 + at1 * (lx21 - lx11);
let xx2 = lx12 + at1 * (lx22 - lx12);
let lrrx = xx1 + an1 * (xx2 - xx1);
10f64.powf(lrrx)
};
rrr[id][ion][iat] = rrx * params.abndd[iat][id]
* params.dens[id] / params.wmm[id] / params.ytot[id];
}
}
}
Frac1Result { rrr }
}
/// Find temperature index in OP table.
///
/// Returns the index `kt1` such that `itemp[kt1] <= kt0 < itemp[kt1+1]`.
fn find_temp_index(kt0: i32, itemp: &[i32], ntt: usize) -> usize {
if ntt == 0 {
return 0;
}
if kt0 < itemp[0] {
return 0;
}
if kt0 >= itemp[ntt - 1] {
return ntt - 1;
}
for it in 0..ntt {
if kt0 == itemp[it] {
return it;
}
}
// Fallback: find bracketing interval
for it in 0..ntt - 1 {
if kt0 >= itemp[it] && kt0 < itemp[it + 1] {
return it;
}
}
ntt - 1
}
/// Find electron density index in OP table.
///
/// Returns the index `kn1` such that `kn1*0.5 <= log10(Ne) < (kn1+1)*0.5`.
fn find_elec_index(kn0: i32) -> usize {
if kn0 < 1 {
0
} else if kn0 >= 60 {
59
} else {
kn0 as usize
}
}
// ============================================================================
// 测试
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_frac1_empty_table() {
let temp = [10000.0];
let elec = [1e14];
let dens = [1e-10];
let wmm = [1.0];
let ytot = [1.0];
let abnd_row = vec![0.0; 1];
let abndd: Vec<&[f64]> = vec![&abnd_row; 30];
let fracop = FracOpData::default();
let params = Frac1Params {
nd: 1,
temp: &temp,
elec: &elec,
dens: &dens,
wmm: &wmm,
ytot: &ytot,
abndd: &abndd,
fracop: &fracop,
max_elements: 30,
};
let result = frac1(&params);
assert_eq!(result.rrr.len(), 1);
assert_eq!(result.rrr[0].len(), MION1);
}
#[test]
fn test_find_temp_index() {
let itemp = [100, 200, 300, 400, 500];
assert_eq!(find_temp_index(50, &itemp, 5), 0); // below range
assert_eq!(find_temp_index(100, &itemp, 5), 0); // exact match
assert_eq!(find_temp_index(300, &itemp, 5), 2); // exact match
assert_eq!(find_temp_index(600, &itemp, 5), 4); // above range
}
#[test]
fn test_find_elec_index() {
assert_eq!(find_elec_index(-1), 0);
assert_eq!(find_elec_index(0), 0);
assert_eq!(find_elec_index(10), 10);
assert_eq!(find_elec_index(70), 59);
}
#[test]
fn test_fracop_default() {
let data = FracOpData::default();
assert_eq!(data.ntt, 0);
assert_eq!(data.frac.len(), MTEMP);
assert_eq!(data.frac[0].len(), MELEC);
assert_eq!(data.frac[0][0].len(), MION1);
}
}
+466
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//! 电离分数数据读取 (FRACTN)。
//!
//! 从 `ioniz.dat` 文件读取 OP 电离分数表,计算各元素的电离分数。
//!
//! # 功能
//!
//! 读取电离势和统计权重数据,结合温度和电子密度网格,
//! 计算各电离态的分数分布。
//!
//! # Fortran 原始代码
//!
//! ```fortran
//! subroutine fractn(iatnum)
//! common/fracop/frac(mtemp,melec,mion1),fracm(mtemp,melec),
//! itemp(mtemp),ntt
//! ...
//! end
//! ```
use std::fs::File;
use std::io::{BufRead, BufReader};
use super::frac1::{MTEMP, MELEC, MION1};
// ============================================================================
// 常量
// ============================================================================
/// 最大数据集数
pub const MDAT: usize = 17;
// ============================================================================
// 数据结构
// ============================================================================
/// FRACTN 输出 - 电离分数表。
#[derive(Debug, Clone)]
pub struct FracOp {
/// 电离分数 [MTEMP][MELEC][MION1]
/// frac[it][ie][ion] = 元素 iatnum 在温度 it、电子密度 ie 下的电离态 ion 分数
pub frac: Vec<Vec<Vec<f64>>>,
/// 负离子分数 [MTEMP][MELEC]
pub fracm: Vec<Vec<f64>>,
/// 温度索引数组 [MTEMP]
pub itemp: Vec<i32>,
/// 有效温度点数
pub ntt: usize,
}
impl FracOp {
/// 创建新的空 FracOp。
pub fn new() -> Self {
Self {
frac: vec![vec![vec![0.0; MION1]; MELEC]; MTEMP],
fracm: vec![vec![0.0; MELEC]; MTEMP],
itemp: vec![0; MTEMP],
ntt: 0,
}
}
}
impl Default for FracOp {
fn default() -> Self {
Self::new()
}
}
// ============================================================================
// 静态数据
// ============================================================================
/// 各元素的数据集索引 (IDAT)
/// 索引从 1 开始(iatnum = 1..30),0 表示无数据
const IDAT: [usize; 31] = [
0, // 占位
1, 2, 0, 0, 0, 3, 4, 5, 0, 6,
7, 8, 9, 10, 0, 11, 0, 12, 0, 13,
0, 0, 0, 14, 15, 16, 0, 17, 0, 0,
];
/// 统计权重 GG(ion, dataset)
/// 使用一维数组存储,索引: (ion-1) * MDAT + (dataset-1)
const GG_DATA: [[f64; MDAT]; MION1] = [
[2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2.],
[0., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1.],
[0., 0., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2.],
[0., 0., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1.],
[0., 0., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2.],
[0., 0., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1.],
[0., 0., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6.],
[0., 0., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9.],
[0., 0., 0., 4., 4., 4., 4., 4., 4., 4., 4., 4., 4., 4., 4., 4., 4.],
[0., 0., 0., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9.],
[0., 0., 0., 0., 0., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1.],
[0., 0., 0., 0., 0., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2., 2.],
[0., 0., 0., 0., 0., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1.],
[0., 0., 0., 0., 0., 0., 0., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6.],
[0., 0., 0., 0., 0., 0., 0., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9.],
[0., 0., 0., 0., 0., 0., 0., 4., 4., 4., 4., 4., 4., 4., 4., 4., 4.],
[0., 0., 0., 0., 0., 0., 0., 9., 9., 9., 9., 9., 9., 9., 9., 9., 9.],
[0., 0., 0., 0., 0., 0., 0., 6., 6., 6., 6., 6., 6., 6., 6., 6., 6.],
[0., 0., 0., 0., 0., 0., 0., 1., 1., 1., 1., 1., 1., 1., 1., 1., 1.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 10., 10., 10., 10., 10., 10., 10., 10.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 21., 21., 21., 21., 21., 21., 21., 21.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 28., 28., 28., 28., 28., 28., 28., 28.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 25., 25., 25., 25., 25., 25., 25., 25.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 6., 6., 6., 6., 6., 6., 6., 6.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 7., 7., 7., 7., 7., 7., 7., 7.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 6., 6., 25., 25., 25., 25., 25., 25.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 30., 30., 30., 30., 30., 30.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 25., 25., 25., 25., 25., 25.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 28., 28., 28., 28., 28., 28.],
[0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 21., 21., 21., 21., 21., 21.],
];
/// 各数据集的电离势 UU(ion, dataset) * 1000 cm^-1
/// 对应 Fortran 的 uu 数组
/// 只有非零值需要存储,按 (dataset_index, ion_index) -> value
fn get_u0(iatnum: usize, ion_idx: usize) -> f64 {
// ion_idx: 1..iatnum (1-indexed)
// 对应 Fortran: u0(i) = uu(i, idat(iatnum)) * 1000.
let dataset = IDAT[iatnum];
if dataset == 0 || ion_idx == 0 || ion_idx > iatnum {
return 0.0;
}
// 各数据集的 UU 值 (已乘 1000)
// 数据集 1: H, He
// 数据集 2: Li, Be
// 数据集 3: C
// 数据集 4: N
// 数据集 5: O
// 数据集 6: Ne
// 数据集 7: Na
// 数据集 8: Mg
// 数据集 9: Al
// 数据集 10: Si
// 数据集 11: S
// 数据集 12: Ar
// 数据集 13: Ca
// 数据集 14: Fe
// 数据集 15: Ni
// 数据集 16: Zn
// 数据集 17: Kr
// 预定义的 UU 数据集 (单位: 1000 cm^-1,已乘 1000)
const U_DATASETS: [[f64; 30]; 18] = [
// 数据集 0 (未使用)
[0.0; 30],
// 数据集 1: H (1 ion)
[109678.7, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 2: Li, Be (2 ions)
[198310.8, 438908.9, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 3: C (6 ions)
[90820.0, 196665.0, 386241.0, 520178.0, 3162395.0, 3952061.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 4: N (7 ions)
[117225.0, 238751.0, 382704.0, 624866.0, 789537.0, 4452758.0, 5380089.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 5: O (8 ions)
[109837.0, 283240.0, 443086.0, 624384.0, 918657.0, 1114008.0, 5963135.0, 7028393.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 6: Ne (10 ions)
[173930.0, 330391.0, 511800.0, 783300.0, 1018000.0, 1273800.0, 1671792.0, 1928462.0,
9645005.0, 10986876.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 7: Na (11 ions)
[41449.0, 381395.0, 577800.0, 797800.0, 1116200.0, 1388500.0, 1681500.0, 2130800.0,
2418700.0, 11817061.0, 13297676.0, 0.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 8: Mg (12 ions)
[61671.0, 121268.0, 646410.0, 881100.0, 1139400.0, 1504300.0, 1814300.0, 2144700.0,
2645200.0, 2964400.0, 14210261.0, 15829951.0, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 9: Al (13 ions)
[48278.0, 151860.0, 229446.0, 967800.0, 1239800.0, 1536300.0, 1947300.0, 2295400.0,
2663400.0, 3214800.0, 3565600.0, 16825022.0, 18584138.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 10: Si (14 ions)
[65748.0, 131838.0, 270139.0, 364093.0, 1345100.0, 1653900.0, 1988400.0, 2445300.0,
2831900.0, 3237800.0, 3839800.0, 4222400.0, 19661693.0, 21560630.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 11: S (16 ions)
[83558.0, 188200.0, 280900.0, 381541.0, 586200.0, 710184.0, 2265900.0, 2647400.0,
3057700.0, 3606100.0, 4071400.0, 4554300.0, 5255900.0, 5703600.0, 26002663.0, 28182535.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 12: Ar (18 ions)
[127110.0, 222848.0, 328600.0, 482400.0, 605100.0, 734040.0, 1002730.0, 1157080.0,
3407300.0, 3860900.0, 4347000.0, 4986600.0, 5533800.0, 6095500.0, 6894200.0, 7404400.0,
33237173.0, 35699936.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 13: Ca (20 ions)
[49306.0, 95752.0, 410642.0, 542600.0, 681600.0, 877400.0, 1026000.0, 1187600.0,
1520640.0, 1704047.0, 4774000.0, 5301000.0, 5861000.0, 6595000.0, 7215000.0, 7860000.0,
8770000.0, 9338000.0, 41366000.0, 44177410.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 14: Fe (24 ions)
[54576.0, 132966.0, 249700.0, 396500.0, 560200.0, 731020.0, 1291900.0, 1490000.0,
1688000.0, 1971000.0, 2184000.0, 2404000.0, 2862000.0, 3098520.0, 8151000.0, 8850000.0,
9560000.0, 10480000.0, 11260000.0, 12070000.0, 13180000.0, 13882000.0, 60344000.0, 63675900.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 15: Ni (25 ions)
[59959.0, 126145.0, 271550.0, 413000.0, 584000.0, 771100.0, 961440.0, 1569000.0,
1789000.0, 2003000.0, 2307000.0, 2536000.0, 2771000.0, 3250000.0, 3509820.0, 9152000.0,
9872000.0, 10620000.0, 11590000.0, 12410000.0, 13260000.0, 14420000.0, 15162000.0, 65660000.0,
69137400.0, 0.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 16: Zn (26 ions)
[63737.0, 130563.0, 247220.0, 442000.0, 605000.0, 799000.0, 1008000.0, 1218380.0,
1884000.0, 2114000.0, 2341000.0, 2668000.0, 2912000.0, 3163000.0, 3686000.0, 3946820.0,
10180000.0, 10985000.0, 11850000.0, 12708000.0, 13620000.0, 14510000.0, 15797000.0, 16500000.0,
71203000.0, 74829600.0, 0.0, 0.0, 0.0, 0.0],
// 数据集 17: Kr (28 ions)
[61600.0, 146542.0, 283800.0, 443000.0, 613500.0, 870000.0, 1070000.0, 1310000.0,
1560000.0, 1812000.0, 2589000.0, 2840000.0, 3100000.0, 3470000.0, 3740000.0, 4020000.0,
4606000.0, 4896200.0, 12430000.0, 13290000.0, 14160000.0, 15280000.0, 16220000.0, 17190000.0,
18510000.0, 19351000.0, 82984000.0, 86909400.0, 0.0, 0.0],
];
let ds = dataset;
if ds == 0 || ion_idx > 30 {
return 0.0;
}
U_DATASETS[ds][ion_idx - 1]
}
// ============================================================================
// FRACTN 主函数
// ============================================================================
/// 读取指定元素的电离分数数据。
///
/// # 参数
///
/// * `iatnum` - 原子序数 (1..30)。如果数据不存在,返回 `None`。
/// * `data_dir` - 数据文件目录(包含 `ioniz.dat`
///
/// # 返回值
///
/// `FracOp` 结构体,包含电离分数表。如果元素无数据,返回 `None`。
///
/// # Fortran 原始代码
///
/// ```fortran
/// subroutine fractn(iatnum)
/// common/fracop/frac(mtemp,melec,mion1),fracm(mtemp,melec),
/// itemp(mtemp),ntt
/// ...
/// end
/// ```
pub fn fractn(iatnum: usize, data_dir: &str) -> Option<FracOp> {
if iatnum == 0 || iatnum > 30 || IDAT[iatnum] == 0 {
return None;
}
let file_path = format!("{}/ioniz.dat", data_dir);
let file = match File::open(&file_path) {
Ok(f) => f,
Err(_) => return None,
};
let reader = BufReader::new(file);
let mut lines = reader.lines();
let mut frac_op = FracOp::new();
// 设置统计权重和电离势
let mut g0 = [0.0f64; MION1 + 2]; // g0(-1:mion1)
g0[iatnum + 1] = 1.0;
for i in 1..=iatnum {
let ig0 = iatnum - i + 1;
g0[ig0] = GG_DATA[i - 1][IDAT[iatnum]];
}
// 读取头行
let _header = lines.next()?.ok()?;
// 读取温度范围
let line = lines.next()?.ok()?;
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 3 {
return None;
}
let it0: i32 = parts[0].parse().ok()?;
let it1: i32 = parts[1].parse().ok()?;
let itstp: i32 = parts[2].parse().ok()?;
let ntt = ((it1 - it0) / itstp + 1) as usize;
frac_op.ntt = ntt;
// 读取各温度点的数据
for it in 0..ntt {
let line = lines.next()?.ok()?;
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 4 {
continue;
}
let itt: i32 = parts[0].parse().ok()?;
let ie0: i32 = parts[1].parse().ok()?;
let ie1: i32 = parts[2].parse().ok()?;
let iestp: i32 = parts[3].parse().ok()?;
frac_op.itemp[it] = itt;
let t = (std::f64::consts::LN_10 * 0.025 * itt as f64).exp();
let safac0 = t.sqrt() * t / 2.07e-16;
let tkcm = 0.69496 * t;
let net = ((ie1 - ie0) / iestp + 1) as usize;
for _ie in 0..net {
let line = lines.next()?.ok()?;
// 格式: 3i4,2x,4(i4,1x,e9.3)
// 简化解析
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 3 {
continue;
}
let iee: i32 = parts[0].parse().ok()?;
let ion0: usize = parts[1].parse().ok()?;
let ion1: usize = parts[2].parse().ok()?;
let ane = (std::f64::consts::LN_10 * 0.25 * iee as f64).exp();
let safac = safac0 / ane;
let ieind = (iee / 2) as usize;
// 读取分数数据
let mut frac0 = [0.0f64; MION1 + 2]; // frac0(-1:mion1)
let mut ioo = [0i32; MION1 + 2]; // ioo(-1:mion1)
// 解析第一组 (最多 4 个)
let n_parse = (ion1 - ion0 + 1).min(4);
for k in 0..n_parse {
let idx = 3 + k * 2;
if idx + 1 < parts.len() {
ioo[ion0 + k] = parts[idx].parse().unwrap_or(0);
frac0[ion0 + k] = parts[idx + 1].parse().unwrap_or(0.0);
}
}
// 如果有多于 4 个电离态,继续读取
let nio = ion1 - ion0;
if nio >= 3 {
let nlin = nio / 4;
for _ilin in 0..nlin {
let line = lines.next()?.ok()?;
let parts: Vec<&str> = line.split_whitespace().collect();
let start_ion = ion0 + 4 * (_ilin + 1);
for k in 0..4 {
let idx = k * 2;
if idx + 1 < parts.len() && start_ion + k <= ion1 {
ioo[start_ion + k] = parts[idx].parse().unwrap_or(0);
frac0[start_ion + k] = parts[idx + 1].parse().unwrap_or(0.0);
}
}
}
}
// 计算电离分数
let mut z0 = [0.0f64; MION1 + 2]; // z0(-1:mion1)
for ion in ion0..=ion1 {
if ion < iatnum {
if ion == ion0 {
z0[ion] = g0[iatnum - ion];
} else {
z0[ion] = frac0[ion] / frac0[ion - 1] * safac * z0[ion - 1];
let u0_val = get_u0(iatnum, iatnum - ion);
if tkcm > 0.0 && u0_val != 0.0 {
z0[ion] *= (-u0_val / tkcm).exp();
}
}
if z0[ion] != 0.0 {
frac_op.frac[it][ieind][iatnum - ion] = frac0[ion] / z0[ion];
}
} else {
// 负离子 H-
let u0hm = 6090.5;
let z0hm = if ion > 0 && frac0[ion - 1] != 0.0 {
frac0[ion] / frac0[ion - 1] * safac
} else {
0.0
};
let z0hm = if tkcm > 0.0 {
z0hm * (-u0hm / tkcm).exp()
} else {
0.0
};
if z0hm != 0.0 {
frac_op.fracm[it][ieind] = frac0[ion] / z0hm;
}
}
}
}
}
Some(frac_op)
}
// ============================================================================
// 测试
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_idat_table() {
// 验证 IDAT 表的正确性
assert_eq!(IDAT[1], 1); // H
assert_eq!(IDAT[2], 2); // He
assert_eq!(IDAT[3], 0); // Li - 无数据
assert_eq!(IDAT[6], 3); // C
assert_eq!(IDAT[7], 4); // N
assert_eq!(IDAT[8], 5); // O
assert_eq!(IDAT[26], 16); // Fe
}
#[test]
fn test_gg_data() {
// 验证统计权重数据
assert_eq!(GG_DATA[0][0], 2.0); // H 基态
assert_eq!(GG_DATA[0][1], 2.0); // He 基态
assert_eq!(GG_DATA[1][1], 1.0); // He+ 基态
}
#[test]
fn test_get_u0() {
// H 的电离势
let u0_h = get_u0(1, 1);
assert!((u0_h - 109678.7).abs() < 1.0);
// 无效输入
let u0_invalid = get_u0(0, 1);
assert_eq!(u0_invalid, 0.0);
}
#[test]
fn test_frac_op_new() {
let frac_op = FracOp::new();
assert_eq!(frac_op.ntt, 0);
assert_eq!(frac_op.frac.len(), MTEMP);
assert_eq!(frac_op.frac[0].len(), MELEC);
assert_eq!(frac_op.frac[0][0].len(), MION1);
}
#[test]
fn test_fractn_no_data_element() {
// Li (原子序数 3) 没有数据
let result = fractn(3, "/nonexistent");
assert!(result.is_none());
}
#[test]
fn test_fractn_invalid_atomic_number() {
let result = fractn(0, "/nonexistent");
assert!(result.is_none());
let result = fractn(31, "/nonexistent");
assert!(result.is_none());
}
}
+146
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@@ -0,0 +1,146 @@
//! Hydrogenic bound-free Gaunt factors.
//!
//! Translated from SYNSPEC `GAUNT` and `GNTK` functions (synspec54.f:3715, 3763).
/// Hydrogenic bound-free Gaunt factor.
///
/// Calculates the bound-free Gaunt factor for hydrogenic ions
/// for principal quantum number `i` and frequency `fr`.
///
/// # Arguments
/// * `i` - Principal quantum number (1-10)
/// * `fr` - Frequency (Hz)
///
/// # Returns
/// The bound-free Gaunt factor.
pub fn gaunt(i: i32, fr: f64) -> f64 {
let x = fr / 2.99793e14;
match i {
1 => {
1.2302628 + x * (-2.9094219e-3 + x * (7.3993579e-6 - 8.7356966e-9 * x))
+ (12.803223 / x - 5.5759888) / x
}
2 => {
1.1595421 + x * (-2.0735860e-3 + 2.7033384e-6 * x)
+ (-1.2709045 + (-2.0244141 / x + 2.1325684) / x) / x
}
3 => {
1.1450949 + x * (-1.9366592e-3 + 2.3572356e-6 * x)
+ (-0.55936432 + (-0.23387146 / x + 0.52471924) / x) / x
}
4 => {
1.1306695 + x * (-1.3482273e-3 + x * (-4.6949424e-6 + 2.3548636e-8 * x))
+ (-0.31190730 + (0.19683564 - 5.4418565e-2 / x) / x) / x
}
5 => {
1.1190904 + x * (-1.0401085e-3 + x * (-6.9943488e-6 + 2.8496742e-8 * x))
+ (-0.16051018 + (5.5545091e-2 - 8.9182854e-3 / x) / x) / x
}
6 => {
1.1168376 + x * (-8.9466573e-4 + x * (-8.8393133e-6 + 3.4696768e-8 * x))
+ (-0.13075417 + (4.1921183e-2 - 5.5303574e-3 / x) / x) / x
}
7 => {
1.1128632 + x * (-7.4833260e-4 + x * (-1.0244504e-5 + 3.8595771e-8 * x))
+ (-9.5441161e-2 + (2.3350812e-2 - 2.2752881e-3 / x) / x) / x
}
8 => {
1.1093137 + x * (-6.2619148e-4 + x * (-1.1342068e-5 + 4.1477731e-8 * x))
+ (-7.1010560e-2 + (1.3298411e-2 - 9.7200274e-4 / x) / x) / x
}
9 => {
1.1078717 + x * (-5.4837392e-4 + x * (-1.2157943e-5 + 4.3796716e-8 * x))
+ (-5.6046560e-2 + (8.5139736e-3 - 4.9576163e-4 / x) / x) / x
}
10 => {
1.1052734 + x * (-4.4341570e-4 + x * (-1.3235905e-5 + 4.7003140e-8 * x))
+ (-4.7326370e-2 + (6.1516856e-3 - 2.9467046e-4 / x) / x) / x
}
_ => 1.0,
}
}
/// Hydrogenic bound-free Gaunt factor (Klaus Werner version).
///
/// Alternative Gaunt factor calculation for low quantum numbers.
///
/// # Arguments
/// * `i` - Principal quantum number (1-3)
/// * `fr` - Frequency (Hz)
///
/// # Returns
/// The bound-free Gaunt factor.
pub fn gntk(i: i32, fr: f64) -> f64 {
let y = 1.0 / fr;
match i {
1 => 0.9916 + y * (2.71852e13 - y * 2.26846e30),
2 => 1.1050 - y * (2.37490e14 - y * 4.07677e28),
3 => 1.1010 - y * (0.98632e14 - y * 1.03540e28),
_ => 1.0,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_gaunt_n1() {
// Use frequency in valid range for Gaunt factor
let result = gaunt(1, 5.0e14);
assert!(result.is_finite());
assert!(result > 0.0);
}
#[test]
fn test_gaunt_n2() {
// Use frequency in valid range for Gaunt factor
let result = gaunt(2, 5.0e14);
assert!(result.is_finite());
assert!(result > 0.0);
}
#[test]
fn test_gaunt_high_n() {
let result = gaunt(10, 3.0e14);
assert!(result.is_finite());
assert!(result > 0.0);
}
#[test]
fn test_gaunt_default() {
// For n > 10, should return 1.0
let result = gaunt(11, 3.0e14);
assert_eq!(result, 1.0);
}
#[test]
fn test_gntk_n1() {
// Use higher frequency for valid GNTK values
let result = gntk(1, 1.0e15);
assert!(result.is_finite());
}
#[test]
fn test_gntk_n2() {
// Use higher frequency for valid GNTK values
let result = gntk(2, 1.0e15);
assert!(result.is_finite());
}
#[test]
fn test_gntk_n3() {
// Use higher frequency for valid GNTK values
let result = gntk(3, 1.0e15);
assert!(result.is_finite());
}
#[test]
fn test_gntk_default() {
// For n > 3, should return 1.0
let result = gntk(4, 3.0e14);
assert_eq!(result, 1.0);
}
}
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//! Read quasi-molecular satellite line profile data.
//!
//! Translated from SYNSPEC `getlal` subroutine (synspec54.f).
//!
//! Reads profile functions for Lyman alpha, beta, gamma, and Balmer alpha,
//! including quasi-molecular satellites. Data files are in `./data/` directory.
use std::fs::File;
use std::io::{BufRead, BufReader};
use std::path::Path;
use super::allard::{AllardData, AllardTable, NNMAX};
// ============================================================================
// Data file names
// ============================================================================
/// Lyman alpha quasi-molecular data file
const LAQUASI_FILE: &str = "laquasi.dat";
/// Lyman beta quasi-molecular data file
const LBQUASI_FILE: &str = "lbquasi.dat";
/// Lyman gamma quasi-molecular data file
const LGQUASI_FILE: &str = "lgquasi.dat";
/// Balmer alpha quasi-molecular data file
const LHQUASI_FILE: &str = "lhquasi.dat";
// ============================================================================
// Helper: read one quasi-molecular table from file
// ============================================================================
/// Read one quasi-molecular table from a data file.
///
/// # File format
/// Line 1: `nx stnne stnch vneu vcha`
/// Lines 2..nx+1: `xl pl[0] pl[1] pl[2] pl[3] pl[4]`
///
/// # Arguments
/// * `path` - Path to data file
///
/// # Returns
/// Populated `AllardTable` or error message.
fn read_table(path: &Path) -> Result<AllardTable, String> {
let file = File::open(path).map_err(|e| format!("Cannot open {}: {}", path.display(), e))?;
let reader = BufReader::new(file);
let mut lines = reader.lines();
// Read header: nx, stnne, stnch, vneu, vcha
let header = lines
.next()
.ok_or_else(|| format!("Empty file: {}", path.display()))?
.map_err(|e| format!("Read error: {}", e))?;
let parts: Vec<f64> = header
.split_whitespace()
.map(|s| s.parse().unwrap_or(0.0))
.collect();
if parts.len() < 5 {
return Err(format!(
"Invalid header in {}: expected 5 values, got {}",
path.display(),
parts.len()
));
}
let nx = parts[0] as usize;
let stnne_raw = parts[1];
let stnch_raw = parts[2];
let vneu = parts[3];
let vcha = parts[4];
// Read data points
let mut xl = Vec::with_capacity(nx);
let mut pl = Vec::with_capacity(nx);
for (i, line_result) in lines.enumerate() {
if i >= nx {
break;
}
let line = line_result.map_err(|e| format!("Read error at line {}: {}", i + 2, e))?;
let values: Vec<f64> = line
.split_whitespace()
.map(|s| s.parse().unwrap_or(0.0))
.collect();
if values.len() < 6 {
return Err(format!(
"Invalid data at line {} in {}: expected 6 values, got {}",
i + 2,
path.display(),
values.len()
));
}
xl.push(values[0]);
let mut row = [0.0f64; NNMAX];
for j in 0..NNMAX {
row[j] = values[j + 1];
}
pl.push(row);
}
// Convert log densities to linear
let stnne = 10.0f64.powf(stnne_raw);
let stnch = 10.0f64.powf(stnch_raw);
Ok(AllardTable {
xl,
pl,
stnne,
stnch,
vneu,
vcha,
nx,
iwarn: false,
})
}
// ============================================================================
// Main entry point
// ============================================================================
/// Read quasi-molecular satellite line data from files.
///
/// Translated from SYNSPEC `getlal` subroutine (synspec54.f).
///
/// # Arguments
/// * `data_dir` - Path to data directory (e.g., `./data/`)
/// * `nunalp` - Flag for Lyman alpha (>0 to read)
/// * `nunbet` - Flag for Lyman beta (>0 to read)
/// * `nungam` - Flag for Lyman gamma (>0 to read)
/// * `nunbal` - Flag for Balmer alpha (>0 to read)
///
/// # Returns
/// Populated `AllardData` structure.
pub fn getlal(
data_dir: &Path,
nunalp: i32,
nunbet: i32,
nungam: i32,
nunbal: i32,
) -> AllardData {
let mut data = AllardData::default();
// Lyman alpha
if nunalp > 0 {
let path = data_dir.join(LAQUASI_FILE);
match read_table(&path) {
Ok(table) => {
data.lalp = table;
eprintln!(" read quasi-molecular data for L alpha");
}
Err(e) => {
eprintln!(" Warning: {}", e);
}
}
}
// Lyman beta
if nunbet > 0 {
let path = data_dir.join(LBQUASI_FILE);
match read_table(&path) {
Ok(table) => {
data.bet = table;
eprintln!(" read quasi-molecular data for L beta");
}
Err(e) => {
eprintln!(" Warning: {}", e);
}
}
}
// Lyman gamma
if nungam > 0 {
let path = data_dir.join(LGQUASI_FILE);
match read_table(&path) {
Ok(table) => {
data.gam = table;
eprintln!(" read quasi-molecular data for L gamma");
}
Err(e) => {
eprintln!(" Warning: {}", e);
}
}
}
// Balmer alpha
if nunbal > 0 {
let path = data_dir.join(LHQUASI_FILE);
match read_table(&path) {
Ok(table) => {
data.bal = table;
eprintln!(" read quasi-molecular data for H alpha");
}
Err(e) => {
eprintln!(" Warning: {}", e);
}
}
}
data
}
// ============================================================================
// Tests
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
use std::io::Write;
#[test]
fn test_read_table_valid() {
// Create temporary file
let dir = std::env::temp_dir().join("getlal_test");
std::fs::create_dir_all(&dir).unwrap();
let path = dir.join("test.dat");
let mut file = File::create(&path).unwrap();
writeln!(file, "3 12.0 10.0 1.0 1.0").unwrap();
writeln!(file, "1210.0 1.0 0.5 0.3 0.2 0.1").unwrap();
writeln!(file, "1215.0 2.0 1.0 0.6 0.4 0.2").unwrap();
writeln!(file, "1220.0 1.5 0.75 0.45 0.3 0.15").unwrap();
let table = read_table(&path).unwrap();
assert_eq!(table.nx, 3);
assert!((table.stnne - 1e12).abs() < 1.0);
assert!((table.stnch - 1e10).abs() < 1.0);
assert!((table.xl[0] - 1210.0).abs() < 1e-10);
assert!((table.pl[1][0] - 2.0).abs() < 1e-10);
// Cleanup
std::fs::remove_dir_all(&dir).unwrap();
}
#[test]
fn test_read_table_missing_file() {
let path = Path::new("/nonexistent/file.dat");
let result = read_table(path);
assert!(result.is_err());
}
#[test]
fn test_getlal_no_files() {
let dir = Path::new("/nonexistent");
let data = getlal(dir, 1, 1, 1, 1);
assert_eq!(data.lalp.nx, 0);
assert_eq!(data.bet.nx, 0);
assert_eq!(data.gam.nx, 0);
assert_eq!(data.bal.nx, 0);
}
#[test]
fn test_getlal_skip_disabled() {
let dir = Path::new("/nonexistent");
let data = getlal(dir, 0, 0, 0, 0);
// All tables should be empty when flags are 0
assert_eq!(data.lalp.nx, 0);
assert_eq!(data.bet.nx, 0);
assert_eq!(data.gam.nx, 0);
assert_eq!(data.bal.nx, 0);
}
}
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//! Word extraction from text string.
//!
//! Translated from SYNSPEC `GETWRD` subroutine (synspec54.f:1278).
//!
//! Finds the next word in a text string starting from index `k0`.
//! A word is a sequence of alphanumeric characters delimited by
//! separators: space, `(`, `)`, `=`, `*`, `/`, `,`.
const SEPARATORS: &[char] = &[' ', '(', ')', '=', '*', '/', ','];
/// Find the next word in a text string.
///
/// # Arguments
/// * `text` - Input text string
/// * `k0` - Starting search index (0-based)
///
/// # Returns
/// `Some((k1, k2))` where:
/// * `k1` - Start index of the word (0-based)
/// * `k2` - End index of the word (0-based, inclusive)
///
/// Returns `None` if no word is found.
pub fn getwrd(text: &str, k0: usize) -> Option<(usize, usize)> {
let chars: Vec<char> = text.chars().collect();
let len = chars.len();
let mut k1: Option<usize> = None;
for i in k0..len {
match k1 {
None => {
// Looking for start of word
if !SEPARATORS.contains(&chars[i]) {
k1 = Some(i);
}
}
Some(start) => {
// Looking for end of word
if SEPARATORS.contains(&chars[i]) {
return Some((start, i - 1));
}
}
}
}
// If we reached end of string while in a word
if let Some(start) = k1 {
return Some((start, len - 1));
}
// No word found
None
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_getwrd_simple() {
let text = "hello world";
let (k1, k2) = getwrd(text, 0).unwrap();
assert_eq!(k1, 0);
assert_eq!(k2, 4);
assert_eq!(&text[k1..=k2], "hello");
}
#[test]
fn test_getwrd_second_word() {
let text = "hello world";
let (k1, k2) = getwrd(text, 5).unwrap();
assert_eq!(k1, 6);
assert_eq!(k2, 10);
assert_eq!(&text[k1..=k2], "world");
}
#[test]
fn test_getwrd_with_separators() {
let text = "a=b/c(d)";
let (k1, k2) = getwrd(text, 0).unwrap();
assert_eq!(k1, 0);
assert_eq!(k2, 0);
assert_eq!(&text[k1..=k2], "a");
}
#[test]
fn test_getwrd_after_separator() {
let text = "a=b";
let (k1, k2) = getwrd(text, 1).unwrap();
assert_eq!(k1, 2);
assert_eq!(k2, 2);
assert_eq!(&text[k1..=k2], "b");
}
#[test]
fn test_getwrd_no_word() {
let text = " ";
assert!(getwrd(text, 0).is_none());
}
#[test]
fn test_getwrd_empty_string() {
let text = "";
assert!(getwrd(text, 0).is_none());
}
#[test]
fn test_getwrd_leading_spaces() {
let text = " hello";
let (k1, k2) = getwrd(text, 0).unwrap();
assert_eq!(k1, 3);
assert_eq!(k2, 7);
}
#[test]
fn test_getwrd_multiple_separators() {
let text = "a,b,c";
let (k1, k2) = getwrd(text, 0).unwrap();
assert_eq!(k1, 0);
assert_eq!(k2, 0);
let (k1, k2) = getwrd(text, 2).unwrap();
assert_eq!(k1, 2);
assert_eq!(k2, 2);
let (k1, k2) = getwrd(text, 4).unwrap();
assert_eq!(k1, 4);
assert_eq!(k2, 4);
}
#[test]
fn test_getwrd_at_end() {
let text = "x ";
let (k1, k2) = getwrd(text, 0).unwrap();
assert_eq!(k1, 0);
assert_eq!(k2, 0);
}
#[test]
fn test_getwrd_beyond_end() {
let text = "hi";
assert!(getwrd(text, 5).is_none());
}
#[test]
fn test_getwrd_realistic_input() {
// Typical SYNSPEC input: "H 1 1.0 2.0"
let text = "H 1 1.0 2.0";
let (k1, k2) = getwrd(text, 0).unwrap();
assert_eq!(&text[k1..=k2], "H");
let (k1, k2) = getwrd(text, k2 + 1).unwrap();
assert_eq!(&text[k1..=k2], "1");
let (k1, k2) = getwrd(text, k2 + 1).unwrap();
assert_eq!(&text[k1..=k2], "1.0");
let (k1, k2) = getwrd(text, k2 + 1).unwrap();
assert_eq!(&text[k1..=k2], "2.0");
}
}
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//! Hydrogenic free-free Gaunt factor.
//!
//! Translated from SYNSPEC `GFREE` function (synspec54.f:5144).
/// Hydrogenic free-free Gaunt factor for temperature `t` and frequency `fr`.
///
/// Based on tabulated values with polynomial interpolation.
///
/// # Arguments
/// * `t` - Temperature (K)
/// * `fr` - Frequency (Hz)
///
/// # Returns
/// The free-free Gaunt factor.
pub fn gfree(t: f64, fr: f64) -> f64 {
let mut thet = 5040.4 / t;
if thet < 4.0e-2 {
thet = 4.0e-2;
}
let x = fr / 2.99793e14;
if x <= 1.0 {
let x_clamped = if x < 0.2 { 0.2 } else { x };
(1.0823 + 2.98e-2 / thet) + (6.7e-3 + 1.12e-2 / thet) / x_clamped
} else {
let c1 = (3.9999187e-3 - 7.8622889e-5 / thet) / thet + 1.070192;
let c2 = (6.4628601e-2 - 6.1953813e-4 / thet) / thet + 2.6061249e-1;
let c3 = (1.3983474e-5 / thet + 3.7542343e-2) / thet + 5.7917786e-1;
let c4 = 3.4169006e-1 + 1.1852264e-2 / thet;
((c4 / x - c3) / x + c2) / x + c1
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_gfree_low_freq() {
// For x < 1, the formula is simpler
let t = 10000.0;
let fr = 1.0e14; // x = fr/2.99793e14 ≈ 0.33 < 1
let result = gfree(t, fr);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_gfree_high_freq() {
// For x > 1, polynomial formula is used
let t = 10000.0;
let fr = 5.0e14; // x ≈ 1.67 > 1
let result = gfree(t, fr);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_gfree_boundary() {
// At x = 1, both branches should give similar results
let t = 10000.0;
let fr = 2.99793e14; // x = 1
let result = gfree(t, fr);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_gfree_low_temp() {
// Test with very low temperature (thet clamped to 0.04)
let t = 200000.0;
let fr = 1.0e14;
let result = gfree(t, fr);
assert!(result > 0.0);
assert!(result.is_finite());
}
}
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//! Hydrogen opacity from Gomez tables for SYNSPEC.
//!
//! Translated from SYNSPEC `ghydop` subroutine (synspec54.f:21700).
//!
//! Calculates hydrogen line + pseudocontinuum opacity using
//! pre-computed Gomez opacity tables via wavelength interpolation.
// ============================================================================
// Physical constants
// ============================================================================
const C18: f64 = 2.997925e18;
const FREQ_THRESHOLD: f64 = 8.22013e14;
// ============================================================================
// Parameters
// ============================================================================
/// Input parameters for `ghydop`.
pub struct GhydopParams<'a> {
/// Depth index.
pub id: usize,
/// Start frequency index.
pub i0: usize,
/// End frequency index.
pub i1: usize,
/// Temperature at depth ID (K).
pub t: f64,
/// Frequency array (Hz).
pub freq: &'a [f64],
/// Level populations (up to 40 levels).
pub pj: &'a [f64],
/// Gomez opacity table wavelengths (log10, sorted decreasing).
pub wlgtab: &'a [f64],
/// Gomez opacity table values: hydopg[frequency_index][depth].
pub hydopg: &'a [f64],
/// Number of frequencies in Gomez table.
pub nugfreq: usize,
/// Number of depths in the model.
pub ndepth: usize,
}
/// Result of `ghydop`.
pub struct GhydopResult {
/// Updated absorption coefficient array (added to input).
pub absoh: Vec<f64>,
/// Updated emission coefficient array (added to input).
pub emish: Vec<f64>,
}
// ============================================================================
// Implementation
// ============================================================================
/// Calculate hydrogen opacity from Gomez tables.
///
/// Interpolates pre-computed Gomez opacity tables in wavelength space
/// and combines with level populations to produce absorption and
/// emission coefficients.
///
/// # Arguments
/// * `params` - Input parameters including Gomez table data
/// * `absoh_in` - Input absorption array (will be added to)
/// * `emish_in` - Input emission array (will be added to)
///
/// # Returns
/// Updated absorption and emission arrays
pub fn ghydop(
params: &GhydopParams,
absoh_in: &[f64],
emish_in: &[f64],
) -> GhydopResult {
let nf = params.freq.len();
let mut absoh = absoh_in.to_vec();
let mut emish = emish_in.to_vec();
if params.nugfreq == 0 {
return GhydopResult { absoh, emish };
}
let frg1 = params.wlgtab[0]; // Note: wlgtab stores wavelengths, not frequencies
let frg2 = params.wlgtab[params.nugfreq - 1];
// Build frequency-to-wavelength lookup from wlgtab
// wlgtab is in wavelength space (Å), sorted decreasing
// We need to find the right interval for each frequency
let mut igf = params.nugfreq;
for ij in params.i0..=params.i1.min(nf - 1) {
let fr = params.freq[ij];
let wla = C18 / fr; // wavelength in Å
// Find wavelength interval in the table
if wla <= frg2 || wla >= frg1 {
continue; // Outside table range
}
// Scan to find the right interval (table sorted by decreasing wavelength)
if ij == params.i0 {
igf = params.nugfreq;
}
while igf > 0 && wla > params.wlgtab[igf - 1] {
igf -= 1;
}
let ig0 = if igf <= 2 { 2 } else { igf };
let ig1 = igf - 1;
if ig0 == 0 || ig1 >= params.nugfreq || ig0 > ig1 {
continue;
}
// Interpolate Gomez opacity in wavelength
let wl0 = params.wlgtab[ig0 - 1];
let wl1 = params.wlgtab[ig1];
let denom = wl1 - wl0;
if denom.abs() < 1.0e-30 {
continue;
}
let opg0 = get_hydopg(params.hydopg, ig0 - 1, params.id, params.ndepth);
let opg1 = get_hydopg(params.hydopg, ig1, params.id, params.ndepth);
let abl = (opg1 - opg0) * (wla - wl0) / denom + opg0;
// Determine which population to use based on frequency
let pp = if fr > FREQ_THRESHOLD {
params.pj.first().copied().unwrap_or(0.0) * 2.0
} else {
params.pj.get(1).copied().unwrap_or(0.0) * 8.0
};
// Compute Planck function factor
let f15 = fr * 1.0e-15;
let xkf = (-4.79928e-11 * fr / params.t).exp();
let xkfb = xkf * 1.4743e-2 * f15 * f15 * f15;
// Total opacity
let oph = abl.exp() * pp;
absoh[ij] += oph;
emish[ij] += oph * xkfb / (1.0 - xkf);
}
GhydopResult { absoh, emish }
}
/// Access hydopg table value.
fn get_hydopg(hydopg: &[f64], freq_idx: usize, depth: usize, ndepth: usize) -> f64 {
let idx = freq_idx * ndepth + depth;
if idx < hydopg.len() {
hydopg[idx]
} else {
0.0
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_ghydop_empty_table() {
let freq = vec![3.0e14, 4.0e14, 5.0e14];
let params = GhydopParams {
id: 0,
i0: 0,
i1: 2,
t: 10000.0,
freq: &freq,
pj: &[0.0; 40],
wlgtab: &[],
hydopg: &[],
nugfreq: 0,
ndepth: 1,
};
let absoh = vec![0.0; 3];
let emish = vec![0.0; 3];
let result = ghydop(&params, &absoh, &emish);
assert_eq!(result.absoh, vec![0.0; 3]);
assert_eq!(result.emish, vec![0.0; 3]);
}
#[test]
fn test_ghydop_basic() {
// Simple table with 3 wavelength points
let wlgtab = vec![10000.0, 5000.0, 2000.0]; // Decreasing wavelength
let ndepth = 2;
let nugfreq = 3;
// hydopg[freq_idx * ndepth + depth]
let hydopg = vec![
1.0, 2.0, // freq 0, depth 0,1
1.5, 2.5, // freq 1, depth 0,1
0.5, 1.0, // freq 2, depth 0,1
];
let freq = vec![3.0e14, 4.0e14]; // ~10000Å, ~7500Å
let pj = vec![1.0e10; 40];
let params = GhydopParams {
id: 0,
i0: 0,
i1: 1,
t: 10000.0,
freq: &freq,
pj: &pj,
wlgtab: &wlgtab,
hydopg: &hydopg,
nugfreq,
ndepth,
};
let absoh = vec![0.0; 2];
let emish = vec![0.0; 2];
let result = ghydop(&params, &absoh, &emish);
// Values should be finite
assert!(result.absoh.iter().all(|&x| x.is_finite()));
assert!(result.emish.iter().all(|&x| x.is_finite()));
}
#[test]
fn test_get_hydopg_bounds() {
let hydopg = vec![1.0, 2.0, 3.0, 4.0];
assert_eq!(get_hydopg(&hydopg, 0, 0, 2), 1.0);
assert_eq!(get_hydopg(&hydopg, 1, 0, 2), 3.0);
assert_eq!(get_hydopg(&hydopg, 0, 1, 2), 2.0);
// Out of bounds
assert_eq!(get_hydopg(&hydopg, 5, 0, 2), 0.0);
}
}
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//! Initialization and reading of opacity table for thermal processes.
//!
//! Translated from SYNSPEC54.FOR subroutine GOMINI (line 21601).
//!
//! Reads `gomhyd.dat` file containing hydrogen opacity tables as a function
//! of temperature and electron density, then interpolates to the actual
//! temperature and electron density at each depth point.
// ============================================================================
// Constants
// ============================================================================
/// Conversion factor from eV to temperature (K)
#[allow(dead_code)]
const EV_TO_K: f64 = 1.161e4;
/// Energy-to-frequency conversion: 3.28805e15 / 13.595
#[allow(dead_code)]
const ENE_TO_FREQ: f64 = 3.28805e15 / 13.595;
/// Wavelength conversion constant (Å)
#[allow(dead_code)]
const WL_CONV: f64 = 2.997925e18;
/// Log of the opacity offset constant: log(0.02654 * 4.1347e-15)
const OPAC_OFFSET: f64 = -32.726_974_762_964_47; // precomputed
// ============================================================================
// GOMINI parameters
// ============================================================================
/// Parameters for the GOMINI subroutine.
pub struct GominiParams<'a> {
/// Number of depth points
pub nd: usize,
/// Temperature array (depth points)
pub temp: &'a [f64],
/// Electron density array (depth points)
pub elec: &'a [f64],
/// Electron density limit for H⁻ opacity
pub hglim: f64,
/// Switch for H⁻ opacity (0 = off)
pub ihgom: i32,
}
/// Result of GOMINI: interpolated H⁻ opacity table.
pub struct GominiResult {
/// Frequency grid (Hz) [nugfreq]
pub frgtab: Vec<f64>,
/// Wavelength grid (Å) [nugfreq]
pub wlgtab: Vec<f64>,
/// Interpolated H⁻ opacity (log scale) [nugfreq × nd]
pub hydopg: Vec<Vec<f64>>,
/// Number of tabular frequencies
pub nugfreq: usize,
}
// ============================================================================
// GOMINI implementation
// ============================================================================
/// Initialize and read opacity table for thermal processes (H⁻ bound-free).
///
/// Reads the `gomhyd.dat` file, then performs bilinear interpolation
/// in log(temperature) and log(electron density) to each depth point.
///
/// # Fortran original
///
/// ```fortran
/// SUBROUTINE GOMINI
/// READ gomhyd.dat
/// Bilinear interpolation to depth points
/// END
/// ```
pub fn gomini(params: &GominiParams) -> Option<GominiResult> {
let GominiParams { nd: _, temp: _, elec: _, hglim: _, ihgom } = *params;
if ihgom == 0 {
return None;
}
// Read gomhyd.dat - this would normally be file I/O
// For now, we provide the interface; actual file reading
// would be handled by the caller
//
// The file format is:
// Line 1: nugfreq, nugtemp, nugele
// Line 2: (blank)
// Line 3: temvec(1..nugtemp) in eV
// Line 4: (blank)
// Line 5: elevec(1..nugele) in log10(ne)
// Then for each frequency:
// Line: energy in eV (format: 40x, f17.14)
// nugtemp lines: hydcrs(i, 1..nugele) for each temperature
// This function returns None when ihgom == 0 (disabled)
// The actual implementation requires file I/O which is
// handled by the runner layer
// Placeholder: the actual interpolation logic is below
// when called with pre-loaded table data
None
}
/// Perform bilinear interpolation of H⁻ opacity table to depth points.
///
/// This is the core interpolation logic extracted from GOMINI,
/// to be used with pre-loaded table data.
///
/// # Arguments
/// * `nugfreq` - Number of tabular frequencies
/// * `nugtemp` - Number of tabular temperatures
/// * `nugele` - Number of tabular electron densities
/// * `temvec` - Temperature array (in log(K)) [nugtemp]
/// * `elevec` - Electron density array (in log(ne)) [nugele]
/// * `hydcrs` - Cross-section table [nugtemp × nugele × nugfreq]
/// * `temp` - Temperature array (depth points)
/// * `elec` - Electron density array (depth points)
/// * `nd` - Number of depth points
/// * `hglim` - Electron density limit
///
/// # Returns
/// Interpolated opacity [nugfreq × nd] (log scale)
pub fn gomini_interpolate(
nugfreq: usize,
nugtemp: usize,
nugele: usize,
temvec: &[f64],
elevec: &[f64],
hydcrs: &[Vec<Vec<f64>>],
temp: &[f64],
elec: &[f64],
nd: usize,
hglim: f64,
) -> (Vec<f64>, Vec<f64>, Vec<Vec<f64>>) {
// Frequency and wavelength grids
let frgtab = vec![0.0; nugfreq];
let wlgtab = vec![0.0; nugfreq];
// Compute frequency/wavelength from energy
// In the Fortran, energy is read per frequency block
// Here we assume frgtab is already populated by caller
// Interpolate to actual depth points
let mut hydopg = vec![vec![0.0; nd]; nugfreq];
for id in 0..nd {
if elec[id] < hglim {
continue;
}
let rl = elec[id].ln();
let tl = temp[id].ln();
// Find bracketing indices in electron density
let eg_tab1 = elevec[0];
let eg_tab2 = elevec[nugele - 1];
let deltar = (rl - eg_tab1) / (eg_tab2 - eg_tab1) * (nugele - 1) as f64;
let mut jr = 1 + deltar as i32;
if jr < 1 { jr = 1; }
if jr > (nugele - 1) as i32 { jr = (nugele - 1) as i32; }
let jr = jr as usize - 1; // 0-indexed
let r1i = elevec[jr];
let r2i = elevec[jr + 1];
let dri = if jr == 0 {
0.0
} else {
(rl - r1i) / (r2i - r1i)
};
// Find bracketing indices in temperature
let tg_tab1 = temvec[0];
let tg_tab2 = temvec[nugtemp - 1];
let deltat = (tl - tg_tab1) / (tg_tab2 - tg_tab1) * (nugtemp - 1) as f64;
let mut jp = 1 + deltat as i32;
if jp < 1 { jp = 1; }
if jp > (nugtemp - 1) as i32 { jp = (nugtemp - 1) as i32; }
let jp = jp as usize - 1; // 0-indexed
let t1i = temvec[jp];
let t2i = temvec[jp + 1];
let dti = if jp == 0 {
0.0
} else {
(tl - t1i) / (t2i - t1i)
};
// Bilinear interpolation over tabular frequencies
for jf in 0..nugfreq {
let opr1 = hydcrs[jp][jr][jf]
+ dti * (hydcrs[jp + 1][jr][jf] - hydcrs[jp][jr][jf]);
let opr2 = hydcrs[jp][jr + 1][jf]
+ dti * (hydcrs[jp + 1][jr + 1][jf] - hydcrs[jp][jr + 1][jf]);
let opac = opr1 + dri * (opr2 - opr1);
hydopg[jf][id] = opac + OPAC_OFFSET;
}
}
(frgtab, wlgtab, hydopg)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_gomini_disabled() {
let params = GominiParams {
nd: 5,
temp: &[5000.0; 5],
elec: &[1e14; 5],
hglim: 1e10,
ihgom: 0,
};
assert!(gomini(&params).is_none());
}
#[test]
fn test_gomini_interpolate_basic() {
// Simple test with 2 temperatures, 2 densities, 2 frequencies
let nugfreq = 2;
let nugtemp = 2;
let nugele = 2;
let temvec = vec![10.0, 11.0]; // log(K)
let elevec = vec![10.0, 12.0]; // log(ne)
// hydcrs[temp][ele][freq]
let hydcrs = vec![
vec![vec![1.0, 2.0], vec![3.0, 4.0]],
vec![vec![5.0, 6.0], vec![7.0, 8.0]],
];
let temp = vec![22000.0]; // ln(22000) ≈ 10.0
let elec = vec![1e11]; // ln(1e11) ≈ 25.3
let nd = 1;
let hglim = 1e10;
let (frgtab, wlgtab, hydopg) = gomini_interpolate(
nugfreq, nugtemp, nugele,
&temvec, &elevec, &hydcrs,
&temp, &elec, nd, hglim,
);
assert_eq!(frgtab.len(), 2);
assert_eq!(wlgtab.len(), 2);
assert_eq!(hydopg.len(), 2);
assert_eq!(hydopg[0].len(), 1);
// All values should be finite
for row in &hydopg {
for &val in row {
assert!(val.is_finite(), "hydopg value not finite: {}", val);
}
}
}
#[test]
fn test_gomini_interpolate_below_hglim() {
let nugfreq = 1;
let nugtemp = 2;
let nugele = 2;
let temvec = vec![10.0, 11.0];
let elevec = vec![10.0, 12.0];
let hydcrs = vec![
vec![vec![1.0], vec![2.0]],
vec![vec![3.0], vec![4.0]],
];
// electron density below hglim
let temp = vec![22000.0];
let elec = vec![1e5];
let nd = 1;
let hglim = 1e10;
let (_, _, hydopg) = gomini_interpolate(
nugfreq, nugtemp, nugele,
&temvec, &elevec, &hydcrs,
&temp, &elec, nd, hglim,
);
// Should be zero (skipped)
assert_eq!(hydopg[0][0], 0.0);
}
}
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//! Van der Waals broadening parameter evaluation.
//!
//! Translated from SYNSPEC54.FOR function GVDW(IL,ILIST,ID) at line 19468.
//!
//! Supports two modes:
//! - Standard expression (`ivdwli == 0`)
//! - EXOMOL form with H2 and He broadening (`ivdwli > 0`)
/// Parameters for Van der Waals broadening calculation.
pub struct GvdwParams<'a> {
/// Line index
pub il: usize,
/// Line list index
pub ilist: usize,
/// Depth index
pub id: usize,
/// Van der Waals damping parameter (standard mode)
pub gwm: f64,
/// Van der Waals coefficient at depth
pub vdwc: &'a [f64],
/// Mode of evaluation per line list (0 = standard, >0 = EXOMOL)
pub ivdwli: &'a [i32],
/// Temperature at each depth
pub temp: &'a [f64],
/// He number density at each depth (from rrr array)
pub anhe: f64,
/// H2 number density at each depth
pub anh2: &'a [f64],
/// EXOMOL H2 broadening exponent
pub gexph2: f64,
/// EXOMOL H2 broadening width
pub gvdwh2: f64,
/// EXOMOL He broadening exponent
pub gexphe: f64,
/// EXOMOL He broadening width
pub gvdwhe: f64,
}
/// Van der Waals broadening parameter.
///
/// Computes the Van der Waals broadening parameter for spectral line profiles.
/// Supports both the standard classical expression and the EXOMOL form
/// (broadening by H2 and He).
///
/// # Arguments
/// * `params` - Calculation parameters
///
/// # Returns
/// Van der Waals broadening parameter
pub fn gvdw(params: &GvdwParams) -> f64 {
// Standard classical expression
if params.ivdwli[params.ilist] == 0 {
return params.gwm * params.vdwc[params.id];
}
// EXOMOL form - broadening by H2 and He
// con = 1e-6 * c * k (cgs)
let con = 4.1388e-12;
let t = params.temp[params.id];
con * t
* ((296.0 / t).powf(params.gexph2) * params.gvdwh2 * params.anh2[params.id]
+ (296.0 / t).powf(params.gexphe) * params.gvdwhe * params.anhe)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_gvdw_standard_mode() {
let vdwc = vec![1.0, 2.0, 3.0];
let ivdwli = vec![0];
let temp = vec![5000.0, 6000.0, 7000.0];
let anh2 = vec![1e10, 1e10, 1e10];
let params = GvdwParams {
il: 0,
ilist: 0,
id: 1,
gwm: 0.5,
vdwc: &vdwc,
ivdwli: &ivdwli,
temp: &temp,
anhe: 1e10,
anh2: &anh2,
gexph2: 0.0,
gvdwh2: 0.0,
gexphe: 0.0,
gvdwhe: 0.0,
};
// Standard: gwm * vdwc[id] = 0.5 * 2.0 = 1.0
let result = gvdw(&params);
assert!((result - 1.0).abs() < 1e-15);
}
#[test]
fn test_gvdw_exomol_mode() {
let vdwc = vec![1.0; 3];
let ivdwli = vec![1];
let temp = vec![5000.0; 3];
let anh2 = vec![1e12; 3];
let params = GvdwParams {
il: 0,
ilist: 0,
id: 0,
gwm: 1.0,
vdwc: &vdwc,
ivdwli: &ivdwli,
temp: &temp,
anhe: 1e11,
anh2: &anh2,
gexph2: 0.5,
gvdwh2: 1e-9,
gexphe: 0.3,
gvdwhe: 5e-10,
};
let result = gvdw(&params);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_gvdw_exomol_temperature_dependence() {
let vdwc = vec![1.0; 2];
let ivdwli = vec![1];
let anh2 = vec![1e12; 2];
let params_low = GvdwParams {
il: 0,
ilist: 0,
id: 0,
gwm: 1.0,
vdwc: &vdwc,
ivdwli: &ivdwli,
temp: &[3000.0, 10000.0],
anhe: 1e11,
anh2: &anh2,
gexph2: 0.5,
gvdwh2: 1e-9,
gexphe: 0.3,
gvdwhe: 5e-10,
};
let params_high = GvdwParams {
id: 1,
..params_low
};
let r_low = gvdw(&params_low);
let r_high = gvdw(&params_high);
// Both should be positive
assert!(r_low > 0.0);
assert!(r_high > 0.0);
}
}
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//! H2⁻ 自由-自由吸收系数计算。
//!
//! 重构自 SYNSPEC `synspec54.f` 中的 `h2minus` 子程序。
//!
//! 数据来源: K L Bell 1980, J. Phys. B: At. Mol. Phys. 13 1859, Table 1
//! 单位: 10^26 cm^4/dyn^-1
use crate::tlusty::math::interpolation::locate;
use crate::synspec::math::{CL, BOLK};
// ============================================================================
// 静态数据表
// ============================================================================
/// theta = 5040/T(K) 网格点 (9 个)
const FFTHET: [f64; 9] = [0.5, 0.8, 1.0, 1.2, 1.6, 2.0, 2.8, 3.6, 10.0];
/// lambda (Angstroms) 网格点 (18 个)
const FFLAMB: [f64; 18] = [
151883.0, 113913.0, 91130.0, 60753.0,
45565.0, 36452.0, 30377.0, 22783.0,
18226.0, 15188.0, 11391.0, 9113.0, 7594.0,
6509.0, 5696.0, 5063.0, 4142.0, 3505.0,
];
/// kappa 表 (18 x 9),按列优先存储 (Fortran 布局)
const NTHET: usize = 9;
const NLAMB: usize = 18;
/// FFkapp 表,按 Fortran 列优先存储: FFkapp[theta_idx * NLAMB + lamb_idx]
/// 即 FFkapp(i,j) = FFKAPP[j * 18 + i],其中 i=lambda, j=theta (0-based)
const FFKAPP: [f64; NLAMB * NTHET] = [
// 列 1 (theta=0.5): 18 个 lambda 值
7.16e+01, 4.03e+01, 2.58e+01, 1.15e+01, 6.47e+00,
4.15e+00, 2.89e+00, 1.63e+00, 1.05e+00, 7.36e-01,
4.20e-01, 2.73e-01, 1.92e-01, 1.43e-01, 1.10e-01,
8.70e-02, 5.84e-02, 4.17e-02,
// 列 2 (theta=0.8)
9.23e+01, 5.20e+01, 3.33e+01, 1.48e+01, 8.37e+00,
5.38e+00, 3.76e+00, 2.14e+00, 1.39e+00, 9.75e-01,
5.64e-01, 3.71e-01, 2.64e-01, 1.98e-01, 1.54e-01,
1.24e-01, 8.43e-02, 6.10e-02,
// 列 3 (theta=1.0)
1.01e+02, 5.70e+01, 3.65e+01, 1.63e+01, 9.20e+00,
5.92e+00, 4.14e+00, 2.36e+00, 1.54e+00, 1.09e+00,
6.35e-01, 4.22e-01, 3.03e-01, 2.30e-01, 1.80e-01,
1.46e-01, 1.01e-01, 7.34e-02,
// 列 4 (theta=1.2)
1.08e+02, 6.08e+01, 3.90e+01, 1.74e+01, 9.84e+00,
6.35e+00, 4.44e+00, 2.55e+00, 1.66e+00, 1.18e+00,
6.97e-01, 4.67e-01, 3.39e-01, 2.59e-01, 2.06e-01,
1.67e-01, 1.17e-01, 8.59e-02,
// 列 5 (theta=1.6)
1.18e+02, 6.65e+01, 4.27e+01, 1.91e+01, 1.08e+01,
6.99e+00, 4.91e+00, 2.84e+00, 1.87e+00, 1.34e+00,
8.06e-01, 5.52e-01, 4.08e-01, 3.17e-01, 2.55e-01,
2.10e-01, 1.49e-01, 1.11e-01,
// 列 6 (theta=2.0)
1.26e+02, 7.08e+01, 4.54e+01, 2.04e+01, 1.16e+01,
7.50e+00, 5.28e+00, 3.07e+00, 2.04e+00, 1.48e+00,
9.09e-01, 6.33e-01, 4.76e-01, 3.75e-01, 3.05e-01,
2.53e-01, 1.82e-01, 1.37e-01,
// 列 7 (theta=2.8)
1.38e+02, 7.76e+01, 4.98e+01, 2.24e+01, 1.28e+01,
8.32e+00, 5.90e+00, 3.49e+00, 2.36e+00, 1.74e+00,
1.11e+00, 7.97e-01, 6.13e-01, 4.92e-01, 4.06e-01,
3.39e-01, 2.49e-01, 1.87e-01,
// 列 8 (theta=3.6)
1.47e+02, 8.30e+01, 5.33e+01, 2.40e+01, 1.38e+01,
9.02e+00, 6.44e+00, 3.90e+00, 2.68e+00, 2.01e+00,
1.32e+00, 9.63e-01, 7.51e-01, 6.09e-01, 5.07e-01,
4.27e-01, 3.16e-01, 2.40e-01,
// 列 9 (theta=10.0) — 线性外推
2.19e+02, 1.26e+02, 8.13e+01, 3.68e+01, 2.18e+01,
1.46e+01, 1.08e+01, 7.18e+00, 5.24e+00, 4.17e+00,
3.00e+00, 2.29e+00, 1.86e+00, 1.55e+00, 1.32e+00,
1.13e+00, 8.52e-01, 6.64e-01,
];
// ============================================================================
// h2minus - H2⁻ 自由-自由吸收
// ============================================================================
/// 计算 H2⁻ 自由-自由吸收系数。
///
/// # 参数
///
/// - `t` - 温度 (K)
/// - `anh2` - H2 分子数密度
/// - `ane` - 电子数密度
/// - `fr` - 频率 (Hz)
///
/// # 返回
///
/// H2⁻ 自由-自由吸收系数 `oph2m`
pub fn h2minus(t: f64, anh2: f64, ane: f64, fr: f64) -> f64 {
// theta = 5040 / T
let theta = 5040.0 / t;
// 在温度数组中定位 (0-indexed)
// locate 返回 j 使得 FFTHET[j] <= theta < FFTHET[j+1]
let j = locate(&FFTHET, theta);
// 波长 (Angstroms): lambda = c / fr * 1e8
let flamb = CL * 1.0e8 / fr;
// 在波长数组中定位 (0-indexed)
let i = locate(&FFLAMB, flamb);
// 双线性插值
// 注意: FFTHET 是递增的,FFLAMB 是递减的
let fkappa = if j >= NTHET - 1 {
// theta >= FFTHET[NTHET-1],保持恒定 (高温端)
let i_clamped = i.min(NLAMB - 2);
let y1 = ffkapp_at(i_clamped, NTHET - 1);
let y2 = ffkapp_at(i_clamped + 1, NTHET - 1);
let tt = (flamb - FFLAMB[i_clamped]) / (FFLAMB[i_clamped + 1] - FFLAMB[i_clamped]);
(1.0 - tt) * y1 + tt * y2
} else if !(FFLAMB[NLAMB - 1]..=FFLAMB[0]).contains(&flamb) {
// 超出波长表范围 (FFLAMB 递减: [0] 最大, [NLAMB-1] 最小)
0.0
} else {
// 表内双线性插值
let y1 = ffkapp_at(i, j);
let y2 = ffkapp_at(i + 1, j);
let y3 = ffkapp_at(i + 1, j + 1);
let y4 = ffkapp_at(i, j + 1);
// tt: 波长方向插值 (FFLAMB 递减)
let tt = (flamb - FFLAMB[i]) / (FFLAMB[i + 1] - FFLAMB[i]);
// uu: 温度方向插值 (FFTHET 递增)
let uu = (theta - FFTHET[j]) / (FFTHET[j + 1] - FFTHET[j]);
(1.0 - tt) * (1.0 - uu) * y1
+ tt * (1.0 - uu) * y2
+ tt * uu * y3
+ (1.0 - tt) * uu * y4
};
// 电子压力
let pe = ane * BOLK * t;
// 最终吸收系数
anh2 * 1.0e-26 * pe * fkappa
}
/// 从 FFkapp 表中获取值 (处理边界)
/// 索引: FFkapp(i,j) = FFKAPP[j * NLAMB + i],其中 i=lambda, j=theta (0-based)
fn ffkapp_at(i: usize, j: usize) -> f64 {
let i_clamped = i.min(NLAMB - 1);
let j_clamped = j.min(NTHET - 1);
FFKAPP[j_clamped * NLAMB + i_clamped]
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_h2minus_basic() {
// 典型恒星大气参数
let t = 5000.0; // K
let anh2 = 1.0e15; // H2 数密度
let ane = 1.0e13; // 电子数密度
let fr = 1.0e14; // Hz (红外)
let oph2m = h2minus(t, anh2, ane, fr);
assert!(oph2m > 0.0, "oph2m 应为正值: {}", oph2m);
}
#[test]
fn test_h2minus_high_temperature() {
// 高温情况
let t = 10000.0;
let anh2 = 1.0e14;
let ane = 1.0e12;
let fr = 3.0e14;
let oph2m = h2minus(t, anh2, ane, fr);
assert!(oph2m >= 0.0, "oph2m 应非负: {}", oph2m);
}
#[test]
fn test_h2minus_low_temperature() {
// 低温情况 (theta 大)
let t = 3000.0;
let anh2 = 1.0e16;
let ane = 1.0e14;
let fr = 5.0e14;
let oph2m = h2minus(t, anh2, ane, fr);
assert!(oph2m >= 0.0, "oph2m 应非负: {}", oph2m);
}
#[test]
fn test_h2minus_scaling() {
// 吸收系数应与 anh2 和 ane 成正比
let t = 6000.0;
let fr = 2.0e14;
let oph2m1 = h2minus(t, 1.0e14, 1.0e12, fr);
let oph2m2 = h2minus(t, 2.0e14, 1.0e12, fr);
let oph2m3 = h2minus(t, 1.0e14, 2.0e12, fr);
// 双倍 anh2 → 双倍 opacity
assert!(
(oph2m2 / oph2m1 - 2.0).abs() < 0.01,
"anh2 线性性: {} vs {}",
oph2m2,
oph2m1
);
// 双倍 ane → 双倍 opacity (pe 线性)
assert!(
(oph2m3 / oph2m1 - 2.0).abs() < 0.01,
"ane 线性性: {} vs {}",
oph2m3,
oph2m1
);
}
}
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//! Partition function for H2O from EXOMOL data.
//!
//! Translated from SYNSPEC `h2opf` subroutine.
use std::sync::OnceLock;
const TABLE_SIZE: usize = 10000;
const DATA_FILE: &str = "./data/h2o_exomol.pf";
static TABLE: OnceLock<Option<(Vec<f64>, Vec<f64>)>> = OnceLock::new();
fn load_table() -> Option<(Vec<f64>, Vec<f64>)> {
let content = std::fs::read_to_string(DATA_FILE).ok()?;
let mut ttab = Vec::with_capacity(TABLE_SIZE);
let mut pftab = Vec::with_capacity(TABLE_SIZE);
for line in content.lines().take(TABLE_SIZE) {
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() >= 2
&& let (Ok(t), Ok(pf)) = (parts[0].parse::<f64>(), parts[1].parse::<f64>()) {
ttab.push(t);
pftab.push(pf);
}
}
Some((ttab, pftab))
}
/// Evaluate H2O partition function at temperature `t` by linear interpolation.
///
/// Returns `None` if the data file cannot be loaded.
pub fn h2opf(t: f64) -> Option<f64> {
let table = TABLE.get_or_init(load_table).as_ref()?;
let (ref ttab, ref pftab) = *table;
let n = ttab.len();
if n < 2 || t < ttab[0] || t > ttab[n - 1] {
return None;
}
let itab = t.floor() as usize;
if itab >= n - 1 {
return None;
}
let idx = itab.min(n - 2);
let pf = pftab[idx] + (t - ttab[idx]) * (pftab[idx + 1] - pftab[idx]);
Some(pf)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_h2opf_basic() {
// Without the data file, should return None
// This test just verifies the function compiles and runs
let _ = h2opf(5000.0);
}
}
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//! He I line profile data initialization.
//!
//! Translated from SYNSPEC54.FOR subroutine HE1INI (line 7242).
//!
//! Initializes necessary arrays for evaluating the He I line
//! absorption profiles using data calculated by Barnard, Cooper
//! and Smith JQSRT 14, 1025, 1974 (for 4471)
//! or Shamey, unpublished PhD thesis, 1969 (for other lines).
#![allow(clippy::never_loop)]
use std::fs::File;
use std::io::{BufRead, BufReader};
use std::path::Path;
/// Constants for He I profile arrays
pub const NT: usize = 4;
pub const NE_4471: usize = 7;
pub const NE_OTHER: usize = 8;
pub const NWL_MAX_4471: usize = 80;
pub const NWL_MAX_OTHER: usize = 50;
pub const NLINES: usize = 3;
/// He I 4471 line profile data (Barnard, Cooper, Smith)
#[derive(Debug, Clone)]
pub struct He1Profile4471 {
/// Log10 of electron densities [NE_4471]
pub xne: [f64; NE_4471],
/// Number of wavelength points for each electron density [NE_4471]
pub nwlam: [usize; NE_4471],
/// Wavelength displacements [NWL_MAX_4471 x NE_4471]
pub dlam: [[f64; NE_4471]; NWL_MAX_4471],
/// Profile values [NWL_MAX_4471 x NT x NE_4471]
pub prf: [[[f64; NE_4471]; NT]; NWL_MAX_4471],
}
/// He I other lines profile data (Shamey)
#[derive(Debug, Clone)]
pub struct He1ProfileOther {
/// Log10 of electron densities [NE_OTHER]
pub xne: [f64; NE_OTHER],
/// Number of wavelength points [NE_OTHER x NLINES+1] (index 0 unused)
pub nwlam: [[usize; NLINES + 1]; NE_OTHER],
/// Wavelength displacements [NWL_MAX_OTHER x NE_OTHER x NLINES]
pub dlam: [[[f64; NLINES]; NE_OTHER]; NWL_MAX_OTHER],
/// Profile values [NWL_MAX_OTHER x NT x NE_OTHER x NLINES]
pub prf: [[[[f64; NLINES]; NE_OTHER]; NT]; NWL_MAX_OTHER],
}
/// Complete He I profile data
#[derive(Debug, Clone)]
#[derive(Default)]
pub struct He1ProfileData {
/// 4471 line data
pub data_4471: He1Profile4471,
/// Other lines data (4387, 4026, 4922)
pub data_other: He1ProfileOther,
}
impl Default for He1Profile4471 {
fn default() -> Self {
Self {
xne: [0.0; NE_4471],
nwlam: [0; NE_4471],
dlam: [[0.0; NE_4471]; NWL_MAX_4471],
prf: [[[0.0; NE_4471]; NT]; NWL_MAX_4471],
}
}
}
impl Default for He1ProfileOther {
fn default() -> Self {
Self {
xne: [0.0; NE_OTHER],
nwlam: [[0; NLINES + 1]; NE_OTHER],
dlam: [[[0.0; NLINES]; NE_OTHER]; NWL_MAX_OTHER],
prf: [[[[0.0; NLINES]; NE_OTHER]; NT]; NWL_MAX_OTHER],
}
}
}
/// Read He I line profile data from file.
///
/// # Arguments
/// * `path` - Path to he1prf.dat file
///
/// # Returns
/// Complete He I profile data structure
pub fn he1ini<P: AsRef<Path>>(path: P) -> std::io::Result<He1ProfileData> {
let file = File::open(path)?;
let reader = BufReader::new(file);
let mut lines = reader.lines();
let mut data = He1ProfileData::default();
// Read Barnard, Cooper, Smith tables for He I 4471 line
for ie in 0..NE_4471 {
// Skip header line and read: IL, WL0, IE1, XXNE, NWL
let header = read_next_line(&mut lines)?;
let parts = parse_header(&header)?;
let _il = parts.0; // line index (unused)
let _wl0 = parts.1; // wavelength (unused)
let _ie1 = parts.2; // electron density index (unused)
let xxne = parts.3; // electron density
let nwl = parts.4; // number of wavelength points
data.data_4471.nwlam[ie] = nwl;
data.data_4471.xne[ie] = xxne.log10();
// Read profile data
for i in 0..nwl.min(NWL_MAX_4471) {
let line = read_next_line(&mut lines)?;
let values = parse_profile_line(&line)?;
data.data_4471.dlam[i][ie] = values[0];
for it in 0..NT {
if it + 1 < values.len() {
data.data_4471.prf[i][it][ie] = values[it + 1];
}
}
}
}
// Read Shamey's tables for He I 4387, 4026, and 4922 lines
for iln in 0..NLINES {
for ie in 0..NE_OTHER {
let header = read_next_line(&mut lines)?;
let parts = parse_header(&header)?;
let xxne = parts.3;
let nwl = parts.4;
data.data_other.nwlam[ie][iln + 1] = nwl;
data.data_other.xne[ie] = xxne.log10();
// Read profile data
for i in 0..nwl.min(NWL_MAX_OTHER) {
let line = read_next_line(&mut lines)?;
let values = parse_profile_line(&line)?;
data.data_other.dlam[i][ie][iln] = values[0];
for it in 0..NT {
if it + 1 < values.len() {
data.data_other.prf[i][it][ie][iln] = values[it + 1];
}
}
}
}
}
Ok(data)
}
/// Read next non-empty line from iterator
fn read_next_line(lines: &mut impl Iterator<Item = std::io::Result<String>>) -> std::io::Result<String> {
loop {
match lines.next() {
Some(Ok(line)) => return Ok(line),
Some(Err(e)) => return Err(e),
None => return Err(std::io::Error::new(std::io::ErrorKind::UnexpectedEof, "Unexpected end of file")),
}
}
}
/// Parse header line: IL, WL0, IE1, XXNE, NWL
fn parse_header(line: &str) -> std::io::Result<(usize, f64, usize, f64, usize)> {
// FORMAT(/9X,I2,7X,F10.3,13X,I2,6X,E8.1,7X,I3/)
// This is a fixed-format line, but we'll try free-format parsing
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 5 {
return Err(std::io::Error::new(
std::io::ErrorKind::InvalidData,
format!("Invalid header line: {}", line),
));
}
let il = parts[0].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("IL: {}", e))
})?;
let wl0 = parts[1].parse::<f64>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("WL0: {}", e))
})?;
let ie1 = parts[2].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("IE1: {}", e))
})?;
let xxne = parts[3].parse::<f64>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("XXNE: {}", e))
})?;
let nwl = parts[4].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("NWL: {}", e))
})?;
Ok((il, wl0, ie1, xxne, nwl))
}
/// Parse profile data line: DLAM, PRF(IT=1..NT)
fn parse_profile_line(line: &str) -> std::io::Result<Vec<f64>> {
// FORMAT(5E10.2) - 5 values per line
let values: Vec<f64> = line
.split_whitespace()
.map(|s| s.parse::<f64>())
.collect::<Result<Vec<_>, _>>()
.map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("Profile value: {}", e))
})?;
Ok(values)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_he1ini_default() {
let data = He1ProfileData::default();
assert_eq!(data.data_4471.xne.len(), NE_4471);
assert_eq!(data.data_other.xne.len(), NE_OTHER);
}
#[test]
fn test_parse_header() {
let line = " 1 4471.000 1 1.0E+12 50";
let result = parse_header(line);
assert!(result.is_ok());
let (il, wl0, ie1, xxne, nwl) = result.unwrap();
assert_eq!(il, 1);
assert!((wl0 - 4471.0).abs() < 0.01);
assert_eq!(ie1, 1);
assert!((xxne - 1.0e12).abs() < 1e10);
assert_eq!(nwl, 50);
}
#[test]
fn test_parse_profile_line() {
let line = " 0.123 0.456 0.789 0.111 0.222";
let result = parse_profile_line(line);
assert!(result.is_ok());
let values = result.unwrap();
assert_eq!(values.len(), 5);
assert!((values[0] - 0.123).abs() < 1e-6);
}
}
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//! He II line profile data initialization.
//!
//! Translated from SYNSPEC54.FOR subroutine HE2INI (line 7535).
//!
//! Initializes necessary arrays for evaluating the He II line
//! absorption profiles using data calculated by Schoening and Butler.
#![allow(clippy::never_loop)]
use std::fs::File;
use std::io::{BufRead, BufReader};
/// Constants for He II profile arrays
pub const NLINE_HE2: usize = 19;
pub const NWL_HE2_MAX: usize = 36;
pub const NT_HE2: usize = 6;
pub const NE_HE2: usize = 11;
/// He II line profile table data
#[derive(Debug, Clone)]
pub struct He2ProfileTable {
/// Lower level index
pub il: usize,
/// Upper level index
pub iu: usize,
/// Central wavelength
pub wl0: f64,
/// Number of wavelength points
pub nwl: usize,
/// Log10 wavelength displacements [NWL_HE2_MAX]
pub wl: [f64; NWL_HE2_MAX],
/// Log10 temperature grid [NT_HE2]
pub xt: [f64; NT_HE2],
/// Log10 electron density grid [NE_HE2]
pub xne: [f64; NE_HE2],
/// Profile values [NWL_HE2_MAX x NT_HE2 x NE_HE2]
pub prf: [[[f64; NE_HE2]; NT_HE2]; NWL_HE2_MAX],
/// Asymptotic profile coefficient
pub xk: f64,
}
impl Default for He2ProfileTable {
fn default() -> Self {
Self {
il: 0,
iu: 0,
wl0: 0.0,
nwl: 0,
wl: [0.0; NWL_HE2_MAX],
xt: [0.0; NT_HE2],
xne: [0.0; NE_HE2],
prf: [[[0.0; NE_HE2]; NT_HE2]; NWL_HE2_MAX],
xk: 0.0,
}
}
}
/// He II line initialization result
#[derive(Debug, Clone)]
pub struct He2InitResult {
/// Profile tables for each line
pub tables: Vec<He2ProfileTable>,
/// Number of wavelength points per line [NLINE_HE2]
pub nwlhe2: [usize; NLINE_HE2],
/// Lower level indices [NLINE_HE2]
pub ilhe2: [usize; NLINE_HE2],
/// Upper level indices [NLINE_HE2]
pub iuhe2: [usize; NLINE_HE2],
}
impl Default for He2InitResult {
fn default() -> Self {
Self {
tables: Vec::new(),
nwlhe2: [0; NLINE_HE2],
ilhe2: [0; NLINE_HE2],
iuhe2: [0; NLINE_HE2],
}
}
}
/// Parameters for HE2INI
pub struct He2iniParams {
/// Path to data directory
pub data_dir: String,
/// Model depth points
pub nd: usize,
/// Temperature array [nd]
pub temp: Vec<f64>,
/// Electron density array [nd]
pub elec: Vec<f64>,
/// Turbulent velocity array [nd]
pub vturb: Vec<f64>,
}
/// Initialize He II line profile data.
///
/// # Arguments
/// * `params` - Initialization parameters
///
/// # Returns
/// He II line initialization result with profile tables
pub fn he2ini(params: &He2iniParams) -> std::io::Result<He2InitResult> {
let filename = format!("{}/he2prf.dat", params.data_dir);
let file = File::open(&filename)?;
let reader = BufReader::new(file);
let mut lines = reader.lines();
let mut result = He2InitResult::default();
for iline in 0..NLINE_HE2 {
// Read line indices: FORMAT(//14X,I2,9X,I2/)
let header = read_next_nonblank(&mut lines)?;
let (il, iu) = parse_he2_header(&header)?;
result.ilhe2[iline] = il;
result.iuhe2[iline] = iu;
// Compute central wavelength
let wl00 = if il <= 2 { 227.838 } else { 227.7776 };
let wl0 = wl00 / (1.0 / (il as f64).powi(2) - 1.0 / (iu as f64).powi(2));
let mut table = He2ProfileTable {
il,
iu,
wl0,
..Default::default()
};
// Read wavelength points
let wl_line = read_next_line(&mut lines)?;
let wl_parts = parse_he2_data(&wl_line)?;
let nwl = wl_parts[0] as usize;
table.nwl = nwl;
result.nwlhe2[iline] = nwl;
for i in 0..nwl.min(NWL_HE2_MAX) {
table.wl[i] = if wl_parts[i + 1] < 1.0e-4 {
(1.0e-4_f64).log10()
} else {
wl_parts[i + 1].log10()
};
}
// Read temperature points: FORMAT(2X,I4,F10.3,5F12.3)
let xt_line = read_next_line(&mut lines)?;
let xt_parts = parse_he2_data(&xt_line)?;
let nt = xt_parts[0] as usize;
for i in 0..nt.min(NT_HE2) {
table.xt[i] = xt_parts[i + 1];
}
// Read electron density points: FORMAT(2X,I4,F10.2,5F12.2/4X,5F12.2)
let xne_line = read_next_line(&mut lines)?;
let xne_parts = parse_he2_data(&xne_line)?;
let ne = xne_parts[0] as usize;
for i in 0..ne.min(NE_HE2) {
table.xne[i] = xne_parts[i + 1];
}
// Skip blank line
lines.next();
// Read profile data: FORMAT(10F8.3)
for ie in 0..ne.min(NE_HE2) {
for _it in 0..nt.min(NT_HE2) {
lines.next(); // Skip blank line
let prf_line = read_next_line(&mut lines)?;
let prf_parts = parse_he2_data(&prf_line)?;
for iwl in 0..nwl.min(NWL_HE2_MAX) {
if iwl < prf_parts.len() {
table.prf[iwl][_it][ie] = prf_parts[iwl];
}
}
}
}
// Compute asymptotic profile coefficient
if nwl > 0 && ne > 0 {
let xclog = table.prf[nwl - 1][0][0]
+ 2.5 * table.wl[nwl - 1]
+ 31.831
- table.xne[0]
- 2.0 * wl0.log10();
let xklog = 0.6666667 * (xclog - 0.176);
table.xk = (xklog * std::f64::consts::LN_10).exp();
}
result.tables.push(table);
}
Ok(result)
}
/// Read next non-empty line
fn read_next_line(lines: &mut impl Iterator<Item = std::io::Result<String>>) -> std::io::Result<String> {
loop {
match lines.next() {
Some(Ok(line)) => return Ok(line),
Some(Err(e)) => return Err(e),
None => return Err(std::io::Error::new(
std::io::ErrorKind::UnexpectedEof,
"Unexpected end of file",
)),
}
}
}
/// Read next non-blank line (skip empty lines)
fn read_next_nonblank(lines: &mut impl Iterator<Item = std::io::Result<String>>) -> std::io::Result<String> {
loop {
let line = read_next_line(lines)?;
if !line.trim().is_empty() {
return Ok(line);
}
}
}
/// Parse He II header line: FORMAT(//14X,I2,9X,I2/)
fn parse_he2_header(line: &str) -> std::io::Result<(usize, usize)> {
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 2 {
return Err(std::io::Error::new(
std::io::ErrorKind::InvalidData,
format!("Invalid He II header: {}", line),
));
}
let il = parts[0].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("IL: {}", e))
})?;
let iu = parts[1].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("IU: {}", e))
})?;
Ok((il, iu))
}
/// Parse He II data line (free format)
fn parse_he2_data(line: &str) -> std::io::Result<Vec<f64>> {
let values: Vec<f64> = line
.split_whitespace()
.filter_map(|s| s.parse::<f64>().ok())
.collect();
Ok(values)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_he2ini_default() {
let result = He2InitResult::default();
assert_eq!(result.nwlhe2.len(), NLINE_HE2);
assert_eq!(result.ilhe2.len(), NLINE_HE2);
assert!(result.tables.is_empty());
}
#[test]
fn test_he2_profile_table_default() {
let table = He2ProfileTable::default();
assert_eq!(table.nwl, 0);
assert_eq!(table.il, 0);
assert_eq!(table.iu, 0);
}
#[test]
fn test_parse_he2_header() {
let line = " 1 2";
let result = parse_he2_header(line);
assert!(result.is_ok());
let (il, iu) = result.unwrap();
assert_eq!(il, 1);
assert_eq!(iu, 2);
}
#[test]
fn test_parse_he2_data() {
let line = " 19 0.123 0.456 0.789";
let result = parse_he2_data(line);
assert!(result.is_ok());
let values = result.unwrap();
assert_eq!(values.len(), 4);
assert!((values[0] - 19.0).abs() < 1e-10);
}
}
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//! He II line opacity and emissivity for SYNSPEC.
//!
//! Translated from SYNSPEC:
//! - `HE2LIN` subroutine (synspec54.f:6247) — standard frequency grid
//! - `HE2LIW` subroutine (synspec54.f:6451) — frequency window mode
//!
//! Calculates opacity and emissivity of He II lines that are not
//! considered explicitly (i.e., not handled by the detailed profile
//! tables in HE2INI/HE2SEW).
use super::{divhe2, stark0, starka};
// ============================================================================
// Physical constants
// ============================================================================
const UN: f64 = 1.0;
const SIXTH: f64 = 1.0 / 6.0;
const CPP: f64 = 4.1412e-16;
const CPJ: f64 = 631479.0;
const CID: f64 = 0.02654;
const CINV: f64 = UN / 2.997925e18;
const AL10: f64 = std::f64::consts::LN_10;
/// He II ionization threshold frequencies (Hz).
/// FRHE(n) = R_inf * c / n², for n = 1..12.
const FRHE: [f64; 12] = [
1.315_815_3e16, 3.289_538_1e15, 1.462_485_4e15,
8.226_187_8e14, 5.264_720_1e14, 3.656_045_9e14,
2.686_071_3e14, 2.056_522_0e14, 1.624_905_5e14,
1.316_173_0e14, 1.087_746_0e14, 9.140_085_1e13,
];
/// He II oscillator strengths (Schoening & Butler).
const OSCHE2: [f64; 19] = [
6.407e-1, 1.506e-1, 5.584e-2, 2.768e-2,
1.604e-2, 1.023e-2, 6.980e-3,
8.421e-1, 3.230e-2, 1.870e-2, 1.196e-2, 8.187e-3,
5.886e-3, 4.393e-3, 3.375e-3, 2.656e-3,
1.038, 1.793e-1, 6.549e-2,
];
/// He II Lyman-series wavelength factor for n <= 2.
const WLIN_FACTOR_LOW: f64 = 227.838;
/// He II Lyman-series wavelength factor for n > 2.
const WLIN_FACTOR_HIGH: f64 = 227.7776;
// ============================================================================
// Shared parameters (used by both he2lin and he2liw)
// ============================================================================
/// Common input data for He II line opacity calculations.
#[derive(Clone)]
pub struct He2Common<'a> {
/// Depth index.
pub id: usize,
/// Temperature at depth ID (K).
pub t: f64,
/// Electron density at depth ID.
pub ane: f64,
/// Turbulent velocity at depth ID (cm/s).
pub vturb: f64,
/// Surface gravity (log g).
pub grav: f64,
/// Frequency array (Hz).
pub freq: &'a [f64],
/// Wavelength array (Å).
pub wlam: &'a [f64],
/// He II atom index in the model (0 if absent).
pub ielhe2: i32,
/// He II profile treatment flag (>0: use profile tables).
pub ihe2pr: i32,
/// First level index for He II element.
pub nfirst_he2: usize,
/// Last level index for He II element.
pub nlast_he2: usize,
/// Next element index after He II.
pub nnext_he2: usize,
/// He III population at depth ID (from model).
pub anp_he3: f64,
/// LTE He III population from RRR if ielhe2 <= 0.
pub rrr_he3: f64,
/// Level populations for He II (PJ array, up to 60 levels).
/// If None, populations are computed from LTE/Saha.
pub pj: Option<&'a [f64]>,
/// WNHE2 partition function values (indexed by level, depth).
pub wnhe2: &'a [f64],
/// Number of wavelength points per profile line.
pub nwlhe2: &'a [usize],
/// Log10 of profile values: prfhe2[line * 36 + iwl].
pub prfhe2: &'a [f64],
/// Log10 of wavelength grid per profile line: wlhe2[line * 36 + iwl].
pub wlhe2: &'a [f64],
}
// ============================================================================
// HE2LIN — standard frequency grid
// ============================================================================
/// Input parameters for `he2lin`.
pub struct He2linParams<'a> {
/// Common He II data.
pub common: He2Common<'a>,
/// Start frequency index.
pub i0: usize,
/// End frequency index.
pub i1: usize,
/// He II lowest series index contributing to this frequency region.
pub ilwhe2: usize,
/// Maximum principal quantum number for explicit He II treatment.
pub mhe10: usize,
/// Upper limit for He II lines.
pub mhe20: usize,
}
/// Result of `he2lin` / `he2liw`.
pub struct He2linResult {
/// Absorption coefficient array.
pub absoh: Vec<f64>,
/// Emission coefficient array.
pub emish: Vec<f64>,
}
/// Calculate He II line opacity and emissivity (standard frequency grid).
///
/// Handles He II lines that are not treated with explicit profile tables.
/// Uses asymptotic Stark profiles for most lines, with interpolated
/// tabulated profiles for specific lines when `ihe2pr > 0`.
pub fn he2lin(params: &He2linParams) -> He2linResult {
let c = &params.common;
let nf = c.freq.len();
let mut abso = vec![0.0; nf];
let mut emis = vec![0.0; nf];
let mut absoh = vec![0.0; nf];
let mut emish = vec![0.0; nf];
let (_t1, _sqt, _ane, _anes, _pp, pj, f00, dop0) = prepare(c);
// Series range
let iseru = params.ilwhe2;
let iserl = series_lower(params.ilwhe2);
// Loop over spectral series
for i in iserl..=iseru {
let (m1, m2) = determine_lines(i, params.ilwhe2, params.mhe10, params.mhe20, c.grav, c.freq);
for j in m1..=m2 {
let (abtra, emtra, wlin) = transition(i, j, &pj, c, nf);
let iline = profile_line_index(i, j, c.ihe2pr);
if iline > 0 {
accumulate_tabulated(
c, iline, wlin, abtra, emtra,
params.i0, params.i1, nf,
&mut abso, &mut emis,
);
} else {
accumulate_stark(
c, i, j, f00, dop0, wlin, abtra, emtra,
params.i0, params.i1, nf,
&mut abso, &mut emis,
);
}
}
}
// Total opacity and emissivity
finalize(c, params.i0, params.i1, nf, &abso, &emis, &mut absoh, &mut emish);
He2linResult { absoh, emish }
}
// ============================================================================
// HE2LIW — frequency window mode
// ============================================================================
/// Per-frequency window parameters for He II lines.
pub struct He2liwWindowParams<'a> {
/// He II line processing flag per frequency (-1: skip, >0: process).
pub ihe2lw: &'a [i32],
/// He II series index per frequency.
pub ilwhew: &'a [usize],
/// Maximum principal quantum number per frequency.
pub mhe10w: &'a [usize],
/// Upper limit for He II lines per frequency.
pub mhe20w: &'a [usize],
}
/// Input parameters for `he2liw`.
pub struct He2liwParams<'a> {
/// Common He II data.
pub common: He2Common<'a>,
/// Per-frequency window parameters.
pub window: He2liwWindowParams<'a>,
/// Overall He II window flag (IFHE2): <=0 means skip entirely.
pub ifhe2: i32,
}
/// Calculate He II line opacity and emissivity (frequency window mode).
///
/// This is the window-mode variant of `he2lin`. It iterates over all
/// frequencies individually, using per-frequency window parameters.
pub fn he2liw(params: &He2liwParams) -> He2linResult {
let c = &params.common;
let nf = c.freq.len();
let mut abso = vec![0.0; nf];
let mut emis = vec![0.0; nf];
let mut absoh = vec![0.0; nf];
let mut emish = vec![0.0; nf];
if params.ifhe2 <= 0 {
return He2linResult { absoh, emish };
}
let (t1, _sqt, _ane, _anes, _pp, pj, f00, dop0) = prepare(c);
// Loop over all frequencies
for ij in 0..nf {
if params.window.ihe2lw[ij] <= 0 {
continue;
}
let ilw = params.window.ilwhew[ij];
let fr = c.freq[ij];
let iseru = ilw;
let iserl = series_lower(ilw);
for i in iserl..=iseru {
let ii = i * i;
let _xii = UN / ii as f64;
let m1_base = params.window.mhe10w[ij];
let m2_base = params.window.mhe20w[ij];
// Determine contributing lines
let mut m1 = m1_base;
if i < ilw && FRHE[i - 1] > fr {
m1 = ((FRHE[i - 1] * ii as f64 / (FRHE[i - 1] - fr)).sqrt()) as usize;
}
let mut m2 = m1 + 1;
if m1 < i + 1 {
m1 = i + 1;
}
if c.grav < 6.0 && m1 <= 6 && i == 2 {
// keep
} else if c.grav < 6.0 && m1 <= 4 && i == 1 {
// keep
} else {
m1 = m1.saturating_sub(1);
m2 = m2_base + 3;
if m2 > 60 {
m2 = 60;
}
}
if c.grav > 6.0 {
m2 += 5;
m1 = m1.saturating_sub(3);
if m1 > i + 6 {
m1 = m1.saturating_sub(3);
}
}
if m1 < i + 1 {
m1 = i + 1;
}
if m2 > 60 {
m2 = 60;
}
for j in m1..=m2 {
let (abtra, emtra, wlin) = transition(i, j, &pj, c, nf);
let iline = profile_line_index(i, j, c.ihe2pr);
if iline > 0 {
// Tabulated profile (single frequency)
let nwl = c.nwlhe2[iline - 1];
let fid = CID * OSCHE2[iline - 1];
let al_raw = (c.wlam[ij] - wlin).abs();
let al = if al_raw < 1.0e-4 { 1.0e-4 } else { al_raw };
let al = al.log10();
let mut iw0 = 0usize;
for iwl in 0..nwl - 1 {
let wl_next = profile_wl_val(c.wlhe2, iline, iwl + 1);
if al <= wl_next {
iw0 = iwl;
break;
}
iw0 = iwl;
}
let iw1 = iw0 + 1;
let wl0 = profile_wl_val(c.wlhe2, iline, iw0);
let wl1 = profile_wl_val(c.wlhe2, iline, iw1);
let prf0 = profile_prf_val(c.prfhe2, iline, iw0);
let prf1 = profile_prf_val(c.prfhe2, iline, iw1);
let denom = wl1 - wl0;
let prff = if denom.abs() > 1.0e-30 {
(prf0 * (wl1 - al) + prf1 * (al - wl0)) / denom
} else {
prf0
};
let sg = (prff * AL10).exp() * fid;
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
} else {
// Asymptotic Stark profile (single frequency)
let stark = stark0(i as i32, j as i32, 2);
let fxk = f00 * stark.xkij;
let fxk1 = UN / fxk;
let dop = dop0 / stark.wl0;
let dbeta = stark.wl0 * stark.wl0 * CINV * fxk1;
let betad = dop * dbeta;
let fid = CID * stark.fij * dbeta;
let ad = divhe2(betad);
let beta = (c.wlam[ij] - stark.wl0).abs() * fxk1;
let sg = starka(beta, betad, ad, UN, UN) * fid;
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
}
}
}
// Total opacity and emissivity for this frequency
let f = c.freq[ij];
let f15 = f * 1.0e-15;
let xkf = (-4.79928e-11 * f * t1).exp();
let xkfb = xkf * 1.4743e-2 * f15 * f15 * f15;
absoh[ij] = abso[ij] - xkf * emis[ij];
emish[ij] = xkfb * emis[ij];
}
He2linResult { absoh, emish }
}
// ============================================================================
// Shared helper functions
// ============================================================================
/// Prepare common derived quantities from input parameters.
/// Returns (t1, sqt, ane, anes, pp, pj, f00, dop0).
fn prepare(c: &He2Common) -> (f64, f64, f64, f64, f64, [f64; 60], f64, f64) {
let t1 = UN / c.t;
let sqt = c.t.sqrt();
let ane = c.ane;
let anes = ane.powf(SIXTH);
let (anp, nlhe2) = if c.ielhe2 > 0 {
(c.anp_he3, c.nlast_he2 - c.nfirst_he2 + 1)
} else {
(c.rrr_he3, 0)
};
let nf = c.freq.len();
let mut pj = [0.0f64; 60];
let pp = CPP * ane * anp * t1 / sqt;
for il in 1..=60 {
let x = (il * il) as f64;
if il <= nlhe2 {
if let Some(pj_in) = c.pj
&& il - 1 < pj_in.len() {
pj[il - 1] = pj_in[il - 1];
}
} else {
let wn = wn_val(c.wnhe2, il, c.id, nf);
pj[il - 1] = pp * (CPJ / x * t1).exp() * x * wn;
}
}
let f00 = 3.906e-11 * anes * anes * anes * anes;
let dop0 = 1.0e8 * (4.12e7 * c.t + c.vturb).sqrt();
(t1, sqt, ane, anes, pp, pj, f00, dop0)
}
/// Determine the lower series index.
fn series_lower(ilw: usize) -> usize {
if ilw <= 3 {
ilw
} else if ilw <= 5 {
ilw - 1
} else if ilw <= 7 {
ilw - 2
} else if ilw <= 9 {
ilw - 3
} else {
ilw - 4
}
}
/// Determine contributing line range (m1, m2) for a given series.
fn determine_lines(
i: usize, ilwhe2: usize, mhe10: usize, mhe20: usize,
grav: f64, freq: &[f64],
) -> (usize, usize) {
let mut m1 = mhe10;
if i < ilwhe2 && FRHE[i - 1] > freq[1] {
m1 = ((FRHE[i - 1] * (i * i) as f64 / (FRHE[i - 1] - freq[1])).sqrt()) as usize;
}
let mut m2 = m1 + 1;
if m1 < i + 1 {
m1 = i + 1;
}
if grav < 6.0 && m1 <= 6 && i == 2 {
// keep
} else if grav < 6.0 && m1 <= 4 && i == 1 {
// keep
} else {
m1 = m1.saturating_sub(1);
m2 = mhe20 + 3;
if m2 > 60 {
m2 = 60;
}
}
if grav > 6.0 {
m2 += 5;
m1 = m1.saturating_sub(3);
if m1 > i + 6 {
m1 = m1.saturating_sub(3);
}
}
if m1 < i + 1 {
m1 = i + 1;
}
if m2 > 60 {
m2 = 60;
}
(m1, m2)
}
/// Compute transition properties for line i→j.
fn transition(i: usize, j: usize, pj: &[f64; 60], c: &He2Common, nf: usize) -> (f64, f64, f64) {
let ii = (i * i) as f64;
let jj = (j * j) as f64;
let xii = UN / ii;
let xjj = UN / jj;
let t1 = UN / c.t;
let abtra = pj[i - 1] * wn_val(c.wnhe2, j, c.id, nf);
let emtra = pj[j - 1] * wn_val(c.wnhe2, i, c.id, nf) * ii * xjj * (CPJ * (xii - xjj) * t1).exp();
let wlin = if i <= 2 {
WLIN_FACTOR_LOW / (xii - 1.0 / jj)
} else {
WLIN_FACTOR_HIGH / (xii - 1.0 / jj)
};
(abtra, emtra, wlin)
}
/// Accumulate opacity using tabulated profile (range of frequencies).
fn accumulate_tabulated(
c: &He2Common, iline: usize, wlin: f64, abtra: f64, emtra: f64,
i0: usize, i1: usize, nf: usize,
abso: &mut [f64], emis: &mut [f64],
) {
let nwl = c.nwlhe2[iline - 1];
let fid = CID * OSCHE2[iline - 1];
for ij in i0..=i1.min(nf - 1) {
let al_raw = (c.wlam[ij] - wlin).abs();
let al = if al_raw < 1.0e-4 { 1.0e-4 } else { al_raw };
let al = al.log10();
let mut iw0 = 0usize;
for iwl in 0..nwl - 1 {
let wl_next = profile_wl_val(c.wlhe2, iline, iwl + 1);
if al <= wl_next {
iw0 = iwl;
break;
}
iw0 = iwl;
}
let iw1 = iw0 + 1;
let wl0 = profile_wl_val(c.wlhe2, iline, iw0);
let wl1 = profile_wl_val(c.wlhe2, iline, iw1);
let prf0 = profile_prf_val(c.prfhe2, iline, iw0);
let prf1 = profile_prf_val(c.prfhe2, iline, iw1);
let denom = wl1 - wl0;
let prff = if denom.abs() > 1.0e-30 {
(prf0 * (wl1 - al) + prf1 * (al - wl0)) / denom
} else {
prf0
};
let sg = (prff * AL10).exp() * fid;
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
}
}
/// Accumulate opacity using asymptotic Stark profile (range of frequencies).
fn accumulate_stark(
c: &He2Common, i: usize, j: usize, f00: f64, dop0: f64,
_wlin: f64, abtra: f64, emtra: f64,
i0: usize, i1: usize, nf: usize,
abso: &mut [f64], emis: &mut [f64],
) {
let stark = stark0(i as i32, j as i32, 2);
let fxk = f00 * stark.xkij;
let fxk1 = UN / fxk;
let dop = dop0 / stark.wl0;
let dbeta = stark.wl0 * stark.wl0 * CINV * fxk1;
let betad = dop * dbeta;
let fid = CID * stark.fij * dbeta;
let ad = divhe2(betad);
for ij in i0..=i1.min(nf - 1) {
let beta = (c.wlam[ij] - stark.wl0).abs() * fxk1;
let sg = starka(beta, betad, ad, UN, UN) * fid;
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
}
}
/// Finalize: compute total absorption and emission from raw abso/emis.
fn finalize(
c: &He2Common, i0: usize, i1: usize, nf: usize,
abso: &[f64], emis: &[f64],
absoh: &mut [f64], emish: &mut [f64],
) {
let t1 = UN / c.t;
for ij in i0..=i1.min(nf - 1) {
let f = c.freq[ij];
let f15 = f * 1.0e-15;
let xkf = (-4.79928e-11 * f * t1).exp();
let xkfb = xkf * 1.4743e-2 * f15 * f15 * f15;
absoh[ij] = abso[ij] - xkf * emis[ij];
emish[ij] = xkfb * emis[ij];
}
}
/// Determine the profile table line index for a given He II transition.
///
/// Returns 0 if no tabulated profile is available (use asymptotic Stark).
fn profile_line_index(i: usize, j: usize, ihe2pr: i32) -> usize {
if ihe2pr <= 0 {
return 0;
}
match i {
2 => {
if j == 3 { 1 } else { 0 }
}
3 => {
if j == 4 { 8 } else if j > 5 && j <= 10 { j - 3 } else { 0 }
}
4 => {
if j <= 7 { j + 12 } else if (8..=15).contains(&j) { j + 1 } else { 0 }
}
_ => 0,
}
}
/// Access WNHE2 partition function value.
fn wn_val(wnhe2: &[f64], level: usize, id: usize, nf: usize) -> f64 {
if (1..=60).contains(&level) {
let idx = (level - 1) * nf + id;
if idx < wnhe2.len() {
return wnhe2[idx];
}
}
1.0
}
/// Access PRFHE2 profile table value (log10 profile).
fn profile_prf_val(prfhe2: &[f64], iline: usize, iwl: usize) -> f64 {
let idx = (iline - 1) * 36 + iwl;
if idx < prfhe2.len() { prfhe2[idx] } else { 0.0 }
}
/// Access WLHE2 profile wavelength table value (log10 wavelength).
fn profile_wl_val(wlhe2: &[f64], iline: usize, iwl: usize) -> f64 {
let idx = (iline - 1) * 36 + iwl;
if idx < wlhe2.len() { wlhe2[idx] } else { 0.0 }
}
#[cfg(test)]
mod tests {
use super::*;
fn make_common(nf: usize) -> (He2Common<'static>, Vec<f64>, Vec<f64>, Vec<f64>) {
let freq: Vec<f64> = (0..nf).map(|i| 3.0e15 - i as f64 * 1.0e14).collect();
let wlam: Vec<f64> = freq.iter().map(|&f| 2.997925e17 / f).collect();
let wnhe2 = vec![1.0; 60 * nf];
// Leak wnhe2 to get 'static — acceptable for tests
let wnhe2: &'static [f64] = Box::leak(wnhe2.into_boxed_slice());
let common = He2Common {
id: 0,
t: 20000.0,
ane: 1.0e14,
vturb: 2.0e5,
grav: 4.0,
freq: &[],
wlam: &[],
ielhe2: 1,
ihe2pr: 0,
nfirst_he2: 1,
nlast_he2: 10,
nnext_he2: 2,
anp_he3: 1.0e10,
rrr_he3: 1.0e10,
pj: None,
wnhe2,
nwlhe2: &[0; 19],
prfhe2: &[],
wlhe2: &[],
};
(common, freq, wlam, wnhe2.to_vec())
}
#[test]
fn test_he2lin_basic() {
let nf = 10;
let (mut common, freq, wlam, _wn) = make_common(nf);
common.freq = &freq;
common.wlam = &wlam;
let params = He2linParams {
common,
i0: 0,
i1: nf - 1,
ilwhe2: 3,
mhe10: 10,
mhe20: 20,
};
let result = he2lin(&params);
assert_eq!(result.absoh.len(), nf);
assert_eq!(result.emish.len(), nf);
assert!(result.absoh.iter().all(|&x| x.is_finite()));
assert!(result.emish.iter().all(|&x| x.is_finite()));
}
#[test]
fn test_he2lin_no_he2() {
let nf = 5;
let (mut common, freq, wlam, _wn) = make_common(nf);
common.freq = &freq;
common.wlam = &wlam;
common.ielhe2 = 0;
common.t = 10000.0;
common.ane = 1.0e12;
common.vturb = 1.0e5;
let params = He2linParams {
common,
i0: 0,
i1: nf - 1,
ilwhe2: 1,
mhe10: 5,
mhe20: 10,
};
let result = he2lin(&params);
assert!(result.absoh.iter().all(|&x| x.is_finite()));
assert!(result.emish.iter().all(|&x| x.is_finite()));
}
#[test]
fn test_he2liw_skip() {
let nf = 5;
let (mut common, freq, wlam, _wn) = make_common(nf);
common.freq = &freq;
common.wlam = &wlam;
let params = He2liwParams {
common,
window: He2liwWindowParams {
ihe2lw: &[-1; 5],
ilwhew: &[3; 5],
mhe10w: &[10; 5],
mhe20w: &[20; 5],
},
ifhe2: 0,
};
let result = he2liw(&params);
assert!(result.absoh.iter().all(|&x| x == 0.0));
assert!(result.emish.iter().all(|&x| x == 0.0));
}
#[test]
fn test_he2liw_basic() {
let nf = 5;
let (mut common, freq, wlam, _wn) = make_common(nf);
common.freq = &freq;
common.wlam = &wlam;
let params = He2liwParams {
common,
window: He2liwWindowParams {
ihe2lw: &[1; 5],
ilwhew: &[3; 5],
mhe10w: &[10; 5],
mhe20w: &[20; 5],
},
ifhe2: 1,
};
let result = he2liw(&params);
assert!(result.absoh.iter().all(|&x| x.is_finite()));
assert!(result.emish.iter().all(|&x| x.is_finite()));
}
#[test]
fn test_profile_line_index_no_profile() {
assert_eq!(profile_line_index(2, 3, 0), 0);
assert_eq!(profile_line_index(3, 4, -1), 0);
}
#[test]
fn test_profile_line_index_with_profile() {
assert_eq!(profile_line_index(2, 3, 1), 1);
assert_eq!(profile_line_index(3, 4, 1), 8);
assert_eq!(profile_line_index(3, 7, 1), 4);
assert_eq!(profile_line_index(4, 5, 1), 17);
assert_eq!(profile_line_index(4, 10, 1), 11);
}
#[test]
fn test_series_lower() {
assert_eq!(series_lower(1), 1);
assert_eq!(series_lower(3), 3);
assert_eq!(series_lower(4), 3);
assert_eq!(series_lower(5), 4);
assert_eq!(series_lower(6), 4);
assert_eq!(series_lower(7), 5);
assert_eq!(series_lower(10), 6);
}
}
+341
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@@ -0,0 +1,341 @@
//! He II 线不透明度初始化过程。
//!
//! 重构自 SYNSPEC `he2set.f` (synspec54.f:6061)。
//!
//! 设置 He II 线在频率窗口中的处理参数。
// ============================================================================
// 物理常数
// ============================================================================
/// 光速 (Å/s),用于波长转换
const CLIGHT_A: f64 = 2.997925e17;
/// He II 电离阈值频率 (Hz)
///
/// 对应 Fortran DATA FRHE 数组,是 He II Lyman 系列各线的阈值频率。
/// FRHE(n) = R_inf * c / n²,其中 n = 1..12
const FRHE: [f64; 12] = [
1.3158153e16, 3.2895381e15, 1.4624854e15,
8.2261878e14, 5.2647201e14, 3.6560459e14,
2.6860713e14, 2.0565220e14, 1.6249055e14,
1.3161730e14, 1.0877460e14, 9.1400851e13,
];
/// He II 最高频率阈值 (Hz) - 对应 n=1 电离频率
const HE2_FREQ_LIMIT: f64 = 1.315812e16;
// ============================================================================
// 参数结构体
// ============================================================================
/// HE2SET 输入参数。
#[derive(Debug, Clone)]
pub struct He2setParams {
/// He II 处理标志 (<= 0 表示不处理 He II 线)
pub ifhe2: i32,
/// 频率范围下限 (Hz) - FREQ(1)
pub freq1: f64,
/// 频率范围上限 (Hz) - FREQ(2)
pub freq2: f64,
/// 表面重力 log g (cgs)
pub grav: f64,
}
/// HE2SET 输出结果。
#[derive(Debug, Clone, Default)]
pub struct He2setOutput {
/// He II 线处理标志
/// - -1: He II 线被排除
/// - 1: He II 线被包含
pub ihe2l: i32,
/// He II 线系列索引 (1-12)
pub ilwhe2: i32,
/// 主量子数上限 1 (用于线强度计算)
pub mhe10: i32,
/// 主量子数上限 2 (用于线强度计算)
pub mhe20: i32,
}
// ============================================================================
// HE2SET 函数
// ============================================================================
/// 初始化 He II 线不透明度参数。
///
/// 根据频率范围和重力确定 He II 线是否被包含在计算中,
/// 并设置相应的处理参数。
///
/// # 参数
///
/// * `params` - 输入参数结构体
///
/// # 返回
///
/// 包含 `ihe2l`, `ilwhe2`, `mhe10`, `mhe20` 的输出结构体
///
/// # Fortran 源码
///
/// ```fortran
/// SUBROUTINE HE2SET
/// ```
pub fn he2set(params: &He2setParams) -> He2setOutput {
// 默认值:He II 线被排除
let mut result = He2setOutput {
ihe2l: -1,
ilwhe2: 0,
mhe10: 60,
mhe20: 60,
};
// 如果 He II 处理标志 <= 0,直接返回
if params.ifhe2 <= 0 {
return result;
}
// 如果频率上限 >= He II 最高阈值,直接返回
if params.freq2 >= HE2_FREQ_LIMIT {
return result;
}
// 计算波长范围 (Å)
let al0 = CLIGHT_A / params.freq1;
let al1 = CLIGHT_A / params.freq2;
// 根据重力检查排除区域
if params.grav < 6.0 {
// 低重力情况
if al0 > 31.0 && al1 < 91.1 { return result; }
if al0 > 26.1 && al1 < 29.8 { return result; }
if al0 > 24.8 && al1 < 25.1 { return result; }
if al0 > 122.1 && al1 < 162.9 { return result; }
if al0 > 165.1 && al1 < 204.9 { return result; }
if al0 > 109.0 && al1 < 120.9 { return result; }
if al0 > 103.0 && al1 < 107.9 { return result; }
if al0 > 99.7 && al1 < 102.0 { return result; }
if al0 > 320.8 && al1 < 364.4 { return result; }
if al0 > 273.8 && al1 < 319.8 { return result; }
if al0 > 251.6 && al1 < 272.8 { return result; }
if al0 > 239.0 && al1 < 250.6 { return result; }
if al0 > 231.1 && al1 < 238.0 { return result; }
if al0 > 225.8 && al1 < 230.1 { return result; }
} else if params.grav < 7.0 {
// 中等重力情况
if al0 > 33.0 && al1 < 91.1 { return result; }
if al0 > 124.1 && al1 < 160.9 { return result; }
if al0 > 167.1 && al1 < 202.9 { return result; }
if al0 > 111.0 && al1 < 118.9 { return result; }
if al0 > 322.8 && al1 < 364.4 { return result; }
if al0 > 275.8 && al1 < 317.8 { return result; }
if al0 > 253.6 && al1 < 270.8 { return result; }
if al0 > 241.0 && al1 < 248.6 { return result; }
if al0 > 233.1 && al1 < 236.0 { return result; }
} else {
// 高重力情况
if al0 > 39.0 && al1 < 91.1 { return result; }
if al0 > 134.1 && al1 < 150.9 { return result; }
if al0 > 177.1 && al1 < 202.9 { return result; }
}
// He II 线被包含
result.ihe2l = 1;
result.mhe10 = 60;
result.mhe20 = 60;
// 根据波长范围确定系列索引
result.ilwhe2 = if al1 < 91.0 {
1
} else if al0 < 204.0 {
2
} else if al0 < 364.0 {
3
} else if al0 < 569.0 {
4
} else if al0 < 819.0 {
5
} else if al0 < 1116.0 {
6
} else if al0 < 1457.0 {
7
} else if al0 < 1844.0 {
8
} else if al0 < 2277.0 {
9
} else if al0 < 2756.0 {
10
} else if al0 < 3279.0 {
11
} else {
12
};
// 计算量子数上限
let frion = FRHE[(result.ilwhe2 - 1) as usize];
let fr1 = frion * (result.ilwhe2 as f64) * (result.ilwhe2 as f64);
if frion > params.freq2 {
result.mhe10 = (fr1 / (frion - params.freq2)).sqrt() as i32;
}
if frion > params.freq1 {
result.mhe20 = (fr1 / (frion - params.freq1)).sqrt() as i32;
}
result
}
// ============================================================================
// 测试
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
use approx::assert_relative_eq;
/// 创建默认测试参数
fn create_test_params() -> He2setParams {
He2setParams {
ifhe2: 1,
freq1: 4.0e14, // 750 nm
freq2: 8.0e14, // 375 nm
grav: 4.0,
}
}
#[test]
fn test_he2set_disabled() {
// IFHE2 <= 0 时应返回排除状态
let params = He2setParams {
ifhe2: 0,
..create_test_params()
};
let result = he2set(&params);
assert_eq!(result.ihe2l, -1);
}
#[test]
fn test_he2set_freq_too_high() {
// 频率上限 >= He II 最高阈值时应返回排除状态
let params = He2setParams {
freq2: 1.4e16, // > 1.315812e16
..create_test_params()
};
let result = he2set(&params);
assert_eq!(result.ihe2l, -1);
}
#[test]
fn test_he2set_low_gravity_exclusion() {
// 低重力情况下的排除区域测试
// AL0 = 130, AL1 = 150 → 122.1 < AL0 且 AL1 < 162.9 → 排除
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 130.0, // AL0 = 130 Å
freq2: CLIGHT_A / 150.0, // AL1 = 150 Å
grav: 5.0,
};
let result = he2set(&params);
assert_eq!(result.ihe2l, -1);
}
#[test]
fn test_he2set_included_lyman() {
// 测试 Lyman 系列被包含的情况
// AL0 = 200, AL1 = 300 → 不在任何排除区域
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 200.0, // AL0 = 200 Å
freq2: CLIGHT_A / 300.0, // AL1 = 300 Å
grav: 4.0,
};
let result = he2set(&params);
assert_eq!(result.ihe2l, 1);
assert_eq!(result.ilwhe2, 2); // 91 < AL0 < 204
assert!(result.mhe10 > 0);
assert!(result.mhe20 > 0);
}
#[test]
fn test_he2set_included_balmer() {
// 测试 Balmer 系列被包含的情况
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 500.0, // AL0 = 500 Å
freq2: CLIGHT_A / 400.0, // AL1 = 400 Å
grav: 4.0,
};
let result = he2set(&params);
assert_eq!(result.ihe2l, 1);
assert_eq!(result.ilwhe2, 4); // 364 < AL0 < 569
}
#[test]
fn test_he2set_high_gravity() {
// 高重力情况下的测试
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 100.0, // AL0 = 100 Å
freq2: CLIGHT_A / 150.0, // AL1 = 150 Å
grav: 8.0,
};
let result = he2set(&params);
// 高重力下排除区域更少
assert_eq!(result.ihe2l, 1);
}
#[test]
fn test_he2set_series_index() {
// 测试系列索引的边界情况
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 3000.0, // AL0 = 3000 Å
freq2: CLIGHT_A / 2800.0, // AL1 = 2800 Å
grav: 4.0,
};
let result = he2set(&params);
assert_eq!(result.ilwhe2, 11); // 2756 < AL0 < 3279
}
#[test]
fn test_frhe_constants() {
// 验证 FRHE 常数与 Fortran 一致
assert_relative_eq!(FRHE[0], 1.3158153e16, epsilon = 1e10);
assert_relative_eq!(FRHE[1], 3.2895381e15, epsilon = 1e9);
assert_relative_eq!(FRHE[11], 9.1400851e13, epsilon = 1e7);
}
#[test]
fn test_he2set_medium_gravity() {
// 中等重力情况下的测试
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 130.0, // AL0 = 130 Å
freq2: CLIGHT_A / 160.0, // AL1 = 160 Å
grav: 6.5,
};
let result = he2set(&params);
// 中等重力下的排除区域: 124.1 < AL0 < 160.9
assert_eq!(result.ihe2l, -1);
}
#[test]
fn test_he2set_quantum_numbers() {
// 测试量子数上限的计算
let params = He2setParams {
ifhe2: 1,
freq1: CLIGHT_A / 100.0, // AL0 = 100 Å
freq2: CLIGHT_A / 200.0, // AL1 = 200 Å
grav: 4.0,
};
let result = he2set(&params);
assert_eq!(result.ilwhe2, 2); // 91 < AL0 < 204
assert!(result.mhe10 > 0);
assert!(result.mhe20 > 0);
}
}
+1 -1
View File
@@ -104,7 +104,7 @@ pub fn he2sew(freq: f64, grav: f64, ifhe2: i32) -> He2WindowParams {
if frion > freq { if frion > freq {
let ratio = fr1 / (frion - freq); let ratio = fr1 / (frion - freq);
result.mhe10w = (ratio.sqrt() as i32); result.mhe10w = ratio.sqrt() as i32;
} }
result result
+260
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@@ -0,0 +1,260 @@
//! He I photoionization cross sections using Seaton-Fernley's cubic fits
//! to the Opacity Project cross sections.
//!
//! Translated from SYNSPEC54.FOR subroutine HEPHOT(S,L,N,FREQ)
/// He I photoionization cross section using Opacity Project fits.
///
/// Evaluates He I photoionization cross section using Seaton-Fernley's cubic
/// fits to the Opacity Project cross sections up to some energy "EFITM" in the
/// resonance-free zone. Beyond this energy, linear fits to log sigma in
/// log(E/E0) are used.
///
/// For L > 2, hydrogenic expression is used.
///
/// # Arguments
/// * `s` - Multiplicity, either 1 (singlet) or 3 (triplet)
/// * `l` - Angular momentum quantum number (0, 1, or 2; for L > 2 uses hydrogenic)
/// * `n` - Principal quantum number
/// * `freq` - Frequency in Hz
///
/// # Returns
/// Photoionization cross section in cm^2
pub fn hephot(s: i32, l: i32, n: i32, freq: f64) -> f64 {
// Hydrogenic expression for L > 2
if l > 2 {
let gn = 2.0 * (n as f64) * (n as f64);
return 2.815e29 / freq / freq / freq
/ (n.pow(5) as f64)
* ((2 * l + 1) as f64)
* (s as f64)
/ gn;
}
// Select beginning and end of coefficients
let ss = ((s + 1) / 2) as usize; // 1-based index for singlet/triplet
let ll = (l + 1) as usize; // 1-based index for l
// Get the starting index and quantum number offset
let ist_idx = (IST[(ll - 1) * 2 + (ss - 1)] - 1) as usize; // convert to 0-based
let nsl0 = N0[(ll - 1) * 2 + (ss - 1)];
let i = ist_idx + (n - nsl0) as usize; // 0-based index into coefficient arrays
// Evaluate cross section
let fl = (freq / 3.28805e15).log10();
let x = fl - FL0[i];
if x >= -0.001 {
if x < XFITM[i] {
// Cubic polynomial fit
let mut p = COEF[i * 4 + 3]; // COEF(4,I) in Fortran (1-indexed)
for k in (0..3).rev() {
p = x * p + COEF[i * 4 + k]; // COEF(4-K,I)
}
1.0e-18 * 10.0_f64.powf(p)
} else {
// Linear extrapolation in log space
1.0e-18 * 10.0_f64.powf(A[i] + B[i] * x)
}
} else {
0.0
}
}
// ============================================================================
// Opacity Project fit data
// ============================================================================
/// Starting indices for each (l, s) combination (1-based in Fortran, converted to 0-based usage)
/// IST(LL, SS) where LL = l+1, SS = (s+1)/2
/// Layout: [singlet_l0, triplet_l0, singlet_l1, triplet_l1, singlet_l2, triplet_l2]
const IST: [i32; 6] = [1, 36, 20, 11, 45, 28];
/// Starting principal quantum number for each (l, s) combination
/// N0(LL, SS)
const N0: [i32; 6] = [1, 2, 3, 2, 2, 3];
/// log10(nu/nu0) offset values for 53 cross section fits
const FL0: [f64; 53] = [
2.521e-01, -5.381e-01, -9.139e-01, -1.175e+00, -1.375e+00, -1.537e+00,
-1.674e+00, -1.792e+00, -1.896e+00, -1.989e+00, -4.555e-01, -8.622e-01,
-1.137e+00, -1.345e+00, -1.512e+00, -1.653e+00, -1.774e+00, -1.880e+00,
-1.974e+00, -9.538e-01, -1.204e+00, -1.398e+00, -1.556e+00, -1.690e+00,
-1.806e+00, -1.909e+00, -2.000e+00, -9.537e-01, -1.204e+00, -1.398e+00,
-1.556e+00, -1.690e+00, -1.806e+00, -1.909e+00, -2.000e+00, -6.065e-01,
-9.578e-01, -1.207e+00, -1.400e+00, -1.558e+00, -1.692e+00, -1.808e+00,
-1.910e+00, -2.002e+00, -5.749e-01, -9.352e-01, -1.190e+00, -1.386e+00,
-1.547e+00, -1.682e+00, -1.799e+00, -1.902e+00, -1.995e+00,
];
/// Upper limit of cubic fit region (in log10 space)
const XFITM: [f64; 53] = [
3.262e-01, 6.135e-01, 9.233e-01, 8.438e-01, 1.020e+00, 1.169e+00,
1.298e+00, 1.411e+00, 1.512e+00, 1.602e+00, 7.228e-01, 1.076e+00,
1.206e+00, 1.404e+00, 1.481e+00, 1.464e+00, 1.581e+00, 1.685e+00,
1.777e+00, 9.586e-01, 1.187e+00, 1.371e+00, 1.524e+00, 1.740e+00,
1.854e+00, 1.955e+00, 2.046e+00, 9.585e-01, 1.041e+00, 1.371e+00,
1.608e+00, 1.739e+00, 1.768e+00, 1.869e+00, 1.803e+00, 7.360e-01,
1.041e+00, 1.272e+00, 1.457e+00, 1.611e+00, 1.741e+00, 1.855e+00,
1.870e+00, 1.804e+00, 9.302e-01, 1.144e+00, 1.028e+00, 1.210e+00,
1.362e+00, 1.646e+00, 1.761e+00, 1.863e+00, 1.954e+00,
];
/// Linear fit coefficients A (53 values)
const A: [f64; 53] = [
6.95319e-01, 1.13101e+00, 1.36313e+00, 1.51684e+00, 1.64767e+00,
1.75643e+00, 1.84458e+00, 1.87243e+00, 1.85628e+00, 1.90889e+00,
9.01802e-01, 1.25389e+00, 1.39033e+00, 1.55226e+00, 1.60658e+00,
1.65930e+00, 1.68855e+00, 1.62477e+00, 1.66726e+00, 1.83599e+00,
2.50403e+00, 3.08564e+00, 3.56545e+00, 4.25922e+00, 4.61346e+00,
4.91417e+00, 5.19211e+00, 1.74181e+00, 2.25756e+00, 2.95625e+00,
3.65899e+00, 4.04397e+00, 4.13410e+00, 4.43538e+00, 4.19583e+00,
1.79027e+00, 2.23543e+00, 2.63942e+00, 3.02461e+00, 3.35018e+00,
3.62067e+00, 3.85218e+00, 3.76689e+00, 3.49318e+00, 1.16294e+00,
1.86467e+00, 2.02110e+00, 2.24231e+00, 2.44240e+00, 2.76594e+00,
2.93230e+00, 3.08109e+00, 3.21069e+00,
];
/// Linear fit coefficients B (53 values)
const B: [f64; 53] = [
-1.29000e+00, -2.15771e+00, -2.13263e+00, -2.10272e+00, -2.10861e+00,
-2.11507e+00, -2.11710e+00, -2.08531e+00, -2.03296e+00, -2.03441e+00,
-1.85905e+00, -2.04057e+00, -2.02189e+00, -2.05930e+00, -2.03403e+00,
-2.02071e+00, -1.99956e+00, -1.92851e+00, -1.92905e+00, -4.58608e+00,
-4.40022e+00, -4.39154e+00, -4.39676e+00, -4.57631e+00, -4.57120e+00,
-4.56188e+00, -4.55915e+00, -4.41218e+00, -4.12940e+00, -4.24401e+00,
-4.40783e+00, -4.39930e+00, -4.25981e+00, -4.26804e+00, -4.00419e+00,
-4.47251e+00, -3.87960e+00, -3.71668e+00, -3.68461e+00, -3.67173e+00,
-3.65991e+00, -3.64968e+00, -3.48666e+00, -3.23985e+00, -2.95758e+00,
-3.07110e+00, -2.87157e+00, -2.83137e+00, -2.82132e+00, -2.91084e+00,
-2.91159e+00, -2.91336e+00, -2.91296e+00,
];
/// Cubic polynomial coefficients COEF(4, 53) stored as flat array
/// COEF[I*4 + j] corresponds to Fortran COEF(j+1, I+1)
const COEF: [f64; 212] = [
// J=1..10
8.734e-01, -1.545e+00, -1.093e+00, 5.918e-01,
9.771e-01, -1.567e+00, -4.739e-01, -1.302e-01,
1.174e+00, -1.638e+00, -2.831e-01, -3.281e-02,
1.324e+00, -1.692e+00, -2.916e-01, 9.027e-02,
1.445e+00, -1.761e+00, -1.902e-01, 4.401e-02,
1.546e+00, -1.817e+00, -1.278e-01, 2.293e-02,
1.635e+00, -1.864e+00, -8.252e-02, 9.854e-03,
1.712e+00, -1.903e+00, -5.206e-02, 2.892e-03,
1.782e+00, -1.936e+00, -2.952e-02, -1.405e-03,
1.845e+00, -1.964e+00, -1.152e-02, -4.487e-03,
// J=11..19
7.377e-01, -9.327e-01, -1.466e+00, 6.891e-01,
9.031e-01, -1.157e+00, -7.151e-01, 1.832e-01,
1.031e+00, -1.313e+00, -4.517e-01, 9.207e-02,
1.135e+00, -1.441e+00, -2.724e-01, 3.105e-02,
1.225e+00, -1.536e+00, -1.725e-01, 7.191e-03,
1.302e+00, -1.602e+00, -1.300e-01, 7.345e-03,
1.372e+00, -1.664e+00, -8.204e-02, -1.643e-03,
1.434e+00, -1.715e+00, -4.646e-02, -7.456e-03,
1.491e+00, -1.760e+00, -1.838e-02, -1.152e-02,
// J=20..27
1.258e+00, -3.442e+00, -4.731e-01, -9.522e-02,
1.553e+00, -2.781e+00, -6.841e-01, -4.083e-03,
1.727e+00, -2.494e+00, -5.785e-01, -6.015e-02,
1.853e+00, -2.347e+00, -4.611e-01, -9.615e-02,
1.955e+00, -2.273e+00, -3.457e-01, -1.245e-01,
2.041e+00, -2.226e+00, -2.669e-01, -1.344e-01,
2.115e+00, -2.200e+00, -1.999e-01, -1.410e-01,
2.182e+00, -2.188e+00, -1.405e-01, -1.460e-01,
// J=28..35
1.267e+00, -3.417e+00, -5.038e-01, -1.797e-02,
1.565e+00, -2.781e+00, -6.497e-01, -5.979e-03,
1.741e+00, -2.479e+00, -6.099e-01, -2.227e-02,
1.870e+00, -2.336e+00, -4.899e-01, -6.616e-02,
1.973e+00, -2.253e+00, -3.972e-01, -8.729e-02,
2.061e+00, -2.212e+00, -3.072e-01, -1.060e-01,
2.137e+00, -2.189e+00, -2.352e-01, -1.171e-01,
2.205e+00, -2.186e+00, -1.621e-01, -1.296e-01,
// J=36..44
1.129e+00, -3.149e+00, -1.910e-01, -5.244e-01,
1.431e+00, -2.511e+00, -3.710e-01, -1.933e-01,
1.620e+00, -2.303e+00, -3.045e-01, -1.391e-01,
1.763e+00, -2.235e+00, -1.829e-01, -1.491e-01,
1.879e+00, -2.215e+00, -9.003e-02, -1.537e-01,
1.978e+00, -2.213e+00, -2.066e-02, -1.541e-01,
2.064e+00, -2.220e+00, 3.258e-02, -1.527e-01,
2.140e+00, -2.225e+00, 6.311e-02, -1.455e-01,
2.208e+00, -2.229e+00, 7.977e-02, -1.357e-01,
// J=45..53
1.204e+00, -2.809e+00, -3.094e-01, 1.100e-01,
1.455e+00, -2.254e+00, -4.795e-01, 6.872e-02,
1.619e+00, -2.109e+00, -3.357e-01, -2.532e-02,
1.747e+00, -2.065e+00, -2.317e-01, -5.224e-02,
1.853e+00, -2.058e+00, -1.517e-01, -6.647e-02,
1.943e+00, -2.055e+00, -1.158e-01, -6.081e-02,
2.023e+00, -2.070e+00, -6.470e-02, -6.800e-02,
2.095e+00, -2.088e+00, -2.357e-02, -7.250e-02,
2.160e+00, -2.107e+00, 1.065e-02, -7.542e-02,
];
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_hephot_below_threshold() {
// Below threshold frequency should return 0
let sigma = hephot(1, 0, 1, 1.0e14);
assert_eq!(sigma, 0.0);
}
#[test]
fn test_hephot_singlet_s_ground() {
// Singlet S state, n=1: threshold is at 3.288e15 * 10^FL0[0] ≈ 5.76e15 Hz
// Use frequency well above threshold
let freq = 8.0e15;
let sigma = hephot(1, 0, 1, freq);
assert!(sigma > 0.0, "Cross section should be positive above threshold");
assert!(sigma < 1.0e-15, "Cross section should be in reasonable range");
}
#[test]
fn test_hephot_triplet_p_n2() {
// Triplet P state, n=2
// IST(2,2)=36, N0(2,2)=2, so i = 36-1 + (2-2) = 35 (0-based)
let freq = 1.0e15;
let sigma = hephot(3, 1, 2, freq);
// May be below or above threshold depending on freq
assert!(sigma >= 0.0);
}
#[test]
fn test_hephot_hydrogenic_l3() {
// For L > 2, should use hydrogenic expression
let freq = 1.0e15;
let sigma = hephot(1, 3, 3, freq);
assert!(sigma > 0.0, "Hydrogenic cross section should be positive");
// Expected: 2.815e29 / freq^3 / n^5 * (2L+1) * S / (2*n^2)
let expected = 2.815e29 / freq.powi(3) / (3_i32.pow(5) as f64) * 7.0 * 1.0 / 18.0;
assert!((sigma - expected).abs() / expected < 1.0e-10);
}
#[test]
fn test_hephot_singlet_d_n2() {
// Singlet D, n=2: IST(3,1)=20, N0(3,1)=3
// i = 20-1 + (2-3) = 18 (0-based)
// But n < N0 gives negative index - this case shouldn't be called
// Let's test n=3 instead
let freq = 1.5e15;
let sigma = hephot(1, 2, 3, freq);
assert!(sigma >= 0.0);
}
#[test]
fn test_hephot_all_multiplicities() {
// Test that both singlet and triplet produce valid results
let freq = 5.0e15;
let s1 = hephot(1, 0, 1, freq); // singlet
let s3 = hephot(3, 0, 2, freq); // triplet
assert!(s1 >= 0.0);
assert!(s3 >= 0.0);
}
}
+163
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@@ -0,0 +1,163 @@
//! 光致电离截面插值(Hidalgo 1968)。
//!
//! 重构自 SYNSPEC `hidalg.f`
//!
//! 使用 Hidalgo (1968, Ap. J., 153, 981) 的波长和光致电离截面数据表,
//! 对给定频率进行线性插值。
/// 波长网格 1 (Å),用于 INDEX < 13 的物种
const WL1: [f64; 20] = [
39.1, 80.9, 97.6, 100.1, 104.3, 107.2, 108.7, 111.9, 113.6, 115.4,
117.1, 119.0, 124.8, 126.9, 129.1, 131.3, 133.6, 136.0, 138.5, 141.1,
];
/// 波长网格 2 (Å),用于 INDEX >= 13 的物种
const WL2: [f64; 20] = [
68.5, 80.9, 100.1, 120.9, 158.8, 165.7, 177.3, 190.6, 200.7, 206.2,
211.9, 218.0, 224.5, 231.3, 246.3, 0.0, 0.0, 0.0, 0.0, 0.0,
];
/// 光致电离截面数据 (Mbarn),20×24 矩阵(列优先存储)
const SIG0: [[f64; 20]; 24] = [
[0.0; 20], // col 1
[
0.0460, 0.2400, 0.3500, 0.3700, 0.4000, 0.4300, 0.4400, 0.4600, 0.4700, 0.4900,
0.5000, 0.5200, 0.5700, 0.6200, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
], // col 2
[0.0; 20], // col 3
[
0.0092, 0.1000, 0.1900, 0.2100, 0.2300, 0.2500, 0.2600, 0.2900, 0.3000, 0.3200,
0.3400, 0.3500, 0.4100, 0.4300, 0.4500, 0.4800, 0.5000, 0.5300, 0.5600, 0.5900,
], // col 4
[
0.3400, 0.4600, 0.6300, 0.7700, 0.9100, 1.080, 0.0, 0.0, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
], // col 5
[0.0; 20], // col 6
[
0.0064, 0.1100, 0.2200, 0.4100, 0.9400, 1.000, 1.300, 1.600, 0.0, 0.0,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
], // col 7
[0.0; 20], // col 8
[
0.0370, 0.0650, 0.1300, 0.2400, 0.5500, 0.6300, 0.7700, 0.9500, 1.100, 1.250,
0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
], // col 9
[0.0; 20], // col 10
[
0.0220, 0.0390, 0.0800, 0.1500, 0.3500, 0.4000, 0.4900, 0.6200, 0.7200, 0.7800,
0.8500, 0.9300, 1.020, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0,
], // col 11
[0.0; 20], // col 12
[0.0; 20], // col 13
[0.0; 20], // col 14
[0.0; 20], // col 15
[0.0; 20], // col 16
[0.0; 20], // col 17
[0.0; 20], // col 18
[0.0; 20], // col 19
[0.0; 20], // col 20
[0.0; 20], // col 21
[0.0; 20], // col 22
[0.0; 20], // col 23
[0.0; 20], // col 24
];
/// 光速 (cm/s)
const C_LIGHT: f64 = 2.997925e18;
/// 截面单位转换因子 (cm^2)
const SIG_FACTOR: f64 = 1.0e-18;
/// Hidalgo (1968) 光致电离截面插值。
///
/// 根据 Hidalgo 数据表,对给定频率进行线性插值。
///
/// # 参数
///
/// * `ib` - 物种标识(负值,`INDEX = -IB - 100`
/// * `fr` - 频率 (Hz)
///
/// # 返回值
///
/// 光致电离截面 (cm^2)
pub fn hidalg(ib: i32, fr: f64) -> f64 {
let index = (-ib - 101) as usize; // 转为 0-indexed
if index >= 24 {
return 0.0;
}
// 根据 INDEX 选择波长网格和数据
let num = if index < 12 { 20 } else { 15 };
let wli = if index < 12 { &WL1 } else { &WL2 };
let sigs = &SIG0[index];
// 将频率转换为波长 (Å)
let wlam = C_LIGHT / fr;
// 查找插值区间
let mut il = 0;
let mut ir = num - 1;
for i in 0..num - 1 {
if wlam >= wli[i] && wlam <= wli[i + 1] {
il = i;
ir = i + 1;
break;
}
}
// 线性插值
let mut sigm = if wli[ir] - wli[il] > 0.0 {
(sigs[ir] - sigs[il]) * (wlam - wli[il]) / (wli[ir] - wli[il]) + sigs[il]
} else {
sigs[il]
};
// 边界处理
if wlam <= wli[0] {
sigm = sigs[0];
}
if wlam >= wli[num - 1] {
sigm = sigs[num - 1];
}
sigm * SIG_FACTOR
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_hidalg_in_range() {
// 测试 H I (IB=-101, INDEX=0) 在有效波长范围内
// 100 Å 对应频率
let fr = C_LIGHT / 100.0;
let result = hidalg(-101, fr);
// H I 数据全为 0,所以结果应为 0
assert!(result >= 0.0);
}
#[test]
fn test_hidalg_species_2() {
// 测试物种 2 (IB=-102, INDEX=1)
let fr = C_LIGHT / 50.0; // 50 Å
let result = hidalg(-102, fr);
assert!(result >= 0.0);
assert!(result.is_finite());
}
#[test]
fn test_hidalg_invalid_index() {
let result = hidalg(-125, C_LIGHT / 100.0);
assert_eq!(result, 0.0);
}
#[test]
fn test_hidalg_above_range() {
// 高于波长范围时返回末值
let fr = C_LIGHT / 200.0;
let result = hidalg(-102, fr);
assert!(result >= 0.0);
}
}
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//! Hydrogen line profile data initialization.
//!
//! Translated from SYNSPEC54.FOR subroutine HYDINI (line 6877).
//!
//! Initializes necessary arrays for evaluating hydrogen line profiles
//! from the Lemke, Tremblay-Bergeron, or Schoening-Butler tables.
#![allow(clippy::never_loop)]
use std::fs::File;
use std::io::{BufRead, BufReader};
use super::stark0::stark0;
/// Constants for hydrogen profile arrays
pub const NLINES_MAX: usize = 22;
pub const NLEVELS: usize = 4;
pub const NWL_MAX: usize = 100;
pub const NT_MAX: usize = 20;
pub const NE_MAX: usize = 20;
/// Hydrogen line profile table data
#[derive(Debug, Clone)]
pub struct HydProfileTable {
/// Line index (i, j)
pub i: usize,
pub j: usize,
/// Central wavelength
pub wl0: f64,
/// Number of wavelength points
pub nwl: usize,
/// Number of temperature points
pub nt: usize,
/// Number of electron density points
pub ne: usize,
/// Log10 wavelength displacements [NWL_MAX]
pub wl: [f64; NWL_MAX],
/// Log10 temperature grid [NT_MAX]
pub xt: [f64; NT_MAX],
/// Log10 electron density grid [NE_MAX]
pub xne: [f64; NE_MAX],
/// Profile values [NWL_MAX x NT_MAX x NE_MAX]
pub prf: [[[f64; NE_MAX]; NT_MAX]; NWL_MAX],
/// Asymptotic profile coefficient
pub xk: f64,
}
impl Default for HydProfileTable {
fn default() -> Self {
Self {
i: 0,
j: 0,
wl0: 0.0,
nwl: 0,
nt: 0,
ne: 0,
wl: [0.0; NWL_MAX],
xt: [0.0; NT_MAX],
xne: [0.0; NE_MAX],
prf: [[[0.0; NE_MAX]; NT_MAX]; NWL_MAX],
xk: 0.0,
}
}
}
/// Hydrogen line initialization result
#[derive(Debug, Clone)]
pub struct HydInitResult {
/// Central wavelengths for lines [NLEVELS x NLINES_MAX]
pub wline: [[f64; NLINES_MAX]; NLEVELS],
/// Line index mapping [NLEVELS x NLINES_MAX]
pub ilin0: [[usize; NLINES_MAX]; NLEVELS],
/// Profile tables
pub tables: Vec<HydProfileTable>,
/// Lemke mode flag
pub ilemke: bool,
/// Number of lines
pub nlihyd: usize,
}
impl Default for HydInitResult {
fn default() -> Self {
Self {
wline: [[0.0; NLINES_MAX]; NLEVELS],
ilin0: [[0; NLINES_MAX]; NLEVELS],
tables: Vec::new(),
ilemke: false,
nlihyd: 0,
}
}
}
/// Hydrogen line profile table source
#[derive(Debug, Clone, Copy, PartialEq)]
pub enum HydTableSource {
/// Schoening-Butler tables (ihydpr < 0)
SchoeningButler,
/// Lemke tables (ihydpr = 21)
Lemke,
/// Tremblay-Bergeron tables (ihydpr = 22)
Tremblay,
}
/// Parameters for HYDINI
pub struct HydiniParams {
/// Table source selection
pub source: HydTableSource,
/// Path to data directory
pub data_dir: String,
/// Model depth points
pub nd: usize,
/// Temperature array [nd]
pub temp: Vec<f64>,
/// Electron density array [nd]
pub elec: Vec<f64>,
/// Turbulent velocity array [nd]
pub vturb: Vec<f64>,
}
/// Initialize hydrogen line profile data.
///
/// # Arguments
/// * `params` - Initialization parameters
///
/// # Returns
/// Hydrogen line initialization result with profile tables
pub fn hydini(params: &HydiniParams) -> std::io::Result<HydInitResult> {
let mut result = HydInitResult::default();
// Initialize central wavelengths using STARK0
for i in 0..NLEVELS {
for j in (i + 1)..NLINES_MAX {
let stark = stark0(i as i32 + 1, j as i32 + 1, 1);
result.wline[i][j] = stark.wl0;
}
}
// Initialize line index mapping
for i in 0..NLEVELS {
for j in 0..NLINES_MAX {
result.ilin0[i][j] = 0;
}
}
match params.source {
HydTableSource::SchoeningButler => {
read_schoening_butler(params, &mut result)?;
}
HydTableSource::Lemke | HydTableSource::Tremblay => {
read_lemke_tremblay(params, &mut result)?;
}
}
Ok(result)
}
/// Read Schoening-Butler tables
fn read_schoening_butler(
params: &HydiniParams,
result: &mut HydInitResult,
) -> std::io::Result<()> {
let filename = format!("{}/hydprf.dat", params.data_dir);
let file = File::open(&filename)?;
let reader = BufReader::new(file);
let mut lines = reader.lines();
// Skip 12 header lines
for _ in 0..12 {
lines.next();
}
let nline = 12;
result.ilemke = false;
for iline in 0..nline {
// Read line indices
let header = read_next_line(&mut lines)?;
let (i, j) = parse_line_indices(&header)?;
let j = if iline == 11 { 10 } else { j }; // Special case for last line
let wl0 = result.wline[i - 1][j - 1];
result.ilin0[i - 1][j - 1] = iline + 1;
let mut table = HydProfileTable {
i,
j,
wl0,
..Default::default()
};
// Read wavelength points
let wl_line = read_next_line(&mut lines)?;
let wl_parts = parse_data_line(&wl_line)?;
let nwl = wl_parts.len() - 1; // First value is character
table.nwl = nwl;
for k in 0..nwl.min(NWL_MAX) {
table.wl[k] = if wl_parts[k + 1] < 1.0e-4 {
(1.0e-4_f64).log10()
} else {
wl_parts[k + 1].log10()
};
}
// Read temperature points
let xt_line = read_next_line(&mut lines)?;
let xt_parts = parse_data_line(&xt_line)?;
let nt = xt_parts.len() - 1;
table.nt = nt;
for k in 0..nt.min(NT_MAX) {
table.xt[k] = xt_parts[k + 1];
}
// Read electron density points
let xne_line = read_next_line(&mut lines)?;
let xne_parts = parse_data_line(&xne_line)?;
let ne = xne_parts.len() - 1;
table.ne = ne;
for k in 0..ne.min(NE_MAX) {
table.xne[k] = xne_parts[k + 1];
}
// Skip blank line
lines.next();
// Read profile data
for ie in 0..ne.min(NE_MAX) {
for it in 0..nt.min(NT_MAX) {
lines.next(); // Skip blank line
let prf_line = read_next_line(&mut lines)?;
let prf_parts = parse_data_line(&prf_line)?;
for iwl in 0..nwl.min(NWL_MAX) {
if iwl < prf_parts.len() {
table.prf[iwl][it][ie] = prf_parts[iwl];
}
}
}
}
// Compute asymptotic profile coefficient
if nwl > 0 && ne > 0 {
let xclog = table.prf[nwl - 1][0][0]
+ 2.5 * table.wl[nwl - 1]
+ 31.5304
- table.xne[0]
- 2.0 * wl0.log10();
let xklog = 0.6666667 * (xclog - 0.176);
table.xk = (xklog * std::f64::consts::LN_10).exp();
}
result.tables.push(table);
}
Ok(())
}
/// Read Lemke or Tremblay tables
fn read_lemke_tremblay(
params: &HydiniParams,
result: &mut HydInitResult,
) -> std::io::Result<()> {
let filename = match params.source {
HydTableSource::Lemke => format!("{}/lemke.dat", params.data_dir),
HydTableSource::Tremblay => format!("{}/tremblay.dat", params.data_dir),
_ => unreachable!(),
};
let file = File::open(&filename)?;
let reader = BufReader::new(file);
let mut lines = reader.lines();
result.ilemke = true;
// Read number of tables
let ntab_line = read_next_line(&mut lines)?;
let ntab: usize = ntab_line.trim().parse().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("NTAB: {}", e))
})?;
let mut iline = 0;
for _ in 0..ntab {
// Read number of lines in this table
let nlly_line = read_next_line(&mut lines)?;
let nlly: usize = nlly_line.trim().parse().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("NLLY: {}", e))
})?;
let ilineb = iline;
// Read line parameters
for _ in 0..nlly {
let param_line = read_next_line(&mut lines)?;
let parts = parse_data_line(&param_line)?;
if parts.len() < 11 {
return Err(std::io::Error::new(
std::io::ErrorKind::InvalidData,
"Invalid Lemke/Tremblay parameter line",
));
}
let i = parts[0] as usize;
let j = parts[1] as usize;
let almin = parts[2];
let anemin = parts[3];
let tmin = parts[4];
let dla = parts[5];
let dle = parts[6];
let dlt = parts[7];
let nwl = parts[8] as usize;
let ne = parts[9] as usize;
let nt = parts[10] as usize;
let wl0 = result.wline[i - 1][j - 1];
result.ilin0[i - 1][j - 1] = iline + 1;
let mut table = HydProfileTable {
i,
j,
wl0,
nwl,
nt,
ne,
..Default::default()
};
// Generate wavelength grid
for iwl in 0..nwl.min(NWL_MAX) {
table.wl[iwl] = almin + (iwl as f64) * dla;
}
// Generate electron density grid
for ie in 0..ne.min(NE_MAX) {
table.xne[ie] = anemin + (ie as f64) * dle;
}
// Generate temperature grid
for it in 0..nt.min(NT_MAX) {
table.xt[it] = tmin + (it as f64) * dlt;
}
result.tables.push(table);
iline += 1;
}
// Read profile data for each line
for ili in 0..nlly {
let ilne = ilineb + ili;
let table = &mut result.tables[ilne];
let nwl = table.nwl;
let ne = table.ne;
let nt = table.nt;
lines.next(); // Skip blank line
for ie in 0..ne.min(NE_MAX) {
for it in 0..nt.min(NT_MAX) {
let prf_line = read_next_line(&mut lines)?;
let parts = parse_data_line(&prf_line)?;
// First value is QLT (quality factor), skip it
for iwl in 0..nwl.min(NWL_MAX) {
if iwl + 1 < parts.len() {
table.prf[iwl][it][ie] = parts[iwl + 1];
}
}
}
}
// Compute asymptotic profile coefficient
if nwl > 0 && ne > 0 {
let xclog = table.prf[nwl - 1][0][0]
+ 2.5 * table.wl[nwl - 1].log10()
+ 31.5304
- table.xne[0]
- 2.0 * table.wl0.log10();
let xklog = 0.6666667 * (xclog - 0.176);
table.xk = (xklog * std::f64::consts::LN_10).exp();
}
}
}
result.nlihyd = iline;
Ok(())
}
/// Read next non-empty line
fn read_next_line(lines: &mut impl Iterator<Item = std::io::Result<String>>) -> std::io::Result<String> {
loop {
match lines.next() {
Some(Ok(line)) => return Ok(line),
Some(Err(e)) => return Err(e),
None => return Err(std::io::Error::new(
std::io::ErrorKind::UnexpectedEof,
"Unexpected end of file",
)),
}
}
}
/// Parse line indices from header: FORMAT(12X,I1,9X,I1)
fn parse_line_indices(line: &str) -> std::io::Result<(usize, usize)> {
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 2 {
return Err(std::io::Error::new(
std::io::ErrorKind::InvalidData,
format!("Invalid line indices: {}", line),
));
}
let i = parts[0].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("I: {}", e))
})?;
let j = parts[1].parse::<usize>().map_err(|e| {
std::io::Error::new(std::io::ErrorKind::InvalidData, format!("J: {}", e))
})?;
Ok((i, j))
}
/// Parse data line (free format)
fn parse_data_line(line: &str) -> std::io::Result<Vec<f64>> {
let values: Vec<f64> = line
.split_whitespace()
.filter_map(|s| s.parse::<f64>().ok())
.collect();
Ok(values)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_hydini_default() {
let result = HydInitResult::default();
assert_eq!(result.wline.len(), NLEVELS);
assert_eq!(result.ilin0.len(), NLEVELS);
assert!(result.tables.is_empty());
}
#[test]
fn test_hyd_profile_table_default() {
let table = HydProfileTable::default();
assert_eq!(table.nwl, 0);
assert_eq!(table.nt, 0);
assert_eq!(table.ne, 0);
}
#[test]
fn test_parse_line_indices() {
let line = " 1 2";
let result = parse_line_indices(line);
assert!(result.is_ok());
let (i, j) = result.unwrap();
assert_eq!(i, 1);
assert_eq!(j, 2);
}
#[test]
fn test_parse_data_line() {
let line = " 1.0 2.0 3.0 4.0";
let result = parse_data_line(line);
assert!(result.is_ok());
let values = result.unwrap();
assert_eq!(values.len(), 4);
assert!((values[0] - 1.0).abs() < 1e-10);
}
}
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//! Hydrogen line opacity calculation for SYNSPEC.
//!
//! Translated from SYNSPEC `HYDLIN` subroutine (synspec54.f:5425).
//!
//! Calculates opacity and emissivity of hydrogen lines including:
//! - Stark broadening (analytic profiles)
//! - Allard quasi-molecular satellite opacity
//! - Far-infrared hydrogen lines
use super::stark0::stark0;
use super::starka::starka;
use super::starkir::starkir;
use super::divstr::divstr;
use super::allard::{self, AllardData};
use super::lyahhe::lyahhe;
/// Physical constants for hydrogen line calculations
const CPP: f64 = 4.1412e-16;
const CPJ: f64 = 157803.0;
const C00: f64 = 1.25e-9;
const CID: f64 = 0.02654;
const CINV: f64 = 1.0 / 2.997925e18;
/// Parameters for hydrogen line opacity calculation
pub struct HydlinParams {
/// Depth index
pub id: usize,
/// Start frequency index
pub i0: usize,
/// End frequency index
pub i1: usize,
/// Number of frequencies
pub nfreq: usize,
/// Wavelength array (Å)
pub wlam: Vec<f64>,
/// Frequency array (Hz)
pub freq: Vec<f64>,
/// Temperature (K)
pub t: f64,
/// Electron density
pub ane: f64,
/// H atom exists
pub iath: i32,
/// Lower level for H lines
pub ilowh: i32,
/// Upper level limit
pub m10: usize,
pub m20: usize,
/// H ground level population
pub pop_h: f64,
/// H continuum level population
pub pop_h_cont: f64,
/// Turbulent velocity
pub vturb: f64,
/// wnHint factors
pub wn_hint: Vec<Vec<f64>>,
/// Quasi-molecular Lyman-alpha flag (>0: include)
pub nunalp: i32,
/// Quasi-molecular Lyman-beta flag (>0: include)
pub nunbet: i32,
/// Quasi-molecular Lyman-gamma flag (>0: include)
pub nungam: i32,
/// Quasi-molecular Balmer flag (>0: include)
pub nunbal: i32,
/// Allard quasi-molecular profile data (optional)
pub allard_data: Option<AllardData>,
/// Neutral H particle density at depth [cm⁻³]
pub hneutr: f64,
/// Ionized H particle density at depth [cm⁻³]
pub hcharg: f64,
/// Lyman-alpha He broadening flag (>0: include)
pub nunhhe: i32,
/// He atom index in atomic data (>0: He present)
pub iathe: i32,
/// He ground level population at depth
pub pop_he: f64,
}
/// Result of hydrogen line opacity calculation
pub struct HydlinResult {
/// Absorption coefficient array
pub absoh: Vec<f64>,
/// Emission coefficient array
pub emish: Vec<f64>,
}
/// Calculate hydrogen line opacity and emissivity.
///
/// Translates the full SYNSPEC HYDLIN subroutine including Stark broadening
/// and infrared lines.
pub fn hydlin(params: &HydlinParams) -> HydlinResult {
let i0 = params.i0;
let i1 = params.i1;
let nfreq = params.nfreq;
let mut absoh = vec![0.0; nfreq];
let mut emish = vec![0.0; nfreq];
// Skip if no hydrogen or empty arrays
if params.iath <= 0 || params.wlam.is_empty() || params.ilowh <= 0 {
return HydlinResult { absoh, emish };
}
let t = params.t;
let t1 = 1.0 / t;
let sqt = t.sqrt();
let ane = params.ane;
let anes = (ane.ln() / 6.0).exp();
// Population of level 2 (for Saha)
let anp = params.pop_h_cont;
let pp = CPP * ane * anp * t1 / sqt;
// Level populations
let nlh = params.wn_hint.len().min(3);
let mut pj = vec![0.0f64; 50];
for il in 0..50 {
let x = ((il + 1) * (il + 1)) as f64;
if il < nlh {
pj[il] = params.pop_h * (-CPJ / x * t1).exp() * x;
} else {
let wn = if il < params.wn_hint.len() && params.id < params.wn_hint[il].len() {
params.wn_hint[il][params.id]
} else {
1.0
};
pj[il] = pp * (CPJ / x * t1).exp() * x * wn;
}
}
// Frequency-independent Stark parameters
let f00 = C00 * anes * anes * anes * anes;
let dop0 = 1.0e8 * (1.65e8 * t + params.vturb).sqrt();
// Determine spectral series range
let iserl = params.ilowh as usize;
let mut iseru = params.ilowh as usize;
if i0 < params.wlam.len() {
let wl = params.wlam[i0];
if wl > 14000.0 { iseru = 4; }
if wl > 22700.0 { iseru = 5; }
if wl > 32800.0 { iseru = 6; }
if wl > 44660.0 { iseru = 7; }
}
// Loop over spectral series
for i in iserl..=iseru.min(40) {
let ii = (i * i) as f64;
let xii = 1.0 / ii;
let popi = if i - 1 < pj.len() { pj[i - 1] } else { 0.0 };
// Determine contributing lines
let m1 = (i + 1).max(params.m10);
let m2 = (i + 4).min(params.m20).min(40);
for j in m1..=m2 {
let jj = (j * j) as f64;
let xjj = 1.0 / jj;
// Transition properties
let wn_j = if j - 1 < params.wn_hint.len() && params.id < params.wn_hint[j - 1].len() {
params.wn_hint[j - 1][params.id]
} else {
1.0
};
let wn_i = if i - 1 < params.wn_hint.len() && params.id < params.wn_hint[i - 1].len() {
params.wn_hint[i - 1][params.id]
} else {
1.0
};
let abtra = popi * wn_j;
let emtra = if j - 1 < pj.len() {
pj[j - 1] * wn_i * ii * xjj * (CPJ * (xii - xjj) * t1).exp()
} else {
0.0
};
// Use analytic Stark profile
let stark = stark0(i as i32, j as i32, 1);
let wl0 = stark.wl0;
let xkij = stark.xkij;
let fij = stark.fij;
// Check if line contributes in this wavelength region
let wlam_i1 = if i1 < params.wlam.len() { params.wlam[i1] } else { 0.0 };
let wlam_i0 = if i0 < params.wlam.len() { params.wlam[i0] } else { 0.0 };
let in_range = (wl0 <= wlam_i1 && 1.25 * wl0 > wlam_i0)
|| (wl0 >= wlam_i0 && 0.75 * wl0 < wlam_i1);
if in_range {
let fxk = f00 * xkij;
if fxk.abs() < 1.0e-30 { continue; }
let fxk1 = 1.0 / fxk;
let dop = dop0 / wl0;
let dbeta = wl0 * wl0 * CINV * fxk1;
let betad = dop * dbeta;
let fid = CID * fij * dbeta;
let (ad, div) = divstr(betad);
// Quasi-molecular opacity check (Lyman alpha/beta/gamma, Balmer alpha)
let lquasi = (i == 1 && j == 2 && params.nunalp > 0)
|| (i == 1 && j == 3 && params.nunbet > 0)
|| (i == 1 && j == 4 && params.nungam > 0)
|| (i == 2 && j == 3 && params.nunbal > 0);
if lquasi && params.allard_data.is_some() {
// Allard quasi-molecular + Stark profile
let ad_ref = params.allard_data.as_ref().unwrap();
for ij in i0..=i1.min(nfreq - 1) {
let wl = params.wlam[ij];
let beta = (wl - wl0).abs() * fxk1;
let sg_allard = allard::allard(ad_ref, wl, params.hneutr, params.hcharg, i as i32, j as i32);
let sg = sg_allard + starka(beta, betad, ad, div, 2.0) * fid;
absoh[ij] += sg * abtra;
emish[ij] += sg * emtra;
}
} else {
// Standard Stark profile
for ij in i0..=i1.min(nfreq - 1) {
let beta = (params.wlam[ij] - wl0).abs() * fxk1;
let sg = if i < 5 {
starka(beta, betad, ad, div, 2.0) * fid
} else {
starkir(ii as i32, jj as i32, t, ane, beta, dbeta) * fid
};
absoh[ij] += sg * abtra;
emish[ij] += sg * emtra;
}
}
}
// Lyman-alpha broadening by helium (Lyahhe)
let lalhhe = i == 1 && j == 2 && params.nunhhe > 0;
if lalhhe && params.iathe > 0 && params.pop_he > 0.0 {
let rel = 1.0 / std::f64::consts::TAU;
for ij in i0..=i1.min(nfreq - 1) {
let sg0 = lyahhe(params.wlam[ij], params.pop_he);
let sg = sg0 * rel;
absoh[ij] += sg * abtra;
emish[ij] += sg * emtra;
}
}
}
}
// Far infrared hydrogen lines
if i1 < nfreq && !params.wlam.is_empty() && params.wlam[i1.min(params.wlam.len() - 1)] > 70000.0 {
for i in 8..=13 {
let ii = (i * i) as f64;
let xii = 1.0 / ii;
for j in (i + 1)..=(i + 4).min(40) {
let jj = (j * j) as f64;
let xjj = 1.0 / jj;
let stark = stark0(i as i32, j as i32, 1);
let wl0 = stark.wl0;
let xkij = stark.xkij;
let fij = stark.fij;
let wlam_i1 = params.wlam[i1.min(params.wlam.len() - 1)];
let wlam_i0 = params.wlam[i0.min(params.wlam.len() - 1)];
let in_range = (wl0 <= wlam_i1 && 1.5 * wl0 > wlam_i0)
|| (wl0 >= wlam_i0 && 0.5 * wl0 < wlam_i1);
if in_range {
let fxk = f00 * xkij;
if fxk.abs() < 1.0e-30 { continue; }
let fxk1 = 1.0 / fxk;
let dop = dop0 / wl0;
let dbeta = wl0 * wl0 * CINV * fxk1;
let _betad = dop * dbeta;
let fid = CID * fij * dbeta;
let wn_j = if j - 1 < params.wn_hint.len() && params.id < params.wn_hint[j - 1].len() {
params.wn_hint[j - 1][params.id]
} else {
1.0
};
let wn_i = if i - 1 < params.wn_hint.len() && params.id < params.wn_hint[i - 1].len() {
params.wn_hint[i - 1][params.id]
} else {
1.0
};
let popi = if i - 1 < pj.len() { pj[i - 1] } else { 0.0 };
let popj = if j - 1 < pj.len() { pj[j - 1] } else { 0.0 };
let abtra = popi * wn_j;
let emtra = popj * wn_i * ii * xjj * (CPJ * (xii - xjj) * t1).exp();
for ij in i0..=i1.min(nfreq - 1) {
let beta = (params.wlam[ij] - wl0).abs() * fxk1;
let sg = starkir(ii as i32, jj as i32, t, ane, beta, dbeta) * fid;
absoh[ij] += sg * abtra;
emish[ij] += sg * emtra;
}
}
}
}
}
// Total opacity and emissivity (stimulated emission correction)
for ij in i0..=i1.min(nfreq - 1) {
let f = params.freq[ij];
let f15 = f * 1.0e-15;
let xkf = (-4.79928e-11 * f * t1).exp();
let xkfb = xkf * 1.4743e-2 * f15 * f15 * f15;
absoh[ij] -= xkf * emish[ij];
emish[ij] *= xkfb;
}
HydlinResult { absoh, emish }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_hydlin_basic() {
let params = HydlinParams {
id: 0,
i0: 0,
i1: 4,
nfreq: 5,
wlam: vec![10000.0, 12000.0, 14000.0, 16000.0, 18000.0],
freq: vec![3.0e14, 2.5e14, 2.14e14, 1.87e14, 1.67e14],
t: 6000.0,
ane: 1.0e13,
iath: 1,
ilowh: 1,
m10: 2,
m20: 10,
pop_h: 1.0e16,
pop_h_cont: 1.0e10,
vturb: 2.0e5,
wn_hint: vec![vec![1.0; 10]; 50],
nunalp: 0,
nunbet: 0,
nungam: 0,
nunbal: 0,
allard_data: None,
hneutr: 0.0,
hcharg: 0.0,
nunhhe: 0,
iathe: 0,
pop_he: 0.0,
};
let result = hydlin(&params);
assert!(result.absoh.iter().all(|&x| x.is_finite()));
assert!(result.emish.iter().all(|&x| x.is_finite()));
}
#[test]
fn test_hydlin_no_hydrogen() {
let params = HydlinParams {
id: 0,
i0: 0,
i1: 4,
nfreq: 5,
wlam: vec![10000.0, 12000.0, 14000.0, 16000.0, 18000.0],
freq: vec![3.0e14, 2.5e14, 2.14e14, 1.87e14, 1.67e14],
t: 6000.0,
ane: 1.0e13,
iath: 0,
ilowh: 1,
m10: 2,
m20: 10,
pop_h: 1.0e16,
pop_h_cont: 1.0e10,
vturb: 2.0e5,
wn_hint: vec![vec![1.0; 10]; 50],
nunalp: 0,
nunbet: 0,
nungam: 0,
nunbal: 0,
allard_data: None,
hneutr: 0.0,
hcharg: 0.0,
nunhhe: 0,
iathe: 0,
pop_he: 0.0,
};
let result = hydlin(&params);
assert!(result.absoh.iter().all(|&x| x == 0.0));
assert!(result.emish.iter().all(|&x| x == 0.0));
}
}
+706
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//! Hydrogen line opacity and emissivity for SYNSPEC (frequency window mode).
//!
//! Translated from SYNSPEC `HYDLIW` subroutine (synspec54.f:5798).
//!
//! Calculates opacity and emissivity of hydrogen lines in the frequency
//! window mode. This is the window-mode variant of `hydlin`.
use super::{allard, divstr, feautr, lyahhe::lyahhe, stark0, starka, FeautrParams};
// ============================================================================
// Physical constants
// ============================================================================
const UN: f64 = 1.0;
const TWO: f64 = 2.0;
const SIXTH: f64 = 1.0 / 6.0;
const CPP: f64 = 4.1412e-16;
const CPJ: f64 = 157803.0;
#[allow(dead_code)]
const CPJ4: f64 = CPJ / 4.0;
const C00: f64 = 1.25e-9;
const CID: f64 = 0.02654;
const CINV: f64 = UN / 2.997925e18;
const AL10: f64 = std::f64::consts::LN_10;
// ============================================================================
// Parameters
// ============================================================================
/// Common input data for hydrogen line opacity calculations.
pub struct HydliwCommon<'a> {
/// Depth index.
pub id: usize,
/// Temperature at depth ID (K).
pub t: f64,
/// Electron density at depth ID.
pub ane: f64,
/// Turbulent velocity at depth ID (cm/s).
pub vturb: f64,
/// Surface gravity (log g).
pub grav: f64,
/// Frequency array (Hz).
pub freq: &'a [f64],
/// Wavelength array (Å).
pub wlam: &'a [f64],
/// H atom exists flag.
pub iath: i32,
/// Lyman line treatment switch.
pub iophli: i32,
/// Lemke profile table flag.
pub ilemke: i32,
/// H ground level population.
pub pop_h_cont: f64,
/// Level populations for H (up to 40 levels).
/// If None, populations are computed from LTE/Saha.
pub pj: Option<&'a [f64]>,
/// WNHINT partition function values (indexed by level, depth).
pub wnhint: &'a [f64],
/// Number of wavelength points per hydrogen profile line.
pub nwlhyd: &'a [usize],
/// Log10 of profile values: prfhyd[line * 54 + iwl].
pub prfhyd: &'a [f64],
/// Log10 of wavelength grid per profile line: wlhyd[line * 54 + iwl].
pub wlhyd: &'a [f64],
/// Line wavelength table wline[i][j] for i<=4, j<=22.
pub wline: &'a [f64],
/// Oscillator strengths osch[i][j] for i<=4, j<=22.
pub osch: &'a [f64],
/// Profile line index table ilin0[i][j] for i<=4, j<=22.
pub ilin0: &'a [i32],
/// Number of NLTE H levels.
pub nlh: usize,
/// H ground level index in model.
pub n0hn: usize,
/// Feautrier parameters for Lyman-alpha.
pub feautr_params: Option<&'a FeautrParams>,
/// Laser delay flag.
pub lasdel: bool,
/// Quasi-molecular Lyman-alpha flag (>0: include).
pub nunalp: i32,
/// Quasi-molecular Lyman-beta flag (>0: include).
pub nunbet: i32,
/// Quasi-molecular Lyman-gamma flag (>0: include).
pub nungam: i32,
/// Quasi-molecular Balmer flag (>0: include).
pub nunbal: i32,
/// Allard quasi-molecular profile data (optional).
/// If None, quasi-molecular opacity is skipped.
pub allard_data: Option<&'a super::AllardData>,
/// Neutral H particle density at depth [cm⁻³].
pub hneutr: f64,
/// Ionized H particle density at depth [cm⁻³].
pub hcharg: f64,
/// Lyman-alpha He broadening flag (>0: include).
pub nunhhe: i32,
/// He atom index in atomic data (>0: He present).
pub iathe: i32,
/// He ground level population at depth.
pub pop_he: f64,
}
/// Per-frequency window parameters for hydrogen lines.
pub struct HydliwWindowParams<'a> {
/// H line processing flag per frequency (-1: skip, >0: process).
pub ihylw: &'a [i32],
/// Lower series index per frequency.
pub ilowhw: &'a [usize],
/// Maximum principal quantum number per frequency.
pub m10w: &'a [usize],
/// Upper limit for H lines per frequency.
pub m20w: &'a [usize],
}
/// Input parameters for `hydliw`.
pub struct HydliwParams<'a> {
/// Common H data.
pub common: HydliwCommon<'a>,
/// Per-frequency window parameters.
pub window: HydliwWindowParams<'a>,
}
/// Result of `hydliw`.
pub struct HydliwResult {
/// Absorption coefficient array.
pub absoh: Vec<f64>,
/// Emission coefficient array.
pub emish: Vec<f64>,
}
// ============================================================================
// Implementation
// ============================================================================
/// Calculate hydrogen line opacity and emissivity (frequency window mode).
pub fn hydliw(params: &HydliwParams) -> HydliwResult {
let c = &params.common;
let nf = c.freq.len();
let mut abso = vec![0.0; nf];
let mut emis = vec![0.0; nf];
let mut absoh = vec![0.0; nf];
let mut emish = vec![0.0; nf];
if c.iath <= 0 {
return HydliwResult { absoh, emish };
}
let t1 = UN / c.t;
let sqt = c.t.sqrt();
let anes = c.ane.powf(SIXTH);
// Populations of the first 40 levels of hydrogen
let mut pj = [0.0f64; 40];
let pp = CPP * c.ane * c.pop_h_cont * t1 / sqt;
for il in 1..=40 {
let x = (il * il) as f64;
if il <= c.nlh {
if let Some(pj_in) = c.pj
&& il - 1 < pj_in.len() {
pj[il - 1] = pj_in[il - 1];
}
} else {
let wn = wn_val(c.wnhint, il, c.id, nf);
pj[il - 1] = pp * (CPJ / x * t1).exp() * x * wn;
}
}
// Frequency- and line-independent Stark parameters
let f00 = C00 * anes * anes * anes * anes;
let dop0 = 1.0e8 * (1.65e8 * c.t + c.vturb).sqrt();
// Loop over all frequencies
for ij in 0..nf {
if params.window.ihylw[ij] <= 0 {
continue;
}
let wl = c.wlam[ij];
let fr = c.freq[ij];
// Determine series range based on wavelength
let (mut iserl, iseru) = series_range_hydrogen(params.window.ilowhw[ij], wl);
if iserl == 3 && iseru == 3 && c.nunbal > 0 {
iserl = 2;
}
abso[ij] = 0.0;
emis[ij] = 0.0;
for i in iserl..=iseru {
let ii = (i * i) as f64;
let xii = UN / ii;
let _popi = pj[i - 1];
// Determine contributing lines
let (m1, m2) = determine_lines_hydrogen(
i, params.window.ilowhw[ij], params.window.m10w[ij],
params.window.m20w[ij], c.grav,
);
for j in m1..=m2 {
// Skip certain Lyman lines if iophli < 0
if i == 1 && j <= 5 && c.iophli < 0 {
continue;
}
let jj = j * j;
let xjj = UN / jj as f64;
// Transition properties
let (abtra, emtra) = transition_hydrogen(i, j, &pj, c, nf, ii, xii, xjj, t1);
// Lyman-alpha broadening by helium (Lyahhe)
let lalhhe = i == 1 && j == 2 && c.nunhhe > 0;
if lalhhe && c.iathe > 0 && c.pop_he > 0.0 {
let rel = 1.0 / std::f64::consts::TAU;
let sg0 = lyahhe(wl, c.pop_he);
let sg = sg0 * rel;
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
}
// Profile line index for tabulated profiles
let iline = if i <= 4 && j <= 22 {
let idx = (i - 1) * 22 + (j - 1);
if idx < c.ilin0.len() { c.ilin0[idx] } else { 0 }
} else {
0
};
// Quasi-molecular opacity check
let lquasi = (i == 1 && j == 2 && c.nunalp > 0)
|| (i == 1 && j == 3 && c.nunbet > 0)
|| (i == 1 && j == 4 && c.nungam > 0)
|| (i == 2 && j == 3 && c.nunbal > 0);
if lquasi && c.allard_data.is_some() {
// Quasi-molecular + Stark profile
let stark = stark0(i as i32, j as i32, 1);
let fxk = f00 * stark.xkij;
let fxk1 = UN / fxk;
let dop = dop0 / stark.wl0;
let dbeta = stark.wl0 * stark.wl0 * CINV * fxk1;
let betad = dop * dbeta;
let fid = CID * stark.fij * dbeta;
let (ad, div) = divstr(betad);
let beta = (wl - stark.wl0).abs() * fxk1;
// Allard quasi-molecular contribution
let ad_data = c.allard_data.unwrap();
let sg_allard = allard(ad_data, wl, c.hneutr, c.hcharg, i as i32, j as i32);
let sg = sg_allard + starka(beta, betad, ad, div, UN) * fid;
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
} else if iline > 0 {
// Tabulated Stark profile
let nwl_idx = iline as usize - 1;
if nwl_idx < c.nwlhyd.len() {
let nwl = c.nwlhyd[nwl_idx];
let wline_idx = (i - 1) * 22 + (j - 1);
let wline_ij = if wline_idx < c.wline.len() {
c.wline[wline_idx]
} else {
0.0
};
let osch_idx = (i - 1) * 22 + (j - 1);
let osch_ij = if osch_idx < c.osch.len() {
c.osch[osch_idx]
} else {
0.0
};
let fid = CID * osch_ij;
let mut al = (wl - wline_ij).abs();
if al < 1.0e-4 {
al = 1.0e-4;
}
if c.ilemke == 1 {
al /= f00;
}
let al = al.log10();
// Find interpolation interval
let mut iw0 = 0usize;
for iwl in 0..nwl - 1 {
let wl_next = profile_wl_val_h(c.wlhyd, nwl_idx, iwl + 1);
if al <= wl_next {
iw0 = iwl;
break;
}
iw0 = iwl;
}
let iw1 = iw0 + 1;
let wl0 = profile_wl_val_h(c.wlhyd, nwl_idx, iw0);
let wl1 = profile_wl_val_h(c.wlhyd, nwl_idx, iw1);
let prf0 = profile_prf_val_h(c.prfhyd, nwl_idx, iw0);
let prf1 = profile_prf_val_h(c.prfhyd, nwl_idx, iw1);
let denom = wl1 - wl0;
let prff = if denom.abs() > 1.0e-30 {
(prf0 * (wl1 - al) + prf1 * (al - wl0)) / denom
} else {
prf0
};
let mut sg = (prff * AL10).exp() * fid;
if c.ilemke == 1 {
sg *= wline_ij * wline_ij * CINV / f00;
}
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
}
} else {
// Asymptotic Stark profile
let stark = stark0(i as i32, j as i32, 1);
let fxk = f00 * stark.xkij;
let fxk1 = UN / fxk;
let dop = dop0 / stark.wl0;
let dbeta = stark.wl0 * stark.wl0 * CINV * fxk1;
let betad = dop * dbeta;
let fid = CID * stark.fij * dbeta;
let (ad, div) = divstr(betad);
let beta = (wl - stark.wl0).abs() * fxk1;
let mut sg = starka(beta, betad, ad, div, TWO) * fid;
// Feautrier Lyman-alpha correction
if c.iophli == 2 && i == 1 && j == 2
&& let Some(fp) = c.feautr_params {
sg *= feautr(fr, fp);
}
abso[ij] += sg * abtra;
emis[ij] += sg * emtra;
}
}
}
// Total opacity and emissivity
let f = c.freq[ij];
let f15 = f * 1.0e-15;
let xkf = (-4.79928e-11 * f * t1).exp();
let xkfb = xkf * 1.4743e-2 * f15 * f15 * f15;
if abso[ij] <= 0.0 && c.lasdel {
abso[ij] = 0.0;
emis[ij] = 0.0;
}
absoh[ij] = abso[ij] - xkf * emis[ij];
emish[ij] = xkfb * emis[ij];
}
HydliwResult { absoh, emish }
}
// ============================================================================
// Helper functions
// ============================================================================
/// Determine series range based on wavelength for hydrogen.
fn series_range_hydrogen(ilow: usize, wl: f64) -> (usize, usize) {
let mut iserl = ilow;
let mut iseru = ilow;
if wl > 17000.0 && wl <= 21000.0 {
iserl = 3; iseru = 4;
} else if wl > 22700.0 && wl <= 29000.0 {
iserl = 4; iseru = 5;
} else if wl > 32800.0 && wl <= 37000.0 {
iserl = 5; iseru = 6;
} else if wl > 37000.0 && wl <= 44600.0 {
iserl = 4; iseru = 6;
} else if wl > 44660.0 && wl <= 58300.0 {
iserl = 5; iseru = 7;
} else if wl > 58300.0 && wl <= 72000.0 {
iserl = 6; iseru = 8;
} else if wl > 72000.0 && wl <= 73800.0 {
iserl = 5; iseru = 8;
} else if wl > 73800.0 && wl <= 77000.0 {
iserl = 5; iseru = 9;
} else if wl > 77000.0 {
iserl = 6; iseru = 9;
}
(iserl, iseru)
}
/// Determine contributing line range for hydrogen.
fn determine_lines_hydrogen(
i: usize, ilowhw: usize, m10w: usize, m20w: usize, grav: f64,
) -> (usize, usize) {
let mut m1 = m10w;
if i < ilowhw {
m1 = ilowhw - 1;
}
let mut m2 = m1 + 1;
if m1 < i + 1 {
m1 = i + 1;
}
if grav < 3.0 {
let threshold = match i {
7 => 16,
6 => 14,
5 => 12,
4 => 10,
3 => 8,
2 => 6,
1 => 4,
_ => 0,
};
if m1 <= threshold && (1..=7).contains(&i) {
// Keep m1 as is
} else {
m1 = m1.saturating_sub(1);
m2 = m20w + 3;
}
} else {
m1 = m1.saturating_sub(1);
m2 = m20w + 3;
}
if m1 < i + 1 {
m1 = i + 1;
}
if grav > 3.0 {
m2 += 5;
m1 = m1.saturating_sub(3);
if m1 > i + 6 {
m1 = m1.saturating_sub(3);
}
}
if grav > 6.0 {
m2 += 2;
m1 = m1.saturating_sub(1);
if m1 > i + 6 {
m1 = m1.saturating_sub(1);
}
}
if m1 < i + 1 {
m1 = i + 1;
}
if m2 > 40 {
m2 = 40;
}
(m1, m2)
}
/// Compute transition properties for hydrogen line i→j.
fn transition_hydrogen(
i: usize, j: usize, pj: &[f64; 40], c: &HydliwCommon, nf: usize,
ii: f64, xii: f64, xjj: f64, t1: f64,
) -> (f64, f64) {
let wn_j = wn_val(c.wnhint, j, c.id, nf);
let wn_i = wn_val(c.wnhint, i, c.id, nf);
let mut abtra = pj[i - 1] * wn_j;
let mut emtra = pj[j - 1] * wn_i * ii * xjj * (CPJ * (xii - xjj) * t1).exp();
// Special handling for low i, j (first two series members)
if i <= 2 && j <= i + 2 {
abtra = pj[i - 1];
emtra = pj[j - 1] * wn_i / wn_j * ii * xjj * (CPJ * (xii - xjj) * t1).exp();
}
(abtra, emtra)
}
/// Access WNHINT partition function value.
fn wn_val(wnhint: &[f64], level: usize, id: usize, nf: usize) -> f64 {
if (1..=40).contains(&level) {
let idx = (level - 1) * nf + id;
if idx < wnhint.len() {
return wnhint[idx];
}
}
1.0
}
/// Access WLHYD profile wavelength table value.
fn profile_wl_val_h(wlhyd: &[f64], line_idx: usize, iwl: usize) -> f64 {
let idx = line_idx * 54 + iwl;
if idx < wlhyd.len() { wlhyd[idx] } else { 0.0 }
}
/// Access PRFHYD profile value.
fn profile_prf_val_h(prfhyd: &[f64], line_idx: usize, iwl: usize) -> f64 {
let idx = line_idx * 54 + iwl;
if idx < prfhyd.len() { prfhyd[idx] } else { 0.0 }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_series_range_hydrogen() {
// Default: just the lower level
assert_eq!(series_range_hydrogen(3, 10000.0), (3, 3));
// Near-IR: Paschen + Brackett
assert_eq!(series_range_hydrogen(1, 18000.0), (3, 4));
// Mid-IR: Brackett
assert_eq!(series_range_hydrogen(1, 25000.0), (4, 5));
// Far-IR
assert_eq!(series_range_hydrogen(1, 50000.0), (5, 7));
}
#[test]
fn test_determine_lines_hydrogen_basic() {
// Low gravity, small i
let (m1, m2) = determine_lines_hydrogen(1, 1, 10, 20, 2.0);
assert!(m1 >= 2);
assert!(m2 >= m1);
}
#[test]
fn test_determine_lines_hydrogen_high_grav() {
let (m1, m2) = determine_lines_hydrogen(3, 3, 10, 20, 7.0);
assert!(m1 >= 4);
assert!(m2 <= 40);
}
#[test]
fn test_hydliw_no_hydrogen() {
let nf = 5;
let freq: Vec<f64> = (0..nf).map(|i| 3.0e15 - i as f64 * 1.0e14).collect();
let wlam: Vec<f64> = freq.iter().map(|&f| 2.997925e17 / f).collect();
let wnhint = vec![1.0; 40 * nf];
let wline = vec![0.0; 4 * 22];
let osch = vec![0.0; 4 * 22];
let ilin0 = vec![0i32; 4 * 22];
let params = HydliwParams {
common: HydliwCommon {
id: 0,
t: 10000.0,
ane: 1.0e12,
vturb: 1.0e5,
grav: 4.0,
freq: &freq,
wlam: &wlam,
iath: 0, // No hydrogen
iophli: 1,
ilemke: 0,
pop_h_cont: 1.0e10,
pj: None,
wnhint: &wnhint,
nwlhyd: &[],
prfhyd: &[],
wlhyd: &[],
wline: &wline,
osch: &osch,
ilin0: &ilin0,
nlh: 10,
n0hn: 0,
feautr_params: None,
lasdel: false,
nunalp: 0,
nunbet: 0,
nungam: 0,
nunbal: 0,
allard_data: None,
hneutr: 0.0,
hcharg: 0.0,
nunhhe: 0,
iathe: 0,
pop_he: 0.0,
},
window: HydliwWindowParams {
ihylw: &[1; 5],
ilowhw: &[1; 5],
m10w: &[5; 5],
m20w: &[15; 5],
},
};
let result = hydliw(&params);
assert!(result.absoh.iter().all(|&x| x == 0.0));
assert!(result.emish.iter().all(|&x| x == 0.0));
}
#[test]
fn test_hydliw_basic() {
let nf = 5;
let freq: Vec<f64> = (0..nf).map(|i| 3.0e15 - i as f64 * 1.0e14).collect();
let wlam: Vec<f64> = freq.iter().map(|&f| 2.997925e17 / f).collect();
let wnhint = vec![1.0; 40 * nf];
let wline = vec![0.0; 4 * 22];
let osch = vec![0.0; 4 * 22];
let ilin0 = vec![0i32; 4 * 22];
let params = HydliwParams {
common: HydliwCommon {
id: 0,
t: 20000.0,
ane: 1.0e14,
vturb: 2.0e5,
grav: 4.0,
freq: &freq,
wlam: &wlam,
iath: 1,
iophli: 1,
ilemke: 0,
pop_h_cont: 1.0e10,
pj: None,
wnhint: &wnhint,
nwlhyd: &[],
prfhyd: &[],
wlhyd: &[],
wline: &wline,
osch: &osch,
ilin0: &ilin0,
nlh: 10,
n0hn: 0,
feautr_params: None,
lasdel: false,
nunalp: 0,
nunbet: 0,
nungam: 0,
nunbal: 0,
allard_data: None,
hneutr: 0.0,
hcharg: 0.0,
nunhhe: 0,
iathe: 0,
pop_he: 0.0,
},
window: HydliwWindowParams {
ihylw: &[1; 5],
ilowhw: &[1; 5],
m10w: &[5; 5],
m20w: &[15; 5],
},
};
let result = hydliw(&params);
assert!(result.absoh.iter().all(|&x| x.is_finite()));
assert!(result.emish.iter().all(|&x| x.is_finite()));
}
#[test]
fn test_hydliw_skip_freq() {
let nf = 3;
let freq: Vec<f64> = (0..nf).map(|i| 3.0e15 - i as f64 * 1.0e14).collect();
let wlam: Vec<f64> = freq.iter().map(|&f| 2.997925e17 / f).collect();
let wnhint = vec![1.0; 40 * nf];
let wline = vec![0.0; 4 * 22];
let osch = vec![0.0; 4 * 22];
let ilin0 = vec![0i32; 4 * 22];
let params = HydliwParams {
common: HydliwCommon {
id: 0,
t: 10000.0,
ane: 1.0e12,
vturb: 1.0e5,
grav: 4.0,
freq: &freq,
wlam: &wlam,
iath: 1,
iophli: 1,
ilemke: 0,
pop_h_cont: 1.0e10,
pj: None,
wnhint: &wnhint,
nwlhyd: &[],
prfhyd: &[],
wlhyd: &[],
wline: &wline,
osch: &osch,
ilin0: &ilin0,
nlh: 10,
n0hn: 0,
feautr_params: None,
lasdel: false,
nunalp: 0,
nunbet: 0,
nungam: 0,
nunbal: 0,
allard_data: None,
hneutr: 0.0,
hcharg: 0.0,
nunhhe: 0,
iathe: 0,
pop_he: 0.0,
},
window: HydliwWindowParams {
ihylw: &[-1, 1, -1], // Skip freq 0 and 2
ilowhw: &[1; 3],
m10w: &[5; 3],
m20w: &[15; 3],
},
};
let result = hydliw(&params);
assert_eq!(result.absoh[0], 0.0);
assert_eq!(result.emish[0], 0.0);
assert_eq!(result.absoh[2], 0.0);
assert_eq!(result.emish[2], 0.0);
}
}
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//! 氢线 Stark 展宽表格插值。
//!
//! 重构自 SYNSPEC `HYDTAB` 子程序 (synspec54.f:7074)。
//!
//! 为给定谱线 I→J 和深度点 ID 插值氢线 Stark 展宽表格。
//! 计算修改后的温度(含湍流速度修正)和电子密度,
//! 然后调用 `inthyd` 进行二维插值。
#![allow(clippy::erasing_op)]
use crate::tlusty::math::hydrogen::inthyd;
use crate::tlusty::state::HydPrf;
/// 参数:氢线表格插值
pub struct HydtabParams<'a> {
/// 跃迁下能级 (1-indexed, Fortran 风格)
pub i: i32,
/// 跃迁上能级 (1-indexed, Fortran 风格)
pub j: i32,
/// 深度索引 (1-indexed)
pub id: usize,
/// 温度数组 (K)
pub temp: &'a [f64],
/// 电子密度数组
pub elec: &'a [f64],
/// 湍流速度数组
pub vturb: &'a [f64],
/// 谱线索引表 ILIN0(i,j) → 谱线编号 (1-indexed, 0 = 无此线)
pub ilin0: &'a [i32],
/// ILIN0 行数 (用于 2D 索引)
pub ilin0_nrows: usize,
/// 谱线中心波长 WLINE(i,j) (Å)
pub wline: &'a [f64],
/// WLINE 行数
pub wline_nrows: usize,
/// 每条谱线的波长点数 NWLH(iline)
pub nwli: &'a [i32],
/// 轮廓数据 PRF(iwl, it, ie, iline) — log10 值
pub prf: &'a [f64],
/// PRF 维度: (nwl_max, nt_max, ne_max)
pub prf_dims: (usize, usize, usize),
/// 波长偏移 WLHYD(iline, iwl)
pub wlhyd: &'a [f64],
/// WLHYD 维度: (nwl_max,)
pub wlhyd_nwl_max: usize,
/// 输出: PRFHYD(iline, id, iwl) — 插值后的轮廓
pub prfhyd: &'a mut [f64],
/// PRFHYD 维度: (nlines, ndepth, nwl_max)
pub prfhyd_dims: (usize, usize, usize),
/// 氢线表格数据 (用于 inthyd)
pub hydprf: &'a HydPrf,
/// 静态 XK 系数 (在 id==1 时计算,后续复用)
pub xk: &'a mut f64,
}
/// 氢线表格插值。
///
/// 为谱线 I→J 在深度点 ID 处插值 Stark 展宽表格。
/// 结果存储在 `params.prfhyd` 数组中。
///
/// # Fortran 原始代码
///
/// ```fortran
/// SUBROUTINE HYDTAB(I,J,ID)
/// ```
pub fn hydtab(params: &mut HydtabParams) {
let i = params.i as usize;
let j = params.j as usize;
let id = params.id; // 1-indexed
// 获取谱线索引 (1-indexed, 0 = 无此线)
let idx = (i - 1) * params.ilin0_nrows + (j - 1);
let iline_1 = params.ilin0[idx]; // 1-indexed
if iline_1 == 0 {
return;
}
let iline = (iline_1 - 1) as usize; // 0-indexed
// 获取波长和波长点数
let wl_idx = (i - 1) * params.wline_nrows + (j - 1);
let wl0 = params.wline[wl_idx];
let nwl = params.nwli[iline] as usize;
// 计算渐近轮廓系数 (仅在第一个深度点)
if id == 1 {
// PRF(NWL, 1, 1, ILINE) — 注意 Fortran 1-indexed
let prf_idx = (nwl - 1) * params.prf_dims.1 * params.prf_dims.2
+ 0 * params.prf_dims.2;
let prf_val = if prf_idx < params.prf.len() {
params.prf[prf_idx]
} else {
0.0
};
// WLHYD(ILINE, NWL)
let wlhyd_idx = iline * params.wlhyd_nwl_max + (nwl - 1);
let wlhyd_val = if wlhyd_idx < params.wlhyd.len() {
params.wlhyd[wlhyd_idx]
} else {
0.0
};
let xclog = prf_val + 2.5 * wlhyd_val - 0.477121;
let xklog = 0.6666667 * xclog;
*params.xk = (xklog * std::f64::consts::LN_10).exp();
}
let xk = *params.xk;
// 修改温度以考虑湍流速度对 Doppler 宽度的影响
let id0 = id - 1; // 0-indexed
let t = params.temp[id0] + 6.06e-9 * params.vturb[id0];
let ane = params.elec[id0];
let tl = t.log10();
let anel = ane.log10();
// Stark 参数
let f00 = 1.25e-9 * ane.powf(0.666666667);
let fxk = f00 * xk;
let dop = 1.0e8 / wl0 * (1.65e8 * t).sqrt();
let dbeta = wl0 * wl0 / 2.997925e18 / fxk;
let _betad = dbeta * dop;
// 对每个波长点调用 INTHYD 插值
for iwl in 0..nwl {
let prof = inthyd(tl, anel, iwl, iline, params.hydprf, dbeta, xk);
// PRFHYD(ILINE, ID, IWL) — 存储结果
let prfhyd_idx = iline * params.prfhyd_dims.1 * params.prfhyd_dims.2
+ (id - 1) * params.prfhyd_dims.2
+ iwl;
if prfhyd_idx < params.prfhyd.len() {
params.prfhyd[prfhyd_idx] = prof;
}
}
}
#[cfg(test)]
mod tests {
use super::*;
use crate::tlusty::state::HydPrf;
fn create_test_params() -> (HydPrf, Vec<f64>, Vec<f64>) {
let mut hydprf = HydPrf::default();
hydprf.nth[0] = 7;
hydprf.neh[0] = 20;
for it in 0..7 {
hydprf.xtlem[it] = 4.0 + it as f64 * 0.1;
}
for ie in 0..20 {
hydprf.xnelem[ie] = 12.0 + ie as f64 * 0.2;
}
for iwl in 0..90 {
hydprf.wlh[iwl] = 4000.0 + iwl as f64 * 10.0;
}
for it in 0..7 {
for ie in 0..20 {
hydprf.set_prfhyd(0, 0, it, ie, -2.0 + it as f64 * 0.1 + ie as f64 * 0.01);
}
}
let mut prf = vec![0.0; 90 * 7 * 20];
for iwl in 0..90 {
for it in 0..7 {
for ie in 0..20 {
let idx = iwl * 7 * 20 + it * 20 + ie;
prf[idx] = -2.0 + it as f64 * 0.1 + ie as f64 * 0.01;
}
}
}
let mut wlhyd = vec![0.0; 90];
for iwl in 0..90 {
wlhyd[iwl] = 0.01 * (iwl + 1) as f64;
}
(hydprf, prf, wlhyd)
}
#[test]
fn test_hydtab_no_line() {
let (hydprf, prf, wlhyd) = create_test_params();
let temp = vec![10000.0, 9000.0];
let elec = vec![1e13, 1e13];
let vturb = vec![1e5, 1e5];
let ilin0 = vec![0i32; 4]; // 2x2, all zero = no line
let wline = vec![1215.67; 4];
let nwlh = vec![90i32];
let mut prfhyd = vec![0.0; 1 * 2 * 90];
let mut xk = 0.0;
let mut params = HydtabParams {
i: 1,
j: 2,
id: 1,
temp: &temp,
elec: &elec,
vturb: &vturb,
ilin0: &ilin0,
ilin0_nrows: 2,
wline: &wline,
wline_nrows: 2,
nwli: &nwlh,
prf: &prf,
prf_dims: (90, 7, 20),
wlhyd: &wlhyd,
wlhyd_nwl_max: 90,
prfhyd: &mut prfhyd,
prfhyd_dims: (1, 2, 90),
hydprf: &hydprf,
xk: &mut xk,
};
hydtab(&mut params);
// ilin0 = 0, should return immediately
assert_eq!(prfhyd[0], 0.0);
}
#[test]
fn test_hydtab_basic() {
let (hydprf, prf, wlhyd) = create_test_params();
let temp = vec![10000.0, 9000.0];
let elec = vec![1e13, 1e13];
let vturb = vec![1e5, 1e5];
let ilin0 = vec![1i32; 4]; // 2x2, line index = 1
let wline = vec![1215.67; 4];
let nwlh = vec![90i32];
let mut prfhyd = vec![0.0; 1 * 2 * 90];
let mut xk = 0.0;
let mut params = HydtabParams {
i: 1,
j: 2,
id: 1,
temp: &temp,
elec: &elec,
vturb: &vturb,
ilin0: &ilin0,
ilin0_nrows: 2,
wline: &wline,
wline_nrows: 2,
nwli: &nwlh,
prf: &prf,
prf_dims: (90, 7, 20),
wlhyd: &wlhyd,
wlhyd_nwl_max: 90,
prfhyd: &mut prfhyd,
prfhyd_dims: (1, 2, 90),
hydprf: &hydprf,
xk: &mut xk,
};
hydtab(&mut params);
// xk should have been computed (id == 1)
assert!(xk > 0.0);
// prfhyd should have been filled with finite values
let has_nonzero = prfhyd.iter().any(|&v| v != 0.0);
assert!(has_nonzero);
}
}
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//! SYNSPEC 氢线窗口初始化。
//!
//! 重构自 SYNSPEC 54 的 HYLSEW 子程序。
/// 氢线窗口参数
#[derive(Debug, Clone)]
pub struct HylsewOutput {
/// 是否包含氢线 (0=否, 1=是)
pub ihylw: i32,
/// 线数参数
pub m20w: i32,
/// 最低主量子数索引
pub ilowhw: i32,
/// 线翼参数
pub m10w: i32,
}
/// 初始化氢线处理窗口。
///
/// 根据频率和重力加速度判断是否包含氢线,并设置相关参数。
///
/// # Arguments
/// * `ij` - 频率索引
/// * `freq` - 频率值 (Hz)
/// * `grav` - 重力加速度 (log g)
///
/// # Returns
/// 氢线窗口参数
pub fn hylsew(_ij: usize, freq: f64, grav: f64) -> HylsewOutput {
let mut output = HylsewOutput {
ihylw: 0,
m20w: 0,
ilowhw: 0,
m10w: 0,
};
// 检查频率是否在氢线范围内
if freq >= 3.28805e15 {
return output;
}
let al0 = 2.997925e17 / freq;
let al1 = al0;
// 根据重力加速度检查波长范围
if grav < 6.0 {
if al0 > 160.0 && al1 < 364.6 {
return output;
}
if al0 > 506.0 && al1 < 630.0 {
return output;
}
if al0 > 680.0 && al1 < 820.3 {
return output;
}
} else {
if al0 > 540.0 && al1 < 600.0 {
return output;
}
if al0 > 720.0 && al1 < 820.3 {
return output;
}
}
// 包含氢线
output.ihylw = 1;
output.m20w = 40;
// 确定最低主量子数
let frion = if al1 < 364.6 {
output.ilowhw = 1;
3.28805e15
} else if al1 < 820.0 {
output.ilowhw = 2;
8.2225e14
} else if al1 < 1458.0 {
output.ilowhw = 3;
3.6544142e14
} else if al1 < 2278.0 {
output.ilowhw = 4;
2.0555837e14
} else if al1 < 3281.0 {
output.ilowhw = 5;
1.315589e14
} else if al1 < 4466.0 {
output.ilowhw = 6;
9.136394e13
} else {
output.ilowhw = 7;
6.7120228e13
};
// 计算线翼参数
if frion > freq {
output.m10w = (3.289017e15 / (frion - freq).abs()).sqrt() as i32;
}
output
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_hylsew_high_freq() {
// 频率太高,不包含氢线
let result = hylsew(1, 4.0e15, 4.0);
assert_eq!(result.ihylw, 0);
}
#[test]
fn test_hylsew_lyman_region() {
// Lyman 系区域
let result = hylsew(1, 3.0e15, 4.0);
assert_eq!(result.ihylw, 1);
assert_eq!(result.ilowhw, 1);
}
#[test]
fn test_hylsew_balmer_region() {
// Balmer 系区域 (500 Å,在 Lyman 极限和 Balmer 极限之间)
let freq = 2.997925e17 / 500.0;
let result = hylsew(1, freq, 4.0);
assert_eq!(result.ihylw, 1);
assert_eq!(result.ilowhw, 2);
}
#[test]
fn test_hylsew_high_gravity() {
// 高重力情况
let freq = 2.997925e17 / 550.0;
let result = hylsew(1, freq, 7.0);
assert_eq!(result.ihylw, 0);
}
}
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//! Output of selected molecular line parameters (identification table).
//!
//! Translated from SYNSPEC54.FOR subroutine IDMTAB (line 16380).
//!
//! Computes and formats molecular line parameters for the identification
//! table output, including equivalent widths and line strengths.
use crate::synspec::math::inibla::CL;
// ============================================================================
// Constants
// ============================================================================
/// Conversion factor: ln(10) for log-gf
const C1: f64 = std::f64::consts::LN_10;
/// Conversion factor: gf offset
const C2: f64 = 4.201_467_2;
/// Conversion factor: energy to temperature
const C3: f64 = 1.438_788_6;
/// Strength category labels
const APB: &str = " ";
const AP0: &str = " .";
const AP1: &str = " *";
const AP2: &str = " **";
const AP3: &str = " ***";
const AP4: &str = "****";
// ============================================================================
// IDMTAB parameters
// ============================================================================
/// Parameters for a single molecular line.
pub struct IdmtabLine {
/// Wavelength (Å)
pub alam: f64,
/// Molecule index
pub imol: usize,
/// Lower excitation potential (cm⁻¹)
pub excl: f64,
/// Log gf value
pub gfm: f64,
/// Van der Waals broadening
pub grm: f64,
/// Stark broadening
pub gsm: f64,
/// Van der Waals broadening (depth-dependent)
pub gvdw: f64,
/// Doppler width
pub dop1: f64,
/// Continuum opacity at line center
pub absta: f64,
/// Stimulated emission factor
pub stim: f64,
/// Molecular population ratio
pub rrmol: f64,
/// Temperature at standard depth (K)
pub temp: f64,
/// Electron density at standard depth
pub elec: f64,
}
/// Result of IDMTAB computation for a single line.
pub struct IdmtabResult {
/// Wavelength (Å)
pub alam: f64,
/// Molecule name
pub molecule: String,
/// Log gf
pub gf: f64,
/// Lower excitation energy (K)
pub excl_k: f64,
/// Line-to-continuum ratio (STR0)
pub str0: f64,
/// Equivalent width (mÅ)
pub eqw: f64,
/// Strength category label
pub apr: &'static str,
/// Depth index
pub id: usize,
/// Total broadening parameter
pub agam: f64,
}
// ============================================================================
// IDMTAB implementation
// ============================================================================
/// Compute molecular line parameters for the identification table.
///
/// For a given molecular line, computes the line strength, equivalent width,
/// and strength category.
///
/// # Fortran original
///
/// ```fortran
/// SUBROUTINE IDMTAB
/// DO IL0=1,NLINML
/// ...compute STR0, EQW, APR...
/// END DO
/// END
/// ```
pub fn idmtab_compute(line: &IdmtabLine) -> IdmtabResult {
let IdmtabLine {
alam, imol: _, excl, gfm, grm, gsm, gvdw,
dop1, absta, stim, rrmol, temp, elec,
} = *line;
// Total broadening parameter
// Fortran: AGAM=(GRM+GSM*ANE+GVDW)*DOP1
let agam = (grm + gsm * elec + gvdw) * dop1;
// Absorption at line center
// Fortran: ABCNT=EXP(GFM-EXCL/TEMP)*RRMOL*DOP1*STIM
let abcnt = (gfm - excl / temp).exp() * rrmol * dop1 * stim;
// Line-to-continuum ratio
// Fortran: STR0=ABCNT/ABSTA
let str0 = if absta > 0.0 { abcnt / absta } else { 0.0 };
// Log gf
let gf = (gfm + C2) / C1;
// Lower excitation energy in K
let excl_k = excl / C3;
// Equivalent width estimate
let ww1 = if str0 <= 1.2 {
0.886 * str0 * (1.0 - str0 * (0.707 - str0 * 0.577))
} else {
str0.ln().sqrt()
};
let ww1 = if str0 > 55.0 {
let ww2 = 0.5 * (std::f64::consts::PI * agam * str0).sqrt();
if ww2 > ww1 { ww2 } else { ww1 }
} else {
ww1
};
// Equivalent width in mÅ
// Fortran: EQW=ALAM/FREQ0*1.E3/DOP1*WW1
// Since ALAM is wavelength and we don't have FREQ0 directly,
// we use the relation: EQW ≈ ALAM * WW1 / (c/ALAM) / DOP1 * 1e3
// Simplified: EQW = ALAM^2 / CL * 1e3 / DOP1 * WW1
let eqw = alam * alam / CL * 1e3 / dop1 * ww1;
// Strength category
let str = eqw * 10.0;
let apr = if str >= 1e4 {
AP4
} else if str >= 1e3 {
AP3
} else if str >= 1e2 {
AP2
} else if str >= 1e1 {
AP1
} else if str >= 1e0 {
AP0
} else {
APB
};
IdmtabResult {
alam,
molecule: String::new(), // Filled by caller
gf,
excl_k,
str0,
eqw,
apr,
id: 0, // Filled by caller
agam,
}
}
#[cfg(test)]
mod tests {
use super::*;
fn create_test_line() -> IdmtabLine {
IdmtabLine {
alam: 5000.0,
imol: 1,
excl: 10000.0,
gfm: -2.0,
grm: 0.1,
gsm: 0.01,
gvdw: 0.05,
dop1: 0.01,
absta: 1e-10,
stim: 1.0,
rrmol: 1e-5,
temp: 10000.0,
elec: 1e14,
}
}
#[test]
fn test_idmtab_basic() {
let line = create_test_line();
let result = idmtab_compute(&line);
assert!(result.alam > 0.0);
assert!(result.str0.is_finite());
assert!(result.eqw.is_finite());
assert!(result.eqw >= 0.0);
assert!(result.agam.is_finite());
}
#[test]
fn test_idmtab_weak_line() {
let mut line = create_test_line();
line.rrmol = 1e-20; // Very weak line
let result = idmtab_compute(&line);
// Weak line should have small STR0
assert!(result.str0 < 1.0);
assert_eq!(result.apr, APB);
}
#[test]
fn test_idmtab_strong_line() {
let mut line = create_test_line();
line.rrmol = 1e10; // Very strong line
line.absta = 1e-20;
let result = idmtab_compute(&line);
// Strong line should have large STR0
assert!(result.str0 > 1.0);
}
#[test]
fn test_idmtab_strength_categories() {
// Test that different strength values produce correct categories
let mut line = create_test_line();
// Weak line
line.rrmol = 1e-15;
let r = idmtab_compute(&line);
if r.str0 <= 1.2 {
// For weak lines, EQW is small
assert!(r.eqw < 1.0 || r.apr == APB);
}
}
}
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//! Output of selected atomic line parameters (identification table).
//!
//! Translated from SYNSPEC54.FOR subroutine IDTAB (line 9636).
//!
//! Computes and formats atomic line parameters for the identification
//! table output, including equivalent widths and line strengths.
use crate::synspec::math::inibla::CL;
// ============================================================================
// Constants
// ============================================================================
/// Conversion factor: ln(10) for log-gf
const C1: f64 = std::f64::consts::LN_10;
/// Conversion factor: gf offset
const C2: f64 = 4.201_467_2;
/// Conversion factor: energy to temperature
const C3: f64 = 1.438_788_6;
/// Ionization stage labels
const TYPION: [&str; 30] = [
" I ", " II ", " III", " IV ", " V ",
" VI ", " VII", "VIII", " IX ", " X ",
" XI ", " XII", "XIII", " XIV", " XV ",
" XVI", "XVII", " 18 ", " XIX", " XX ",
" XXI", "XXII", " 23 ", "XXIV", "XXV ",
"XXVI", " 27 ", " 28 ", "XXIX", " XXX",
];
/// Strength category labels
const APB: &str = " ";
const AP0: &str = " .";
const AP1: &str = " *";
const AP2: &str = " **";
const AP3: &str = " ***";
const AP4: &str = "****";
// ============================================================================
// IDTAB parameters
// ============================================================================
/// Parameters for a single atomic line.
pub struct IdtabLine {
/// Line index
pub il: usize,
/// Wavelength (Å)
pub alam: f64,
/// Atom index
pub iat: usize,
/// Ionization stage (1-based)
pub ion: usize,
/// Lower excitation potential (cm⁻¹)
pub excl: f64,
/// Log gf value
pub gf0: f64,
/// Doppler width
pub dop1: f64,
/// Continuum opacity at line center
pub absta: f64,
/// Stimulated emission factor
pub stim: f64,
/// Population ratio RRR
pub rrr: f64,
/// Total broadening parameter (from PROFIL)
pub agam: f64,
/// Temperature at standard depth (K)
pub temp: f64,
/// Standard depth index
pub idstd: usize,
/// Reference depth index
pub id: usize,
/// Lower level index
pub ilown: usize,
/// Upper level index
pub iupn: usize,
/// First level index for the element
pub nfirst: usize,
/// Element index for the lower level
pub iel: usize,
}
/// Result of IDTAB computation for a single line.
pub struct IdtabResult {
/// Wavelength (Å)
pub alam: f64,
/// Atom name
pub atom: String,
/// Ionization stage label
pub ion_label: &'static str,
/// Log gf
pub gf: f64,
/// Lower excitation energy (K)
pub excl_k: f64,
/// Line-to-continuum ratio (STR0)
pub str0: f64,
/// Equivalent width (mÅ)
pub eqw: f64,
/// Strength category label
pub apr: &'static str,
/// Lower level index (relative)
pub ill: usize,
/// Upper level index (relative)
pub ilu: usize,
/// Depth index
pub id: usize,
}
// ============================================================================
// IDTAB implementation
// ============================================================================
/// Compute atomic line parameters for the identification table.
///
/// For a given atomic line, computes the line strength, equivalent width,
/// and strength category.
///
/// # Fortran original
///
/// ```fortran
/// SUBROUTINE IDTAB
/// DO IL0=1,NLIN
/// ...compute STR0, EQW, APR...
/// END DO
/// END
/// ```
pub fn idtab_compute(line: &IdtabLine) -> IdtabResult {
let IdtabLine {
il: _, alam, iat: _, ion, excl, gf0, dop1, absta, stim, rrr,
agam, temp, idstd: _, id, ilown, iupn, nfirst, iel: _,
} = *line;
// Absorption at line center
// Fortran: ABCNT=EXP(GF0-EXCL/TEMP)*RRR*STIM
let abcnt = (gf0 - excl / temp).exp() * rrr * stim;
// Line-to-continuum ratio
// Fortran: STR0=ABCNT*DOP1/ABSTA
let str0 = if absta > 0.0 {
abcnt * dop1 / absta
} else {
0.0
};
// Log gf
let gf = (gf0 + C2) / C1;
// Lower excitation energy in K
let excl_k = excl / C3;
// Equivalent width estimate
let ww1 = if str0 <= 1.2 {
0.886 * str0 * (1.0 - str0 * (0.707 - str0 * 0.577))
} else {
str0.ln().sqrt()
};
let ww1 = if str0 > 55.0 {
let ww2 = 0.5 * (std::f64::consts::PI * agam * str0).sqrt();
if ww2 > ww1 { ww2 } else { ww1 }
} else {
ww1
};
// Equivalent width in mÅ
// Fortran: EQW=ALAM/FREQ0*1.E3/DOP1*WW1
// FREQ0 = CL/ALAM, so EQW = ALAM^2/CL * 1e3 / DOP1 * WW1
let eqw = alam * alam / CL * 1e3 / dop1 * ww1;
// Strength category
let str = eqw * 10.0;
let apr = if str >= 1e4 {
AP4
} else if str >= 1e3 {
AP3
} else if str >= 1e2 {
AP2
} else if str >= 1e1 {
AP1
} else if str >= 1e0 {
AP0
} else {
APB
};
// Relative level indices
let ill = if ilown > 0 { ilown - nfirst + 1 } else { 0 };
let ilu = if iupn > 0 { iupn - nfirst + 1 } else { 0 };
// Ionization stage label (1-based index)
let ion_label = if (1..=30).contains(&ion) {
TYPION[ion - 1]
} else {
" ?? "
};
IdtabResult {
alam,
atom: String::new(), // Filled by caller
ion_label,
gf,
excl_k,
str0,
eqw,
apr,
ill,
ilu,
id,
}
}
#[cfg(test)]
mod tests {
use super::*;
fn create_test_line() -> IdtabLine {
IdtabLine {
il: 1,
alam: 5000.0,
iat: 1,
ion: 1,
excl: 10000.0,
gf0: -1.0,
dop1: 0.01,
absta: 1e-10,
stim: 1.0,
rrr: 1e-3,
agam: 0.1,
temp: 10000.0,
idstd: 35,
id: 35,
ilown: 1,
iupn: 5,
nfirst: 1,
iel: 1,
}
}
#[test]
fn test_idtab_basic() {
let line = create_test_line();
let result = idtab_compute(&line);
assert!(result.alam > 0.0);
assert!(result.str0.is_finite());
assert!(result.eqw.is_finite());
assert!(result.eqw >= 0.0);
assert!(result.alam.is_finite());
assert_eq!(result.ion_label, " I ");
}
#[test]
fn test_idtab_ion_labels() {
let mut line = create_test_line();
line.ion = 1;
assert_eq!(idtab_compute(&line).ion_label, " I ");
line.ion = 2;
assert_eq!(idtab_compute(&line).ion_label, " II ");
line.ion = 26;
assert_eq!(idtab_compute(&line).ion_label, "XXVI");
}
#[test]
fn test_idtab_level_indices() {
let mut line = create_test_line();
line.ilown = 10;
line.iupn = 15;
line.nfirst = 8;
let result = idtab_compute(&line);
assert_eq!(result.ill, 3); // 10 - 8 + 1
assert_eq!(result.ilu, 8); // 15 - 8 + 1
}
#[test]
fn test_idtab_weak_line() {
let mut line = create_test_line();
line.rrr = 1e-20;
let result = idtab_compute(&line);
assert!(result.str0 < 1.0);
}
}
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//! ingrid — 不透明度网格计算的状态参数设置。
//!
//! Fortran 原始签名: SUBROUTINE INGRID(MODE,INEXT,IGRD)
//!
//! 设置不透明度表计算的温度和密度网格。
//!
//! 注意: Fortran 版本直接操作文件 I/O 和 COMMON 块。
//! Rust 版本提供纯计算核心函数。
/// 密度参数类型
#[derive(Debug, Clone, Copy, PartialEq)]
pub enum DensityParameterType {
/// 电子密度
ElectronDensity = 0,
/// 质量密度 (idens < 10)
MassDensity = 1,
/// 可变密度 (idens >= 20)
Variable = 2,
}
/// 不透明度网格参数
#[derive(Debug, Clone)]
pub struct OpacityGridParams {
/// 最低温度 (K)
pub temp1: f64,
/// 最高温度 (K)
pub temp2: f64,
/// 温度点数
pub ntemp: usize,
/// 密度参数类型
pub dens_type: DensityParameterType,
/// 最低密度
pub dens1: f64,
/// 最高密度
pub dens2: f64,
/// 密度点数
pub ndens: usize,
/// 频率点数
pub nfgrid: usize,
/// 最短波长 (nm)
pub wlam1: f64,
/// 最长波长 (nm)
pub wlam2: f64,
}
/// 生成对数等距温度网格
///
/// Fortran 原始逻辑:
/// ```fortran
/// at1=log(temp1)
/// at2=log(temp2)
/// dt=(at2-at1)/(ntemp-1)
/// do i=1,ntemp
/// tempg(i)=exp(at1+(i-1)*dt)
/// end do
/// ```
pub fn generate_temperature_grid(temp1: f64, temp2: f64, ntemp: usize) -> Vec<f64> {
if temp1 <= 0.0 {
return vec![temp1; ntemp];
}
let at1 = temp1.ln();
let at2 = temp2.ln();
let dt = if ntemp > 1 { (at2 - at1) / (ntemp - 1) as f64 } else { 0.0 };
(0..ntemp)
.map(|i| (at1 + i as f64 * dt).exp())
.collect()
}
/// 生成对数等距密度网格(均匀分布)
///
/// Fortran 原始逻辑:
/// ```fortran
/// at1=log(dens1)
/// at2=log(dens2)
/// dr=(at2-at1)/(ndens-1)
/// do i=1,ntemp
/// do j=1,ndens
/// densg(i,j)=exp(at1+(j-1)*dr)
/// end do
/// end do
/// ```
pub fn generate_density_grid_uniform(
dens1: f64,
dens2: f64,
ndens: usize,
ntemp: usize,
) -> Vec<Vec<f64>> {
let at1 = dens1.ln();
let at2 = dens2.ln();
let dr = if ndens > 1 { (at2 - at1) / (ndens - 1) as f64 } else { 0.0 };
(0..ntemp)
.map(|_| {
(0..ndens)
.map(|j| (at1 + j as f64 * dr).exp())
.collect()
})
.collect()
}
/// 生成可变密度网格(密度范围随温度变化)
///
/// Fortran 原始逻辑:
/// ```fortran
/// do i=1,ntemp
/// dens1=rhol1+(rhou1-rhol1)/(at2-at1)*(templ(i)-at1)
/// dens2=rhol2+(rhou2-rhol2)/(at2-at1)*(templ(i)-at1)
/// dr=(dens2-dens1)/(ndens-1)
/// do j=1,ndens
/// densg(i,j)=exp(dens1+(j-1)*dr)
/// end do
/// end do
/// ```
pub fn generate_density_grid_variable(
temp_grid: &[f64],
dens_lower: (f64, f64), // (at_low_T, at_high_T)
dens_upper: (f64, f64), // (at_low_T, at_high_T)
ndens: usize,
) -> Vec<Vec<f64>> {
let ntemp = temp_grid.len();
if ntemp == 0 {
return Vec::new();
}
let at1 = temp_grid[0].ln();
let at2 = temp_grid[ntemp - 1].ln();
let dt_range = at2 - at1;
let rhol1 = dens_lower.0.ln();
let rhol2 = dens_lower.1.ln();
let rhou1 = dens_upper.0.ln();
let rhou2 = dens_upper.1.ln();
(0..ntemp)
.map(|i| {
let templ_i = temp_grid[i].ln();
let frac = if dt_range.abs() > 1e-30 {
(templ_i - at1) / dt_range
} else {
0.0
};
let dens1 = rhol1 + (rhou1 - rhol1) * frac;
let dens2 = rhol2 + (rhou2 - rhol2) * frac;
let dr = if ndens > 1 { (dens2 - dens1) / (ndens - 1) as f64 } else { 0.0 };
(0..ndens)
.map(|j| (dens1 + j as f64 * dr).exp())
.collect()
})
.collect()
}
/// 从模型大气设置网格(温度和密度来自模型)
///
/// Fortran 原始逻辑:
/// ```fortran
/// call inpmod
/// ntemp=nd
/// ndens=1
/// do it=1,ntemp
/// tempg(it)=temp(it)
/// densg0(it)=dens(it)
/// densg(it,1)=dens(it)
/// elecm(it)=elec(it)
/// end do
/// ```
pub fn set_grid_from_model(
temps: &[f64],
dens: &[f64],
elec: &[f64],
) -> (Vec<f64>, Vec<f64>, Vec<Vec<f64>>, Vec<f64>) {
let _ntemp = temps.len();
let tempg = temps.to_vec();
let densg0 = dens.to_vec();
let densg = dens.iter().map(|&d| vec![d]).collect();
let elecm = elec.to_vec();
(tempg, densg0, densg, elecm)
}
/// 不透明度表插值结果
#[derive(Debug, Clone)]
pub struct InterpolatedOpacity {
/// 波长网格 (nm)
pub wavelengths: Vec<f64>,
/// 不透明度(对数)
pub log_opacity: Vec<f64>,
}
/// 对数空间平均插值
///
/// Fortran 原始逻辑:
/// ```fortran
/// if(isum.gt.0) then
/// abgrd(ijgrd)=log(sum/float(isum))
/// ```
pub fn log_average_interpolation(
wltab: &[f64],
absop: &[f64],
wlgrid: &[f64],
) -> Vec<f64> {
let nfgrid = wlgrid.len();
let nfr = wltab.len();
let mut abgrd = vec![0.0; nfgrid];
let mut ij = 0;
for ijgrd in 0..nfgrid {
let wlgr = if ijgrd + 1 < nfgrid {
0.5 * (wlgrid[ijgrd] + wlgrid[ijgrd + 1])
} else {
wlgrid[ijgrd]
};
let mut sum = 0.0_f64;
let mut isum = 0;
while ij < nfr && wltab[ij] <= wlgr {
sum += absop[ij].exp();
isum += 1;
ij += 1;
}
if isum > 0 {
abgrd[ijgrd] = (sum / isum as f64).ln();
} else if ij < nfr {
// 线性插值
let abl = absop[ij];
let wlt = wltab[ij];
if ij + 1 < nfr {
let abl_next = absop[ij + 1];
let wlt_next = wltab[ij + 1];
abgrd[ijgrd] = abl + (abl_next - abl) / (wlt_next - wlt) * (wlgr - wlt);
} else {
abgrd[ijgrd] = abl;
}
}
}
// 最后一个点复制前一个
if nfgrid > 1 {
abgrd[nfgrid - 1] = abgrd[nfgrid - 2];
}
abgrd
}
/// 网格遍历状态
#[derive(Debug, Clone)]
pub struct GridTraversalState {
/// 当前温度索引
pub indext: usize,
/// 当前密度索引
pub indexn: usize,
/// 是否还有下一个网格点
pub inext: bool,
}
/// 编排函数: 不透明度网格初始化和推进。
///
/// Fortran 原始逻辑: SUBROUTINE INGRID(MODE,INEXT,IGRD)
///
/// # 模式
/// - `mode=0`: 初始化 — 读取网格参数,设置温度/密度网格
/// - `mode=1`: 推进 — 存储当前结果,推进到下一个网格点
pub struct IngridParams<'a> {
/// 模式 (0=init, 1=advance)
pub mode: i32,
/// 网格参数 (mode=0 时使用)
pub grid_params: Option<&'a OpacityGridParams>,
/// 温度网格 (mode=1 时使用)
pub temperatures: &'a [f64],
/// 密度网格 (mode=1 时使用)
pub densities: &'a [Vec<f64>],
/// 每温度点密度数 (mode=1 时使用)
pub nden: &'a [usize],
/// 当前不透明度数据 (mode=1 时使用)
pub absop: &'a [f64],
/// 当前波长表 (mode=1 时使用)
pub wltab: &'a [f64],
/// 目标波长网格 (mode=1 时使用)
pub wlgrid: &'a [f64],
/// 插值模式 (0=average, 1=intrp)
pub inttab: i32,
}
pub struct IngridResult {
/// 是否还有下一个网格点
pub inext: bool,
/// 温度网格
pub tempg: Vec<f64>,
/// 密度网格 [temp_idx][dens_idx]
pub densg: Vec<Vec<f64>>,
/// 电子密度网格 [temp_idx][dens_idx]
pub elecgr: Vec<Vec<f64>>,
/// 插值后的不透明度 (对数)
pub abgrd: Vec<f64>,
/// 当前温度索引
pub indext: usize,
/// 当前密度索引
pub indexn: usize,
}
pub fn ingrid(params: &IngridParams) -> IngridResult {
if params.mode == 0 {
// Initialization mode
let gp = params.grid_params.unwrap();
let tempg = generate_temperature_grid(gp.temp1, gp.temp2, gp.ntemp);
let densg = match gp.dens_type {
DensityParameterType::ElectronDensity | DensityParameterType::MassDensity => {
generate_density_grid_uniform(gp.dens1, gp.dens2, gp.ndens, gp.ntemp)
}
DensityParameterType::Variable => {
// Variable density: use provided dens1/dens2 as bounds
generate_density_grid_uniform(gp.dens1, gp.dens2, gp.ndens, gp.ntemp)
}
};
let elecgr = vec![vec![0.0; gp.ndens]; gp.ntemp];
IngridResult {
inext: gp.ntemp > 1 || gp.ndens > 1,
tempg,
densg,
elecgr,
abgrd: vec![0.0; gp.nfgrid],
indext: 0,
indexn: 0,
}
} else {
// Advance mode: interpolate opacity and move to next grid point
let ntemp = params.temperatures.len();
let nden = params.nden;
// Interpolate opacity to grid
let abgrd = if params.inttab == 1 {
log_average_interpolation(params.wltab, params.absop, params.wlgrid)
} else {
log_average_interpolation(params.wltab, params.absop, params.wlgrid)
};
// Advance grid state
let mut state = GridTraversalState {
indext: 0,
indexn: 0,
inext: true,
};
advance_grid_point(&mut state, ntemp, nden);
IngridResult {
inext: state.inext,
tempg: params.temperatures.to_vec(),
densg: params.densities.to_vec(),
elecgr: vec![vec![0.0; nden.len()]; ntemp],
abgrd,
indext: state.indext,
indexn: state.indexn,
}
}
}
/// 推进到下一个网格点
///
/// Fortran 原始逻辑 (1-indexed):
/// ```fortran
/// if(indexn.lt.ndens) then
/// indexn=indexn+1
/// inext=1
/// else
/// indexn=1
/// if(indext.lt.ntemp) then
/// indext=indext+1
/// inext=1
/// else
/// inext=0
/// end if
/// end if
/// ```
///
/// Rust 版本使用 0-indexed: indexn 从 0 到 ndens-1
pub fn advance_grid_point(
state: &mut GridTraversalState,
ntemp: usize,
ndens: &[usize],
) {
let current_ndens = ndens[state.indext];
if state.indexn < current_ndens - 1 {
// 还有更多密度点
state.indexn += 1;
state.inext = true;
} else {
// 当前温度的所有密度点完成
state.indexn = 0;
if state.indext < ntemp - 1 {
// 还有更多温度点
state.indext += 1;
state.inext = true;
} else {
// 所有网格点完成
state.inext = false;
}
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_generate_temperature_grid() {
let grid = generate_temperature_grid(5000.0, 50000.0, 10);
assert_eq!(grid.len(), 10);
assert!((grid[0] - 5000.0).abs() < 1e-10);
assert!((grid[9] - 50000.0).abs() < 1e-3);
// 对数等距
let ratio = grid[1] / grid[0];
for i in 1..9 {
assert!((grid[i + 1] / grid[i] - ratio).abs() < 1e-10);
}
}
#[test]
fn test_generate_temperature_grid_negative() {
let grid = generate_temperature_grid(-1.0, 50000.0, 5);
assert_eq!(grid.len(), 5);
// temp1 <= 0 → 所有值为 temp1
for &t in &grid {
assert_eq!(t, -1.0);
}
}
#[test]
fn test_generate_density_grid_uniform() {
let grid = generate_density_grid_uniform(1e-10, 1e-6, 5, 3);
assert_eq!(grid.len(), 3);
assert_eq!(grid[0].len(), 5);
assert!((grid[0][0] - 1e-10).abs() < 1e-20);
assert!((grid[0][4] - 1e-6).abs() < 1e-15);
// 所有温度的密度网格相同
assert_eq!(grid[0], grid[1]);
assert_eq!(grid[1], grid[2]);
}
#[test]
fn test_generate_density_grid_variable() {
let temps = vec![5000.0, 10000.0, 20000.0];
let grid = generate_density_grid_variable(
&temps,
(1e-10, 1e-8), // 低端密度随温度变化
(1e-6, 1e-4), // 高端密度随温度变化
5,
);
assert_eq!(grid.len(), 3);
assert_eq!(grid[0].len(), 5);
// 低温的密度范围不同于高温
assert!(grid[0][0] != grid[2][0]);
}
#[test]
fn test_set_grid_from_model() {
let temps = vec![5000.0, 10000.0];
let dens = vec![1e-8, 1e-7];
let elec = vec![1e-10, 1e-9];
let (tempg, densg0, densg, elecm) = set_grid_from_model(&temps, &dens, &elec);
assert_eq!(tempg, temps);
assert_eq!(densg0, dens);
assert_eq!(elecm, elec);
assert_eq!(densg.len(), 2);
assert_eq!(densg[0], vec![1e-8]);
}
#[test]
fn test_log_average_interpolation() {
let wltab = vec![100.0, 200.0, 300.0, 400.0, 500.0];
let absop = vec![0.0, 1.0, 2.0, 1.0, 0.0];
let wlgrid = vec![150.0, 250.0, 350.0, 450.0];
let result = log_average_interpolation(&wltab, &absop, &wlgrid);
assert_eq!(result.len(), 4);
// 所有值应该是有限的
for &v in &result {
assert!(v.is_finite());
}
}
#[test]
fn test_advance_grid_point() {
let mut state = GridTraversalState {
indext: 0,
indexn: 0,
inext: true,
};
let ndens = vec![3, 3, 3];
// 第一次推进: indexn 0 → 1
advance_grid_point(&mut state, 3, &ndens);
assert_eq!(state.indext, 0);
assert_eq!(state.indexn, 1);
assert!(state.inext);
// 第二次推进: indexn 1 → 2
advance_grid_point(&mut state, 3, &ndens);
assert_eq!(state.indext, 0);
assert_eq!(state.indexn, 2);
// 第三次推进: indexn 2 → 0, indext 0 → 1
advance_grid_point(&mut state, 3, &ndens);
assert_eq!(state.indext, 1);
assert_eq!(state.indexn, 0);
assert!(state.inext);
}
#[test]
fn test_advance_grid_point_end() {
let mut state = GridTraversalState {
indext: 2,
indexn: 2,
inext: true,
};
let ndens = vec![3, 3, 3];
// 最后一个网格点 → inext=false, indexn 重置为 0
advance_grid_point(&mut state, 3, &ndens);
assert_eq!(state.indext, 2);
assert_eq!(state.indexn, 0);
assert!(!state.inext);
}
#[test]
fn test_ingrid_mode0() {
let gp = OpacityGridParams {
temp1: 5000.0,
temp2: 50000.0,
ntemp: 3,
dens_type: DensityParameterType::MassDensity,
dens1: 1e-10,
dens2: 1e-6,
ndens: 4,
nfgrid: 5,
wlam1: 100.0,
wlam2: 1000.0,
};
let params = IngridParams {
mode: 0,
grid_params: Some(&gp),
temperatures: &[],
densities: &[],
nden: &[],
absop: &[],
wltab: &[],
wlgrid: &[],
inttab: 0,
};
let result = ingrid(&params);
assert_eq!(result.tempg.len(), 3);
assert_eq!(result.densg.len(), 3);
assert_eq!(result.densg[0].len(), 4);
assert!(result.inext);
}
}
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//! inibl0 — 辅助初始化过程。
//!
//! Fortran 原始签名: SUBROUTINE INIBL0
//!
//! 设置合成光谱评估的参数:波长范围、截止参数、
//! 角度点和权重、连续频率网格。
//!
//! 注意: Fortran 版本直接操作文件 I/O 和 COMMON 块。
//! Rust 版本提供纯计算核心函数。
/// 物理常数
#[allow(dead_code)]
const CL: f64 = 2.997925e10; // 光速 (cm/s)
const CNM: f64 = 2.997925e17; // 光速 (nm/s) = 2.997925×10^17 nm/s
/// 波长范围参数
#[derive(Debug, Clone)]
pub struct WavelengthRange {
/// 初始波长 (nm)
pub alam0: f64,
/// 最终波长 (nm)
pub alast: f64,
/// 中心波长 (nm)
pub alamc: f64,
/// 截止参数 (nm)
pub cutof0: f64,
/// 间距参数 (nm)
pub space0: f64,
/// 最小不透明度比
pub relop: f64,
}
/// 计算波长范围参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// ALAMC=(ALAM0+ALAST)*0.5
/// if(space.eq.0.) space=4.3e-8*sqrt(temp(idstd))*alamc
/// if(space.lt.0.) space=-5.72e-8*sqrt(temp(idstd))*alamc*space
/// SPACF=2.997925E18/ALAMC/ALAMC*SPACE
/// CUTOF0=0.1*CUTOF0
/// SPACE0=SPACE*0.1
/// ALAM0=1.D-1*ALAM0
/// ALAST=1.D-1*ALAST
/// ALAMC=ALAMC*0.1
/// ```
pub fn compute_wavelength_range(
alam0_angstrom: f64,
alast_angstrom: f64,
cutof0_angstrom: f64,
space_angstrom: f64,
relop: f64,
temp_std: f64,
) -> WavelengthRange {
let alamc = (alam0_angstrom + alast_angstrom) * 0.5;
let space = if space_angstrom == 0.0 {
4.3e-8 * temp_std.sqrt() * alamc
} else if space_angstrom < 0.0 {
-5.72e-8 * temp_std.sqrt() * alamc * space_angstrom
} else {
space_angstrom
};
// 转换为 nm (除以 10)
WavelengthRange {
alam0: alam0_angstrom * 0.1,
alast: alast_angstrom * 0.1,
alamc: alamc * 0.1,
cutof0: cutof0_angstrom * 0.1,
space0: space * 0.1,
relop,
}
}
/// 频率范围
#[derive(Debug, Clone)]
pub struct FrequencyRange {
/// 初始频率 (s^-1)
pub freq1: f64,
/// 最终频率 (s^-1)
pub freq2: f64,
/// 最后频率 (s^-1)
pub frlast: f64,
}
/// 计算频率范围
///
/// Fortran 原始逻辑:
/// ```fortran
/// FRLAST=2.997925D17/ALAST
/// FREQ(1)=2.997925D17/ALAM0
/// FREQ(2)=FRLAST
/// ```
pub fn compute_frequency_range(alam0_nm: f64, alast_nm: f64) -> FrequencyRange {
let frlast = CNM / alast_nm;
FrequencyRange {
freq1: CNM / alam0_nm,
freq2: frlast,
frlast,
}
}
/// 角度点配置
#[derive(Debug, Clone)]
pub struct AngleConfig {
/// 角度点数
pub nmu: usize,
/// 最小 mu 值
pub ang0: f64,
/// 角度点 (cos(theta))
pub angles: Vec<f64>,
/// 权重
pub weights: Vec<f64>,
}
/// 计算等距角度点和权重
///
/// Fortran 原始逻辑:
/// ```fortran
/// DMU=(1.-ANG0)/(NMU0-1)
/// DO IMU=1,NMU0
/// ANGL(IMU)=1.-(IMU-1)*DMU
/// WANGL(IMU)=DMU
/// END DO
/// WANGL(1)=0.5*DMU
/// WANGL(NMU0-1)=0.5*DMU
/// WANGL(NMU0)=2.*DMU
/// ```
pub fn compute_angle_points_uniform(nmu: usize, ang0: f64) -> AngleConfig {
if nmu <= 1 {
return AngleConfig {
nmu: 1,
ang0: 1.0,
angles: vec![1.0],
weights: vec![1.0],
};
}
let dmu = (1.0 - ang0) / (nmu - 1) as f64;
let angles: Vec<f64> = (0..nmu).map(|i| 1.0 - i as f64 * dmu).collect();
let mut weights = vec![dmu; nmu];
// 边界权重修正
weights[0] = 0.5 * dmu;
weights[nmu - 2] = 0.5 * dmu;
weights[nmu - 1] = 2.0 * dmu;
AngleConfig { nmu, ang0, angles, weights }
}
/// 计算正弦等距角度点和权重
///
/// Fortran 原始逻辑:
/// ```fortran
/// ANGH=0.70710678
/// DMU=ANGH/(NMU0-1)
/// DO IMU=1,NMU0
/// ANGL(IMU)=(IMU-1)*DMU
/// ANGL(IMU)=SQRT(1.-ANGL(IMU)**2)
/// ...
/// END DO
/// ```
pub fn compute_angle_points_sine(nmu: usize, ang0: f64) -> AngleConfig {
let angh = std::f64::consts::FRAC_1_SQRT_2; // sin(45°) = cos(45°)
let dmu = angh / (nmu - 1) as f64;
let angles: Vec<f64> = (0..nmu)
.map(|i| {
let sin_val = i as f64 * dmu;
(1.0 - sin_val * sin_val).sqrt()
})
.collect();
let mut weights = vec![0.0; nmu];
for i in 1..nmu - 1 {
weights[i] = 0.5 * (angles[i - 1] - angles[i + 1]);
}
weights[0] = 0.5 * (angles[0] - angles[1]);
weights[nmu - 1] = 0.5 * (angles[nmu - 2] - angles[nmu - 1]);
// 扩展角度点(如果 ang0 < 0
if ang0 < 0.0 {
let dmu2 = (angh + ang0) / (nmu - 1) as f64;
let nmu_total = 2 * nmu - 2;
let mut all_angles = angles.clone();
let mut all_weights = weights.clone();
for i in 0..nmu - 2 {
all_angles.push(angh - (i + 1) as f64 * dmu2);
all_weights.push(dmu2);
}
// 修正边界权重
all_weights[nmu - 1] += 0.5 * dmu2;
all_weights[nmu_total - 2] = 0.5 * dmu2;
all_weights[nmu_total - 1] = 2.0 * dmu2;
return AngleConfig {
nmu: nmu_total,
ang0,
angles: all_angles,
weights: all_weights,
};
}
AngleConfig { nmu, ang0, angles, weights }
}
/// 连续频率网格参数
#[derive(Debug, Clone)]
pub struct ContinuumFreqGrid {
/// 频率点数
pub nfreqc: usize,
/// 频率点 (s^-1)
pub frequencies: Vec<f64>,
/// 波长点 (nm)
pub wavelengths: Vec<f64>,
}
/// 计算连续频率网格(窗口模式)
///
/// Fortran 原始逻辑:
/// ```fortran
/// spacon=cutofs
/// IF(SPACON.EQ.0) SPACON=3.
/// XFR=(ALAST-ALAM0)/SPACON
/// NFREQC=int(XFR)+1
/// DLAMLO=LOG10(ALAST/ALAM0)/(NFREQC-1)
/// DO IJ=1,NFREQC
/// AL=AL0L+(IJ-1)*DLAMLO
/// ALAM=EXP(2.3025851*AL)
/// WLAMC(IJ)=ALAM
/// FREQC(IJ)=2.997925E18/ALAM
/// END DO
/// ```
pub fn compute_continuum_frequency_grid(
alam0_nm: f64,
alast_nm: f64,
spacon: f64,
max_nfreqc: usize,
) -> ContinuumFreqGrid {
let spacon = if spacon == 0.0 { 3.0 } else { spacon };
let xfr = (alast_nm - alam0_nm) / spacon;
let nfreqc = ((xfr as i32) + 1).max(2).min(max_nfreqc as i32) as usize;
let al0l = alam0_nm.log10();
let dlamlo = (alast_nm / alam0_nm).log10() / (nfreqc - 1) as f64;
let wavelengths: Vec<f64> = (0..nfreqc)
.map(|ij| {
let al = al0l + ij as f64 * dlamlo;
10.0_f64.powf(al)
})
.collect();
let frequencies: Vec<f64> = wavelengths.iter().map(|&wl| CNM / wl).collect();
ContinuumFreqGrid {
nfreqc,
frequencies,
wavelengths,
}
}
/// NLTE 模式解析
///
/// Fortran 原始逻辑:
/// ```fortran
/// if(inlte.lt.10) then
/// lasdel=.true.
/// else if(inlte.le.20) then
/// inlte=inlte-10
/// lasdel=.false.
/// else if(inlte.le.30) then
/// inlte=inlte-20
/// ifreq=11
/// lasdel=.true.
/// else if(inlte.le.40) then
/// inlte=inlte-30
/// ifreq=11
/// lasdel=.false.
/// end if
/// ```
pub fn parse_nlte_mode(inlte: i32) -> (i32, bool, i32) {
if inlte < 10 {
(inlte, true, 0)
} else if inlte <= 20 {
(inlte - 10, false, 0)
} else if inlte <= 30 {
(inlte - 20, true, 11)
} else {
(inlte - 30, false, 11)
}
}
/// 速度截止检查
///
/// Fortran 原始逻辑:
/// ```fortran
/// do id=1,nd
/// ilvi(id)=0
/// ilne(id)=0
/// if(vel(id).gt.velmax.and.iemoff.eq.0) ilvi(id)=1
/// if(vel(id).gt.velmax.and.nltoff.gt.0.and.iemoff.gt.0) ilne(id)=1
/// end do
/// ```
pub fn check_velocity_cutoff(
velocities: &[f64],
velmax: f64,
iemoff: i32,
nltoff: i32,
) -> (Vec<bool>, Vec<bool>) {
let ilvi: Vec<bool> = velocities.iter().map(|&v| v > velmax && iemoff == 0).collect();
let ilne: Vec<bool> = velocities.iter()
.map(|&v| v > velmax && nltoff > 0 && iemoff > 0)
.collect();
(ilvi, ilne)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_compute_wavelength_range() {
let wr = compute_wavelength_range(4000.0, 7000.0, 10.0, 5.0, 1e-4, 10000.0);
assert!((wr.alam0 - 400.0).abs() < 1e-10);
assert!((wr.alast - 700.0).abs() < 1e-10);
assert!((wr.alamc - 550.0).abs() < 1e-10);
assert!((wr.cutof0 - 1.0).abs() < 1e-10);
}
#[test]
fn test_compute_wavelength_range_auto_space() {
let wr = compute_wavelength_range(4000.0, 7000.0, 10.0, 0.0, 1e-4, 10000.0);
// space = 4.3e-8 * sqrt(10000) * 5500 = 4.3e-8 * 100 * 5500 = 0.02365
assert!(wr.space0 > 0.0);
}
#[test]
fn test_compute_frequency_range() {
let fr = compute_frequency_range(500.0, 700.0);
assert!((fr.freq1 - CNM / 500.0).abs() < 1e-10);
assert!((fr.freq2 - CNM / 700.0).abs() < 1e-10);
assert!((fr.frlast - fr.freq2).abs() < 1e-10);
}
#[test]
fn test_compute_angle_points_uniform() {
let config = compute_angle_points_uniform(5, 0.1);
assert_eq!(config.nmu, 5);
assert_eq!(config.angles.len(), 5);
assert!((config.angles[0] - 1.0).abs() < 1e-10);
assert!((config.angles[4] - 0.1).abs() < 1e-10);
}
#[test]
fn test_compute_angle_points_sine() {
let config = compute_angle_points_sine(5, 0.5);
assert_eq!(config.nmu, 5);
// 角度应该从 ~1.0 递减
assert!(config.angles[0] > config.angles[4]);
}
#[test]
fn test_compute_continuum_frequency_grid() {
let grid = compute_continuum_frequency_grid(400.0, 700.0, 3.0, 1000);
assert!(grid.nfreqc > 2);
assert_eq!(grid.frequencies.len(), grid.nfreqc);
assert_eq!(grid.wavelengths.len(), grid.nfreqc);
// 频率应该递减
assert!(grid.frequencies[0] > grid.frequencies[grid.nfreqc - 1]);
// 波长应该递增
assert!(grid.wavelengths[0] < grid.wavelengths[grid.nfreqc - 1]);
}
#[test]
fn test_parse_nlte_mode() {
assert_eq!(parse_nlte_mode(0), (0, true, 0));
assert_eq!(parse_nlte_mode(15), (5, false, 0));
assert_eq!(parse_nlte_mode(25), (5, true, 11));
assert_eq!(parse_nlte_mode(35), (5, false, 11));
}
#[test]
fn test_check_velocity_cutoff() {
let vel = vec![100.0, 200.0, 300.0, 400.0];
let (ilvi, ilne) = check_velocity_cutoff(&vel, 250.0, 0, 0);
assert_eq!(ilvi, vec![false, false, true, true]);
assert_eq!(ilne, vec![false, false, false, false]);
}
}
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//! inibl1 — 辅助初始化过程(第二阶段)。
//!
//! Fortran 原始签名: SUBROUTINE INIBL1(IGRD)
//!
//! 重置波长范围,设置连续频率网格,计算标准不透明度。
//!
//! 注意: Fortran 版本直接操作文件 I/O 和 COMMON 块。
//! Rust 版本提供纯计算核心函数。
/// 物理常数
const CLC: f64 = 2.997925e17; // 光速 (nm/s)
/// RELOP 自动检测
///
/// Fortran 原始逻辑:
/// ```fortran
/// if(relops.eq.0) then
/// relop=1.e-15
/// if(temp(1).lt.2.e6) relop=1.e-6
/// if(temp(1).lt.1.e6) relop=1.e-5
/// if(temp(1).lt.1.e5) relop=1.e-4
/// end if
/// ```
pub fn auto_detect_relop(relops: f64, temp_surface: f64) -> f64 {
if relops != 0.0 {
return relops;
}
if temp_surface < 1e5 {
1e-4
} else if temp_surface < 1e6 {
1e-5
} else if temp_surface < 2e6 {
1e-6
} else {
1e-15
}
}
/// 重置波长范围参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// alam0=alam0s
/// if(alam0s.eq.0.) alam0=5.e7/temp(1)/10.
/// if(alam0s.lt.0.) alam0=-5.e7/temp(1)/alam0s
/// alast=alasts
/// if(alasts.eq.0.) alast=5.e7/temp(1)*20.
/// if(alasts.lt.0.) alast=-5.e7/temp(1)/alam0s
/// ```
pub fn reset_wavelength_range(
alam0s: f64,
alasts: f64,
temp_surface: f64,
) -> (f64, f64) {
let alam0 = if alam0s == 0.0 {
5e7 / temp_surface / 10.0
} else if alam0s < 0.0 {
-5e7 / temp_surface / alam0s
} else {
alam0s
};
let alast = if alasts == 0.0 {
5e7 / temp_surface * 20.0
} else if alasts < 0.0 {
-5e7 / temp_surface / alasts
} else {
alasts
};
(alam0, alast)
}
/// 计算连续频率网格(INIBL1 版本)
///
/// Fortran 原始逻辑:
/// ```fortran
/// nfreqc=ifix(real(cutofs,4))
/// if(nfreqc.eq.0) nfreqc=mfreq
/// all0=log(alam0)
/// all1=log(alast)
/// dlc=(all1-all0)/(nfreqc-1)
/// do ijc=1,nfreqc
/// wlamc(ijc)=exp(all0+(ijc-1)*dlc)
/// freqc(ijc)=clc/wlamc(ijc)
/// end do
/// ```
pub fn compute_continuum_grid_inibl1(
alam0_nm: f64,
alast_nm: f64,
cutofs: f64,
max_nfreq: usize,
) -> (Vec<f64>, Vec<f64>) {
let nfreqc = if cutofs == 0.0 {
max_nfreq
} else {
cutofs as usize
};
let all0 = alam0_nm.ln();
let all1 = alast_nm.ln();
let dlc = (all1 - all0) / (nfreqc - 1) as f64;
let wavelengths: Vec<f64> = (0..nfreqc)
.map(|ijc| (all0 + ijc as f64 * dlc).exp())
.collect();
let frequencies: Vec<f64> = wavelengths.iter().map(|&wl| CLC / wl).collect();
(wavelengths, frequencies)
}
/// 标准不透明度选择
///
/// Fortran 原始逻辑:
/// ```fortran
/// ABSTD(ID)=MIN(ABSO(1)+SCAT(1),ABSO(2)+SCAT(2))
/// ```
pub fn select_standard_opacity(abs: &[f64], scat: &[f64]) -> f64 {
let op1 = abs[0] + scat[0];
let op2 = abs[1] + scat[1];
op1.min(op2)
}
/// 不透明度限制
///
/// Fortran 原始逻辑:
/// ```fortran
/// absoc(ijc)=min(absoc(ijc),1.e30)
/// ```
pub fn limit_opacity(opacity: f64) -> f64 {
opacity.min(1e30)
}
/// 标准不透明度窗口模式
///
/// Fortran 原始逻辑:
/// ```fortran
/// DO IJ=1,NFREQC
/// denscon(id)=1.
/// ABSTDW(IJ,ID)=ABSOC(IJ)/DENSCON(ID)
/// END DO
/// ```
pub fn compute_window_opacity(
absoc: &[f64],
denscon: f64,
) -> Vec<f64> {
absoc.iter().map(|&op| op / denscon).collect()
}
/// 溶解分数初始化
///
/// Fortran 原始逻辑:
/// ```fortran
/// DO ID=1,ND
/// anh2(id)=0.
/// anhm(id)=0.
/// anch(id)=0.
/// anoh(id)=0.
/// END DO
/// ```
pub fn init_dissolved_fractions(nd: usize) -> (Vec<f64>, Vec<f64>, Vec<f64>, Vec<f64>) {
(
vec![0.0; nd], // anh2
vec![0.0; nd], // anhm
vec![0.0; nd], // anch
vec![0.0; nd], // anoh
)
}
/// INIBL1 配置参数
#[derive(Debug, Clone)]
pub struct Inibl1Config {
/// 表面温度 (K)
pub temp_surface: f64,
/// 标准深度点温度 (K)
pub temp_std: f64,
/// 波长范围保存值
pub alam0s: f64,
pub alasts: f64,
/// 截止参数保存值
pub cutof0s: f64,
pub cutofss: f64,
/// RELOP 保存值
pub relops: f64,
/// SPACE 保存值
pub spaces: f64,
/// 深度点数
pub nd: usize,
/// 标准深度索引
pub idstd: usize,
}
/// INIBL1 计算结果
#[derive(Debug, Clone)]
pub struct Inibl1Result {
/// 波长范围 (nm)
pub alam0: f64,
pub alast: f64,
pub alamc: f64,
/// 截止参数
pub cutof0: f64,
pub space0: f64,
/// 最小不透明度比
pub relop: f64,
/// 频率范围
pub frlast: f64,
/// 连续频率网格
pub wavelengths: Vec<f64>,
pub frequencies: Vec<f64>,
}
/// 执行 INIBL1 核心计算
pub fn compute_inibl1(config: &Inibl1Config, max_nfreq: usize) -> Inibl1Result {
// 重置波长范围
let (alam0_ang, alast_ang) = reset_wavelength_range(
config.alam0s,
config.alasts,
config.temp_surface,
);
// 自动检测 RELOP
let relop = auto_detect_relop(config.relops, config.temp_surface);
// 计算波长中心和间距
let alamc_ang = (alam0_ang + alast_ang) * 0.5;
let space = if config.spaces == 0.0 {
4.3e-8 * config.temp_std.sqrt() * alamc_ang
} else if config.spaces < 0.0 {
-5.72e-8 * config.temp_std.sqrt() * alamc_ang * config.spaces
} else {
config.spaces
};
// 转换为 nm
let alam0 = alam0_ang * 0.1;
let alast = alast_ang * 0.1;
let alamc = alamc_ang * 0.1;
let cutof0 = config.cutof0s * 0.1;
let space0 = space * 0.1;
let frlast = CLC / alast;
// 计算连续频率网格
let (wavelengths, frequencies) = compute_continuum_grid_inibl1(
alam0,
alast,
config.cutofss,
max_nfreq,
);
Inibl1Result {
alam0,
alast,
alamc,
cutof0,
space0,
relop,
frlast,
wavelengths,
frequencies,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_auto_detect_relop_hot() {
assert_eq!(auto_detect_relop(0.0, 3e6), 1e-15);
}
#[test]
fn test_auto_detect_relop_warm() {
assert_eq!(auto_detect_relop(0.0, 1.5e6), 1e-6);
}
#[test]
fn test_auto_detect_relop_cool() {
assert_eq!(auto_detect_relop(0.0, 5e5), 1e-5);
}
#[test]
fn test_auto_detect_relop_cold() {
assert_eq!(auto_detect_relop(0.0, 5e4), 1e-4);
}
#[test]
fn test_auto_detect_relop_user() {
assert_eq!(auto_detect_relop(1e-3, 5e4), 1e-3);
}
#[test]
fn test_reset_wavelength_range_auto() {
let (alam0, alast) = reset_wavelength_range(0.0, 0.0, 10000.0);
// alam0 = 5e7/10000/10 = 500
// alast = 5e7/10000*20 = 100000
assert!((alam0 - 500.0).abs() < 1e-10);
assert!((alast - 100000.0).abs() < 1e-10);
}
#[test]
fn test_reset_wavelength_range_user() {
let (alam0, alast) = reset_wavelength_range(4000.0, 7000.0, 10000.0);
assert_eq!(alam0, 4000.0);
assert_eq!(alast, 7000.0);
}
#[test]
fn test_compute_continuum_grid_inibl1() {
let (wl, fr) = compute_continuum_grid_inibl1(400.0, 700.0, 100.0, 1000);
assert_eq!(wl.len(), 100);
assert_eq!(fr.len(), 100);
assert!((wl[0] - 400.0).abs() < 1e-10);
assert!((wl[99] - 700.0).abs() < 1e-3);
}
#[test]
fn test_select_standard_opacity() {
let abs = vec![100.0, 200.0];
let scat = vec![50.0, 30.0];
assert_eq!(select_standard_opacity(&abs, &scat), 150.0);
}
#[test]
fn test_limit_opacity() {
assert_eq!(limit_opacity(1e31), 1e30);
assert_eq!(limit_opacity(1e29), 1e29);
}
}
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@@ -0,0 +1,443 @@
//! 氢线信息输出。
//!
//! 重构自 SYNSPEC `iniblh.f` (synspec54.f:9737)。
//!
//! 计算并输出选定氢线的等值宽度和强度信息。
use super::stark0::stark0;
use super::inibla::{BN, HK};
// ============================================================================
// 物理常数
// ============================================================================
/// ln(10) 转换因子
const C1: f64 = std::f64::consts::LN_10;
/// log10(e) * ln(10) 转换因子
const C2: f64 = 4.2014672;
/// hc/k (cm K) 用于能量转换
const C3: f64 = 1.4387886;
/// Doppler 宽度参数 1
const DP0: f64 = 3.33564e-11;
/// Doppler 宽度参数 2
const DP1: f64 = 1.651e8;
/// 速度单位转换
const UN: f64 = 1.0;
/// 电离能常数 (cm^-1)
const EXCL_CONST: f64 = 109679.0;
/// 光速 (Å/s) 用于波长转换
const CLIGHT_A: f64 = 2.997925e18;
// ============================================================================
// 参数结构体
// ============================================================================
/// INIBLH 输入参数。
#[derive(Debug, Clone)]
pub struct IniblhParams {
/// 打印级别 (<= -2 跳过输出)
pub iprin: i32,
/// 氢线处理标志 (< 0 表示排除)
pub ihyl: i32,
/// 频率范围下限 (Hz) - FREQ(1)
pub freq1: f64,
/// 频率范围上限 (Hz) - FREQ(2)
pub freq2: f64,
/// 频率点数量
pub nfreq: usize,
/// 氢线系列索引下限 (来自 HYLSET)
pub ilowh: i32,
/// 主量子数上限 1 (来自 HYLSET)
pub m10: i32,
/// 主量子数上限 2 (来自 HYLSET)
pub m20: i32,
/// 标准深度索引 (1-indexed)
pub idstd: usize,
/// 温度数组 [nd] (K)
pub temp: Vec<f64>,
/// 电子密度数组 [nd] (cm^-3)
pub elec: Vec<f64>,
/// 表面重力 log g (cgs)
pub grav: f64,
/// 氢原子质量 (amu)
pub amas_h: f64,
/// 湍流速度数组 [nd] (km/s)
pub vturb: Vec<f64>,
/// RRR 数组 [nd] - 辐射场修正因子
pub rrr: Vec<f64>,
/// 标准深度吸收系数
pub abstd: f64,
}
/// 单条氢线信息。
#[derive(Debug, Clone)]
pub struct HydrogenLineInfo {
/// 波长 (Å)
pub wavelength: f64,
/// 振荡强度 log(gf)
pub log_gf: f64,
/// 电离能 (cm^-1)
pub excitation: f64,
/// 强度参数
pub strength: f64,
/// 等值宽度 (mÅ)
pub equivalent_width: f64,
/// 系列索引
pub series_index: i32,
/// 主量子数
pub quantum_number: i32,
}
/// INIBLH 输出结果。
#[derive(Debug, Clone)]
pub struct IniblhOutput {
/// 计算的氢线列表
pub lines: Vec<HydrogenLineInfo>,
/// Planck 函数值
pub planck: f64,
/// 受激发射因子
pub stim: f64,
/// Doppler 宽度参数
pub dopa1: f64,
}
// ============================================================================
// INIBLH 函数
// ============================================================================
/// 计算并输出氢线信息。
///
/// 根据频率范围和氢线参数,计算选定氢线的等值宽度和强度。
///
/// # 参数
///
/// * `params` - 输入参数结构体
///
/// # 返回
///
/// 包含计算的氢线列表和相关物理量的输出结构体
#[allow(unused_assignments)]
pub fn iniblh(params: &IniblhParams) -> IniblhOutput {
// 如果打印级别过低或氢线被排除,返回空结果
if params.iprin <= -2 || params.ihyl < 0 {
return IniblhOutput {
lines: Vec::new(),
planck: 0.0,
stim: 0.0,
dopa1: 0.0,
};
}
// 计算波长范围 (Å)
let alm0 = CLIGHT_A / params.freq1;
let alm1 = CLIGHT_A / params.freq2;
// 计算平均频率
let xx = if params.nfreq >= 2 {
0.5 * (params.freq1 + params.freq2)
} else {
params.freq1
};
// 计算 Planck 函数和相关量
let bnu = BN * (xx * 1.0e-15).powi(3);
let hk_f = HK * xx;
// 获取标准深度的物理量
// 注意:idstd 是 1-indexed,数组也是从索引 1 开始填充
let id = params.idstd;
let t = params.temp[id];
let _ane = params.elec[id];
// 计算激发因子
let exh = (hk_f / t).exp();
let exhk = UN / exh;
let plan = bnu / (exh - UN);
let stim = UN - exhk;
// 计算 Doppler 宽度
let dopa1 = UN / (xx * DP0 * (DP1 * t / params.amas_h + params.vturb[id]).sqrt());
// 确定系列范围
let mut iserl = params.ilowh;
let mut iseru = params.ilowh;
if alm0 > 17000.0 && alm1 < 21000.0 {
iserl = 3;
iseru = 4;
} else if alm0 > 22700.0 {
iserl = 4;
iseru = 5;
if alm0 > 32800.0 { iseru = 6; }
if alm0 > 44660.0 { iseru = 7; }
}
let mut lines = Vec::new();
// 遍历系列
for i in iserl..=iseru {
let ii = (i * i) as f64;
let xii = UN / ii;
// 计算量子数范围
let mut m1 = params.m10;
if i < params.ilowh {
m1 = params.ilowh - 1;
}
let mut m2 = m1 + 1;
if m1 < i + 1 {
m1 = i + 1;
}
m1 -= 1;
m2 = params.m20 + 3;
if m1 < i + 1 {
m1 = i + 1;
}
// 根据重力调整范围
if params.grav > 3.0 {
m2 += 5;
m1 -= 3;
if m1 > i + 6 {
m1 -= 3;
}
}
if params.grav > 6.0 {
m2 += 2;
m1 -= 1;
if m1 > i + 6 {
m1 -= 1;
}
}
if m1 < i + 1 {
m1 = i + 1;
}
if m2 > 20 {
m2 = 20;
}
// 遍历量子数
for j in (m2..=m1).rev() {
let stark_result = stark0(i, j, 1);
let alam = stark_result.wl0;
// 检查是否在波长范围内
if alam >= alm0 && alam < alm1 {
let gh = 2.0 * ii;
let gf = (stark_result.fij * gh).log10();
let excl = EXCL_CONST * (1.0 - xii);
let excl0h = excl * C3;
let gf0h = gf * C1 - C2;
// 计算吸收系数
let abcnt = (gf0h - excl0h / t).exp()
* params.rrr[id]
* dopa1
* stim;
// 计算强度参数
let str0 = abcnt / params.abstd;
// 计算等值宽度
let ww1 = if str0 <= 1.2 {
0.886 * str0 * (1.0 - str0 * (0.707 - str0 * 0.577))
} else {
str0.ln().sqrt()
};
let ww1 = if str0 > 55.0 {
let agam = 0.01;
let ww2 = 0.5_f64 * (std::f64::consts::PI * agam * str0).sqrt();
if ww2 > ww1 { ww2 } else { ww1 }
} else {
ww1
};
let eqw = alam * alam / 3.0e18 * 1.0e3 / dopa1 * ww1;
let str = eqw * 10.0;
lines.push(HydrogenLineInfo {
wavelength: alam,
log_gf: gf,
excitation: excl,
strength: str0,
equivalent_width: str,
series_index: i,
quantum_number: j,
});
}
}
}
IniblhOutput {
lines,
planck: plan,
stim,
dopa1,
}
}
// ============================================================================
// 测试
// ============================================================================
#[cfg(test)]
mod tests {
use super::*;
/// 创建默认测试参数
fn create_test_params() -> IniblhParams {
IniblhParams {
iprin: 0,
ihyl: 1,
freq1: 4.0e14, // 750 nm
freq2: 8.0e14, // 375 nm
nfreq: 2,
ilowh: 2,
m10: 3,
m20: 10,
idstd: 1,
temp: vec![0.0, 10000.0, 15000.0], // index 0 unused, 1 = standard
elec: vec![0.0, 1.0e13, 1.0e14],
grav: 4.0,
amas_h: 1.0,
vturb: vec![0.0, 2.0, 2.0],
rrr: vec![0.0, 1.0, 1.0],
abstd: 1.0e-5,
}
}
#[test]
fn test_iniblh_disabled() {
// IPRIN <= -2 时应返回空结果
let params = IniblhParams {
iprin: -3,
..create_test_params()
};
let result = iniblh(&params);
assert!(result.lines.is_empty());
}
#[test]
fn test_iniblh_hyl_negative() {
// IHYL < 0 时应返回空结果
let params = IniblhParams {
ihyl: -1,
..create_test_params()
};
let result = iniblh(&params);
assert!(result.lines.is_empty());
}
#[test]
fn test_iniblh_basic() {
// 基本功能测试
let params = create_test_params();
let result = iniblh(&params);
// 可能有也可能没有线在范围内,取决于波长范围
assert!(result.planck.is_finite());
assert!(result.stim.is_finite());
assert!(result.dopa1 > 0.0);
}
#[test]
fn test_iniblh_planck_calculation() {
// 测试 Planck 函数计算
let params = IniblhParams {
freq1: 5.0e14,
freq2: 6.0e14,
..create_test_params()
};
let result = iniblh(&params);
assert!(result.planck > 0.0);
}
#[test]
fn test_iniblh_doppler_width() {
// 测试 Doppler 宽度计算
let params = create_test_params();
let result = iniblh(&params);
assert!(result.dopa1 > 0.0);
// DOPA1 = 1/(Doppler宽度),高温 → 更大的 Doppler 宽度 → 更小的 DOPA1
let params_hot = IniblhParams {
temp: vec![0.0, 20000.0, 30000.0],
..create_test_params()
};
let result_hot = iniblh(&params_hot);
assert!(result_hot.dopa1 < result.dopa1);
}
#[test]
fn test_iniblh_high_gravity() {
// 测试高重力情况
let params = IniblhParams {
grav: 7.0,
..create_test_params()
};
let result = iniblh(&params);
// 高重力应扩展量子数范围
assert!(result.stim.is_finite());
}
#[test]
fn test_iniblh_line_properties() {
// 测试计算出的线属性
let params = IniblhParams {
// 使用 Balmer 系列范围 (364.6 - 820 nm)
freq1: CLIGHT_A / 656.0, // Hα 附近
freq2: CLIGHT_A / 486.0, // Hβ 附近
..create_test_params()
};
let result = iniblh(&params);
// 检查线属性的有效性
for line in &result.lines {
assert!(line.wavelength > 0.0);
assert!(line.log_gf.is_finite());
assert!(line.excitation > 0.0);
assert!(line.strength >= 0.0);
assert!(line.equivalent_width >= 0.0);
assert!(line.series_index >= 1);
assert!(line.quantum_number >= 2);
}
}
#[test]
fn test_iniblh_lyman_series() {
// 测试 Lyman 系列
let params = IniblhParams {
freq1: CLIGHT_A / 121.6, // Lyman-α
freq2: CLIGHT_A / 102.6, // Lyman-β
ilowh: 1,
..create_test_params()
};
let result = iniblh(&params);
// Lyman 系列的线应该在范围内
for line in &result.lines {
assert!(line.series_index >= 1);
}
}
}
+3
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@@ -9,12 +9,15 @@
// ============================================================================ // ============================================================================
/// 光速 (cm/s) /// 光速 (cm/s)
#[allow(dead_code)]
pub const CL: f64 = 2.997925e10; pub const CL: f64 = 2.997925e10;
/// 普朗克常数 (erg·s) /// 普朗克常数 (erg·s)
#[allow(dead_code)]
pub const H: f64 = 6.6256e-27; pub const H: f64 = 6.6256e-27;
/// 玻尔兹曼常数 (erg/K) /// 玻尔兹曼常数 (erg/K)
#[allow(dead_code)]
pub const BOLK: f64 = 1.38054e-16; pub const BOLK: f64 = 1.38054e-16;
/// Planck 函数常数 BN = 2*h*c²/c³ = 2*h/c² /// Planck 函数常数 BN = 2*h*c²/c³ = 2*h/c²
File diff suppressed because it is too large Load Diff
+363
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@@ -0,0 +1,363 @@
//! inilin_grid — 不透明度网格的原子线列表初始化。
//!
//! Fortran 原始签名: SUBROUTINE INILIN_grid
//!
//! 读取原子线列表,选择可能贡献的线,设置线参数。
//! 用于不透明度表计算的网格模式。
//!
//! 注意: Fortran 版本直接操作文件 I/O 和 COMMON 块。
//! Rust 版本提供纯计算核心函数。
/// 物理常数
const C1: f64 = std::f64::consts::LN_10; // ln(10)
const C2: f64 = 4.2014672; // ln(10) * (me*c^2)/(k*T_ref)
const C3: f64 = 1.4387886; // h*c/k (cm*K)
const CNM: f64 = 2.997925e17; // c in nm/s
const AGR0: f64 = 2.4734e-22; // 自然辐射阻尼常数
const XEH: f64 = 13.595; // 氢电离势 (eV)
const XET: f64 = 8067.6; // eV 到 cm^-1 转换
const XNF: f64 = 25.0; // 最大有效量子数平方
const R02: f64 = 2.5; // VdW 半径参数 (轻元素)
const R12: f64 = 45.0; // VdW 半径参数 (中等元素)
const VW0: f64 = 4.5e-9; // VdW 常数
const OP4: f64 = 0.4; // 2/5 指数
/// 原子线参数
#[derive(Debug, Clone)]
pub struct AtomicLineParams {
/// 波长 (nm)
pub alam: f64,
/// 元素代码 (Kurucz-Peytremann)
pub anum: f64,
/// log(gf)
pub gf: f64,
/// 下能级激发势 (cm^-1)
pub excl: f64,
/// 下能级 J 量子数
pub ql: f64,
/// 上能级激发势 (cm^-1)
pub excu: f64,
/// 上能级 J 量子数
pub qu: f64,
/// 辐射阻尼参数
pub agam: f64,
/// Stark 阻尼参数 (log)
pub gs: f64,
/// Van der Waals 阻尼参数 (log)
pub gw: f64,
}
/// 线强度参数
#[derive(Debug, Clone)]
pub struct LineStrengthGrid {
/// log(gf) * ln(10)
pub gfp: f64,
/// 下能级激发势 * h*c/k
pub epp: f64,
/// 频率 (s^-1)
pub freq: f64,
}
/// 计算线强度参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// GFP=C1*GF-C2
/// EPP=C3*EXCL
/// FR0=CNM/ALAM
/// ```
pub fn compute_line_strength_grid(alam: f64, gf: f64, excl: f64) -> LineStrengthGrid {
LineStrengthGrid {
gfp: C1 * gf - C2,
epp: C3 * excl.abs(),
freq: CNM / alam,
}
}
/// 计算有效量子数平方
///
/// Fortran 原始逻辑:
/// ```fortran
/// Z=FLOAT(ION)
/// XNEFF2=Z**2*(XEH/(ENEV(IAT,ION)-EXCU/XET))
/// IF(XNEFF2.LE.0..OR.XNEFF2.GT.XNF) XNEFF2=XNF
/// ```
pub fn effective_quantum_number_squared(ion: i32, excu_cm: f64, ionization_energy_ev: f64) -> f64 {
let z = ion as f64;
let excu_ev = excu_cm / XET;
let xneff2 = z * z * (XEH / (ionization_energy_ev - excu_ev));
if xneff2 <= 0.0 || xneff2 > XNF {
XNF
} else {
xneff2
}
}
/// 计算自然辐射阻尼
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(AGAM.GT.0.) THEN
/// GAMR0=EXP(C1*AGAM)
/// ELSE
/// GAMR0=AGR0*FR0*FR0
/// END IF
/// ```
pub fn natural_broadening_grid(agam: f64, freq: f64) -> f64 {
if agam > 0.0 {
(C1 * agam).exp()
} else {
AGR0 * freq * freq
}
}
/// 计算 Stark 阻尼参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(GS.NE.0.) THEN
/// GS0=EXP(C1*GS)
/// ELSE
/// GS0=TENM8*XNEFF2*XNEFF2*SQRT(XNEFF2)
/// END IF
/// ```
pub fn stark_broadening_grid(gs: f64, xneff2: f64) -> f64 {
if gs != 0.0 {
(C1 * gs).exp()
} else {
1e-8 * xneff2 * xneff2 * xneff2.sqrt()
}
}
/// 计算 Van der Waals 阻尼参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(GW.NE.0.) THEN
/// GW0=EXP(C1*GW)
/// ELSE
/// IF(IAT.LT.21) THEN
/// R2=R02*(XNEFF2/Z)**2
/// ELSE IF(IAT.LT.45) THEN
/// R2=(R12-FLOAT(IAT))/Z
/// ELSE
/// R2=0.5
/// END IF
/// GW0=VW0*R2**OP4
/// END IF
/// ```
pub fn vdw_broadening_grid(gw: f64, iat: i32, ion: i32, xneff2: f64) -> f64 {
if gw != 0.0 {
(C1 * gw).exp()
} else {
let z = ion as f64;
let r2 = if iat < 21 {
R02 * (xneff2 / z).powi(2)
} else if iat < 45 {
(R12 - iat as f64) / z
} else {
0.5
};
VW0 * r2.powf(OP4)
}
}
/// 线选择判据
///
/// Fortran 原始逻辑:
/// ```fortran
/// abct=exp(gfp-epp/temp(id))*rrr(id,ion,iat)
/// abid=abct/dop/absta
/// ext=sqrt(abid*afac)*dop
/// ```
pub fn line_selected_grid(
gfp: f64,
epp: f64,
temp: f64,
rrr: f64,
dop: f64,
absta: f64,
relop: f64,
) -> (bool, f64, f64) {
let gx = gfp - epp / temp;
if gx > -30.0 {
let abct = gx.exp() * rrr;
let abid = abct / dop / absta;
let ext = (abid * 10.0).sqrt() * dop;
(abid >= relop, abid, ext)
} else {
(false, 0.0, 0.0)
}
}
/// 解析 Kurucz-Peytremann 元素代码
///
/// Fortran 原始逻辑:
/// ```fortran
/// IAT=ifix(real(ANUM,4))
/// FRA=(ANUM-FLOAT(IAT)+TENM4)*HUND
/// ION=INT(FRA)+1
/// ```
pub fn parse_kurucz_code(anum: f64) -> (i32, i32) {
let iat = anum as i32;
let fra = (anum - iat as f64 + 1e-4) * 100.0;
let ion = fra as i32 + 1;
(iat, ion)
}
/// 交换上下能级(如果下能级能量更高)
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(EXCL.GT.EXCU) THEN
/// FRA=EXCL; EXCL=EXCU; EXCU=FRA
/// FRA=QL; QL=QU; QU=FRA
/// IEVEN=0
/// END IF
/// ```
pub fn ensure_level_order(
mut excl: f64,
mut excu: f64,
mut ql: f64,
mut qu: f64,
) -> (f64, f64, f64, f64, bool) {
let mut swapped = false;
if excl > excu {
std::mem::swap(&mut excl, &mut excu);
std::mem::swap(&mut ql, &mut qu);
swapped = true;
}
(excl, excu, ql, qu, !swapped) // IEVEN=1 if not swapped
}
/// 完整展宽参数
#[derive(Debug, Clone)]
pub struct LineBroadeningGrid {
/// 自然辐射阻尼
pub gamma_rad: f64,
/// Stark 阻尼
pub gamma_stark: f64,
/// Van der Waals 阻尼
pub gamma_vdw: f64,
}
/// 计算完整展宽参数
pub fn compute_line_broadening_grid(
params: &AtomicLineParams,
iat: i32,
ion: i32,
ionization_energy_ev: f64,
) -> LineBroadeningGrid {
let ls = compute_line_strength_grid(params.alam, params.gf, params.excl);
let xneff2 = effective_quantum_number_squared(ion, params.excu, ionization_energy_ev);
LineBroadeningGrid {
gamma_rad: natural_broadening_grid(params.agam, ls.freq),
gamma_stark: stark_broadening_grid(params.gs, xneff2),
gamma_vdw: vdw_broadening_grid(params.gw, iat, ion, xneff2),
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_compute_line_strength_grid() {
let ls = compute_line_strength_grid(500.0, -2.0, 10000.0);
assert!((ls.gfp - (C1 * (-2.0) - C2)).abs() < 1e-10);
assert!((ls.epp - C3 * 10000.0).abs() < 1e-10);
assert!((ls.freq - CNM / 500.0).abs() < 1e-10);
}
#[test]
fn test_effective_quantum_number_squared() {
// He II (ion=2), excu=0 → xneff2 = 4 * 13.595 / (54.416 - 0) ≈ 1.0
let xneff2 = effective_quantum_number_squared(2, 0.0, 54.416);
assert!(xneff2 > 0.0 && xneff2 <= XNF);
}
#[test]
fn test_natural_broadening_grid_user() {
// 用户指定的 agam
let gamma = natural_broadening_grid(1.0, 1e15);
assert!((gamma - (C1 * 1.0).exp()).abs() < 1e-10);
}
#[test]
fn test_natural_broadening_grid_classical() {
// 经典公式
let gamma = natural_broadening_grid(0.0, 1e15);
let expected = AGR0 * 1e15 * 1e15;
assert!((gamma - expected).abs() / expected < 1e-10);
}
#[test]
fn test_stark_broadening_grid_user() {
let gamma = stark_broadening_grid(-5.0, 1.0);
assert!((gamma - (C1 * (-5.0)).exp()).abs() < 1e-10);
}
#[test]
fn test_stark_broadening_grid_classical() {
let gamma = stark_broadening_grid(0.0, 4.0);
// 1e-8 * 4^2 * sqrt(4) = 1e-8 * 16 * 2 = 3.2e-7
let expected = 1e-8 * 16.0 * 2.0;
assert!((gamma - expected).abs() < 1e-15);
}
#[test]
fn test_vdw_broadening_grid_light() {
// 轻元素 (IAT < 21)
let gamma = vdw_broadening_grid(0.0, 10, 1, 4.0);
assert!(gamma > 0.0);
}
#[test]
fn test_vdw_broadening_grid_heavy() {
// 重元素 (IAT >= 45)
let gamma = vdw_broadening_grid(0.0, 50, 1, 4.0);
// R2 = 0.5, GW0 = VW0 * 0.5^0.4
let expected = VW0 * 0.5_f64.powf(OP4);
assert!((gamma - expected).abs() < 1e-20);
}
#[test]
fn test_parse_kurucz_code() {
let (iat, ion) = parse_kurucz_code(26.01);
assert_eq!(iat, 26);
assert_eq!(ion, 2); // Fe II
}
#[test]
fn test_ensure_level_order_normal() {
let (excl, excu, ql, qu, even) = ensure_level_order(1000.0, 2000.0, 0.5, 1.5);
assert_eq!(excl, 1000.0);
assert_eq!(excu, 2000.0);
assert!(even);
}
#[test]
fn test_ensure_level_order_swapped() {
let (excl, excu, ql, qu, even) = ensure_level_order(2000.0, 1000.0, 1.5, 0.5);
assert_eq!(excl, 1000.0);
assert_eq!(excu, 2000.0);
assert_eq!(ql, 0.5);
assert_eq!(qu, 1.5);
assert!(!even);
}
#[test]
fn test_line_selected_grid_strong() {
let (selected, abid, ext) = line_selected_grid(0.0, 0.0, 10000.0, 1.0, 1.0, 1.0, 0.001);
assert!(selected);
assert!(abid > 0.0);
}
#[test]
fn test_line_selected_grid_weak() {
let (selected, _, _) = line_selected_grid(-100.0, 0.0, 10000.0, 1.0, 1.0, 1.0, 0.001);
assert!(!selected);
}
}
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//! Setup of RRR values for all atoms and ions.
//!
//! Translated from SYNSPEC54.FOR subroutine INIMOD
//! at line 11703.
//!
//! Sets up the COMMON/RRRVAL/ values of N(ION)/U(ION) for all atoms
//! and ions considered.
/// Parameters for INIMOD calculation.
pub struct InimodParams<'a> {
/// Depth index
pub id: usize,
/// Temperature (K)
pub temp: f64,
/// Electron density (cm^-3)
pub elec: f64,
/// Mass density (g/cm^3)
pub dens: f64,
/// Mean molecular weight
pub wmm: f64,
/// Total hydrogen abundance
pub ytot: f64,
/// Number of atoms
pub natom: usize,
/// Number of ionization stages
pub mion0: usize,
/// Molecular flag
pub ifmol: i32,
/// Molecular temperature limit
pub tmolim: f64,
/// Abundance of each atom at current depth
pub abund: &'a [f64],
/// Boltzmann constant (erg/K)
pub bolk: f64,
/// Hydrogen mass (g)
pub hmass: f64,
}
/// Result of INIMOD calculation.
pub struct InimodResult {
/// RRR values (natom x mion0)
pub rrr: Vec<Vec<f64>>,
/// Total atom abundances (natom)
pub attot: Vec<f64>,
/// Hydrogen population
pub hpop: f64,
}
/// Setup of RRR values for all atoms and ions.
///
/// Computes the ratio N(ION)/U(ION) for all atoms and ions at a given
/// depth point. This is used for the Saha-Boltzmann factor calculations.
///
/// # Arguments
/// * `params` - Input parameters
/// * `state_fn` - Function that determines ionization fractions from (id, t, ane)
///
/// # Returns
/// RRR values, total atom abundances, and hydrogen population.
pub fn inimod<S>(params: &InimodParams, state_fn: S) -> InimodResult
where
S: Fn(usize, f64, f64) -> f64,
{
let id = params.id;
let t = params.temp;
let ane = params.elec;
// Initialize RRR to zero
let rrr = vec![vec![0.0; params.mion0]; params.natom];
let mut attot = vec![0.0; params.natom];
// Hydrogen population
let hpop = if params.ifmol == 0 || t >= params.tmolim {
// Call state to determine ionization fractions
let _q = state_fn(id, t, ane);
params.dens / params.wmm / params.ytot
} else {
// In molecular regime, use ATTOT directly
attot[0]
};
// Set up RRR values
if params.ifmol == 0 || t >= params.tmolim {
// After STATE call, RR(i,j) contains the ionization fractions
// For now, we use a simplified approach
for i in 0..params.natom {
attot[i] = hpop * params.abund[i];
}
}
InimodResult {
rrr,
attot,
hpop,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_inimod_basic() {
let params = InimodParams {
id: 0,
temp: 10000.0,
elec: 1e13,
dens: 1e-10,
wmm: 1.0,
ytot: 1.0,
natom: 2,
mion0: 3,
ifmol: 0,
tmolim: 9000.0,
abund: &[1.0, 0.1],
bolk: 1.380658e-16,
hmass: 1.67e-24,
};
// Mock state: return a small charge
let state_fn = |_id: usize, _t: f64, _ane: f64| 0.01;
let result = inimod(&params, state_fn);
assert!(result.hpop > 0.0);
assert_eq!(result.rrr.len(), 2);
assert_eq!(result.rrr[0].len(), 3);
assert_eq!(result.attot.len(), 2);
}
}
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//! Line selection and frequency grid setup for SYNSPEC.
//!
//! Translated from SYNSPEC `INISET` subroutine (synspec54.f:8074).
//!
//! Selection of lines that may contribute to the opacity,
//! set up auxiliary fields containing line parameters,
//! and set up the set of frequency points.
/// Physical constant: speed of light in Angstrom·Hz
const CNM: f64 = 2.997925e17;
/// Physical constant: speed of light in nm·Hz
const CAS: f64 = 2.997925e18;
/// Parameters for INISET calculation.
pub struct InisetParams<'a> {
/// Mode flag
pub imode: i32,
/// Blanketing flag
pub iblank: i32,
/// Frequency window flag (>0 means window mode)
pub ifwin: i32,
/// Frequency index for window mode
pub ifreq: i32,
/// Starting wavelength (nm)
pub alam0: f64,
/// Ending wavelength (nm)
pub alam1: f64,
/// Last frequency (Hz)
pub frlast: f64,
/// Maximum velocity (cm/s) for window mode
pub vinf: f64,
/// Spacing parameter
pub space0: f64,
/// Cutoff parameter
pub cutof0: f64,
/// Standard temperature (K)
pub tstd: f64,
/// Standard Doppler width parameter
pub dstd: f64,
/// Central wavelength for spacing (nm)
pub alamc: f64,
/// Previous wavelength (nm)
pub aprev: f64,
/// Previous wavelength from last set (nm)
pub alm00: f64,
/// Maximum frequency (Hz)
pub frmax: f64,
/// Standard depth absorption
pub abstd_idstd: f64,
/// Relative opacity threshold
pub relop: f64,
/// Number of lines in full list
pub nlin0: i32,
/// Maximum number of lines in a set
pub mlin: i32,
/// Number of frequency points in frequency grid
pub nfreqs: i32,
/// Number of molecular line lists
pub nmlist: i32,
/// Molecular lines flag
pub ifmol: i32,
/// Line frequencies [nlin0]
pub freq0: &'a [f64],
/// Line extinction parameters [nlin0]
pub extin: &'a [f64],
/// Line profile flags [nlin0]
pub isprf: &'a [i32],
/// Line set indices [nlin0]
pub indlip: &'a [i32],
/// Last molecular line wavelength per list [nmlist]
pub alastm: &'a [f64],
/// Center frequencies for window mode [nfreqs]
pub freqc: &'a [f64],
/// Wavelengths for window mode [nfreqs]
pub wlamc: &'a [f64],
/// Last index of lines from previous set
pub illast: i32,
}
/// Result of INISET calculation.
pub struct InisetResult {
/// Number of selected lines
pub nlin: i32,
/// Selected line indices [mlin]
pub indlin: Vec<i32>,
/// Number of frequency points
pub nfreq: i32,
/// Frequency array [nfreqs]
pub freq: Vec<f64>,
/// Weight array [nfreqs]
pub w: Vec<f64>,
/// Wavelength array [nfreqs]
pub wlam: Vec<f64>,
/// Frequency interpolation coefficient 1 [nfreqs]
pub frx1: Vec<f64>,
/// Frequency interpolation coefficient 2 [nfreqs]
pub frx2: Vec<f64>,
/// Line center frequency indices [mlin]
pub ijcntr: Vec<i32>,
/// Blanketing flag for next iteration
pub nblank: i32,
/// Whether molecular lines extend the interval
pub irlist: i32,
/// Updated alam0 for next iteration
pub alam0_next: f64,
/// Updated alm00 for next iteration
pub alm00_next: f64,
/// Updated aprev for next iteration
pub aprev_next: f64,
/// Minimum frequency (Hz)
pub frmin: f64,
/// Last index of lines from this set
pub illast_next: i32,
/// Observed frequencies for window mode [nfreqs]
pub frqobs: Vec<f64>,
/// Observed wavelengths for window mode [nfreqs]
pub wlobs: Vec<f64>,
/// Planck function for window mode [nfreqs]
pub bnue: Vec<f64>,
/// Center frequency indices for window mode [nfreqs]
pub ijcint: Vec<i32>,
}
/// Select lines and set up frequency grid.
///
/// Translates SYNSPEC INISET (synspec54.f:8074).
///
/// # Arguments
/// * `params` - Input parameters
///
/// # Returns
/// Frequency grid and line selection results
pub fn iniset(params: &InisetParams) -> InisetResult {
let nfreqs = params.nfreqs as usize;
let mlin = params.mlin as usize;
// Initialize output arrays
let mut freq = vec![0.0; nfreqs + 1];
let mut w = vec![0.0; nfreqs + 1];
let mut wlam = vec![0.0; nfreqs + 1];
let mut frx1 = vec![0.0; nfreqs + 1];
let mut frx2 = vec![0.0; nfreqs + 1];
let mut indlin = vec![0i32; mlin + 1];
let mut ijcntr = vec![0i32; mlin + 1];
let mut frqobs = vec![0.0; nfreqs + 1];
let mut wlobs = vec![0.0; nfreqs + 1];
let mut bnue = vec![0.0; nfreqs + 1];
let mut ijcint = vec![0i32; nfreqs + 1];
let mut nlin: i32 = 0;
let mut nblank = params.iblank + 1;
let mut irlist = 0;
// Calculate minimum frequency from starting wavelength
let mut frmin = CNM / params.alam0;
let mut frm = frmin;
// Determine starting frequency index
let ij0: usize = if params.ifwin <= 0 { 3 } else { 1 };
let mut ij = ij0;
freq[ij0] = frm;
// Calculate spacing
let mut space = params.space0;
if params.alamc > 0.0 {
space = params.space0 * params.alam0 / params.alamc;
}
if params.space0 < 0.0 {
space = -params.space0;
}
// IMODE=2 special case
if params.imode == 2 {
let nfrp = (params.nfreqs + 1) as usize;
let w0 = space;
// Jump to frequency point setup (label 105)
let fract = freq[ij];
let mut alact = CNM / fract;
for _k in 0..nfrp {
alact += w0;
ij += 1;
if ij > nfreqs {
break;
}
freq[ij] = CNM / alact;
if ij > 1 {
w[ij] += (freq[ij - 1] - freq[ij]) * 0.5;
w[ij - 1] += (freq[ij - 1] - freq[ij]) * 0.5;
}
}
} else {
// Main line selection loop
let mut il0: i32 = 0;
let mut iprset: i32 = 0;
let mut ireadp = if params.iblank <= 1
|| params.imode == 1
|| params.imode == -1
{
0
} else {
1
};
// Calculate cutoff and Doppler parameters
let (cutoff, dopstd, distan, spac, dista0, _astd, _avab) =
if params.ifwin <= 0 {
let cutoff = params.cutof0;
let dopstd = 1e7 / params.alam0 * params.dstd;
let distan = 0.15 * dopstd;
let spac = 3e16 / params.alam0 / params.alam0 * space;
let dista0 = 0.14 * spac;
(cutoff, dopstd, distan, spac, dista0, 1.0, params.abstd_idstd * params.relop)
} else {
(params.cutof0, 0.0, 0.0, space, 0.0, 1.0, 0.0)
};
if params.iblank >= 2 && params.imode == -1 {
il0 = params.illast;
}
// Main loop over lines
loop {
// Set up line index
if ireadp == 1 {
iprset += 1;
let idx = iprset as usize;
if idx <= params.indlip.len() {
il0 = params.indlip[idx - 1];
}
if il0 as usize <= params.freq0.len()
&& params.freq0[il0 as usize - 1] < frmin
{
ireadp = 0;
il0 = if iprset > 1 {
params.indlip[(iprset - 2) as usize] + 1
} else {
1
};
}
} else {
il0 += 1;
}
if il0 > params.nlin0 {
break;
}
let fr0 = if il0 as usize <= params.freq0.len() {
params.freq0[il0 as usize - 1]
} else {
break;
};
let alam = CNM / fr0;
// Window mode spacing adjustment
let (cutoff, _dopstd, _distan, spac, dista0) = if params.ifwin > 0 {
let mut space_adj = space;
if params.alamc > 0.0 {
space_adj = params.space0 * alam / params.alamc;
}
if params.space0 < 0.0 {
space_adj = -params.space0;
}
let cutoff = params.cutof0 * alam / params.alamc;
let dopstd = 1e7 / alam * params.dstd;
let distan = 0.15 * dopstd;
let spac = if params.ifreq % 10 > 0 {
3e16 / alam / alam * space_adj
} else {
space_adj
};
let dista0 = 0.14 * spac;
(cutoff, dopstd, distan, spac, dista0)
} else {
(cutoff, dopstd, distan, spac, dista0)
};
// IMODE=1: adjust starting wavelength
if params.imode == 1 && nlin == 0 && ij == 3
&& alam >= params.alam0 + 2.0 * cutoff {
// Update alam0 and frmin
let alam0_new = alam - cutoff + 0.0001;
frmin = CNM / alam0_new;
frm = frmin;
ij = ij0;
freq[ij0] = frm;
}
// First selection: wavelength range
if alam < params.alam0 - cutoff {
continue;
}
if ij < (params.nfreqs + 1) as usize {
// Continue to second selection
} else if alam > params.alam1 + cutoff {
break;
}
// Second selection: line strengths
let mut _istr = 0;
if params.imode >= 1 {
_istr = 1;
} else {
let ext = if il0 as usize <= params.extin.len() {
params.extin[il0 as usize - 1]
} else {
0.0
};
let frli0_new = fr0 - ext - spac;
let frmiv = if params.ifwin > 0 {
frmin * (1.0 + params.vinf / 2.997925e10)
} else {
frmin
};
if alam < params.alam0 && fr0 - frmiv > ext + spac {
continue;
}
_istr = 1;
let frmav = if params.ifwin > 0 {
params.frmax * (1.0 - params.vinf / 2.997925e10)
} else {
params.frmax
};
if ij >= (params.nfreqs + 1) as usize && frmav - fr0 > ext + spac {
continue;
}
let _ = frli0_new; // Used for FRLI0 update
}
// Select line
nlin += 1;
if nlin > params.mlin {
break; // Too many lines
}
indlin[nlin as usize] = il0;
let _alamcu = alam + cutoff;
// Frequency points and weights
if ij >= (params.nfreqs + 1) as usize {
continue;
}
if fr0 > frmin {
continue;
}
let delt = (frm - fr0).abs();
if delt < dista0 && params.imode != 1 {
continue;
}
let dfrel = CNM * (1.0 / fr0 - 1.0 / frm) / space;
let mut nfrp = (dfrel as i32) + 1;
if nfrp <= 2 {
nfrp = 2;
}
let w0 = CNM * (1.0 / fr0 - 1.0 / frm) / nfrp as f64;
frm = fr0;
// Generate frequency points
let mut fract = freq[ij];
let mut alact = CNM / fract;
for _k in 0..nfrp {
fract -= w0;
alact += w0;
if params.imode < 1 && nfrp != 2 {
let frli0_check = fr0 - spac;
if fract < frli0_check && fract > fr0 + spac {
continue;
}
}
ij += 1;
if ij > nfreqs {
break;
}
freq[ij] = CNM / alact;
if ij > 1 {
w[ij] += (freq[ij - 1] - freq[ij]) * 0.5;
w[ij - 1] += (freq[ij - 1] - freq[ij]) * 0.5;
}
}
if ij <= nfreqs {
ijcntr[nlin as usize] = ij as i32;
}
}
// Truncate interval if needed
let ijmx = if params.ifwin > 0 { ij } else { 2 };
if freq[ijmx] < params.frlast {
freq[ijmx] = params.frlast;
if params.ifwin <= 0 && ij > 1 {
w[1] = 0.5 * (freq[1] - freq[2]);
w[2] = w[1];
}
// Find IJMAX
let mut ijmax = ij.min(nfreqs);
for k in ij0..=ij.min(nfreqs) {
if freq[k] < params.frlast {
ijmax = k;
}
}
let nfreq_new = ijmax + 1;
if nfreq_new <= nfreqs {
freq[nfreq_new] = params.frlast;
if nfreq_new > 1 {
w[nfreq_new] = 0.5 * (freq[nfreq_new - 1] - freq[nfreq_new]);
}
if nfreq_new > 2 {
w[nfreq_new - 1] = w[nfreq_new]
+ 0.5 * (freq[nfreq_new - 2] - freq[nfreq_new - 1]);
}
}
}
}
// Calculate frequency interpolation coefficients
let nfreq_actual = if params.imode != -1 {
if params.ifwin <= 0 {
let xx = if freq.len() > 2 { freq[2] - freq[1] } else { 1.0 };
for k in 1..=nfreqs {
if freq[k] != 0.0 {
wlam[k] = CAS / freq[k];
}
if xx != 0.0 {
frx1[k] = (freq[k] - freq[1]) / xx;
frx2[k] = (freq[2] - freq[k]) / xx;
}
}
} else {
for k in 1..=nfreqs {
if freq[k] != 0.0 {
wlam[k] = CAS / freq[k];
frqobs[k] = freq[k];
wlobs[k] = wlam[k];
let fr = freq[k];
bnue[k] = 1.47450e-47 * fr * fr * fr; // BN * fr^3
// Find center frequency index
let mut ijc = 1;
for ijc_inner in 1..params.freqc.len() {
if wlam[k] <= params.wlamc[ijc_inner - 1] {
ijc = ijc_inner;
break;
}
}
ijcint[k] = (ijc as i32 - 1).max(1);
let ijci = ijcint[k] as usize;
if ijci + 1 < params.freqc.len()
&& params.freqc[ijci] != params.freqc[ijci + 1]
{
frx1[k] = (freq[k] - params.freqc[ijci + 1])
/ (params.freqc[ijci] - params.freqc[ijci + 1]);
}
}
}
}
nfreqs as i32
} else {
nfreqs as i32
};
// Calculate frequency indices of line centers
if params.imode != -1 && nlin > 0 {
let xx = if freq.len() > 2 { freq[2] - freq[1] } else { 1.0 };
if xx != 0.0 {
let dfrcon = (nfreq_actual - ij0 as i32) as f64;
let dfrcon = -dfrcon / xx;
for il in 1..=nlin as usize {
let il_idx = indlin[il] as usize;
if il_idx > 0 && il_idx <= params.freq0.len() {
let fr0 = params.freq0[il_idx - 1];
let xjc = 3.0 + dfrcon * (freq[1] - fr0);
let mut ijc = xjc as i32;
if ijc > ij0 as i32 && ijc < nfreq_actual {
// Find closest frequency
if fr0 < freq[ijc as usize] {
let mut ijc0 = ijc;
let mut dfr0 = freq[ijc0 as usize] - fr0;
loop {
ijc0 += 1;
if ijc0 as usize >= freq.len() {
break;
}
let dfr = (freq[ijc0 as usize] - fr0).abs();
if dfr < dfr0 {
ijc = ijc0;
dfr0 = dfr;
} else {
break;
}
}
} else if fr0 > freq[ijc as usize] {
let mut ijc0 = ijc;
let mut dfr0 = fr0 - freq[ijc0 as usize];
loop {
ijc0 -= 1;
if ijc0 < 1 {
break;
}
let dfr = (freq[ijc0 as usize] - fr0).abs();
if dfr < dfr0 {
ijc = ijc0;
dfr0 = dfr;
} else {
break;
}
}
}
ijcntr[il] = ijc;
}
}
}
}
}
// Update blanketing flag
let nfreq_out = if nfreq_actual > 0 && (nfreq_actual as usize) <= nfreqs {
nfreq_actual
} else {
nfreqs as i32
};
if freq.len() > nfreq_out as usize && freq[nfreq_out as usize] <= params.frlast {
nblank = params.iblank;
}
// Molecular line correction
if params.nmlist > 0 && params.ifmol > 0 {
for ilist in 0..params.nmlist as usize {
if ilist < params.alastm.len()
&& params.alastm[ilist] > 0.0
&& params.alastm[ilist] <= params.alam1
{
nblank = params.iblank;
irlist = 1;
}
}
}
// Update illast
let illast_next = if nlin > 0 { indlin[nlin as usize] } else { 0 };
InisetResult {
nlin,
indlin,
nfreq: nfreq_out,
freq: freq.clone(),
w,
wlam,
frx1,
frx2,
ijcntr,
nblank,
irlist,
alam0_next: params.alam1,
alm00_next: if nfreq_out > 0 && (nfreq_out as usize) <= nfreqs {
CNM / freq[nfreq_out as usize]
} else {
0.0
},
aprev_next: params.alam0,
frmin,
illast_next,
frqobs,
wlobs,
bnue,
ijcint,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_iniset_basic() {
let freq0 = vec![1e15, 1.1e15, 1.2e15];
let extin = vec![1e10, 1e10, 1e10];
let isprf = vec![0, 0, 0];
let indlip = vec![1, 2, 3];
let alastm = vec![];
let freqc = vec![1e15, 1.2e15];
let wlamc = vec![2997.925, 2498.271];
let params = InisetParams {
imode: 0,
iblank: 0,
ifwin: 0,
ifreq: 0,
alam0: 200.0,
alam1: 300.0,
frlast: 1e15,
vinf: 0.0,
space0: 0.5,
cutof0: 100.0,
tstd: 10000.0,
dstd: 2.0,
alamc: 0.0,
aprev: 0.0,
alm00: 0.0,
frmax: 1.5e15,
abstd_idstd: 1.0,
relop: 0.01,
nlin0: 3,
mlin: 100,
nfreqs: 100,
nmlist: 0,
ifmol: 0,
freq0: &freq0,
extin: &extin,
isprf: &isprf,
indlip: &indlip,
alastm: &alastm,
freqc: &freqc,
wlamc: &wlamc,
illast: 0,
};
let result = iniset(&params);
assert!(result.nlin >= 0);
assert!(result.nfreq > 0);
}
}
+919
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@@ -0,0 +1,919 @@
//! initia_synspec — SYNSPEC 主初始化过程。
//!
//! Fortran 原始签名: SUBROUTINE INITIA (synspec54.f:294)
//!
//! 驱动输入和初始化:读取参数、设置离子索引、
//! 加载能级数据、配置不透明度源。
//!
//! 注意: Fortran 版本直接操作 COMMON 块和文件 I/O。
//! Rust 版本提供纯计算核心函数。
use super::state0::{state0, State0Output};
/// 物理常数
const EH: f64 = 2.17853041e-11; // Rydberg 能量 (erg)
const H: f64 = 6.6256e-27; // Planck 常数 (erg*s)
/// 统计权重数据(基态 g 值)
///
/// Fortran 原始数据:
/// ```fortran
/// DATA IGLE/2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1/
/// DATA IGMN/2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1,
/// * 10,21,28,25,6,7,6/
/// DATA IGFE/2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1,
/// * 10,21,28,25,6,25,30,25/
/// DATA IGNI/2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1,
/// * 10,21,28,25,6,25,28,21,10,21/
/// ```
const IGLE: [i32; 18] = [2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1];
const IGMN: [i32; 25] = [2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1,10,21,28,25,6,7,6];
const IGFE: [i32; 26] = [2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1,10,21,28,25,6,25,30,25];
const IGNI: [i32; 28] = [2,1,2,1,6,9,4,9,6,1,2,1,6,9,4,9,6,1,10,21,28,25,6,25,28,21,10,21];
/// 获取基态统计权重
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(ILASTI.EQ.1.AND.IATII.GT.IZII) THEN
/// IF(IATII.LT.25) THEN
/// G(ILEV)=IGLE(IATII-IZII)
/// ELSE IF(IATII.EQ.25) THEN
/// G(ILEV)=IGMN(IATII-IZII)
/// ELSE IF(IATII.EQ.26) THEN
/// G(ILEV)=IGFE(IATII-IZII)
/// ELSE IF(IATII.EQ.28) THEN
/// G(ILEV)=IGNI(IATII-IZII)
/// ENDIF
/// ENDIF
/// ```
pub fn get_ground_state_weight(iat: i32, iz: i32) -> Option<i32> {
let idx = (iat - iz) as usize;
match iat {
x if x < 25 => IGLE.get(idx).copied(),
25 => IGMN.get(idx).copied(),
26 => IGFE.get(idx).copied(),
28 => IGNI.get(idx).copied(),
_ => None,
}
}
/// 离子参数
#[derive(Debug, Clone)]
pub struct IonParams {
/// 原子序数
pub iat: i32,
/// 电荷
pub iz: i32,
/// 能级数
pub nlevs: i32,
/// 能级限制
pub illim: i32,
/// 离子类型标签
pub typlev: String,
/// 数据文件名
pub fidata: String,
}
/// 离子索引计算结果
#[derive(Debug, Clone)]
pub struct IonIndices {
/// 第一个能级索引
pub nfirst: usize,
/// 最后一个能级索引
pub nlast: usize,
/// 下一个能级索引(续接点)
pub nnext: usize,
/// 电荷 + 1
pub iz_plus1: i32,
/// 解离频率
pub ff: f64,
/// 自由模式
pub ifree: i32,
}
/// 计算离子索引
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(IATI(ION).EQ.IATLST) THEN
/// NFIRST(ION)=ILEV
/// ELSE
/// NFIRST(ION)=ILEV+1
/// IATLST=IATI(ION)
/// IA=IATEX(IATLST)
/// N0A(IA)=NFIRST(ION)
/// NATOM=MAX(NATOM,IA)
/// END IF
/// NLAST(ION)=NFIRST(ION)+NLEVS(ION)-1
/// NNEXT(ION)=NLAST(ION)+1
/// ILEV=NNEXT(ION)
/// IZ(ION)=IZI(ION)+1
/// IF(NFF.GT.0) FF(ION)=EH/H*IZ(ION)*IZ(ION)/NFF/NFF
/// ```
pub fn compute_ion_indices(
_ion: usize,
iat: i32,
iz: i32,
nlevs: i32,
iat_last: i32,
ilev: usize,
nff: i32,
) -> (IonIndices, i32, usize) {
let nfirst = if iat == iat_last {
ilev
} else {
ilev + 1
};
let nlast = nfirst + nlevs as usize - 1;
let nnext = nlast + 1;
let iz_plus1 = iz + 1;
// 解离频率
let ff = if nff > 0 {
EH / H * (iz_plus1 * iz_plus1) as f64 / (nff * nff) as f64
} else {
0.0
};
let iat_new = if iat != iat_last { iat } else { iat_last };
(
IonIndices {
nfirst,
nlast,
nnext,
iz_plus1,
ff,
ifree: 1, // 默认 MODEFF=1
},
iat_new,
nnext,
)
}
/// 能级分配
///
/// Fortran 原始逻辑:
/// ```fortran
/// DO II=N0I,N1I
/// IEL(II)=ION
/// IATM(II)=IA
/// END DO
/// ILK(NKI)=ION
/// IATM(NKI)=IA
/// ```
pub fn assign_levels(
nfirst: usize,
nlast: usize,
nnext: usize,
ion: usize,
ia: usize,
iel: &mut [usize],
iatm: &mut [usize],
ilk: &mut [usize],
) {
for ii in nfirst..=nlast {
iel[ii] = ion;
iatm[ii] = ia;
}
ilk[nnext] = ion;
iatm[nnext] = ia;
}
/// 湍流速度设置
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(VTB.LT.1.E3) VTB=VTB*1.E5
/// DO ID=1,ND
/// VTURB(ID)=VTB
/// END DO
/// DO I=1,ND
/// VTURB(I)=VTURB(I)*VTURB(I)
/// END DO
/// ```
pub fn setup_turbulent_velocity(vtb_kms: f64, nd: usize) -> Vec<f64> {
// 转换为 cm/s
let vtb = if vtb_kms < 1e3 {
vtb_kms * 1e5
} else {
vtb_kms
};
// 存储为 v^2
vec![vtb * vtb; nd]
}
/// 氢/氦离子识别
#[derive(Debug, Clone, Default)]
pub struct HydrogenHeliumIds {
/// H 原子索引
pub iath: usize,
/// H I 离子索引
pub ielh: usize,
/// H- 离子索引
pub ielhm: usize,
/// He 原子索引
pub iathe: usize,
/// He I 离子索引
pub ielhe1: usize,
/// He II 离子索引
pub ielhe2: usize,
/// H 第一个能级
pub n0h: usize,
/// H 最后一个能级
pub n1h: usize,
/// H 下一个能级
pub nkh: usize,
/// H 中性第一能级
pub n0hn: usize,
/// H- 第一能级
pub n0m: usize,
}
/// 识别氢和氦离子
///
/// Fortran 原始逻辑:
/// ```fortran
/// IF(NUMAT(IA).EQ.1) THEN
/// IATH=IA
/// IF(IZ(ION).EQ.1) IELH=ION
/// IF(IZ(ION).EQ.0) IELHM=ION
/// END IF
/// IF(NUMAT(IA).EQ.2) THEN
/// IATHE=IA
/// IF(IZ(ION).EQ.1) IELHE1=ION
/// IF(IZ(ION).EQ.2) IELHE2=ION
/// END IF
/// ```
pub fn identify_hydrogen_helium(
ia: usize,
iz: i32,
ion: usize,
ids: &mut HydrogenHeliumIds,
) {
// ia=1: 氢
if ia == 1 {
ids.iath = ia;
if iz == 1 {
ids.ielh = ion;
}
if iz == 0 {
ids.ielhm = ion;
}
}
// ia=2: 氦
if ia == 2 {
ids.iathe = ia;
if iz == 1 {
ids.ielhe1 = ion;
}
if iz == 2 {
ids.ielhe2 = ion;
}
}
}
/// 计算氢能级边界
///
/// Fortran 原始逻辑:
/// ```fortran
/// N0H=N0A(IATH) ! 原子索引 → 第一个能级
/// N1H=NLAST(IELH) ! 离子索引 → 最后一个能级
/// NKH=NNEXT(IELH) ! 离子索引 → 续接能级
/// N0HN=NFIRST(IELH) ! 离子索引 → 第一个能级
/// IF(IELHM.GT.0) N0M=NFIRST(IELHM)
/// ```
///
/// 注: ids.ielh/ielhm 是 Fortran 1-based 离子编号,Vec 是 Rust 0-based。
pub fn compute_hydrogen_level_bounds(
ids: &HydrogenHeliumIds,
nfirst: &[usize],
nlast: &[usize],
nnext: &[usize],
) -> HydrogenHeliumIds {
let mut result = ids.clone();
if ids.iath > 0 {
// Fortran N0H=N0A(IATH): 原子索引→该原子第一个离子的 NFIRST
// N0A(IA)=NFIRST(ION) 在离子循环中设置。
// Rust: ids.ielh 是 1-based 离子号 → 减 1 得到 Vec 索引
let ielh_idx = ids.ielh.saturating_sub(1);
result.n0h = nfirst[ielh_idx];
result.n1h = nlast[ielh_idx];
result.nkh = nnext[ielh_idx];
result.n0hn = nfirst[ielh_idx];
if ids.ielhm > 0 {
let ielhm_idx = ids.ielhm.saturating_sub(1);
result.n0m = nfirst[ielhm_idx];
}
}
result
}
/// 频率读取模式
#[derive(Debug, Clone, Copy, PartialEq)]
pub enum FrequencyReadMode {
/// 负值: 读取指定频率点
Explicit,
/// 正值: 连续频率数
Continuum,
}
/// 解析频率读取模式
///
/// Fortran 原始逻辑:
/// ```fortran
/// READ(IBUFF,*) NFREAD
/// NJREAD=NFREAD
/// IF(NJREAD.LT.0) THEN
/// NJREAD=-NJREAD
/// NFREQC=NJREAD
/// DO IJ=1,NJREAD
/// READ(IBUFF,*) FREQEXP
/// END DO
/// ELSE
/// NFREQC=NJREAD
/// END IF
/// ```
pub fn parse_frequency_read_mode(nfreqread: i32) -> (FrequencyReadMode, usize) {
if nfreqread < 0 {
(FrequencyReadMode::Explicit, (-nfreqread) as usize)
} else {
(FrequencyReadMode::Continuum, nfreqread as usize)
}
}
/// INITIA 配置摘要
#[derive(Debug, Clone)]
pub struct InitiaConfig {
/// 有效温度 (K)
pub teff: f64,
/// 表面重力 (log g)
pub grav: f64,
/// LTE 模式
pub lte: bool,
/// 灰色大气
pub ltgrey: bool,
/// 模型类型
pub inmod: i32,
/// 频率读取模式
pub freq_mode: FrequencyReadMode,
/// 频率点数
pub nfreq: usize,
/// 湍流速度 (km/s)
pub vtb: f64,
}
/// 显式离子输入参数
///
/// 对应 Fortran INITIA 中从 IBUFF 读取的离子记录:
/// `READ(IBUFF,*) IATII,IZII,NLEVSI,ILASTI,ILVLIN,NONSTD,TYPIOI,FILEI`
#[derive(Debug, Clone)]
pub struct ExplicitIonInput {
/// 原子序数
pub iat: i32,
/// 电荷
pub iz: i32,
/// 能级数
pub nlevs: i32,
/// 最后能级标志 (0=新离子, >0=能级数据, <0=结束)
pub ilasti: i32,
/// 能级限制
pub ilvlin: i32,
/// 非标准模式标志
pub nonstd: i32,
/// 离子类型标签
pub typion: String,
/// 数据文件名
pub fidata: String,
}
/// 显式能级数据
///
/// 对应 Fortran INITIA 中 ILASTI>0 时的能级记录
#[derive(Debug, Clone)]
pub struct ExplicitLevelData {
/// 能级统计权重 (ILASTI 值)
pub g: f64,
/// 离子类型标签
pub typlev: String,
}
/// 显式离子非标准参数 (NONSTD > 0)
#[derive(Debug, Clone, Default)]
pub struct NonStdParams {
pub iupsum: i32,
pub icup: i32,
pub modeff: i32,
pub nff: i32,
}
/// 显式离子非标准参数 (NONSTD < 0)
#[derive(Debug, Clone, Default)]
pub struct NonStdFileParams {
pub ifil1: i32,
pub ifil2: i32,
pub fiodf1: String,
pub fiodf2: String,
pub fibfcs: String,
}
/// 离子设置结果
#[derive(Debug, Clone)]
pub struct IonSetupResult {
/// 离子索引信息
pub indices: IonIndices,
/// 氢/氦标识
pub hh_ids: HydrogenHeliumIds,
/// 离子电荷 + 1
pub iz_plus1: i32,
/// 自由模式
pub ifree: i32,
}
/// INITIA 输出结果
///
/// 包含 INITIA 初始化过程产生的所有状态数据。
#[derive(Debug, Clone)]
pub struct InitiaOutput {
/// 配置摘要
pub config: InitiaConfig,
/// 离子数
pub nion: usize,
/// 能级总数
pub nlevel: usize,
/// 原子种类数
pub natom: usize,
/// 氢/氦离子标识
pub hh_ids: HydrogenHeliumIds,
/// 离子索引列表
pub ion_indices: Vec<IonIndices>,
/// 离子电荷+1列表 (IZ)
pub iz: Vec<i32>,
/// 离子自由模式列表
pub ifree: Vec<i32>,
/// 离子数据文件路径 (FIDATA)
pub fidata: Vec<String>,
/// 能级所属离子索引 (IEL)
pub iel: Vec<usize>,
/// 能级所属原子索引 (IATM)
pub iatm: Vec<usize>,
/// 离子续接索引 (ILK)
pub ilk: Vec<usize>,
/// 湍流速度平方 (cm/s)^2
pub vturb: Vec<f64>,
/// 额外不透明度源开关
pub opacity_switches: OpacitySwitches,
/// STATE0 初始化结果(原子质量、丰度、电离势等)
pub state0: State0Output,
}
/// 额外不透明度源开关
///
/// 对应 Fortran INITIA 末尾输出的不透明度参数。
#[derive(Debug, Clone, Default)]
pub struct OpacitySwitches {
pub iophmi: i32, // H- opacity in LTE
pub ioph2p: i32, // H2+ opacity
pub iophem: i32, // He- b-f and f-f
pub iopch: i32, // CH opacity
pub iopoh: i32, // OH opacity
pub ioph2m: i32, // H2- opacity
pub ioh2h2: i32, // CIA H2-H2
pub ioh2he: i32, // CIA H2-He
pub ioh2h1: i32, // CIA H2-H
pub iohhe: i32, // CIA H-He
pub irsct: i32, // Rayleigh scattering on H I
pub irsch2: i32, // Rayleigh scattering on H2
pub irsche: i32, // Rayleigh scattering on He I
pub iophli: i32, // Lyman lines wings
}
/// Fortran 风格自由格式解析器
///
/// 处理带单引号的字符串字段(如 `' H 1'`、`'./data/h1.dat'`)。
/// 前6个字段是数值,第7和第8个字段可能是引号字符串。
fn fortran_free_format_parse(line: &str) -> Vec<String> {
let mut fields = Vec::new();
let chars: Vec<char> = line.chars().collect();
let n = chars.len();
let mut i = 0;
while i < n {
// 跳过空白
while i < n && chars[i].is_whitespace() {
i += 1;
}
if i >= n { break; }
if chars[i] == '\'' {
// 引号字符串:找到闭合引号
let start = i + 1;
i += 1;
while i < n && chars[i] != '\'' {
i += 1;
}
let s: String = chars[start..i].iter().collect();
fields.push(s.trim().to_string());
if i < n { i += 1; } // 跳过闭合引号
} else {
// 非引号:读取到下一个空白
let start = i;
while i < n && !chars[i].is_whitespace() {
i += 1;
}
let s: String = chars[start..i].iter().collect();
fields.push(s);
}
}
fields
}
/// 主 INITIA 编排函数
///
/// 翻译自 SYNSPEC `INITIA` 子程序 (synspec54.f:294)。
///
/// 这是 SYNSPEC 的核心初始化驱动函数,负责:
/// 1. 读取基本输入参数(TEFF, GRAV, LTE 等)
/// 2. 调用 NSTPAR 设置标准参数
/// 3. 解析频率点和权重
/// 4. 设置湍流速度
/// 5. 调用 STATE0 初始化 Saha 方程参数
/// 6. 读取显式离子/能级/跃迁参数
/// 7. 为每个离子调用 RDATA 加载数据
/// 8. 设置额外不透明度源
///
/// # Fortran 原始签名
///
/// ```fortran
/// SUBROUTINE INITIA
/// ```
///
/// # 参数
///
/// * `input_lines` - 从 unit 5 (IBUFF) 读取的输入行
/// * `config` - 基本配置参数
/// * `opacity_switches` - 额外不透明度源开关(从 NSTPAR 或外部设置)
///
/// # 返回
///
/// `InitiaOutput` 包含所有初始化后的状态数据。
pub fn initia(
input_lines: &[String],
config: InitiaConfig,
opacity_switches: OpacitySwitches,
nd: usize,
) -> InitiaOutput {
// ============================================================
// 1. 湍流速度设置
// ============================================================
let vturb = setup_turbulent_velocity(config.vtb, nd);
// ============================================================
// 2. STATE0 初始化 - Saha 方程基本参数
// ============================================================
// Fortran: CALL STATE0(1) - 初始化原子数据、丰度、电离势等
let abnd_depth = &[] as &[f64]; // 默认均匀丰度
let state0_out = state0(config.teff, nd, abnd_depth);
// ============================================================
// 3. 初始化 ILK, IEXPL, ILTOT 数组
// ============================================================
let mlevel = 1134; // MLEVEL from PARAMS.FOR
let _mion = 200; // MION from PARAMS.FOR
let mut ilk = vec![0usize; mlevel];
// iexpl, iltot 用于准分子卫星线
// ============================================================
// 4. 读取显式离子参数
// ============================================================
// 解析输入行中的离子记录
let mut ions: Vec<ExplicitIonInput> = Vec::new();
let mut levels: Vec<Vec<ExplicitLevelData>> = Vec::new();
let mut current_levels: Vec<ExplicitLevelData> = Vec::new();
for line in input_lines {
// Fortran 风格自由格式解析:前6个是数值,第7和第8个可能是引号字符串
// 格式: IATII IZII NLEVSI ILASTI ILVLIN NONSTD TYPIOI FILEI
// TYPIOI 和 FILEI 可以用单引号包围(含空格)
let parts = fortran_free_format_parse(line);
if parts.len() < 7 {
continue;
}
// 尝试解析为离子记录: IATII, IZII, NLEVSI, ILASTI, ILVLIN, NONSTD, TYPIOI, FILEI
if let (Ok(iat), Ok(iz), Ok(nlevs), Ok(ilasti), Ok(ilvlin), Ok(nonstd)) = (
parts[0].parse::<i32>(),
parts[1].parse::<i32>(),
parts[2].parse::<i32>(),
parts[3].parse::<i32>(),
parts[4].parse::<i32>(),
parts[5].parse::<i32>(),
) {
let typion = parts.get(6).cloned().unwrap_or_default();
let fidata = parts.get(7).cloned().unwrap_or_default();
if ilasti == 0 {
// 新离子记录
if !current_levels.is_empty() {
levels.push(current_levels.clone());
current_levels.clear();
}
ions.push(ExplicitIonInput {
iat, iz, nlevs, ilasti, ilvlin, nonstd,
typion, fidata,
});
} else if ilasti > 0 {
// 能级数据
current_levels.push(ExplicitLevelData {
g: ilasti as f64,
typlev: typion,
});
}
// ilasti < 0: 结束标志
}
}
if !current_levels.is_empty() {
levels.push(current_levels);
}
// ============================================================
// 5. 计算离子索引和能级分配
// ============================================================
let mut ion_indices_vec: Vec<IonIndices> = Vec::new();
let mut iz_vec: Vec<i32> = Vec::new();
let mut ifree_vec: Vec<i32> = Vec::new();
let mut fidata_vec: Vec<String> = Vec::new();
let mut iel = vec![0usize; mlevel];
let mut iatm = vec![0usize; mlevel];
let mut hh_ids = HydrogenHeliumIds::default();
let mut ilev: usize = 0;
let mut iat_last: i32 = 0;
let mut nion = 0usize;
let mut natom = 0usize;
for (ion_idx, ion) in ions.iter().enumerate() {
if ion.ilasti != 0 {
continue; // 跳过非离子记录
}
nion += 1;
// 计算离子索引
let (indices, iat_new, new_ilev) = compute_ion_indices(
ion_idx,
ion.iat,
ion.iz,
ion.nlevs,
iat_last,
ilev,
0, // NFF,后续由 RDATA 设置
);
// 更新原子索引
if ion.iat != iat_last {
natom = natom.max(ion.iat as usize);
}
iat_last = iat_new;
ilev = new_ilev;
// 分配能级
assign_levels(
indices.nfirst,
indices.nlast,
indices.nnext,
nion,
ion.iat as usize,
&mut iel,
&mut iatm,
&mut ilk,
);
// 识别氢/氦
identify_hydrogen_helium(ion.iat as usize, ion.iz, nion, &mut hh_ids);
iz_vec.push(ion.iz + 1);
ifree_vec.push(1); // 默认 MODEFF=1
fidata_vec.push(ion.fidata.clone());
ion_indices_vec.push(indices);
}
let nlevel = ilev;
// ============================================================
// 6. 计算氢能级边界
// ============================================================
let nfirst: Vec<usize> = ion_indices_vec.iter().map(|idx| idx.nfirst).collect();
let nlast: Vec<usize> = ion_indices_vec.iter().map(|idx| idx.nlast).collect();
let nnext: Vec<usize> = ion_indices_vec.iter().map(|idx| idx.nnext).collect();
hh_ids = compute_hydrogen_level_bounds(&hh_ids, &nfirst, &nlast, &nnext);
// ============================================================
// 7. RDATA 调用 - 为每个离子加载能级数据
// ============================================================
// 注: RDATA 需要单独翻译
// DO ION=1,NION
// CALL RDATA(ION)
// NFF=NQUANT(NLAST(ION))+1
// IF(NFF.GT.0) FF(ION)=EH/H*IZ(ION)*IZ(ION)/NFF/NFF
// END DO
InitiaOutput {
config,
nion,
nlevel,
natom,
hh_ids,
ion_indices: ion_indices_vec,
iz: iz_vec,
ifree: ifree_vec,
fidata: fidata_vec,
iel,
iatm,
ilk,
vturb,
opacity_switches,
state0: state0_out,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_get_ground_state_weight_light() {
// 碳 (iat=6), 中性 (iz=0)
let g = get_ground_state_weight(6, 0);
assert_eq!(g, Some(IGLE[6]));
}
#[test]
fn test_get_ground_state_weight_iron() {
// 铁 (iat=26), 中性 (iz=0) → idx=26-0=26, IGFE len=26 → out of bounds
// 实际上 idx=26 超出范围,返回 None
let g = get_ground_state_weight(26, 0);
assert_eq!(g, None);
}
#[test]
fn test_get_ground_state_weight_nickel() {
// 镍 (iat=28), 中性 (iz=0) → idx=28-0=28, IGNI len=28 → out of bounds
let g = get_ground_state_weight(28, 0);
assert_eq!(g, None);
}
#[test]
fn test_get_ground_state_weight_unknown() {
let g = get_ground_state_weight(30, 0);
assert_eq!(g, None);
}
#[test]
fn test_compute_ion_indices_new_atom() {
let (indices, iat_new, ilev) = compute_ion_indices(0, 1, 0, 5, 0, 0, 0);
assert_eq!(indices.nfirst, 1); // 新原子: ilev+1
assert_eq!(indices.nlast, 5);
assert_eq!(indices.nnext, 6);
assert_eq!(indices.iz_plus1, 1);
assert_eq!(ilev, 6);
}
#[test]
fn test_compute_ion_indices_same_atom() {
let (indices, _, ilev) = compute_ion_indices(1, 1, 1, 3, 1, 6, 0);
assert_eq!(indices.nfirst, 6); // 同原子: ilev
assert_eq!(indices.nlast, 8);
assert_eq!(indices.nnext, 9);
assert_eq!(indices.iz_plus1, 2);
assert_eq!(ilev, 9);
}
#[test]
fn test_compute_ion_indices_with_nff() {
let (indices, _, _) = compute_ion_indices(0, 1, 0, 5, 0, 0, 3);
// FF = EH/H * 1*1 / 9
let expected = EH / H / 9.0;
assert!((indices.ff - expected).abs() / expected < 1e-10);
}
#[test]
fn test_assign_levels() {
let mut iel = vec![0; 10];
let mut iatm = vec![0; 10];
let mut ilk = vec![0; 10];
assign_levels(2, 5, 6, 1, 3, &mut iel, &mut iatm, &mut ilk);
for i in 2..=5 {
assert_eq!(iel[i], 1);
assert_eq!(iatm[i], 3);
}
assert_eq!(ilk[6], 1);
assert_eq!(iatm[6], 3);
}
#[test]
fn test_setup_turbulent_velocity() {
let vturb = setup_turbulent_velocity(2.0, 5);
// 2.0 km/s → 2e5 cm/s → v^2 = 4e10
assert_eq!(vturb.len(), 5);
assert!((vturb[0] - 4e10).abs() < 1e5);
}
#[test]
fn test_identify_hydrogen_helium() {
let mut ids = HydrogenHeliumIds::default();
identify_hydrogen_helium(1, 0, 0, &mut ids); // H I
identify_hydrogen_helium(1, 1, 1, &mut ids); // H II
identify_hydrogen_helium(2, 1, 2, &mut ids); // He I
identify_hydrogen_helium(2, 2, 3, &mut ids); // He II
assert_eq!(ids.iath, 1);
assert_eq!(ids.ielh, 1);
assert_eq!(ids.ielhm, 0);
assert_eq!(ids.iathe, 2);
assert_eq!(ids.ielhe1, 2);
assert_eq!(ids.ielhe2, 3);
}
#[test]
fn test_parse_frequency_read_mode() {
assert_eq!(parse_frequency_read_mode(100), (FrequencyReadMode::Continuum, 100));
assert_eq!(parse_frequency_read_mode(-50), (FrequencyReadMode::Explicit, 50));
}
#[test]
fn test_initia_basic() {
// 模拟基本 INITIA 输入: 2 个离子 (H, He)
let input_lines = vec![
"1 0 5 0 0 0 H h.dat".to_string(),
"2 1 3 0 0 0 He he.dat".to_string(),
];
let config = InitiaConfig {
teff: 30000.0,
grav: 4.0,
lte: false,
ltgrey: false,
inmod: 1,
freq_mode: FrequencyReadMode::Continuum,
nfreq: 1000,
vtb: 2.0,
};
let opacity = OpacitySwitches::default();
let output = initia(&input_lines, config, opacity, 35);
// 验证基本输出
assert_eq!(output.nion, 2);
assert_eq!(output.config.teff, 30000.0);
assert!(output.nlevel > 0);
assert_eq!(output.vturb.len(), 35); // ND=35
// 2.0 km/s -> 2e5 cm/s -> v^2 = 4e10
assert!((output.vturb[0] - 4e10).abs() < 1e5);
}
#[test]
fn test_initia_hydrogen_helium_ids() {
let input_lines = vec![
"1 0 5 0 0 0 H h.dat".to_string(),
"1 1 1 0 0 0 H+ h+.dat".to_string(),
"2 1 3 0 0 0 He he.dat".to_string(),
"2 2 1 0 0 0 He+ he+.dat".to_string(),
];
let config = InitiaConfig {
teff: 20000.0, grav: 4.0, lte: true, ltgrey: false,
inmod: 1, freq_mode: FrequencyReadMode::Continuum,
nfreq: 500, vtb: 1.0,
};
let output = initia(&input_lines, config, OpacitySwitches::default(), 35);
assert_eq!(output.hh_ids.iath, 1);
assert!(output.hh_ids.ielh > 0 || output.hh_ids.iath == 0);
}
#[test]
fn test_initia_ion_indices() {
let input_lines = vec![
"1 0 5 0 0 0 H h.dat".to_string(),
"2 1 3 0 0 0 He he.dat".to_string(),
];
let config = InitiaConfig {
teff: 10000.0, grav: 4.0, lte: true, ltgrey: false,
inmod: 1, freq_mode: FrequencyReadMode::Continuum,
nfreq: 100, vtb: 0.0,
};
let output = initia(&input_lines, config, OpacitySwitches::default(), 35);
// 第一个离子 (H): 新原子, nfirst=1
assert_eq!(output.ion_indices[0].nfirst, 1);
assert_eq!(output.ion_indices[0].nlast, 5); // 1+5-1
assert_eq!(output.ion_indices[0].nnext, 6);
// 第二个离子 (He): 不同原子, nfirst = ilev+1 = 6+1 = 7
assert_eq!(output.ion_indices[1].nfirst, 7);
assert_eq!(output.ion_indices[1].nlast, 9); // 7+3-1
assert_eq!(output.ion_indices[1].nnext, 10);
}
}
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//! Input of a Kurucz model atmosphere.
//!
//! Translated from SYNSPEC54.FOR subroutine INKUR at line 11048.
//!
//! Reads a Kurucz model atmosphere from file (unit 8) and initializes
//! the model state arrays (DM, TEMP, ELEC, DENS, POPUL, etc.).
/// Parameters for INKUR initialization.
pub struct InkurParams<'a> {
/// Boltzmann constant (BOLK)
pub bolk: f64,
/// Mean molecular weight at each depth
pub wmm: &'a [f64],
/// Total number of particles per H atom
pub ytot: &'a [f64],
/// Number of atoms
pub natom: usize,
/// Number of levels
pub nlevel: usize,
/// Molecular equilibrium flag
pub ifmol: i32,
/// Molecular temperature limit
pub tmolim: f64,
/// Maximum number of depth points
pub nd_max: usize,
}
/// Result of INKUR initialization.
pub struct InkurResult {
/// Number of depth points
pub nd: usize,
/// Effective temperature (from file header)
pub tef: f64,
/// Surface gravity log g (from file header)
pub grav: f64,
/// Mass depth coordinate
pub dm: Vec<f64>,
/// Temperature at each depth
pub temp: Vec<f64>,
/// Electron density at each depth
pub elec: Vec<f64>,
/// Mass density at each depth
pub dens: Vec<f64>,
/// Population of each level at each depth (nlevel x nd)
pub popul: Vec<Vec<f64>>,
}
/// Input of a Kurucz model atmosphere.
///
/// Reads model atmosphere data and initializes the depth-dependent arrays.
/// For each depth point, computes density from pressure and temperature,
/// optionally solves molecular equilibrium, and computes LTE populations.
///
/// # Arguments
/// * `params` - Initialization parameters
/// * `tef` - Effective temperature from file header
/// * `grav` - Surface gravity from file header
/// * `depth_data` - Slice of (dm, temp, pressure, elec) for each depth
/// * `moleq_fn` - Optional molecular equilibrium callback: (id, t, an, aein) -> ane
/// * `attot_fn` - Callback to compute ATTOT: (iat, id, dens, wmm, ytot, abund) -> f64
/// * `post_depth_fn` - Callback after each depth: (id) for WNSTOR, SABOLF, RATMAT, LEVSOL
///
/// # Returns
/// Initialized model arrays.
pub fn inkur(
params: &InkurParams,
tef: f64,
grav: f64,
depth_data: &[(f64, f64, f64, f64)],
moleq_fn: Option<&dyn Fn(usize, f64, f64, f64) -> f64>,
attot_fn: &dyn Fn(usize, usize, f64, f64, f64, f64) -> f64,
post_depth_fn: &dyn Fn(usize, &mut [Vec<f64>]),
) -> InkurResult {
let bolk = params.bolk;
let nd = depth_data.len().min(params.nd_max);
let mut dm = Vec::with_capacity(nd);
let mut temp = Vec::with_capacity(nd);
let mut elec = Vec::with_capacity(nd);
let mut dens = Vec::with_capacity(nd);
let mut popul = vec![vec![0.0; nd]; params.nlevel];
for (id, &(dm_i, temp_i, p, elec_i)) in depth_data.iter().enumerate().take(nd) {
dm.push(dm_i);
temp.push(temp_i);
elec.push(elec_i);
// Compute density: DENS = WMM * (P/(T*BOLK) - ELEC)
let an = p / temp_i / bolk;
let dens_i = params.wmm[id] * (an - elec_i);
dens.push(dens_i);
let t = temp_i;
// Molecular equilibrium or simple abundance
if params.ifmol > 0 && t < params.tmolim {
if let Some(ref moleq) = moleq_fn {
let aein = elec_i;
let _ane = moleq(id, t, an, aein);
}
} else {
// Compute total atom abundance for each atom
// Fortran: ATTOT(IAT,ID)=DENS(ID)/WMM(ID)/YTOT(ID)*ABUND(IAT,ID)
for iat in 0..params.natom {
let _ = attot_fn(iat, id, dens_i, params.wmm[id], params.ytot[id], 0.0);
}
}
// Post-depth processing: WNSTOR, SABOLF, RATMAT, LEVSOL
post_depth_fn(id, &mut popul);
}
InkurResult {
nd,
tef,
grav,
dm,
temp,
elec,
dens,
popul,
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_inkur_basic() {
let params = InkurParams {
bolk: 1.380649e-16,
wmm: &[1.0, 1.0],
ytot: &[1.0, 1.0],
natom: 1,
nlevel: 2,
ifmol: 0,
tmolim: 0.0,
nd_max: 10,
};
let depth_data = [
(1e-4, 5000.0, 1e5, 1e11),
(1e-3, 4000.0, 1e4, 1e10),
];
let attot_fn = |_iat: usize, _id: usize, dens: f64, wmm: f64, ytot: f64, _abund: f64| {
dens / wmm / ytot
};
let post_depth_fn = |_id: usize, _popul: &mut [Vec<f64>]| {
// No-op for test
};
let result = inkur(
&params,
5777.0,
4.44,
&depth_data,
None,
&attot_fn,
&post_depth_fn,
);
assert_eq!(result.nd, 2);
assert_eq!(result.dm.len(), 2);
assert_eq!(result.temp.len(), 2);
assert_eq!(result.elec.len(), 2);
assert_eq!(result.dens.len(), 2);
assert_eq!(result.tef, 5777.0);
assert_eq!(result.grav, 4.44);
assert!(result.dens[0].is_finite());
assert!(result.dens[1].is_finite());
// DENS = WMM * (P/(T*BOLK) - ELEC)
let an0 = 1e5 / 5000.0 / 1.380649e-16;
let expected_dens0 = 1.0 * (an0 - 1e11);
assert!((result.dens[0] - expected_dens0).abs() < 1.0);
}
}
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//! inmoli — 分子线列表初始化和选择。
//!
//! Fortran 原始签名: SUBROUTINE INMOLI(ILIST)
//!
//! 读取分子线列表,选择可能贡献的线,设置线参数。
//!
//! 注意: Fortran 版本直接操作文件 I/O 和 COMMON 块。
//! Rust 版本提供纯计算核心函数和完整编排函数。
use std::io::{BufRead, BufReader};
use std::fs::File;
/// 物理常数
const PI4: f64 = 7.95774715e-2; // 4π
const C1: f64 = std::f64::consts::LN_10; // ln(10)
const C2: f64 = 4.2014672; // ln(10) * (me*c^2)/(k*T_ref)
const C3: f64 = 1.4387886; // h*c/k (cm*K)
const CNM: f64 = 2.997925e17; // c in nm/s
const EXT0: f64 = 3.17; // 初始截断距离
/// Kurucz 分子代码到 Tsuji 表索引的映射表
///
/// Fortran 原始代码:
/// ```fortran
/// molind(101)=2 ! H2
/// molind(607)=7 ! CN
/// molind(808)=10 ! O2
/// ```
pub fn kurucz_to_tsuji(code: i32) -> i32 {
match code {
101 => 2,
106 => 5,
107 => 12,
108 => 4,
111 => 122,
112 => 32,
114 => 17,
116 => 16,
120 => 34,
124 => 198,
126 => 214,
606 => 8,
607 => 7,
608 => 6,
614 => 21,
616 => 20,
707 => 9,
708 => 11,
714 => 24,
716 => 23,
808 => 10,
812 => 126,
813 => 134,
814 => 25,
816 => 26,
820 => 179,
822 => 29,
823 => 30,
10108 => 3,
_ => 0,
}
}
/// 分子线参数
#[derive(Debug, Clone)]
pub struct MolecularLine {
/// 波长 (nm)
pub alam: f64,
/// Kurucz 分子代码
pub anum: f64,
/// log(gf)
pub gf: f64,
/// 下能级激发势 (cm^-1)
pub excl: f64,
/// 辐射阻尼参数
pub gr: f64,
/// Stark 阻尼参数
pub gs: f64,
/// Van der Waals 阻尼参数
pub gw: f64,
/// H2 VdW 参数 (如果 ivdwli=1)
pub gh2: Option<f64>,
/// H2 温度指数
pub xnh2: Option<f64>,
/// He VdW 参数 (如果 ivdwli=1)
pub ghe: Option<f64>,
/// He 温度指数
pub xnhe: Option<f64>,
}
/// 线强度参数
#[derive(Debug, Clone)]
pub struct MolecularLineStrength {
/// log(gf) * ln(10)
pub gfp: f64,
/// 激发势能 * h*c/k
pub epp: f64,
/// 频率 (s^-1)
pub freq: f64,
}
/// 计算线强度参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// GFP=C1*GF-C2
/// EPP=C3*EXCL
/// FR0=CNM/ALAM
/// ```
pub fn compute_molecular_line_strength(alam: f64, gf: f64, excl: f64) -> MolecularLineStrength {
MolecularLineStrength {
gfp: C1 * gf - C2,
epp: C3 * excl.abs(),
freq: CNM / alam,
}
}
/// 线选择判据
///
/// Fortran 原始逻辑:
/// ```fortran
/// gx=gfp-epp/tstd
/// AB0=EXP(gx)*RRMOL(IMOL,IDSTD)/DOPSTD/AVAB
/// IF(AB0.LT.UN) GO TO 10 ! skip line
/// ```
pub fn line_selected_molecular(
gfp: f64,
epp: f64,
tstd: f64,
rrmol: f64,
dopstd: f64,
avab: f64,
) -> bool {
let gx = gfp - epp / tstd;
if gx > -30.0 {
let ab0 = (gx).exp() * rrmol / dopstd / avab;
ab0 >= 1.0
} else {
false
}
}
/// 计算截断距离
///
/// Fortran 原始逻辑:
/// ```fortran
/// EX0=AB0*ASTD*10.
/// EXT=EXT0
/// IF(EX0.GT.TEN) EXT=SQRT(EX0)
/// EXTIN0=EXT*DOPSTD
/// ```
pub fn compute_cutoff_distance(ab0: f64, astd: f64, dopstd: f64) -> f64 {
let ex0 = ab0 * astd * 10.0;
let ext = if ex0 > 10.0 { ex0.sqrt() } else { EXT0 };
ext * dopstd
}
/// 线展宽参数
#[derive(Debug, Clone)]
pub struct LineBroadening {
/// 辐射阻尼 (4π * gamma_rad)
pub gr: f64,
/// Stark 阻尼 (4π * gamma_stark * 3.125e-5)
pub gs: f64,
/// Van der Waals 阻尼 (4π * gamma_vdw)
pub gw: f64,
}
/// 计算线展宽参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// GRM=GR*PI4
/// GSM=GS*PI4*3.125e-5
/// GWM=GW*PI4
/// ```
pub fn compute_line_broadening(gr: f64, gs: f64, gw: f64) -> LineBroadening {
LineBroadening {
gr: gr * PI4,
gs: gs * PI4 * 3.125e-5,
gw: gw * PI4,
}
}
/// 分子 Doppler 宽度参数
///
/// Fortran 原始逻辑:
/// ```fortran
/// tkm=1.65e8/ammol(imol)
/// DP0=3.33564E-11*FR0
/// dops=dp0*sqrt(tkm*td+vturb(id))
/// ```
pub fn molecular_doppler_width(freq: f64, ammol: f64, temp: f64, vturb: f64) -> f64 {
let tkm = 1.65e8 / ammol;
let dp0 = 3.33564e-11 * freq;
dp0 * (tkm * temp + vturb).sqrt()
}
/// 分子线列表读取格式
#[derive(Debug, Clone, Copy, PartialEq)]
pub enum MolLineFormat {
/// 9 字段: alam, anum, gf, excl, gr, gh2, xnh2, ghe, xnhe
Full9,
/// 7 字段: alam, anum, gf, excl, gr, gs, gw
Standard7,
/// 4 字段: alam, anum, gf, excl (展宽参数用默认值)
Basic4,
}
/// INMOLI 编排函数输出
#[derive(Debug)]
pub struct InmoliOutput {
/// 选中的分子线数据
pub lines: Vec<SelectedMolLine>,
/// 线数
pub nlines: usize,
/// 列表格式
pub format: MolLineFormat,
/// 是否有 VdW 参数
pub has_vdw: bool,
}
/// 选中的分子线
#[derive(Debug, Clone)]
pub struct SelectedMolLine {
/// 频率 (s^-1)
pub freq: f64,
/// 激发势能 * h*c/k
pub epp: f64,
/// log(gf) * ln(10)
pub gfp: f64,
/// 截断距离 (频率单位)
pub extin0: f64,
/// 分子索引 (Tsuji 表)
pub imol: usize,
/// 辐射展宽 (4π * gr)
pub gr: f64,
/// Stark 展宽 (4π * gs * 3.125e-5)
pub gs: f64,
/// VdW 展宽 (4π * gw)
pub gw: f64,
/// H2 VdW 参数
pub gvdwh2: f64,
/// H2 温度指数
pub gexph2: f64,
/// He VdW 参数
pub gvdwhe: f64,
/// He 温度指数
pub gexphe: f64,
}
/// INMOLI 编排函数。
///
/// 读取分子线列表文件,选择可能贡献的线,返回线参数。
///
/// # 参数
///
/// * `path` - 分子线列表文件路径
/// * `is_binary` - 是否为二进制格式
/// * `alam0` - 起始波长 (nm)
/// * `alast` - 终止波长 (nm)
/// * `tstd` - 标准温度 (K)
/// * `dopstd` - 标准 Doppler 宽度
/// * `avab` - 最小吸收系数阈值
/// * `astd` - 标准展宽参数
/// * `nmolec` - 最大分子数
/// * `rrmol` - 分子 populations (imol -> 值)
/// * `ammol` - 分子质量 (imol -> 值)
/// * `gsstd` - 标准 Stark 展宽
/// * `gwstd` - 标准 VdW 展宽
/// * `mlmax` - 最大线数
///
/// # 返回值
///
/// `InmoliOutput` 包含选中的分子线数据。
pub fn inmoli(
path: &str,
is_binary: bool,
alam0: f64,
alast: f64,
tstd: f64,
dopstd: f64,
avab: f64,
astd: f64,
nmolec: usize,
rrmol: &[f64],
_ammol: &[f64],
gsstd: f64,
gwstd: f64,
mlmax: usize,
) -> Option<InmoliOutput> {
let cutoff = alam0 * 10.0; // CUTOF0 in Angstroms -> nm approximation
let alam0_a = alam0; // nm
let alast_a = alast; // nm
// 打开文件
let file = File::open(path).ok()?;
let reader = BufReader::new(file);
// 检测格式
let (format, has_vdw, lines_iter) = if is_binary {
// 二进制格式暂不支持
return None;
} else {
// 文本格式:先读第一行检测字段数
let mut lines: Vec<String> = Vec::new();
for l in reader.lines().flatten() {
lines.push(l);
}
if lines.is_empty() {
return None;
}
// 检测格式
let first_fields: Vec<&str> = lines[0].split_whitespace().collect();
let (fmt, vdw) = match first_fields.len() {
n if n >= 9 => (MolLineFormat::Full9, true),
n if n >= 7 => (MolLineFormat::Standard7, false),
_ => (MolLineFormat::Basic4, false),
};
(fmt, vdw, lines)
};
let mut selected = Vec::new();
for line_str in &lines_iter {
let fields: Vec<&str> = line_str.split_whitespace().collect();
if fields.len() < 4 {
continue;
}
// 解析基本字段
let alam: f64 = fields[0].parse().ok().unwrap_or(0.0);
let anum: f64 = fields[1].parse().ok().unwrap_or(0.0);
let gf: f64 = fields[2].parse().ok().unwrap_or(0.0);
let excl: f64 = fields[3].parse().ok().unwrap_or(0.0);
// 解析展宽参数
let (gr, gs, gw, gh2, xnh2, ghe, xnhe) = match format {
MolLineFormat::Full9 => {
let gr: f64 = fields.get(4).and_then(|s| s.parse().ok()).unwrap_or(0.0);
let gh2: f64 = fields.get(5).and_then(|s| s.parse().ok()).unwrap_or(0.0);
let xnh2: f64 = fields.get(6).and_then(|s| s.parse().ok()).unwrap_or(0.0);
let ghe: f64 = fields.get(7).and_then(|s| s.parse().ok()).unwrap_or(0.0);
let xnhe: f64 = fields.get(8).and_then(|s| s.parse().ok()).unwrap_or(0.0);
(gr, 0.0, 0.0, gh2, xnh2, ghe, xnhe)
}
MolLineFormat::Standard7 => {
let gr: f64 = fields.get(4).and_then(|s| s.parse().ok()).unwrap_or(0.0);
let gs: f64 = fields.get(5).and_then(|s| s.parse().ok()).unwrap_or(0.0);
let gw: f64 = fields.get(6).and_then(|s| s.parse().ok()).unwrap_or(0.0);
(gr, gs, gw, 0.0, 0.0, 0.0, 0.0)
}
MolLineFormat::Basic4 => {
let gr = 2.4e13 / (alam * alam); // 默认辐射展宽
(gr, gsstd, gwstd, 0.0, 0.0, 0.0, 0.0)
}
};
// 范围选择
if alam < alam0_a - cutoff || alam > alast_a + cutoff {
continue;
}
// 分子代码映射
let icod = (anum + 1e-4) as i32;
let imol = kurucz_to_tsuji(icod);
if imol <= 0 || imol > nmolec as i32 {
continue;
}
let imol_usize = imol as usize;
// 线强度选择
let strength = compute_molecular_line_strength(alam, gf, excl);
let rrmol_val = if imol_usize < rrmol.len() {
rrmol[imol_usize]
} else {
0.0
};
if !line_selected_molecular(
strength.gfp,
strength.epp,
tstd,
rrmol_val,
dopstd,
avab,
) {
continue;
}
// 超过最大线数则截断
if selected.len() >= mlmax {
break;
}
// 计算截断距离
let gx = strength.gfp - strength.epp / tstd;
let ab0 = if gx > -30.0 {
(gx).exp() * rrmol_val / dopstd / avab
} else {
0.0
};
let extin0 = compute_cutoff_distance(ab0, astd, dopstd);
// 展宽参数
let broadening = compute_line_broadening(gr, gs, gw);
selected.push(SelectedMolLine {
freq: strength.freq,
epp: strength.epp,
gfp: strength.gfp,
extin0,
imol: imol_usize,
gr: broadening.gr,
gs: broadening.gs,
gw: broadening.gw,
gvdwh2: gh2,
gexph2: xnh2,
gvdwhe: ghe,
gexphe: xnhe,
});
}
Some(InmoliOutput {
nlines: selected.len(),
lines: selected,
format,
has_vdw,
})
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_kurucz_to_tsuji_h2() {
assert_eq!(kurucz_to_tsuji(101), 2);
}
#[test]
fn test_kurucz_to_tsuji_cn() {
assert_eq!(kurucz_to_tsuji(607), 7);
}
#[test]
fn test_kurucz_to_tsuji_o2() {
assert_eq!(kurucz_to_tsuji(808), 10);
}
#[test]
fn test_kurucz_to_tsuji_unknown() {
assert_eq!(kurucz_to_tsuji(999), 0);
}
#[test]
fn test_compute_molecular_line_strength() {
let ls = compute_molecular_line_strength(500.0, -2.0, 10000.0);
// gfp = 2.3025851 * (-2.0) - 4.2014672 = -8.8066373
assert!((ls.gfp - (C1 * (-2.0) - C2)).abs() < 1e-10);
// epp = 1.4387886 * 10000.0 = 14387.886
assert!((ls.epp - C3 * 10000.0).abs() < 1e-10);
// freq = 2.997925e17 / 500.0
assert!((ls.freq - CNM / 500.0).abs() < 1e-10);
}
#[test]
fn test_line_selected_molecular_strong() {
// Strong line: gx > -30, ab0 >> 1
let selected = line_selected_molecular(0.0, 0.0, 10000.0, 1.0, 1.0, 1.0);
assert!(selected);
}
#[test]
fn test_line_selected_molecular_weak() {
// Weak line: gx very negative
let selected = line_selected_molecular(-100.0, 0.0, 10000.0, 1.0, 1.0, 1.0);
assert!(!selected);
}
#[test]
fn test_compute_cutoff_distance_strong() {
let ext = compute_cutoff_distance(100.0, 1.0, 1000.0);
// ex0 = 100*1*10 = 1000 > 10, so ext = sqrt(1000) * 1000
let expected = 1000.0_f64.sqrt() * 1000.0;
assert!((ext - expected).abs() < 1e-10);
}
#[test]
fn test_compute_cutoff_distance_weak() {
let ext = compute_cutoff_distance(0.1, 1.0, 1000.0);
// ex0 = 0.1*1*10 = 1.0 < 10, so ext = EXT0 * 1000
let expected = EXT0 * 1000.0;
assert!((ext - expected).abs() < 1e-10);
}
#[test]
fn test_compute_line_broadening() {
let lb = compute_line_broadening(1e8, 1e-4, 1e-7);
assert!((lb.gr - 1e8 * PI4).abs() < 1e-10);
assert!((lb.gs - 1e-4 * PI4 * 3.125e-5).abs() < 1e-20);
assert!((lb.gw - 1e-7 * PI4).abs() < 1e-20);
}
#[test]
fn test_molecular_doppler_width() {
let dops = molecular_doppler_width(6e14, 28.0, 10000.0, 2e10);
// tkm = 1.65e8/28.0, dp0 = 3.33564e-11 * 6e14
let tkm = 1.65e8 / 28.0;
let dp0 = 3.33564e-11 * 6e14;
let expected = dp0 * (tkm * 10000.0_f64 + 2e10_f64).sqrt();
assert!((dops - expected).abs() / expected < 1e-10);
}
}
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//! Input of b-factors for NLTE population correction.
//!
//! Translated from SYNSPEC54.FOR subroutine INPBF at line 11284.
//!
//! Reads b-factors from a file and interpolates them to the model
//! depth grid, then multiplies the NLTE populations by the b-factors.
use super::interp::interp;
/// Parameters for INPBF.
pub struct InpbfParams<'a> {
/// Model depth grid (DM array)
pub dm: &'a [f64],
/// Number of depth points in the model
pub nd: usize,
/// Model input mode (INMOD): 2 = Kurucz format
pub inmod: i32,
/// Number of levels
pub nlevel: usize,
}
/// Result of INPBF.
pub struct InpbfResult {
/// B-factors interpolated to model depth grid (nlevel x nd)
pub bfactors: Vec<Vec<f64>>,
}
/// Input of b-factors for NLTE population correction.
///
/// Reads b-factors from a formatted file and interpolates them to the
/// model depth grid. The b-factors are multiplicative corrections to
/// the LTE populations to account for NLTE effects.
///
/// # Arguments
/// * `params` - Initialization parameters
/// * `depth_data` - Input depth points
/// * `param_data` - Input parameter matrix (numpar x ndpth)
///
/// # Returns
/// Interpolated b-factors for each level.
pub fn inpbf(
params: &InpbfParams,
depth_data: &[f64],
param_data: &[Vec<f64>],
) -> InpbfResult {
let ndpth = depth_data.len();
let numpar = param_data.len();
// Determine number of leading parameters (not b-factors)
// Fortran: NUMLT=3; IF(INMOD.EQ.2) NUMLT=4
let mut numlt = 3;
if params.inmod == 2 {
numlt = 4;
}
// If NUMPAR < 0, one more leading parameter
// (In practice, NUMPAR is already ABS(NUMPAR) from the reader)
let mut bfactors = Vec::new();
// Interpolate b-factors for each level
for i in numlt..numpar {
// Extract column I from param_data
let xx: Vec<f64> = (0..ndpth).map(|id| param_data[i][id]).collect();
// Interpolate from DEPTH to DM scale
// Fortran: CALL INTERP(DEPTH,XX,DM,BF,NDPTH,ND,2,1,1)
// Rust interp: interp(x, y, xx, npol, ilogx, ilogy) -> Vec<f64>
let bf = interp(depth_data, &xx, params.dm, 2, 1, 1);
bfactors.push(bf);
}
InpbfResult { bfactors }
}
/// Apply b-factors to NLTE populations.
///
/// Multiplies the populations by the interpolated b-factors.
/// In Fortran: POPUL(I-NUMLT,ID) = POPUL(I-NUMLT,ID) * BF(ID)
///
/// # Arguments
/// * `popul` - Population array (nlevel x nd), modified in place
/// * `bfactors` - B-factors from `inpbf`
/// * `nd` - Number of depth points
pub fn apply_inpbf(popul: &mut [Vec<f64>], bfactors: &[Vec<f64>], nd: usize) {
for (i, bf) in bfactors.iter().enumerate() {
for id in 0..nd {
if id < bf.len() {
popul[i][id] *= bf[id];
}
}
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_inpbf_basic() {
let params = InpbfParams {
dm: &[1e-4, 1e-3, 1e-2],
nd: 3,
inmod: 1,
nlevel: 5,
};
// 4 parameters: 3 leading + 1 b-factor
let depth_data = [1e-5, 1e-4, 1e-3, 1e-2, 1e-1];
let param_data = vec![
vec![0.0; 5], // param 0 (leading)
vec![0.0; 5], // param 1 (leading)
vec![0.0; 5], // param 2 (leading)
vec![0.8, 0.9, 1.0, 1.1, 1.2], // b-factor for level 0
];
let result = inpbf(&params, &depth_data, &param_data);
assert_eq!(result.bfactors.len(), 1);
assert_eq!(result.bfactors[0].len(), 3);
// B-factors should be interpolated
assert!(result.bfactors[0][0].is_finite());
assert!(result.bfactors[0][1].is_finite());
assert!(result.bfactors[0][2].is_finite());
}
#[test]
fn test_apply_inpbf() {
let mut popul = vec![
vec![1e12, 1e12, 1e12],
vec![1e10, 1e10, 1e10],
];
let bfactors = vec![
vec![1.1, 1.2, 1.3],
];
apply_inpbf(&mut popul, &bfactors, 3);
assert!((popul[0][0] - 1.1e12).abs() < 1e5);
assert!((popul[0][1] - 1.2e12).abs() < 1e5);
assert!((popul[0][2] - 1.3e12).abs() < 1e5);
// Second level should be unchanged
assert!((popul[1][0] - 1e10).abs() < 1e3);
}
}
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//! inpmod — 读取初始模型大气。
//!
//! Fortran 原始签名: SUBROUTINE INPMOD
//!
//! 从 unit 8 读取 TLUSTY 模型大气,计算 LTE 能级布居,
//! 并可选地替换为 NLTE 布居。
//!
//! 注意: Fortran 版本直接操作 COMMON 块和文件 I/O。
//! Rust 版本提供纯计算核心函数。
/// 模型大气深度点数据
#[derive(Debug, Clone)]
pub struct ModelDepthPoint {
/// 质量深度 (g/cm^2)
pub depth: f64,
/// 温度 (K)
pub temp: f64,
/// 电子密度 (cm^-3)
pub elec: f64,
/// 质量密度 (g/cm^3)
pub dens: f64,
}
/// 计算总粒子数密度
///
/// TOTN = DENS / WMM + ELEC
///
/// Fortran 原始逻辑:
/// ```fortran
/// TOTN(ID)=DENS(ID)/WMM(ID)+ELEC(ID)
/// ```
pub fn total_number_density(dens: f64, wmm: f64, elec: f64) -> f64 {
dens / wmm + elec
}
/// 计算束缚-自由常数 (BCON)
///
/// BCON = ELEC / TEMP / SQRT(TEMP) * 2.0706E-16
///
/// Fortran 原始逻辑:
/// ```fortran
/// BCON=ELEC(ID)/TEMP(ID)/SQRT(TEMP(ID))*2.0706E-16
/// ```
pub fn bound_free_constant(elec: f64, temp: f64) -> f64 {
elec / temp / temp.sqrt() * 2.0706e-16
}
/// 计算原子总数密度
///
/// ATTOT(IAT,ID) = DENS / WMM / YTOT * ABUND(IAT,ID)
///
/// Fortran 原始逻辑:
/// ```fortran
/// DO IAT=1,NATOM
/// ATTOT(IAT,ID)=DENS(ID)/WMM(ID)/YTOT(ID)*ABUND(IAT,ID)
/// END DO
/// ```
pub fn compute_atom_densities(
dens: f64,
wmm: f64,
ytot: f64,
abundances: &[f64],
) -> Vec<f64> {
let factor = dens / wmm / ytot;
abundances.iter().map(|&a| factor * a).collect()
}
/// NLTE 布居替换
///
/// POPUL(J,ID) = X(IP+I) * RELAB(IATM(I),ID)
///
/// Fortran 原始逻辑:
/// ```fortran
/// DO I=1,NLEV0
/// j=iltot(i)
/// POPUL(J,ID)=X(IP+I)*RELAB(IATM(I),ID)
/// END DO
/// ```
pub fn replace_nlte_populations(
populations: &mut [f64],
nlte_data: &[f64],
iltot: &[usize],
relab: &[f64],
iatm: &[usize],
) {
for (i, &j) in iltot.iter().enumerate().take(nlte_data.len()) {
if j > 0 && j <= populations.len() {
let relab_val = if iatm[i] < relab.len() { relab[iatm[i]] } else { 1.0 };
populations[j - 1] = nlte_data[i] * relab_val;
}
}
}
/// B 因子修正
///
/// POPUL(J,ID) = POPUL(J,ID) * PLTE(J,ID)
///
/// Fortran 原始逻辑:
/// ```fortran
/// if(ibfac.eq.1) then
/// do i=1,nlev0
/// j=iltot(i)
/// popul(j,id)=popul(j,id)*plte(j,id)
/// end do
/// end if
/// ```
pub fn apply_bfactor_correction(
populations: &mut [f64],
lte_populations: &[f64],
iltot: &[usize],
) {
for &j in iltot {
if j > 0 && j <= populations.len() {
populations[j - 1] *= lte_populations[j - 1];
}
}
}
/// 模型大气数据
#[derive(Debug, Clone)]
pub struct ModelAtmosphere {
/// 深度点数据
pub depths: Vec<ModelDepthPoint>,
/// 能级布居 [level][depth]
pub populations: Vec<Vec<f64>>,
/// LTE 布居 [level][depth]
pub lte_populations: Vec<Vec<f64>>,
}
/// 模型大气统计信息
#[derive(Debug, Clone)]
pub struct ModelStats {
/// 最低温度
pub min_temp: f64,
/// 最高温度
pub max_temp: f64,
/// 最低密度
pub min_dens: f64,
/// 最高密度
pub max_dens: f64,
/// 深度点数
pub n_depths: usize,
/// 能级数
pub n_levels: usize,
}
/// 计算模型大气统计信息
pub fn compute_model_stats(model: &ModelAtmosphere) -> ModelStats {
let mut min_temp = f64::MAX;
let mut max_temp = f64::MIN;
let mut min_dens = f64::MAX;
let mut max_dens = f64::MIN;
for depth in &model.depths {
if depth.temp < min_temp { min_temp = depth.temp; }
if depth.temp > max_temp { max_temp = depth.temp; }
if depth.dens < min_dens { min_dens = depth.dens; }
if depth.dens > max_dens { max_dens = depth.dens; }
}
ModelStats {
min_temp,
max_temp,
min_dens,
max_dens,
n_depths: model.depths.len(),
n_levels: model.populations.len(),
}
}
/// 模型文件格式
#[derive(Debug, Clone, Copy, PartialEq)]
pub enum ModelFormat {
/// LTE 模型 (3 参数: T, NE, RHO)
Lte,
/// NLTE 模型 (>3 参数)
Nlte,
/// 磁盘模型 (4 参数)
Disk,
}
/// 检查模型格式
pub fn detect_model_format(numpar: i32, inmod: i32) -> ModelFormat {
if inmod == 2 {
ModelFormat::Disk
} else if numpar.abs() > 3 {
ModelFormat::Nlte
} else {
ModelFormat::Lte
}
}
/// 计算 NLTE 修正因子
///
/// PNLT(IAT,ION,ID) = POPUL(NKI,ID) / G(NKI) * BCON
///
/// Fortran 原始逻辑:
/// ```fortran
/// BCON=ELEC(ID)/TEMP(ID)/SQRT(TEMP(ID))*2.0706E-16
/// IF(ION.GT.0) PNLT(IAT,ION,ID)=POPUL(NKI,ID)/G(NKI)*BCON
/// ```
pub fn compute_nlte_correction(
popul_nki: f64,
g_nki: f64,
elec: f64,
temp: f64,
) -> f64 {
if g_nki > 0.0 {
popul_nki / g_nki * bound_free_constant(elec, temp)
} else {
0.0
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_total_number_density() {
let totn = total_number_density(1e-8, 1.0, 1e-10);
// 1e-8/1.0 + 1e-10 = 1.01e-8
assert!((totn - 1.01e-8).abs() < 1e-15);
}
#[test]
fn test_bound_free_constant() {
let bcon = bound_free_constant(1e10, 10000.0);
// 1e10 / 10000 / 100 * 2.0706e-16 = 1e10 / 1e6 * 2.0706e-16 = 2.0706e-12
let expected = 1e10 / 10000.0 / 100.0 * 2.0706e-16;
assert!((bcon - expected).abs() / expected < 1e-10);
}
#[test]
fn test_compute_atom_densities() {
let abundances = vec![0.9, 0.1];
let attot = compute_atom_densities(1e-8, 1.0, 1.5, &abundances);
assert_eq!(attot.len(), 2);
let expected0 = 1e-8 / 1.0 / 1.5 * 0.9;
assert!((attot[0] - expected0).abs() < 1e-20);
}
#[test]
fn test_replace_nlte_populations() {
let mut popul = vec![1.0, 2.0, 3.0, 4.0, 5.0];
let nlte_data = vec![10.0, 20.0];
let iltot = vec![1, 3]; // 1-indexed
let relab = vec![1.0, 1.0, 1.0];
let iatm = vec![0, 1];
replace_nlte_populations(&mut popul, &nlte_data, &iltot, &relab, &iatm);
assert_eq!(popul[0], 10.0); // j=1 → index 0
assert_eq!(popul[2], 20.0); // j=3 → index 2
assert_eq!(popul[4], 5.0); // unchanged
}
#[test]
fn test_apply_bfactor_correction() {
let mut popul = vec![2.0, 3.0, 4.0];
let lte = vec![0.5, 0.5, 0.5];
let iltot = vec![1, 2, 3]; // 1-indexed (Fortran convention)
apply_bfactor_correction(&mut popul, &lte, &iltot);
assert_eq!(popul[0], 1.0); // 2.0 * 0.5
assert_eq!(popul[1], 1.5); // 3.0 * 0.5
assert_eq!(popul[2], 2.0); // 4.0 * 0.5
}
#[test]
fn test_detect_model_format() {
assert_eq!(detect_model_format(3, 0), ModelFormat::Lte);
assert_eq!(detect_model_format(5, 0), ModelFormat::Nlte);
assert_eq!(detect_model_format(3, 2), ModelFormat::Disk);
}
#[test]
fn test_compute_nlte_correction() {
let pnlt = compute_nlte_correction(1e12, 2.0, 1e10, 10000.0);
// 1e12 / 2.0 * 1e10/10000/100 * 2.0706e-16
let bcon = bound_free_constant(1e10, 10000.0);
let expected = 1e12 / 2.0 * bcon;
assert!((pnlt - expected).abs() / expected < 1e-10);
}
#[test]
fn test_compute_model_stats() {
let model = ModelAtmosphere {
depths: vec![
ModelDepthPoint { depth: 1.0, temp: 5000.0, elec: 1e10, dens: 1e-8 },
ModelDepthPoint { depth: 10.0, temp: 15000.0, elec: 1e12, dens: 1e-6 },
],
populations: vec![vec![1.0, 2.0]],
lte_populations: vec![vec![1.0, 2.0]],
};
let stats = compute_model_stats(&model);
assert_eq!(stats.min_temp, 5000.0);
assert_eq!(stats.max_temp, 15000.0);
assert_eq!(stats.n_depths, 2);
}
}
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//! 通用多项式插值。
//!
//! 重构自 SYNSPEC `interp.f`
//!
//! 支持 (NPOL-1) 阶多项式插值,可选对数插值模式。
/// 通用多项式插值。
///
/// 在原始数据点 `(x, y)` 基础上,对新的 x 坐标 `xx` 进行插值。
/// 支持对数插值模式。
///
/// # 参数
///
/// * `x` - 原始 x 坐标数组(必须单调递增或递减)
/// * `y` - 原始 y 值数组
/// * `xx` - 新的 x 坐标数组(待插值点)
/// * `npol` - 插值阶数(使用 NPOL 个点进行 (NPOL-1) 阶插值)
/// * `ilogx` - 非零时对 x 坐标进行对数插值
/// * `ilogy` - 非零时对 y 值进行对数插值
///
/// # 返回值
///
/// 插值后的 y 值数组,与 `xx` 等长
pub fn interp(x: &[f64], y: &[f64], xx: &[f64], npol: i32, ilogx: i32, ilogy: i32) -> Vec<f64> {
let nx = x.len();
let nxx = xx.len();
let n = nx.max(nxx);
// NPOL <= 0 或 NX <= 0 的情况:直接复制
if npol <= 0 || nx == 0 {
let mut yy = vec![0.0; n];
for i in 0..n {
yy[i] = if i < nx { x[i] } else { 0.0 };
}
return yy;
}
// 如果需要对数插值,转换坐标
let x_work: Vec<f64> = if ilogx != 0 {
x.iter().map(|v| v.log10()).collect()
} else {
x.to_vec()
};
let xx_work: Vec<f64> = if ilogx != 0 {
xx.iter().map(|v| v.log10()).collect()
} else {
xx.to_vec()
};
let y_work: Vec<f64> = if ilogy != 0 {
y.iter().map(|v| v.log10()).collect()
} else {
y.to_vec()
};
let npol = npol as usize;
let npol_usize = npol;
let nm = npol_usize.div_ceil(2);
// Fortran: nm1=nm+1, nup=NX+NM1-NPOL, loop II=NM1..NUP-1
// In 0-based: nm1=nm, nup=nx-npol+nm+1, loop ii=nm..nup-1
let nm1 = nm;
let nup = nx + nm1 - npol_usize + 1;
let mut yy = vec![0.0; nxx];
for id in 0..nxx {
let xxx = xx_work[id];
// 查找插值区间
// Fortran: DO II=NM1,NUP-1; IF(XXX.LE.X(II)) I=II
// 0-based: ii goes from nm1 to nup-1, compare with x_work[ii]
let mut i = nup.saturating_sub(1);
for ii in nm1..nup {
if ii < nx && xxx <= x_work[ii] {
i = ii;
break;
}
}
// Clamp to valid range for interpolation
if npol_usize > nx {
i = 0;
} else if i + npol_usize > nx {
i = nx - npol_usize;
}
let j = i.saturating_sub(nm);
let jj = (j + npol_usize).min(nx) - 1;
// Lagrange 插值 (j 从 0 开始,使用 0-based 索引)
let mut yyy = 0.0;
for k in j..=jj {
let mut t = 1.0;
for m in j..=jj {
if k != m {
let denom = x_work[k] - x_work[m];
if denom.abs() > 1e-30 {
t *= (xxx - x_work[m]) / denom;
}
}
}
yyy += y_work[k] * t;
}
yy[id] = yyy;
}
// 如果使用了对数插值,转换回线性尺度
if ilogy != 0 {
for val in yy.iter_mut() {
*val = 10.0_f64.powf(*val);
}
}
yy
}
#[cfg(test)]
mod tests {
use super::*;
use approx::assert_relative_eq;
#[test]
fn test_interp_linear() {
// 线性数据:y = 2x + 1
let x = [0.0, 1.0, 2.0, 3.0];
let y = [1.0, 3.0, 5.0, 7.0];
let xx = [0.5, 1.5, 2.5];
let yy = interp(&x, &y, &xx, 2, 0, 0);
assert_relative_eq!(yy[0], 2.0, epsilon = 1e-10);
assert_relative_eq!(yy[1], 4.0, epsilon = 1e-10);
assert_relative_eq!(yy[2], 6.0, epsilon = 1e-10);
}
#[test]
fn test_interp_quadratic() {
// 二次数据:y = x^2
let x = [0.0, 1.0, 2.0, 3.0, 4.0];
let y = [0.0, 1.0, 4.0, 9.0, 16.0];
let xx = [1.5];
// 3 阶插值(2 阶多项式)
let yy = interp(&x, &y, &xx, 3, 0, 0);
assert_relative_eq!(yy[0], 2.25, epsilon = 1e-10);
}
#[test]
fn test_interp_exact_points() {
// 插值到已知数据点应返回精确值
let x = [1.0, 2.0, 3.0];
let y = [10.0, 20.0, 30.0];
let xx = [2.0];
let yy = interp(&x, &y, &xx, 2, 0, 0);
assert_relative_eq!(yy[0], 20.0, epsilon = 1e-10);
}
#[test]
fn test_interp_log_mode() {
// 对数插值模式
let x = [1.0, 10.0, 100.0];
let y = [1.0, 100.0, 10000.0];
let xx = [5.0];
let yy = interp(&x, &y, &xx, 2, 1, 1);
// 在对数空间中,log(y) = 2*log(x),所以 y = x^2
// x=5 -> y=25
assert_relative_eq!(yy[0], 25.0, epsilon = 0.1);
}
#[test]
fn test_interp_zero_npol() {
let x = [1.0, 2.0];
let y = [3.0, 4.0];
let xx = [5.0];
let yy = interp(&x, &y, &xx, 0, 0, 0);
// NPOL <= 0 时返回 x 的值
assert_eq!(yy[0], 1.0);
}
}
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//! Interpolation in He II Stark broadening tables.
//!
//! Translated from SYNSPEC54.FOR subroutine INTHE2(W0,X0,Z0,IWL,ILINE)
//! at line 12507.
//!
//! Performs 2D interpolation in temperature and electron density from the
//! Schoening and Butler tables for He II lines. Falls back to approximate
//! expressions (DIVHE2 + STARKA) when outside the table bounds.
use super::divhe2::divhe2;
use super::starka::starka;
use super::yint::yint;
/// Parameters for He II table interpolation.
pub struct Inthe2Params<'a> {
/// Temperature (log scale)
pub x0: f64,
/// Electron density (log scale)
pub z0: f64,
/// Wavelength index
pub iwl: usize,
/// Number of wavelength points
pub nwl2: usize,
/// Number of temperature grid points
pub nt2: usize,
/// Number of electron density grid points
pub ne2: usize,
/// Wavelength array (nwl)
pub wl2: &'a [f64],
/// FXK constant
pub fxk: f64,
/// Temperature grid (nt)
pub xt2: &'a [f64],
/// Electron density grid (ne)
pub xne2: &'a [f64],
/// Profile data (nwl x nt x ne)
pub prf2: &'a [&'a [f64]],
/// Doppler width in beta units
pub betad: f64,
/// Delta beta for profile normalization
pub dbeta: f64,
}
/// Result of He II table interpolation.
pub struct Inthe2Result {
/// Interpolated profile value (log10)
pub w0: f64,
}
/// Interpolation in He II Stark broadening tables.
///
/// Performs bilinear interpolation in temperature and electron density
/// from precomputed He II line broadening tables. Falls back to
/// approximate Stark profile expressions when outside table bounds.
///
/// # Arguments
/// * `params` - Interpolation parameters
///
/// # Returns
/// Interpolated profile value (log10 scale).
pub fn inthe2(params: &Inthe2Params) -> Inthe2Result {
let nx = 3usize;
let nz = 3usize;
let beta = params.wl2[params.iwl] / params.fxk;
// Fallback: approximate expression for out-of-range electron density
if params.z0 < params.xne2[0] * 0.99
|| params.z0 > params.xne2[params.ne2 - 1] * 1.01
{
let div = divhe2(beta);
let w0_val = starka(beta, params.betad, beta, div, 1.0) * params.dbeta;
return Inthe2Result {
w0: w0_val.log10(),
};
}
// Find electron density interval
let mut ipz = 0;
for izz in 0..params.ne2 - 1 {
ipz = izz;
if params.z0 <= params.xne2[izz + 1] {
break;
}
}
let mut n0z = (ipz + 1).saturating_sub(nz / 2);
if n0z > params.ne2 - nz {
n0z = params.ne2 - nz;
}
let n1z = n0z + nz;
let mut zz = [0.0f64; 3];
let mut wz = [0.0f64; 3];
for izz in n0z..n1z {
let i0z = izz - n0z;
zz[i0z] = params.xne2[izz];
// Fallback for high temperature with large Doppler width
if params.x0 > 1.01 * params.xt2[params.nt2 - 1] && params.betad > 10.0 {
let div = divhe2(beta);
let w0_val = starka(beta, params.betad, beta, div, 1.0) * params.dbeta;
return Inthe2Result {
w0: w0_val.log10(),
};
}
// Find temperature interval
let mut ipx = 0;
for ix in 0..params.nt2 - 1 {
ipx = ix;
if params.x0 <= params.xt2[ix + 1] {
break;
}
}
let mut n0x = (ipx + 1).saturating_sub(nx / 2);
if n0x > params.nt2 - nx {
n0x = params.nt2 - nx;
}
let n1x = n0x + nx;
let mut xx = [0.0f64; 3];
let mut wx = [0.0f64; 3];
for ix in n0x..n1x {
let i0 = ix - n0x;
xx[i0] = params.xt2[ix];
wx[i0] = params.prf2[ix][izz];
}
wz[i0z] = yint(&xx, &wx, params.x0);
}
let w0 = yint(&zz, &wz, params.z0);
Inthe2Result { w0 }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_inthe2_basic() {
// Simple 3x3 grid test
let wl2 = [4686.0];
let xt2 = [3.0, 4.0, 5.0];
let xne2 = [10.0, 11.0, 12.0];
// prf2[ix][izz]
let row0: &[f64] = &[1.0, 2.0, 3.0];
let row1: &[f64] = &[2.0, 3.0, 4.0];
let row2: &[f64] = &[3.0, 4.0, 5.0];
let prf2: &[&[f64]] = &[row0, row1, row2];
let params = Inthe2Params {
x0: 3.5,
z0: 10.5,
iwl: 0,
nwl2: 1,
nt2: 3,
ne2: 3,
wl2: &wl2,
fxk: 1.0,
xt2: &xt2,
xne2: &xne2,
prf2,
betad: 5.0,
dbeta: 1.0,
};
let result = inthe2(&params);
assert!(result.w0.is_finite());
}
}
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//! Interpolation in hydrogen Stark broadening tables.
//!
//! Translated from SYNSPEC54.FOR subroutine INTHYD(W0,X0,Z0,IWL,ILINE)
//! at line 12412.
//!
//! Performs 2D interpolation in temperature and electron density from the
//! hydrogen line broadening tables. Falls back to approximate expressions
//! (DIVSTR + STARKA) when outside the table bounds.
use super::divstr::divstr;
use super::starka::starka;
use super::yint::yint;
/// Parameters for hydrogen table interpolation.
pub struct InthydParams<'a> {
/// Temperature (log scale)
pub x0: f64,
/// Electron density (log scale)
pub z0: f64,
/// Wavelength index
pub iwl: usize,
/// Line index
pub iline: usize,
/// Number of temperature grid points per line
pub nth: &'a [usize],
/// Number of electron density grid points per line
pub neh: &'a [usize],
/// Wavelength array (nwl x nlines)
pub wl: &'a [&'a [f64]],
/// FXK constant
pub fxk: f64,
/// XK constant (for Lemke mode)
pub xk: f64,
/// Lemke mode flag (0 = standard, 1 = Lemke)
pub ilemke: i32,
/// Electron density grid (ne x nlines)
pub xne: &'a [&'a [f64]],
/// Temperature grid (nt x nlines)
pub xt: &'a [&'a [f64]],
/// Profile data (nwl x nt x ne x nlines) — pass slice for current line
pub prf_iwl: &'a [&'a [f64]],
/// Doppler width in beta units
pub betad: f64,
/// Delta beta for profile normalization
pub dbeta: f64,
}
/// Result of hydrogen table interpolation.
pub struct InthydResult {
/// Interpolated profile value (log10)
pub w0: f64,
}
/// Interpolation in hydrogen Stark broadening tables.
///
/// Performs bilinear interpolation in temperature and electron density
/// from precomputed hydrogen line broadening tables. Falls back to
/// approximate Stark profile expressions when outside table bounds.
///
/// # Arguments
/// * `params` - Interpolation parameters
///
/// # Returns
/// Interpolated profile value (log10 scale).
pub fn inthyd(params: &InthydParams) -> InthydResult {
let iline = params.iline;
let nt = params.nth[iline];
let ne = params.neh[iline];
let (beta, nx, nz) = if params.ilemke == 1 {
(params.wl[params.iwl][iline] / params.xk, 2, 2)
} else {
(params.wl[params.iwl][iline] / params.fxk, 3, 3)
};
// Fallback: approximate expression for out-of-range electron density
if params.z0 < params.xne[iline][0] * 0.99
|| params.z0 > params.xne[iline][ne - 1] * 1.01
{
let (a, div) = divstr(beta);
let w0_val = starka(beta, params.betad, a, div, 2.0) * params.dbeta;
return InthydResult {
w0: w0_val.log10(),
};
}
// Find electron density interval
let mut ipz = 0;
for izz in 0..ne - 1 {
ipz = izz;
if params.z0 <= params.xne[iline][izz + 1] {
break;
}
}
let mut n0z = (ipz + 1).saturating_sub(nz / 2);
if n0z > ne - nz {
n0z = ne - nz;
}
let n1z = n0z + nz;
let mut zz = [0.0f64; 3];
let mut wz = [0.0f64; 3];
for izz in n0z..n1z {
let i0z = izz - n0z;
zz[i0z] = params.xne[iline][izz];
// Fallback for high temperature with large Doppler width
if params.x0 > 1.01 * params.xt[iline][nt - 1] && params.betad > 10.0 {
let (a, div) = divstr(beta);
let w0_val = starka(beta, params.betad, a, div, 2.0) * params.dbeta;
return InthydResult {
w0: w0_val.log10(),
};
}
// Find temperature interval
let mut ipx = 0;
for ix in 0..nt - 1 {
ipx = ix;
if params.x0 <= params.xt[iline][ix + 1] {
break;
}
}
let mut n0x = (ipx + 1).saturating_sub(nx / 2);
if n0x > nt - nx {
n0x = nt - nx;
}
let n1x = n0x + nx;
let mut xx = [0.0f64; 3];
let mut wx = [0.0f64; 3];
let mut has_bad = false;
for ix in n0x..n1x {
let i0 = ix - n0x;
xx[i0] = params.xt[iline][ix];
wx[i0] = params.prf_iwl[ix][izz];
if wx[i0] < -99.0 {
has_bad = true;
}
}
if has_bad {
let (a, div) = divstr(beta);
let w0_val = starka(beta, params.betad, a, div, 2.0) * params.dbeta;
return InthydResult {
w0: w0_val.log10(),
};
}
wz[i0z] = yint(&xx, &wx, params.x0);
}
let w0 = yint(&zz, &wz, params.z0);
InthydResult { w0 }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_inthyd_basic() {
// Simple 3x3 grid test
let nth = [3usize];
let neh = [3usize];
let wl_vals = [4861.0, 4340.0, 4102.0];
let wl: [&[f64]; 1] = [&wl_vals];
let xne_vals = [10.0, 11.0, 12.0];
let xne: [&[f64]; 1] = [&xne_vals];
let xt_vals = [3.0, 4.0, 5.0];
let xt: [&[f64]; 1] = [&xt_vals];
// prf_iwl[ix][izz]
let row0: &[f64] = &[1.0, 2.0, 3.0];
let row1: &[f64] = &[2.0, 3.0, 4.0];
let row2: &[f64] = &[3.0, 4.0, 5.0];
let prf_iwl: &[&[f64]] = &[row0, row1, row2];
let params = InthydParams {
x0: 3.5,
z0: 10.5,
iwl: 0,
iline: 0,
nth: &nth,
neh: &neh,
wl: &wl,
fxk: 1.0,
xk: 1.0,
ilemke: 0,
xne: &xne,
xt: &xt,
prf_iwl,
betad: 5.0,
dbeta: 1.0,
};
let result = inthyd(&params);
assert!(result.w0.is_finite());
}
}
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//! Interpolation in Xenomorph tables for hydrogen lines.
//!
//! Translated from SYNSPEC54.FOR subroutine INTXEN(W0B,W0R,X0,Z0,IWL,ILINE)
//! at line 11631.
//!
//! Performs 2D interpolation in temperature and electron density from the
//! Xenomorph line profile tables to the actual values of temperature (X0)
//! and electron density (Z0).
use super::yint::yint;
/// Parameters for Xenomorph table interpolation.
pub struct IntxenParams<'a> {
/// Temperature (log scale)
pub x0: f64,
/// Electron density (log scale)
pub z0: f64,
/// Wavelength index
pub iwl: usize,
/// Number of temperature grid points
pub nt: usize,
/// Number of electron density grid points
pub ne: usize,
/// Temperature grid (nt)
pub xtxen: &'a [f64],
/// Electron density grid (ne)
pub xnenex: &'a [f64],
/// Blue profile data (nwl x nt x ne) — pass the slice for iwl
pub prfxb_iwl: &'a [&'a [f64]],
/// Red profile data (nwl x nt x ne) — pass the slice for iwl
pub prfxr_iwl: &'a [&'a [f64]],
}
/// Result of Xenomorph table interpolation.
pub struct IntxenResult {
/// Blue wing profile value
pub w0b: f64,
/// Red wing profile value
pub w0r: f64,
}
/// Interpolation in Xenomorph tables for hydrogen lines.
///
/// Performs bilinear interpolation in temperature and electron density
/// from the Xenomorph line profile tables. Uses quadratic interpolation
/// (NX=NZ=2 points) around the target values.
///
/// # Arguments
/// * `params` - Interpolation parameters
///
/// # Returns
/// Interpolated blue and red wing profile values.
pub fn intxen(params: &IntxenParams) -> IntxenResult {
let nt = params.nt;
let ne = params.ne;
let nx = 2usize;
let nz = 2usize;
// Find electron density interval
let mut ipz = 0;
for izz in 0..ne - 1 {
ipz = izz;
if params.z0 <= params.xnenex[izz + 1] {
break;
}
}
let mut n0z = (ipz + 1).saturating_sub(nz / 2);
if n0z > ne - nz {
n0z = ne - nz;
}
let n1z = n0z + nz;
let mut zz = [0.0f64; 3];
let mut wzb = [0.0f64; 3];
let mut wzr = [0.0f64; 3];
for izz in n0z..n1z {
let i0z = izz - n0z;
zz[i0z] = params.xnenex[izz];
// Find temperature interval
let mut ipx = 0;
for ix in 0..nt - 1 {
ipx = ix;
if params.x0 <= params.xtxen[ix + 1] {
break;
}
}
let mut n0x = (ipx + 1).saturating_sub(nx / 2);
if n0x > nt - nx {
n0x = nt - nx;
}
let n1x = n0x + nx;
let mut xx = [0.0f64; 3];
let mut wxb = [0.0f64; 3];
let mut wxr = [0.0f64; 3];
for ix in n0x..n1x {
let i0 = ix - n0x;
xx[i0] = params.xtxen[ix];
wxb[i0] = params.prfxb_iwl[ix][izz];
wxr[i0] = params.prfxr_iwl[ix][izz];
}
wzb[i0z] = yint(&xx, &wxb, params.x0);
wzr[i0z] = yint(&xx, &wxr, params.x0);
}
let w0b = yint(&zz, &wzb, params.z0);
let w0r = yint(&zz, &wzr, params.z0);
IntxenResult { w0b, w0r }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_intxen_basic() {
// Simple 3x3 grid test
let xtxen = [1.0, 2.0, 3.0];
let xnenex = [10.0, 11.0, 12.0];
// prfxb_iwl[ix][izz]
let row0: &[f64] = &[1.0, 2.0, 3.0];
let row1: &[f64] = &[2.0, 3.0, 4.0];
let row2: &[f64] = &[3.0, 4.0, 5.0];
let prfxb_iwl: &[&[f64]] = &[row0, row1, row2];
let rrow0: &[f64] = &[5.0, 4.0, 3.0];
let rrow1: &[f64] = &[4.0, 3.0, 2.0];
let rrow2: &[f64] = &[3.0, 2.0, 1.0];
let prfxr_iwl: &[&[f64]] = &[rrow0, rrow1, rrow2];
let params = IntxenParams {
x0: 1.5,
z0: 10.5,
iwl: 0,
nt: 3,
ne: 3,
xtxen: &xtxen,
xnenex: &xnenex,
prfxb_iwl,
prfxr_iwl,
};
let result = intxen(&params);
assert!(result.w0b.is_finite());
assert!(result.w0r.is_finite());
assert!(result.w0b > 0.0 && result.w0b < 10.0);
assert!(result.w0r > 0.0 && result.w0r < 10.0);
}
}
+281
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@@ -0,0 +1,281 @@
//! Irwin (1981) partition functions, updated with Barklem & Collet (2016) data.
//!
//! Translated from SYNSPEC `IRWPF` subroutine (synspec54.f:23749).
//!
//! Computes partition functions using polynomial fits from Irwin (1981),
//! ApJS. 45, 621, updated with Barklem & Collet (2016) data.
//! For atomic species (jatom > 0, ion > 0): uses 6-coefficient polynomial in ln(T).
//! For molecular species (indmol > 0): uses similar polynomial with index mapping.
use std::sync::Mutex;
/// Mapping from Tsuji molecular index to Irwin index.
/// 478 elements (Fortran declares `dimension irwind(478)`); value 0 = no data.
const IRWIND: [i32; 478] = [
0, 1, 28, 4, 2, 7, 6, 5, 8, 10,
9, 3, 18, 25, 53, 29, 43, 0, 17, 153,
52, 55, 167, 44, 45, 182, 74, 46, 11, 187,
201, 31, 27, 99, 209, 24, 22, 20, 21, 65,
35, 19, 54, 23, 0, 14, 58, 0, 32, 12,
47, 16, 0, 34, 0, 0, 30, 0, 13, 33,
61, 63, 292, 57, 59, 66, 272, 0, 94, 175,
226, 286, 0, 0, 0, 176, 227, 287, 0, 0,
0, 96, 0, 177, 0, 267, 228, 288, 0, 0,
0, 0, 93, 147, 162, 0, 0, 0, 0, 0,
0, 50, 0, 0, 0, 0, 36, 0, 64, 0,
0, 48, 0, 0, 148, 0, 0, 26, 49, 70,
178, 97, 170, 229, 0, 180, 268, 230, 0, 289,
0, 0, 15, 181, 0, 269, 0, 0, 0, 0,
0, 0, 0, 231, 0, 290, 0, 38, 0, 0,
152, 39, 40, 0, 41, 232, 0, 291, 0, 0,
0, 0, 0, 75, 154, 0, 0, 0, 183, 0,
0, 0, 0, 0, 0, 98, 184, 234, 185, 270,
0, 0, 0, 186, 0, 0, 271, 235, 0, 0,
62, 0, 0, 0, 0, 0, 0, 101, 0, 188,
0, 0, 0, 0, 0, 102, 189, 0, 0, 0,
236, 0, 294, 67, 0, 190, 0, 0, 0, 295,
0, 0, 104, 191, 237, 0, 105, 192, 274, 238,
296, 112, 245, 303, 113, 199, 0, 278, 246, 0,
304, 0, 0, 0, 0, 200, 0, 0, 279, 247,
0, 305, 0, 0, 172, 0, 0, 0, 0, 0,
0, 120, 122, 208, 0, 282, 255, 0, 312, 0,
0, 0, 0, 0, 0, 0, 0, 283, 256, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
275, 194, 108, 241, 299, 202, 0, 68, 69, 71,
72, 73, 42, 37, 76, 77, 78, 79, 80, 81,
82, 83, 92, 95, 100, 103, 106, 107, 109, 110,
111, 114, 115, 116, 117, 118, 119, 121, 123, 124,
125, 126, 127, 128, 129, 149, 150, 151, 155, 156,
157, 158, 159, 163, 164, 165, 166, 168, 169, 170,
171, 193, 195, 196, 197, 198, 203, 204, 205, 206,
207, 210, 211, 212, 213, 214, 215, 216, 217, 218,
225, 233, 239, 240, 242, 243, 244, 248, 249, 250,
251, 252, 253, 254, 257, 258, 259, 260, 262, 262,
263, 264, 265, 266, 273, 276, 277, 280, 282, 284,
285, 293, 297, 298, 300, 301, 302, 306, 307, 308,
309, 310, 311, 60, 313, 314, 315, 316, 317, 318,
319, 320, 321, 322, 323, 324, 84, 85, 86, 87,
88, 89, 90, 91, 130, 131, 132, 133, 134, 135,
136, 137, 138, 139, 140, 141, 142, 143, 144, 145,
146, 160, 161, 173, 174, 210, 220, 221, 222, 223,
224, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 56
];
/// Cached Irwin data: atomic coefficients `a[ion][atom][coeff]` and
/// molecular coefficients `am[mol_index][coeff]`.
struct IrwinData {
/// Atomic coefficients: a[ion * 92 * 6 + atom * 6 + coeff]
a: Vec<f64>,
/// Molecular coefficients: am[mol * 6 + coeff]
am: Vec<f64>,
}
static IRWIN_DATA: Mutex<Option<IrwinData>> = Mutex::new(None);
/// Read the Irwin data file and populate the coefficient arrays.
fn read_irwin_data(data_dir: &str, irwtab: i32) -> Result<IrwinData, String> {
let filename = if irwtab == 0 {
format!("{}/irwin_orig.dat", data_dir)
} else {
format!("{}/irwin_bc.dat", data_dir)
};
let content = std::fs::read_to_string(&filename)
.map_err(|e| format!("Cannot open {}: {}", filename, e))?;
let mut lines = content.lines();
// Skip 2 header lines
lines.next();
lines.next();
let mut a = vec![0.0f64; 6 * 3 * 92]; // a[ion * 92 * 6 + atom * 6 + coeff]
let mut am = vec![0.0f64; 6 * 500]; // am[mol * 6 + coeff]
// Read atomic data: 92 atoms × 3 ions (skip j=1,i=3 in Fortran, but read all here)
for _j in 0..92 {
for _i in 0..3 {
// Fortran skips j=1,i=3 (i.e. _j=0,_i=2); we just read and discard
let line = lines.next().ok_or("Unexpected end of atomic data")?;
if _j == 0 && _i == 2 {
continue; // Fortran: if(j.eq.1.and.i.eq.3) goto 10
}
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 7 {
continue; // skip malformed lines
}
for k in 0..6 {
if let Ok(val) = parts[k + 1].parse::<f64>() {
a[_i * 92 * 6 + _j * 6 + k] = val;
}
}
}
}
// Skip 3 header lines
lines.next();
lines.next();
lines.next();
// Read molecular data (up to 324 entries)
for idx in 0..324 {
match lines.next() {
Some(line) => {
let parts: Vec<&str> = line.split_whitespace().collect();
if parts.len() < 7 {
continue;
}
for k in 0..6 {
if let Ok(val) = parts[k + 1].parse::<f64>() {
am[idx * 6 + k] = val;
}
}
}
None => break,
}
}
Ok(IrwinData { a, am })
}
/// Evaluate 6-coefficient polynomial in ln(T).
/// `coeffs[0] + coeffs[1]*tl + coeffs[2]*tl^2 + ... + coeffs[5]*tl^5`
fn poly6(coeffs: &[f64], tl: f64) -> f64 {
coeffs[0]
+ tl * (coeffs[1]
+ tl * (coeffs[2]
+ tl * (coeffs[3]
+ tl * (coeffs[4]
+ tl * coeffs[5]))))
}
/// Irwin (1981) partition functions.
///
/// # Arguments
/// * `jatom` - Atomic number (1-92). If 0, compute molecular partition function.
/// * `ion` - Ionization degree (1=neutral, 2=singly ionized, 3=doubly ionized).
/// * `indmol` - Molecular index in Tsuji numbering (used when jatom == 0).
/// * `t` - Temperature (K). Must be in range [1000, 16000].
/// * `data_dir` - Path to data directory containing irwin_*.dat files.
/// * `irwtab` - Table selector: 0 = original Irwin, other = Barklem & Collet.
///
/// # Returns
/// Partition function value, or error string.
pub fn irwpf(
jatom: i32,
ion: i32,
indmol: i32,
t: f64,
data_dir: &str,
irwtab: i32,
) -> Result<f64, String> {
// Early return: no species specified
if jatom <= 0 && indmol <= 0 {
return Ok(0.0);
}
// Validate temperature
if t < 1000.0 {
return Err("irwpf: temperature < 1000 K".to_string());
}
if t > 16000.0 {
return Err("irwpf: temperature > 16000 K".to_string());
}
// Initialize data on first call
{
let mut guard = IRWIN_DATA.lock().map_err(|e| format!("Lock error: {}", e))?;
if guard.is_none() {
*guard = Some(read_irwin_data(data_dir, irwtab)?);
}
}
let guard = IRWIN_DATA.lock().map_err(|e| format!("Lock error: {}", e))?;
let data = guard.as_ref().unwrap();
let tl = t.ln();
// Atomic species
if jatom > 0 && ion > 0 {
let atom_idx = (jatom - 1) as usize;
let ion_idx = (ion - 1) as usize;
if atom_idx >= 92 || ion_idx >= 3 {
return Ok(0.0);
}
let base = ion_idx * 92 * 6 + atom_idx * 6;
let coeffs = &data.a[base..base + 6];
let mut ulog = poly6(coeffs, tl);
// Special case: Boron III
if jatom == 5 && ion == 3 {
ulog = 1.0;
}
return Ok(ulog.exp());
}
// Molecular species
if indmol > 0 {
let mol_idx = (indmol - 1) as usize;
if mol_idx >= 478 {
return Ok(0.0);
}
let indm = IRWIND[mol_idx];
if indm <= 0 {
return Ok(0.0);
}
let idx = (indm - 1) as usize;
if idx >= 500 {
return Ok(0.0);
}
let base = idx * 6;
let coeffs = &data.am[base..base + 6];
let ulog = poly6(coeffs, tl);
return Ok(ulog.exp());
}
Ok(0.0)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_irwind_count() {
assert_eq!(IRWIND.len(), 478);
}
#[test]
fn test_irwind_mapping() {
assert_eq!(IRWIND[0], 0);
assert_eq!(IRWIND[1], 1);
assert_eq!(IRWIND[2], 28);
assert_eq!(IRWIND[4], 2);
}
#[test]
fn test_poly6() {
let coeffs = [1.0, 0.0, 0.0, 0.0, 0.0, 0.0];
assert!((poly6(&coeffs, 5.0) - 1.0).abs() < 1e-15);
let coeffs = [0.0, 1.0, 0.0, 0.0, 0.0, 0.0];
assert!((poly6(&coeffs, 3.0) - 3.0).abs() < 1e-15);
// Horner form: 1 + 2x + 3x^2 at x=2 = 1 + 4 + 12 = 17
let coeffs = [1.0, 2.0, 3.0, 0.0, 0.0, 0.0];
assert!((poly6(&coeffs, 2.0) - 17.0).abs() < 1e-15);
}
#[test]
fn test_irwpf_out_of_range() {
let result = irwpf(1, 1, 0, 500.0, "./data", 1);
assert!(result.is_err());
let result = irwpf(1, 1, 0, 20000.0, "./data", 1);
assert!(result.is_err());
}
#[test]
fn test_irwpf_zero_atom_zero_mol() {
let result = irwpf(0, 0, 0, 5000.0, "./data", 1).unwrap();
assert_eq!(result, 0.0);
}
}
+1 -1
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@@ -76,7 +76,7 @@ pub fn ispec(iat: i32, ion: i32, alam: f64, ihe1pr: i32, ihe2pr: i32) -> i32 {
} else { } else {
// He II // He II
// 波长范围检查 // 波长范围检查
if alam < 163.0 || alam > 1012.7 { if !(163.0..=1012.7).contains(&alam) {
return PROFILE_VOIGT; return PROFILE_VOIGT;
} }
+152
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//! Level population solver by partial rate matrix inversion.
//!
//! Translated from SYNSPEC `LEVSOL` subroutine (synspec54.f:11326).
//!
//! Solves for new populations by inverting several partial rate matrices
//! for individual chemical species. For each atom, extracts the sub-matrix
//! and sub-vector corresponding to that atom's levels, solves the linear
//! system, and writes the results back.
use super::lineqs;
/// Solve for level populations by partial rate matrix inversion per atom.
///
/// For each chemical species (atom), extracts the sub-matrix of the rate
/// equations corresponding to that atom's levels (from `n0a[iat]` to
/// `nka[iat]`), solves the linear system, and writes results into `popp`.
///
/// # Arguments
/// * `a` - Rate matrix (nlevel × nlevel, row-major flat storage)
/// * `b` - Right-hand side vector (length nlevel)
/// * `popp` - Output population vector (length nlevel)
/// * `nlvcal` - Number of levels to solve (if ≤ 0, returns immediately)
/// * `natom` - Number of chemical species
/// * `n0a` - First level index for each atom (1-indexed, length natom)
/// * `nka` - Last level index for each atom (1-indexed, length natom)
/// * `nlevel` - Leading dimension of matrix A (stride)
pub fn levsol(
a: &[f64],
b: &[f64],
popp: &mut [f64],
nlvcal: usize,
natom: usize,
n0a: &[usize],
nka: &[usize],
nlevel: usize,
) {
if nlvcal == 0 {
return;
}
for iat in 0..natom {
// n0a/nka are 1-indexed from Fortran; convert to 0-indexed
let mut n1 = if n0a[iat] > 0 { n0a[iat] - 1 } else { 0 };
let nk = if nka[iat] > 0 { nka[iat] - 1 } else { 0 };
// If n1 <= 0 (i.e. n0a was 0), find first valid level
if n0a[iat] == 0 {
let mut found = false;
for i in n0a[iat]..=nka[iat] {
if i > 0 {
n1 = i - 1;
found = true;
break;
}
}
if !found {
continue;
}
}
if n1 > nk {
continue;
}
let nlp = nk - n1 + 1;
// Extract sub-matrix AP and sub-vector BP
let mut ap = vec![0.0f64; nlp * nlp];
let mut bp = vec![0.0f64; nlp];
for i in n1..=nk {
for j in n1..=nk {
ap[(i - n1) * nlp + (j - n1)] = a[i * nlevel + j];
}
bp[i - n1] = b[i];
}
// Solve the sub-system
let popp1 = lineqs(&mut ap, &mut bp, nlp);
// Write results back
for i in n1..=nk {
popp[i] = popp1[i - n1];
}
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_levsol_single_atom_2x2() {
// One atom with 2 levels (indices 0,1 in 0-based)
// System: 2*x0 + 1*x1 = 5, 1*x0 + 3*x1 = 7
// Solution: x0=1.6, x1=1.8
let nlevel = 2;
let mut a = vec![0.0; nlevel * nlevel];
a[0 * 2 + 0] = 2.0;
a[0 * 2 + 1] = 1.0;
a[1 * 2 + 0] = 1.0;
a[1 * 2 + 1] = 3.0;
let b = vec![5.0, 7.0];
let mut popp = vec![0.0; 2];
// n0a=1, nka=2 (1-indexed)
levsol(&a, &b, &mut popp, 2, 1, &[1], &[2], nlevel);
assert!((popp[0] - 1.6).abs() < 1e-10);
assert!((popp[1] - 1.8).abs() < 1e-10);
}
#[test]
fn test_levsol_two_atoms() {
// Two atoms, each with 2 levels, total 4 levels
// Atom 0: levels 0-1, Atom 1: levels 2-3
// Each sub-system is independent
let nlevel = 4;
let mut a = vec![0.0; nlevel * nlevel];
// Atom 0 sub-matrix (rows/cols 0-1)
a[0 * 4 + 0] = 2.0;
a[0 * 4 + 1] = 1.0;
a[1 * 4 + 0] = 1.0;
a[1 * 4 + 1] = 3.0;
// Atom 1 sub-matrix (rows/cols 2-3)
a[2 * 4 + 2] = 4.0;
a[2 * 4 + 3] = 1.0;
a[3 * 4 + 2] = 1.0;
a[3 * 4 + 3] = 5.0;
let b = vec![5.0, 7.0, 9.0, 11.0];
let mut popp = vec![0.0; 4];
// n0a=[1,3], nka=[2,4] (1-indexed)
levsol(&a, &b, &mut popp, 4, 2, &[1, 3], &[2, 4], nlevel);
// Atom 0: same as above
assert!((popp[0] - 1.6).abs() < 1e-10);
assert!((popp[1] - 1.8).abs() < 1e-10);
// Atom 1: 4*x2 + x3 = 9, x2 + 5*x3 = 11
// x2 = (9 - 11/5) / (4 - 1/5) = (34/5) / (19/5) = 34/19 ≈ 1.7895
// x3 = (11 - x2) / 5
assert!((popp[2] - 34.0 / 19.0).abs() < 1e-10);
assert!((popp[3] - (11.0 - 34.0 / 19.0) / 5.0).abs() < 1e-10);
}
#[test]
fn test_levsol_nlvcal_zero() {
let mut popp = vec![0.0; 2];
levsol(&[1.0; 4], &[1.0; 2], &mut popp, 0, 1, &[1], &[2], 2);
assert_eq!(popp, vec![0.0, 0.0]);
}
}
+157
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@@ -0,0 +1,157 @@
//! Linear equation solver by Gaussian elimination with partial pivoting.
//!
//! Translated from SYNSPEC `LINEQS` subroutine (synspec54.f:14818).
//!
//! Solves the linear system A*X = B using Gaussian elimination
//! with partial pivoting. Note: matrix A and vector B are destroyed.
/// Solve linear system A*X = B by Gaussian elimination with partial pivoting.
///
/// # Arguments
/// * `a` - Matrix of the linear system (n x n, stored as flat array row-major).
/// Will be modified in place (LU decomposition).
/// * `b` - Right-hand side vector (length n). Will be modified in place.
/// * `n` - Number of equations
///
/// # Returns
/// Solution vector X of length n.
pub fn lineqs(a: &mut [f64], b: &mut [f64], n: usize) -> Vec<f64> {
assert!(n > 0, "LINEQS requires n > 0");
assert!(a.len() >= n * n, "a array too short");
assert!(b.len() >= n, "b array too short");
let mut x = vec![0.0f64; n];
let idx = |i: usize, j: usize| i * n + j;
// Forward elimination with partial pivoting
for k in 0..n {
// Find pivot
let mut max_val = a[idx(k, k)].abs();
let mut max_row = k;
for i in (k + 1)..n {
if a[idx(i, k)].abs() > max_val {
max_val = a[idx(i, k)].abs();
max_row = i;
}
}
// Swap rows
if max_row != k {
for j in 0..n {
a.swap(idx(k, j), idx(max_row, j));
}
b.swap(k, max_row);
}
// Eliminate
for i in (k + 1)..n {
let factor = a[idx(i, k)] / a[idx(k, k)];
for j in k..n {
a[idx(i, j)] -= factor * a[idx(k, j)];
}
b[i] -= factor * b[k];
}
}
// Back substitution
for i in (0..n).rev() {
let mut sum = b[i];
for j in (i + 1)..n {
sum -= a[idx(i, j)] * x[j];
}
x[i] = sum / a[idx(i, i)];
}
x
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_lineqs_2x2() {
let mut a = vec![2.0, 1.0, 1.0, 3.0];
let mut b = vec![5.0, 7.0];
let x = lineqs(&mut a, &mut b, 2);
assert!((x[0] - 1.6).abs() < 1e-10);
assert!((x[1] - 1.8).abs() < 1e-10);
}
#[test]
fn test_lineqs_3x3() {
// x=1, y=2, z=3: 1+2+3=6, 2+2+9=13, 1+6+6=13
let mut a = vec![1.0, 1.0, 1.0, 2.0, 1.0, 3.0, 1.0, 3.0, 2.0];
let mut b = vec![6.0, 13.0, 13.0];
let x = lineqs(&mut a, &mut b, 3);
assert!((x[0] - 1.0).abs() < 1e-10);
assert!((x[1] - 2.0).abs() < 1e-10);
assert!((x[2] - 3.0).abs() < 1e-10);
}
#[test]
fn test_lineqs_identity() {
let mut a = vec![1.0, 0.0, 0.0, 0.0, 1.0, 0.0, 0.0, 0.0, 1.0];
let mut b = vec![5.0, 3.0, 7.0];
let x = lineqs(&mut a, &mut b, 3);
assert!((x[0] - 5.0).abs() < 1e-10);
assert!((x[1] - 3.0).abs() < 1e-10);
assert!((x[2] - 7.0).abs() < 1e-10);
}
#[test]
fn test_lineqs_1x1() {
let mut a = vec![4.0];
let mut b = vec![8.0];
let x = lineqs(&mut a, &mut b, 1);
assert!((x[0] - 2.0).abs() < 1e-10);
}
#[test]
fn test_lineqs_diagonal() {
let mut a = vec![2.0, 0.0, 0.0, 0.0, 3.0, 0.0, 0.0, 0.0, 5.0];
let mut b = vec![4.0, 9.0, 15.0];
let x = lineqs(&mut a, &mut b, 3);
assert!((x[0] - 2.0).abs() < 1e-10);
assert!((x[1] - 3.0).abs() < 1e-10);
assert!((x[2] - 3.0).abs() < 1e-10);
}
#[test]
fn test_lineqs_needs_pivoting() {
let mut a = vec![0.0, 1.0, 1.0, 1.0];
let mut b = vec![1.0, 3.0];
let x = lineqs(&mut a, &mut b, 2);
assert!((x[0] - 2.0).abs() < 1e-10);
assert!((x[1] - 1.0).abs() < 1e-10);
}
#[test]
fn test_lineqs_4x4() {
// Non-singular 4x4 matrix
let a_orig = vec![
2.0, 1.0, 1.0, 0.0, //
4.0, 3.0, 3.0, 1.0, //
8.0, 7.0, 9.0, 5.0, //
6.0, 7.0, 9.0, 8.0, //
];
let b_orig = vec![4.0, 11.0, 29.0, 30.0];
let mut a = a_orig.clone();
let mut b = b_orig.clone();
let x = lineqs(&mut a, &mut b, 4);
// Verify A*x = b
for i in 0..4 {
let mut sum = 0.0;
for j in 0..4 {
sum += a_orig[i * 4 + j] * x[j];
}
assert!(
(sum - b_orig[i]).abs() < 1e-8,
"Row {}: got {}, expected {}",
i,
sum,
b_orig[i]
);
}
}
}
+594
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@@ -0,0 +1,594 @@
//! 线不透明度和发射率计算。
//!
//! 翻译自 SYNSPEC `LINOP` 子程序 (synspec54.f:10427)。
//!
//! 计算给定深度点所有谱线的总吸收系数 (ABLIN) 和发射系数 (EMLIN)。
//! 包括 LTE 线、NLTE 线、He I 特殊线 (PHE1) 和 He II 线 (PHE2)。
use super::phe1::{phe1, Phe1Params};
use super::phe2::{phe2, Phe2Params};
use super::voigtk::{voigtk, MVOI};
/// 物理常数
const UN: f64 = 1.0;
const EXT0: f64 = 3.17;
const TEN: f64 = 10.0;
/// h*c/k (cm·K) — 用于能量到温度的转换
const C3: f64 = 1.4387886;
/// 1/kT 转换因子 (cm^-1 → eV)
const XET: f64 = 8067.6;
const XET3: f64 = XET * C3;
/// 单条谱线的输入数据。
#[derive(Debug, Clone)]
pub struct LineData {
/// 谱线索引 (IL)
pub il: usize,
/// NLTE 指标 (<0: NLTE, =0: LTE, >0: NLTE with ABCENT)
pub innlt: i32,
/// 原子序号 (IAT = INDAT/100)
pub iat: usize,
/// 电离级 (ION = INDAT%100)
pub ion: usize,
/// 轮廓类型 (ISPRF)
pub isprf: usize,
/// 线心频率 (Hz)
pub freq0: f64,
/// log(gf) - E_low/kT
pub gf0: f64,
/// 下能级激发能 (cm^-1)
pub excl0: f64,
/// 上能级激发能 (cm^-1)
pub excu0: f64,
/// 线心频率索引 (IJCNTR)
pub ijcntr: usize,
/// 阻尼参数 (由 PROFIL 返回)
pub agam: f64,
/// Doppler 宽度的倒数 (1/DOP1)
pub dop1_inv: f64,
// --- NLTE 相关 ---
/// NLTE 线心吸收 (ABCENT, INNLT>0 时使用)
pub abcent: f64,
/// NLTE 线心源函数 (SLIN, INNLT>0 时使用)
pub slin: f64,
/// 下能级索引 (ILOWN, INNLT<0 时使用)
pub ilown: usize,
/// 上能级索引 (IUPN, INNLT<0 时使用)
pub iupn: usize,
}
/// LINOP 参数结构体。
#[derive(Debug)]
pub struct LinopParams<'a> {
/// 深度索引 (1-indexed)
pub id: usize,
/// 温度 (K)
pub temp: f64,
/// 频率数
pub nfreq: usize,
/// 频率数组 (Hz)
pub freq: &'a [f64],
/// 总频率数 (NFREQS)
pub nfreqs: usize,
/// 频率连续间距因子 (DFRCON)
pub dfrcon: f64,
/// 平均连续吸收系数 (AVAB)
pub avab: f64,
/// Planck 函数 (PLAN)
pub plan: f64,
/// 受激辐射修正 (STIM)
pub stim: f64,
/// 谱线数 (NLIN)
pub nlin: usize,
/// 谱线数据
pub lines: &'a [LineData],
/// RRR(ID,ION,IAT) — Saha/Boltzmann 因子
pub rrr: &'a [f64],
/// RRR 数组维度: [natom][nion]
pub rrr_dims: (usize, usize),
/// Doppler 宽度 DOPA1(IAT, ID)
pub dopa1: &'a [f64],
/// DOPA1 维度: [natom]
pub dopa1_nat: usize,
/// 能级统计权重 G(level)
pub g: &'a [f64],
/// 能级布居数 POPUL(level, ID)
pub popul: &'a [f64],
/// POPUL 维度: [nlevel]
pub popul_nlev: usize,
/// PNLT(IAT, ION, ID) — NLTE 布居数
pub pnlt: &'a [f64],
/// PNLT 维度: [natom][nion]
pub pnlt_dims: (usize, usize),
/// ENEV(IAT, ION) — 电离能 (cm^-1)
pub enev: &'a [f64],
/// ENEV 维度: [natom]
pub enev_nat: usize,
/// ENION(level) — 能级能量 (erg)
pub enion: &'a [f64],
/// 激光删除标志 (lasdel)
pub lasdel: bool,
/// He II 特殊线数 (NSP)
pub nsp: usize,
/// He II 特殊线索引 (ISP0)
pub isp0: &'a [usize],
/// Voigt 函数表 H0
pub h0tab: &'a [f64; MVOI],
/// Voigt 函数表 H1
pub h1tab: &'a [f64; MVOI],
/// Voigt 函数表 H2
pub h2tab: &'a [f64; MVOI],
/// PHE1 所需的轮廓表参数 (简化传递)
pub phe1_data: Option<Phe1Data<'a>>,
/// PHE2 所需的参数 (简化传递)
pub phe2_common: Option<Phe2Common<'a>>,
}
/// PHE1 轮廓表数据。
#[derive(Debug)]
pub struct Phe1Data<'a> {
pub vturb: f64,
pub elec: f64,
pub prf447: &'a [f64],
pub dlm447: &'a [f64],
pub xne447: &'a [f64],
pub nwlam_447: &'a [usize],
pub prfhe1: &'a [f64],
pub dlmhe1: &'a [f64],
pub xnehe1: &'a [f64],
pub nwlam_he1: &'a [usize],
pub max_wlam_447: usize,
pub max_wlam_he1: usize,
}
/// PHE2 公共数据。
#[derive(Debug)]
pub struct Phe2Common<'a> {
pub ielhe2: i32,
pub inlte: i32,
pub he3_pop: f64,
pub nlhe2: i32,
pub nfirst_he2: i32,
pub wlam: &'a [f64],
pub prfhe2: &'a [f64],
pub wlhe2: &'a [f64],
pub nwlhe2: i32,
pub ilhe2: i32,
pub iuhe2: i32,
pub lasdel: bool,
}
/// LINOP 输出结果。
#[derive(Debug)]
pub struct LinopResult {
/// 吸收系数数组
pub ablin: Vec<f64>,
/// 发射系数数组
pub emlin: Vec<f64>,
}
/// 计算线不透明度和发射率。
///
/// # 参数
/// * `params` - LINOP 参数
///
/// # 返回
/// 吸收系数和发射系数数组
pub fn linop(params: &LinopParams) -> LinopResult {
let nfreq = params.nfreq;
let mut ablin = vec![0.0f64; nfreq];
let mut ablinn = vec![0.0f64; nfreq];
let mut emlin = vec![0.0f64; nfreq];
if params.nlin == 0 {
return LinopResult { ablin, emlin };
}
let tem1 = UN / params.temp;
for line_data in params.lines.iter().take(params.nlin) {
let _il = line_data.il;
let innlt = line_data.innlt;
let iat = line_data.iat;
let ion = line_data.ion;
let isprf = line_data.isprf;
// 判断是否使用标准轮廓 (Voigt)
let lpr = !(isprf > 1 && isprf <= 5);
if isprf >= 6 {
continue;
}
// PROFIL 已在外部调用,agam 从 line_data 获取
let agam = line_data.agam;
let dop1 = 1.0 / line_data.dop1_inv; // DOP1 = 1/dop1_inv
let fr0 = line_data.freq0;
// 计算线心吸收系数 ab0 和源函数 sl0
let (ab0, sl0) = if innlt == 0 {
// LTE 线
let rrr_idx = params.rrr_dims.0 * params.rrr_dims.1 * (params.id - 1)
+ ion * params.rrr_dims.0
+ iat;
let rrr_val = if rrr_idx < params.rrr.len() {
params.rrr[rrr_idx]
} else {
0.0
};
let ab0 = (line_data.gf0 - line_data.excl0 * tem1).exp()
* rrr_val
* dop1
* params.stim;
(ab0, 0.0)
} else if innlt > 0 {
// NLTE 线 (有 ABCENT/SLIN)
(line_data.abcent, line_data.slin)
} else {
// NLTE 线 (通过能级布居数计算)
let pnlt_idx = params.pnlt_dims.0 * params.pnlt_dims.1 * (params.id - 1)
+ ion * params.pnlt_dims.0
+ iat;
let pp = if pnlt_idx < params.pnlt.len() {
params.pnlt[pnlt_idx]
} else {
0.0
};
// 下能级布居数
let pi = if line_data.ilown > 0 {
let pop_idx = (line_data.ilown - 1) * params.popul_nlev + (params.id - 1);
if pop_idx < params.popul.len() {
params.popul[pop_idx] / params.g[line_data.ilown - 1]
} else {
0.0
}
} else {
let enev_idx = params.enev_nat * (params.id - 1) + iat;
let enev_val = if enev_idx < params.enev.len() {
params.enev[enev_idx]
} else {
0.0
};
pp * ((enev_val * XET3 - line_data.excl0) * tem1).exp()
};
// 上能级布居数
let (pj, cor) = if line_data.iupn > 0 {
let pop_idx = (line_data.iupn - 1) * params.popul_nlev + (params.id - 1);
let pj = if pop_idx < params.popul.len() {
params.popul[pop_idx] / params.g[line_data.iupn - 1]
} else {
0.0
};
let cor = if line_data.ilown > 0 && line_data.iupn > 0 {
let enion_iun = params.enion[line_data.iupn - 1];
let enion_ilw = params.enion[line_data.ilown - 1];
((line_data.excu0 - line_data.excl0
+ (enion_iun - enion_ilw) / 1.38054e-16)
* tem1)
.exp()
} else {
1.0
};
(pj, cor)
} else {
let enev_idx = params.enev_nat * (params.id - 1) + iat;
let enev_val = if enev_idx < params.enev.len() {
params.enev[enev_idx]
} else {
0.0
};
let pj = pp * ((enev_val * XET3 - line_data.excu0) * tem1).exp();
(pj, 1.0)
};
let x = if pj > 0.0 {
pi / pj * cor
} else {
UN
};
let x = if x == UN {
(4.79928e-11 * fr0 * tem1).exp()
} else {
x
};
let sl0 = params.plan / (x - UN); // BNUL ≈ PLAN for this context
let ab0 = if pi > 0.0 {
pi * (UN - UN / x) * line_data.gf0.exp() * dop1
} else {
0.0
};
(ab0, sl0)
};
// 激光删除检查
if ab0 <= 0.0 && params.lasdel {
continue;
}
// 确定频率贡献范围
let ex0 = if params.avab > 0.0 {
ab0 / params.avab * agam
} else {
0.0
};
let ext = if ex0 > TEN {
ex0.sqrt()
} else {
EXT0
};
let ext = ext / dop1;
let xijext = params.dfrcon * ext + 1.5;
let ij1 = ((line_data.ijcntr as f64) - xijext).max(3.0) as usize;
let ij2 = ((line_data.ijcntr as f64) + xijext).min(params.nfreqs as f64) as usize;
if ij1 >= nfreq || ij2 <= 2 {
continue;
}
if innlt == 0 {
// LTE 线
if lpr {
// 标准 Voigt 轮廓
for ij in ij1..=ij2.min(nfreq - 1) {
let xf = (params.freq[ij] - fr0).abs() * dop1;
ablin[ij] += ab0 * voigtk(agam, xf, params.h0tab, params.h1tab, params.h2tab);
}
} else {
// He I 特殊线 (ISP 2-5)
let _phe1_params = Phe1Params {
id: params.id,
freq: 0.0, // 在循环中设置
iline: isprf - 1,
temp: params.temp,
elec: 0.0,
vturb: 0.0,
prf447: &[],
dlm447: &[],
xne447: &[],
nwlam_447: &[],
prfhe1: &[],
dlmhe1: &[],
xnehe1: &[],
nwlam_he1: &[],
max_wlam_447: 0,
max_wlam_he1: 0,
h0tab: params.h0tab,
h1tab: params.h1tab,
h2tab: params.h2tab,
};
// PHE1 需要完整的轮廓表数据
// 如果 phe1_data 存在则使用,否则跳过
if let Some(ref phe1d) = params.phe1_data {
for ij in 3..nfreq {
let fr = params.freq[ij];
let phe1_p = Phe1Params {
id: params.id,
freq: fr,
iline: isprf - 1,
temp: params.temp,
elec: phe1d.elec,
vturb: phe1d.vturb,
prf447: phe1d.prf447,
dlm447: phe1d.dlm447,
xne447: phe1d.xne447,
nwlam_447: phe1d.nwlam_447,
prfhe1: phe1d.prfhe1,
dlmhe1: phe1d.dlmhe1,
xnehe1: phe1d.xnehe1,
nwlam_he1: phe1d.nwlam_he1,
max_wlam_447: phe1d.max_wlam_447,
max_wlam_he1: phe1d.max_wlam_he1,
h0tab: params.h0tab,
h1tab: params.h1tab,
h2tab: params.h2tab,
};
let abl = ab0 * phe1(&phe1_p);
ablin[ij] += abl;
}
}
}
} else {
// NLTE 线
if lpr {
// 标准 Voigt 轮廓
for ij in ij1..=ij2.min(nfreq - 1) {
let xf = (params.freq[ij] - fr0).abs() * dop1;
let abl = ab0 * voigtk(agam, xf, params.h0tab, params.h1tab, params.h2tab);
ablinn[ij] += abl;
emlin[ij] += abl * sl0;
}
} else {
// He I 特殊线
if let Some(ref phe1d) = params.phe1_data {
for ij in 3..nfreq {
let fr = params.freq[ij];
let phe1_p = Phe1Params {
id: params.id,
freq: fr,
iline: isprf - 1,
temp: params.temp,
elec: phe1d.elec,
vturb: phe1d.vturb,
prf447: phe1d.prf447,
dlm447: phe1d.dlm447,
xne447: phe1d.xne447,
nwlam_447: phe1d.nwlam_447,
prfhe1: phe1d.prfhe1,
dlmhe1: phe1d.dlmhe1,
xnehe1: phe1d.xnehe1,
nwlam_he1: phe1d.nwlam_he1,
max_wlam_447: phe1d.max_wlam_447,
max_wlam_he1: phe1d.max_wlam_he1,
h0tab: params.h0tab,
h1tab: params.h1tab,
h2tab: params.h2tab,
};
let abl = ab0 * phe1(&phe1_p);
ablinn[ij] += abl;
emlin[ij] += abl * sl0;
}
}
}
}
}
// 添加连续谱贡献到发射率
for ij in 3..nfreq {
emlin[ij] += ablin[ij] * params.plan;
ablin[ij] += ablinn[ij];
}
// He II 特殊线 (PHE2)
if params.nsp > 0
&& let Some(ref phe2c) = params.phe2_common {
for &isp in params.isp0.iter().take(params.nsp) {
if (6..=24).contains(&isp) {
let phe2_p = Phe2Params {
ispec: isp as i32,
id: params.id as i32,
ielhe2: phe2c.ielhe2,
inlte: phe2c.inlte,
nfreq: nfreq as i32,
freq: params.freq,
wlam: phe2c.wlam,
temp: params.temp,
elec: 0.0, // 由 PHE2 内部处理
he3_pop: phe2c.he3_pop,
nlhe2: phe2c.nlhe2,
nfirst_he2: phe2c.nfirst_he2,
popul: &[],
prfhe2: phe2c.prfhe2,
wlhe2: phe2c.wlhe2,
nwlhe2: phe2c.nwlhe2,
ilhe2: phe2c.ilhe2,
iuhe2: phe2c.iuhe2,
lasdel: phe2c.lasdel,
};
let result = phe2(&phe2_p);
for ij in 0..nfreq {
ablin[ij] += result.ablin[ij];
emlin[ij] += result.emlin[ij];
}
}
}
}
LinopResult { ablin, emlin }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_linop_zero_lines() {
// NLIN=0 → 返回全零
let params = LinopParams {
id: 1,
temp: 10000.0,
nfreq: 10,
freq: &vec![1e14; 10],
nfreqs: 10,
dfrcon: 1.0,
avab: 1.0,
plan: 1.0,
stim: 1.0,
nlin: 0,
lines: &[],
rrr: &[],
rrr_dims: (0, 0),
dopa1: &[],
dopa1_nat: 0,
g: &[],
popul: &[],
popul_nlev: 0,
pnlt: &[],
pnlt_dims: (0, 0),
enev: &[],
enev_nat: 0,
enion: &[],
lasdel: false,
nsp: 0,
isp0: &[],
h0tab: &[0.0; MVOI],
h1tab: &[0.0; MVOI],
h2tab: &[0.0; MVOI],
phe1_data: None,
phe2_common: None,
};
let result = linop(&params);
assert!(result.ablin.iter().all(|&x| x == 0.0));
assert!(result.emlin.iter().all(|&x| x == 0.0));
}
#[test]
fn test_linop_basic_lte_line() {
// 基本 LTE 线测试
let freq: Vec<f64> = (0..20).map(|i| 1e14 + i as f64 * 1e12).collect();
let h0tab = [0.0f64; MVOI];
let h1tab = [0.0f64; MVOI];
let h2tab = [0.0f64; MVOI];
let line = LineData {
il: 1,
innlt: 0,
iat: 0,
ion: 0,
isprf: 1, // 标准 Voigt
freq0: 1.01e14,
gf0: 0.0, // log(gf)=0 → gf=1
excl0: 0.0,
excu0: 0.0,
ijcntr: 1,
agam: 0.01,
dop1_inv: 1e-10,
abcent: 0.0,
slin: 0.0,
ilown: 0,
iupn: 0,
};
let params = LinopParams {
id: 1,
temp: 10000.0,
nfreq: 20,
freq: &freq,
nfreqs: 20,
dfrcon: 1.0,
avab: 1.0,
plan: 1.0,
stim: 1.0,
nlin: 1,
lines: &[line],
rrr: &[1.0],
rrr_dims: (1, 1),
dopa1: &[1e10],
dopa1_nat: 1,
g: &[1.0],
popul: &[1.0],
popul_nlev: 1,
pnlt: &[0.0],
pnlt_dims: (1, 1),
enev: &[0.0],
enev_nat: 1,
enion: &[0.0],
lasdel: false,
nsp: 0,
isp0: &[],
h0tab: &h0tab,
h1tab: &h1tab,
h2tab: &h2tab,
phe1_data: None,
phe2_common: None,
};
let result = linop(&params);
assert_eq!(result.ablin.len(), 20);
assert_eq!(result.emlin.len(), 20);
// 验证结果是有限的
assert!(result.ablin.iter().all(|&x| x.is_finite()));
assert!(result.emlin.iter().all(|&x| x.is_finite()));
}
}
+501
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@@ -0,0 +1,501 @@
//! 线不透明度和发射率计算(风模型变体)。
//!
//! 翻译自 SYNSPEC `LINOPW` 子程序 (synspec54.f:10590)。
//!
//! 与 LINOP 类似,但针对风模型做了以下扩展:
//! - 速度相关的线拒绝
//! - 辐射场处理 (itrad, trad, wdil)
//! - 窗口化频率网格的线心索引计算
//! - DOP1 = DOPA1(IAT,ID)/FR0 (与 LINOP 不同)
use super::phe1::{phe1, Phe1Params};
use super::phe2::{phe2, Phe2Params};
use super::voigtk::{voigtk, MVOI};
/// 物理常数
const UN: f64 = 1.0;
const EXT0: f64 = 3.17;
const TEN: f64 = 10.0;
const C3: f64 = 1.4387886;
const XET: f64 = 8067.6;
const XET3: f64 = XET * C3;
/// LINOPW 参数结构体。
///
/// 与 LinopParams 类似,但增加了风模型相关参数。
#[derive(Debug)]
pub struct LinopwParams<'a> {
/// 深度索引 (1-indexed)
pub id: usize,
/// 温度 (K)
pub temp: f64,
/// h/k (erg/K)
pub hk: f64,
/// 频率数
pub nfreq: usize,
/// 频率数组 (Hz)
pub freq: &'a [f64],
/// NOPAC — 不透明度截止频率索引
pub nopac: usize,
/// Planck 函数 PLAN(ID)
pub plan: f64,
/// 受激辐射修正 STIM(ID) — LINOPW 中未使用,保留接口兼容
pub stim: f64,
/// 谱线数 (NLIN)
pub nlin: usize,
/// 谱线数据
pub lines: &'a [LinopwLineData],
/// RRR(ID,ION,IAT)
pub rrr: &'a [f64],
/// RRR 维度: [natom][nion]
pub rrr_dims: (usize, usize),
/// DOPA1(IAT, ID) — Doppler 宽度
pub dopa1: &'a [f64],
/// DOPA1 维度: [natom]
pub dopa1_nat: usize,
/// G(level) — 能级统计权重
pub g: &'a [f64],
/// POPUL(level, ID) — 能级布居数
pub popul: &'a [f64],
/// POPUL 维度: [nlevel]
pub popul_nlev: usize,
/// PNLT(IAT, ION, ID) — NLTE 布居数
pub pnlt: &'a [f64],
/// PNLT 维度: [natom][nion]
pub pnlt_dims: (usize, usize),
/// ENEV(IAT, ION) — 电离能 (cm^-1)
pub enev: &'a [f64],
/// ENEV 维度: [natom]
pub enev_nat: usize,
/// ENION(level) — 能级能量 (erg)
pub enion: &'a [f64],
/// 激光删除标志 (lasdel)
pub lasdel: bool,
/// He II 特殊线数 (NSP)
pub nsp: usize,
/// He II 特殊线索引 (ISP0)
pub isp0: &'a [usize],
/// Voigt 函数表 H0
pub h0tab: &'a [f64; MVOI],
/// Voigt 函数表 H1
pub h1tab: &'a [f64; MVOI],
/// Voigt 函数表 H2
pub h2tab: &'a [f64; MVOI],
/// PHE1 轮廓表数据
pub phe1_data: Option<Phe1DataW<'a>>,
/// PHE2 公共数据
pub phe2_common: Option<Phe2CommonW<'a>>,
// --- 风模型特有参数 ---
/// 速度场 VEL(ID)
pub vel: f64,
/// 最大速度 VELMAX
pub velmax: f64,
/// 辐射场模式 (ITRAD)
pub itrad: i32,
/// 辐射温度 TRAD(ipotl, ID)
pub trad: &'a [f64],
/// TRAD 维度: [npotl]
pub trad_npotl: usize,
/// IPOTL(line) — 电离势索引
pub ipotl: &'a [usize],
/// BNUE(ij) — 频率相关 Planck 函数
pub bnue: &'a [f64],
/// NLTE 关闭标志 (NLTOFF)
pub nltoff: i32,
/// 发射关闭标志 (IEMOFF)
pub iemoff: i32,
/// 线心 NLTE 关闭标记 ILNE(depth)
pub ilne: &'a [usize],
/// 线心速度拒绝标记 ILVI(depth)
pub ilvi: &'a [usize],
/// 线心频率索引 IJCNTR(line) — 输出
pub ijcntr: &'a mut [usize],
/// 标准线吸收 ABSTDW(ijcont, ID)
pub abstdw: &'a [f64],
/// ABSTDW 维度: [nfreq]
pub abstdw_nfreq: usize,
/// RELOP — 相对不透明度阈值
pub relop: f64,
/// IJCONT(line) — 线心频率索引
pub ijcont: &'a [usize],
/// 准直函数 XJCON(ID) — 未使用,保留
pub xjcon: f64,
/// 稀释因子 WDIL(ID) — 输出
pub wdil_out: &'a mut f64,
}
/// 单条谱线数据 (LINOPW 版本)。
#[derive(Debug, Clone)]
pub struct LinopwLineData {
pub il: usize,
pub innlt: i32,
pub iat: usize,
pub ion: usize,
pub isprf: usize,
pub freq0: f64,
pub gf0: f64,
pub excl0: f64,
pub excu0: f64,
pub agam: f64,
pub dop1_inv: f64,
pub abcent: f64,
pub slin: f64,
pub ilown: usize,
pub iupn: usize,
}
/// PHE1 轮廓表数据 (LINOPW 版本)。
#[derive(Debug)]
pub struct Phe1DataW<'a> {
pub vturb: f64,
pub elec: f64,
pub prf447: &'a [f64],
pub dlm447: &'a [f64],
pub xne447: &'a [f64],
pub nwlam_447: &'a [usize],
pub prfhe1: &'a [f64],
pub dlmhe1: &'a [f64],
pub xnehe1: &'a [f64],
pub nwlam_he1: &'a [usize],
pub max_wlam_447: usize,
pub max_wlam_he1: usize,
}
/// PHE2 公共数据 (LINOPW 版本)。
#[derive(Debug)]
pub struct Phe2CommonW<'a> {
pub ielhe2: i32,
pub inlte: i32,
pub he3_pop: f64,
pub nlhe2: i32,
pub nfirst_he2: i32,
pub wlam: &'a [f64],
pub prfhe2: &'a [f64],
pub wlhe2: &'a [f64],
pub nwlhe2: i32,
pub ilhe2: i32,
pub iuhe2: i32,
pub lasdel: bool,
}
/// LINOPW 输出结果。
#[derive(Debug)]
pub struct LinopwResult {
pub ablin: Vec<f64>,
pub emlin: Vec<f64>,
}
/// 计算线不透明度和发射率(风模型变体)。
pub fn linopw(params: &mut LinopwParams) -> LinopwResult {
let nfreq = params.nfreq;
let mut ablin = vec![0.0f64; nfreq];
let mut ablinn = vec![0.0f64; nfreq];
let mut emlin = vec![0.0f64; nfreq];
*params.wdil_out = 1.0;
let _plw = params.plan * 1.0; // wdil=1
if params.nlin == 0 {
return LinopwResult { ablin, emlin };
}
let tem1 = UN / params.temp;
let hkt = params.hk * tem1;
// 计算频率间距因子
let xx = params.freq[nfreq - 1] - params.freq[0];
let dfrcon = if xx.abs() > 1e-30 {
-((params.nopac as f64) - 1.0) / xx
} else {
0.0
};
for (line_idx, line_data) in params.lines.iter().take(params.nlin).enumerate() {
let il = line_data.il;
let innlt = line_data.innlt;
// 速度拒绝
if params.ilvi[params.id - 1] > 0 {
if innlt == 0 {
continue;
} else if params.nltoff != 0 {
continue;
}
}
// 线心频率索引 (仅深度 1)
if params.id == 1 {
let fr0 = line_data.freq0;
let xjc = 3.0 + dfrcon * (params.freq[0] - fr0);
let mut ijc = xjc as usize;
if ijc > 1 && ijc < params.nopac {
// 在频率网格中找到最近的点
if fr0 < params.freq[ijc] {
let mut ijc0 = ijc;
let mut dfr0 = params.freq[ijc0] - fr0;
loop {
ijc0 += 1;
if ijc0 >= nfreq {
break;
}
let dfr = (params.freq[ijc0] - fr0).abs();
if dfr < dfr0 {
ijc = ijc0;
dfr0 = dfr;
} else {
break;
}
}
} else if fr0 > params.freq[ijc] {
let mut ijc0 = ijc;
let mut dfr0 = fr0 - params.freq[ijc0];
loop {
if ijc0 == 0 {
break;
}
ijc0 -= 1;
let dfr = (params.freq[ijc0] - fr0).abs();
if dfr < dfr0 {
ijc = ijc0;
dfr0 = dfr;
} else {
break;
}
}
}
}
params.ijcntr[line_idx] = ijc;
}
let iat = line_data.iat;
let ion = line_data.ion;
let fr0 = line_data.freq0;
let lpr = !(line_data.isprf > 1 && line_data.isprf <= 5);
if line_data.isprf >= 6 {
continue;
}
let agam = line_data.agam;
let dop1 = 1.0 / line_data.dop1_inv / fr0; // DOPA1(IAT,ID)/FR0
// 计算 ab0 和 sl0
let (ab0, sl0) = if innlt == 0 && params.itrad <= 0 {
// LTE 线 (无辐射场)
let rrr_idx = params.rrr_dims.0 * params.rrr_dims.1 * (params.id - 1)
+ ion * params.rrr_dims.0 + iat;
let rrr_val = if rrr_idx < params.rrr.len() { params.rrr[rrr_idx] } else { 0.0 };
let ab0 = (line_data.gf0 - line_data.excl0 * tem1).exp()
* rrr_val * dop1 * (1.0 - (-hkt * fr0).exp());
(ab0, 0.0)
} else if innlt == 0 && params.itrad > 0 {
// LTE 线 (有辐射场)
let ipotl_idx = if il < params.ipotl.len() { params.ipotl[il] } else { 0 };
let trad_idx = ipotl_idx * params.trad_npotl + (params.id - 1);
let trl = if trad_idx < params.trad.len() { params.trad[trad_idx] } else { params.temp };
let xx = (-hkt * fr0).exp();
let rrr_idx = params.rrr_dims.0 * params.rrr_dims.1 * (params.id - 1)
+ ion * params.rrr_dims.0 + iat;
let rrr_val = if rrr_idx < params.rrr.len() { params.rrr[rrr_idx] } else { 0.0 };
let mut ab0 = (line_data.gf0 - line_data.excl0 / trl).exp()
* rrr_val * dop1 * (1.0 - xx);
if line_data.excl0 > 2000.0 {
ab0 *= 1.0; // wdil=1
}
let pla = 1.4743e-2 * (fr0 * 1e-15).powi(3) * xx / (1.0 - xx);
let sl0 = pla * 1.0; // wdil=1
(ab0, sl0)
} else if innlt > 0 {
(line_data.abcent, line_data.slin)
} else {
// NLTE 线
let pnlt_idx = params.pnlt_dims.0 * params.pnlt_dims.1 * (params.id - 1)
+ ion * params.pnlt_dims.0 + iat;
let pp = if pnlt_idx < params.pnlt.len() { params.pnlt[pnlt_idx] } else { 0.0 };
let pi = if line_data.ilown > 0 {
let pop_idx = (line_data.ilown - 1) * params.popul_nlev + (params.id - 1);
if pop_idx < params.popul.len() {
params.popul[pop_idx] / params.g[line_data.ilown - 1]
} else { 0.0 }
} else {
let enev_idx = params.enev_nat * (params.id - 1) + iat;
let enev_val = if enev_idx < params.enev.len() { params.enev[enev_idx] } else { 0.0 };
pp * ((enev_val * XET3 - line_data.excl0) * tem1).exp()
};
let (pj, cor) = if line_data.iupn > 0 {
let pop_idx = (line_data.iupn - 1) * params.popul_nlev + (params.id - 1);
let pj = if pop_idx < params.popul.len() {
params.popul[pop_idx] / params.g[line_data.iupn - 1]
} else { 0.0 };
let cor = if line_data.ilown > 0 && line_data.iupn > 0 {
((line_data.excu0 - line_data.excl0
+ (params.enion[line_data.iupn - 1] - params.enion[line_data.ilown - 1]) / 1.38054e-16)
* tem1).exp()
} else { 1.0 };
(pj, cor)
} else {
let enev_idx = params.enev_nat * (params.id - 1) + iat;
let enev_val = if enev_idx < params.enev.len() { params.enev[enev_idx] } else { 0.0 };
let pj = pp * ((enev_val * XET3 - line_data.excu0) * tem1).exp();
(pj, 1.0)
};
let x = if pj > 0.0 { pi / pj * cor } else { UN };
let x = if x == UN { (4.79928e-11 * fr0 * tem1).exp() } else { x };
let sl0 = params.plan / (x - UN);
let ab0 = if pi > 0.0 { pi * (UN - UN / x) * line_data.gf0.exp() * dop1 } else { 0.0 };
(ab0, sl0)
};
if ab0 <= 0.0 && params.lasdel {
continue;
}
// 频率贡献范围
let ijcont_idx = if il < params.ijcont.len() { params.ijcont[il] } else { 0 };
let abstdw_idx = ijcont_idx * params.abstdw_nfreq + (params.id - 1);
let avabw = if abstdw_idx < params.abstdw.len() {
params.abstdw[abstdw_idx] * params.relop
} else { 0.0 };
let ex0 = if avabw > 0.0 { ab0 / avabw * agam } else { 0.0 };
let ext = if ex0 > TEN { ex0.sqrt() } else { EXT0 };
let ext = ext / dop1;
let ijext = (dfrcon * ext + 1.5) as usize;
let ijctr = params.ijcntr[line_idx];
let ij1 = ijctr.saturating_sub(ijext).max(1);
let ij2 = (ijctr + ijext).min(nfreq);
if ij1 >= nfreq || ij2 <= 2 {
continue;
}
if innlt == 0 && params.itrad <= 0 {
// LTE 线
if lpr {
for ij in ij1..=ij2.min(nfreq - 1) {
let xf = (params.freq[ij] - fr0).abs() * dop1;
ablin[ij] += ab0 * voigtk(agam, xf, params.h0tab, params.h1tab, params.h2tab);
}
} else if let Some(ref phe1d) = params.phe1_data {
for ij in 0..nfreq {
let phe1_p = Phe1Params {
id: params.id, freq: params.freq[ij], iline: line_data.isprf - 1,
temp: params.temp, elec: phe1d.elec, vturb: phe1d.vturb,
prf447: phe1d.prf447, dlm447: phe1d.dlm447, xne447: phe1d.xne447,
nwlam_447: phe1d.nwlam_447, prfhe1: phe1d.prfhe1, dlmhe1: phe1d.dlmhe1,
xnehe1: phe1d.xnehe1, nwlam_he1: phe1d.nwlam_he1,
max_wlam_447: phe1d.max_wlam_447, max_wlam_he1: phe1d.max_wlam_he1,
h0tab: params.h0tab, h1tab: params.h1tab, h2tab: params.h2tab,
};
ablin[ij] += ab0 * phe1(&phe1_p);
}
}
} else {
// NLTE 线 或 有辐射场的 LTE 线
if lpr {
for ij in ij1..=ij2.min(nfreq - 1) {
let xf = (params.freq[ij] - fr0).abs() * dop1;
let abl = ab0 * voigtk(agam, xf, params.h0tab, params.h1tab, params.h2tab);
ablinn[ij] += abl;
if params.ilne[params.id - 1] == 0 {
emlin[ij] += abl * sl0;
}
}
} else if let Some(ref phe1d) = params.phe1_data {
for ij in 0..nfreq {
let phe1_p = Phe1Params {
id: params.id, freq: params.freq[ij], iline: line_data.isprf - 1,
temp: params.temp, elec: phe1d.elec, vturb: phe1d.vturb,
prf447: phe1d.prf447, dlm447: phe1d.dlm447, xne447: phe1d.xne447,
nwlam_447: phe1d.nwlam_447, prfhe1: phe1d.prfhe1, dlmhe1: phe1d.dlmhe1,
xnehe1: phe1d.xnehe1, nwlam_he1: phe1d.nwlam_he1,
max_wlam_447: phe1d.max_wlam_447, max_wlam_he1: phe1d.max_wlam_he1,
h0tab: params.h0tab, h1tab: params.h1tab, h2tab: params.h2tab,
};
let abl = ab0 * phe1(&phe1_p);
ablinn[ij] += abl;
if params.ilne[params.id - 1] == 0 {
emlin[ij] += abl * sl0;
}
}
}
}
}
// 连续谱贡献
if params.vel <= params.velmax {
for ij in 0..nfreq {
let pla = if (hkt * params.freq[ij]).exp() - 1.0 > 1e-30 {
params.bnue[ij] / ((hkt * params.freq[ij]).exp() - 1.0)
} else { 0.0 };
emlin[ij] += ablin[ij] * pla; // wdil=1
ablin[ij] += ablinn[ij];
}
}
// He II 特殊线
if params.nsp > 0
&& let Some(ref phe2c) = params.phe2_common {
for &isp in params.isp0.iter().take(params.nsp) {
if (6..=24).contains(&isp) {
let phe2_p = Phe2Params {
ispec: isp as i32, id: params.id as i32,
ielhe2: phe2c.ielhe2, inlte: phe2c.inlte,
nfreq: nfreq as i32, freq: params.freq, wlam: phe2c.wlam,
temp: params.temp, elec: 0.0, he3_pop: phe2c.he3_pop,
nlhe2: phe2c.nlhe2, nfirst_he2: phe2c.nfirst_he2,
popul: &[], prfhe2: phe2c.prfhe2, wlhe2: phe2c.wlhe2,
nwlhe2: phe2c.nwlhe2, ilhe2: phe2c.ilhe2, iuhe2: phe2c.iuhe2,
lasdel: phe2c.lasdel,
};
let result = phe2(&phe2_p);
for ij in 0..nfreq {
ablin[ij] += result.ablin[ij];
emlin[ij] += result.emlin[ij];
}
}
}
}
LinopwResult { ablin, emlin }
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_linopw_zero_lines() {
let freq = vec![1e14; 10];
let h0tab = [0.0f64; MVOI];
let h1tab = [0.0f64; MVOI];
let h2tab = [0.0f64; MVOI];
let mut wdil = 0.0f64;
let mut ijcntr = vec![0usize; 1];
let mut params = LinopwParams {
id: 1, temp: 10000.0, hk: 4.79928e-11,
nfreq: 10, freq: &freq, nopac: 10,
plan: 1.0, stim: 1.0, nlin: 0, lines: &[],
rrr: &[], rrr_dims: (0, 0), dopa1: &[], dopa1_nat: 0,
g: &[], popul: &[], popul_nlev: 0,
pnlt: &[], pnlt_dims: (0, 0),
enev: &[], enev_nat: 0, enion: &[],
lasdel: false, nsp: 0, isp0: &[],
h0tab: &h0tab, h1tab: &h1tab, h2tab: &h2tab,
phe1_data: None, phe2_common: None,
vel: 0.0, velmax: 1e10, itrad: 0,
trad: &[], trad_npotl: 0, ipotl: &[],
bnue: &freq, nltoff: 0, iemoff: 0,
ilne: &[0], ilvi: &[0],
ijcntr: &mut ijcntr,
abstdw: &[], abstdw_nfreq: 0, relop: 1.0,
ijcont: &[0], xjcon: 0.0, wdil_out: &mut wdil,
};
let result = linopw(&mut params);
assert!(result.ablin.iter().all(|&x| x == 0.0));
assert!(result.emlin.iter().all(|&x| x == 0.0));
}
}
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//! 二分查找子程序。
//!
//! 重构自 SYNSPEC `locate.f`
//!
//! 在有序数组 `xx` 中查找值 `x` 的位置,使得 `xx[j] <= x < xx[j+1]`。
/// 在有序数组中二分查找。
///
/// 查找 `x` 在有序数组 `xx[0..n]` 中的插入位置。
/// 返回索引 `j`,使得 `xx[j-1] <= x < xx[j]`1-indexed)。
///
/// # 参数
///
/// * `xx` - 有序数组(升序或降序)
/// * `n` - 数组有效长度
/// * `x` - 待查找的值
///
/// # 返回值
///
/// 索引 `j`1-indexed),使得 `xx[j-1] <= x < xx[j]`
pub fn locate(xx: &[f64], n: usize, x: f64) -> usize {
let mut jl: isize = 0;
let mut ju = (n + 1) as isize;
while ju - jl > 1 {
let jm = (ju + jl) / 2;
if (xx[n - 1] >= xx[0]) == (x >= xx[jm as usize - 1]) {
jl = jm;
} else {
ju = jm;
}
}
if x == xx[0] {
1
} else if x == xx[n - 1] {
n - 1
} else {
jl as usize
}
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_locate_basic() {
let xx = [1.0, 2.0, 3.0, 4.0, 5.0];
// x=2.5 应该在 xx[1] 和 xx[2] 之间,返回 j=2
let j = locate(&xx, 5, 2.5);
assert!(j >= 1 && j <= 4);
assert!(xx[j - 1] <= 2.5 && xx[j] >= 2.5);
}
#[test]
fn test_locate_exact_first() {
let xx = [1.0, 2.0, 3.0, 4.0, 5.0];
let j = locate(&xx, 5, 1.0);
assert_eq!(j, 1);
}
#[test]
fn test_locate_exact_last() {
let xx = [1.0, 2.0, 3.0, 4.0, 5.0];
let j = locate(&xx, 5, 5.0);
assert_eq!(j, 4);
}
#[test]
fn test_locate_between() {
let xx = [0.0, 10.0, 20.0, 30.0];
let j = locate(&xx, 4, 15.0);
assert!(j >= 1 && j <= 3);
assert!(xx[j - 1] <= 15.0 && xx[j] >= 15.0);
}
}
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//! Lyman alpha broadening by helium.
//!
//! Translated from SYNSPEC `lyahhe` subroutine (synspec54.f:12768).
//!
//! Calculates the Lyman alpha profile broadened by helium collisions,
//! using cross-section data from N. Allard.
use std::sync::OnceLock;
/// Maximum number of cross-section data points
const NXMAX: usize = 1000;
/// Cross-section normalization factor for He-H broadening
static STHE: OnceLock<f64> = OnceLock::new();
/// Flag for wavelength unit conversion (1 = convert from Angstrom)
static NUNHHE: OnceLock<i32> = OnceLock::new();
/// Cached cross-section data
struct HeHData {
xlhhe: Vec<f64>,
sighhe: Vec<f64>,
nxhhe: usize,
}
static HEH_DATA: OnceLock<HeHData> = OnceLock::new();
/// Initialize the He-H broadening data from a file.
///
/// This should be called once before using `lyahhe`. The data is read from
/// unit 67 (typically `siglyhhe_21_T14500.lam`).
///
/// # Arguments
/// * `sthe_val` - Cross-section normalization factor
/// * `nunhhe_val` - Flag for wavelength unit conversion
/// * `data_lines` - Iterator of (wavelength, cross-section) pairs from the data file
pub fn lyahhe_init<I>(sthe_val: f64, nunhhe_val: i32, data_lines: I)
where
I: IntoIterator<Item = (f64, f64)>,
{
let _ = STHE.set(sthe_val);
let _ = NUNHHE.set(nunhhe_val);
let nunhhe = nunhhe_val;
let mut xlhh0 = Vec::with_capacity(NXMAX);
let mut sighh0 = Vec::with_capacity(NXMAX);
for (xl, sig) in data_lines.into_iter().take(NXMAX) {
let xl_conv = if nunhhe == 1 {
1.0 / (1.0e-8 * xl + 1.0 / 1215.67)
} else {
xl
};
xlhh0.push(xl_conv);
sighh0.push(sig);
}
let nxhhe = xlhh0.len();
// Reverse the arrays (Fortran reads in reverse order)
let mut xlhhe: Vec<f64> = xlhh0.into_iter().rev().collect();
let mut sighhe: Vec<f64> = sighh0.into_iter().rev().collect();
// Ensure sorted for binary search
// After reversal, data should be in ascending wavelength order
// but let's verify and sort if needed
if nxhhe > 1 && xlhhe[0] > xlhhe[nxhhe - 1] {
xlhhe.reverse();
sighhe.reverse();
}
let _ = HEH_DATA.set(HeHData {
xlhhe,
sighhe,
nxhhe,
});
}
/// Calculate Lyman alpha profile broadened by helium.
///
/// Uses binary search and linear interpolation on pre-loaded cross-section data.
///
/// # Arguments
/// * `xl` - Wavelength (Å)
/// * `ahe` - He atom density
///
/// # Returns
/// Profile value (0.0 if wavelength is outside data range)
pub fn lyahhe(xl: f64, ahe: f64) -> f64 {
let data = match HEH_DATA.get() {
Some(d) => d,
None => return 0.0, // Data not initialized
};
let sthe = match STHE.get() {
Some(&s) => s,
None => return 0.0,
};
if data.nxhhe == 0 {
return 0.0;
}
let prof = 0.0_f64;
// Check bounds
if xl > data.xlhhe[data.nxhhe - 1] {
return prof;
}
// Binary search for the interval
let mut jl = 0usize;
let mut ju = data.nxhhe;
while ju - jl > 1 {
let jm = (ju + jl) / 2;
if (data.xlhhe[data.nxhhe - 1] > data.xlhhe[0]) == (xl > data.xlhhe[jm]) {
jl = jm;
} else {
ju = jm;
}
}
let mut j = jl;
if j == 0 {
j = 1;
}
if j >= data.nxhhe {
j = data.nxhhe - 1;
}
// Linear interpolation
let denom = data.xlhhe[j] - data.xlhhe[j - 1];
if denom.abs() < 1.0e-30 {
return 0.0;
}
let a1 = (xl - data.xlhhe[j - 1]) / denom;
let s1 = (1.0 - a1) * data.sighhe[j - 1] + a1 * data.sighhe[j];
s1 * ahe / sthe * std::f64::consts::TAU
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_lyahhe_not_initialized() {
// Without initialization, should return 0.0
let result = lyahhe(1215.67, 1.0e20);
assert_eq!(result, 0.0);
}
#[test]
fn test_lyahhe_basic() {
// Initialize with synthetic data
let data = vec![
(1215.0, 1.0e-20),
(1215.5, 2.0e-20),
(1215.67, 5.0e-20),
(1216.0, 3.0e-20),
(1216.5, 1.0e-20),
];
lyahhe_init(1.0e21, 0, data);
// Test interpolation at known point
let result = lyahhe(1215.67, 1.0e20);
assert!(result > 0.0);
assert!(result.is_finite());
}
#[test]
fn test_lyahhe_outside_range() {
let data = vec![
(1215.0, 1.0e-20),
(1216.0, 3.0e-20),
];
lyahhe_init(1.0e21, 0, data);
// Wavelength outside range should return 0.0
let result = lyahhe(1220.0, 1.0e20);
assert_eq!(result, 0.0);
}
}
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//! Lyman line wings opacity.
//!
//! Translated from SYNSPEC `LYMLIN` subroutine (synspec54.f:5183).
//!
//! Calculates opacity of Lyman lines (alpha - delta) with
//! approximate partial redistribution.
/// Lyman line frequencies (Hz)
const FRLY: [f64; 4] = [
2.4660375e15, // Lyman alpha
2.9227111e15, // Lyman beta
3.0825469e15, // Lyman gamma
3.156528e15, // Lyman delta
];
/// BNLY coefficients
const BNLY: [f64; 4] = [5.527e-2, 4.090e-2, 2.699e-2, 1.855e-2];
/// Natural broadening coefficients
const SN: [f64; 4] = [1.308e5, 5.280e3, 5.847e2, 1.078e2];
/// Resonance broadening coefficients
const SR: [f64; 4] = [1.218e-16, 9.196e-17, 1.058e-16, 1.296e-16];
/// Stark broadening coefficients (SS)
const SS: [f64; 4] = [9.478e-3, 1.600e-2, 1.441e-2, 1.547e-2];
/// Stark broadening coefficients (GS)
const GS: [f64; 4] = [7.237e-8, 5.432e-6, 5.821e-5, 4.027e-4];
/// Damping constants
const GA: [f64; 4] = [1.000, 1.791, 2.362, 2.801];
/// Parameters for Lyman line wings calculation
pub struct LymlinParams {
/// Depth index
pub id: usize,
/// Frequency (Hz)
pub freq: f64,
/// H ground level population
pub pop_h: f64,
/// Excited level populations (index 0 = level 2, etc.)
pub pop_excited: [f64; 4],
/// Temperature (K)
pub t: f64,
/// Electron density
pub ane: f64,
/// Hydrogen atom exists
pub iath: i32,
/// Lyman line treatment switch
pub iophli: i32,
/// wnHint factors for each level
pub wn_hint: [f64; 5],
}
/// Result of Lyman line wings calculation
pub struct LymlinResult {
/// Absorption coefficient
pub ably: f64,
/// Emission coefficient
pub emly: f64,
/// Scattering coefficient
pub scly: f64,
}
/// Configuration for Lyman line treatment
struct LymlinConfig {
ifstrk: i32,
ifnat: i32,
ifres: i32,
ifprd: i32,
ifsti: i32,
}
use std::sync::OnceLock;
static LYMLIN_CONFIG: OnceLock<LymlinConfig> = OnceLock::new();
fn get_lymlin_config(iophli: i32) -> &'static LymlinConfig {
LYMLIN_CONFIG.get_or_init(|| {
let mut config = LymlinConfig {
ifstrk: 0,
ifnat: 1,
ifres: 1,
ifprd: 0,
ifsti: 0,
};
if iophli < 0 {
config.ifstrk = 1;
config.ifprd = 1;
}
config
})
}
/// Calculate Lyman line wings opacity.
///
/// Computes opacity contributions from Lyman alpha through delta lines
/// using approximate partial redistribution.
///
/// # Arguments
/// * `params` - Input parameters
///
/// # Returns
/// Absorption, emission, and scattering coefficients
pub fn lymlin(params: &LymlinParams) -> LymlinResult {
let mut ably = 0.0;
let mut emly = 0.0;
let mut scly = 0.0;
if params.iath <= 0 {
return LymlinResult { ably, emly, scly };
}
let config = get_lymlin_config(params.iophli);
if params.freq > 3.3e15 {
return LymlinResult { ably, emly, scly };
}
let p = params.pop_h;
let t = params.t;
let ane = params.ane;
for i in 0..4 {
let mut dfr = (FRLY[i] - params.freq).abs();
if dfr <= 5.0e11 {
dfr = 1.0e12;
}
let dfr2 = dfr * dfr;
let dfrs = dfr.sqrt();
let cor = (2.0 * params.freq / (params.freq + FRLY[i])).powi(2);
let mut f = 1.0;
if params.iophli.abs() == 2 {
f = feautr_lyman(params.freq, params.id, t, ane);
}
let mut stark = SS[i] * ane * f / dfr2 / dfrs;
if config.ifstrk == 0 {
stark = 0.0;
}
let mut sn_val = SN[i];
if config.ifnat == 0 {
sn_val = 0.0;
}
let mut sr_val = SR[i];
if config.ifres == 0 {
sr_val = 0.0;
}
let mut sgly = sn_val * (1.0 + sr_val * p) * cor / dfr2 + stark;
sgly *= params.wn_hint[i + 1];
let mut gama = 1.0 / (GA[i] + GS[i] * ane * f / dfrs);
if config.ifprd == 0 {
gama = 0.0;
}
ably += p * sgly;
emly += params.pop_excited[i] * sgly * BNLY[i] * (1.0 - gama);
if config.ifsti != 0 {
ably -= params.pop_excited[i] * sgly / ((i + 2) * (i + 2)) as f64;
}
scly += p * sgly * gama;
}
LymlinResult { ably, emly, scly }
}
/// Lyman-alpha Stark broadening after N. Feautrier.
///
/// Interpolates in tabulated Stark broadening profiles.
/// This is a simplified version used specifically in LYMLIN.
///
/// # Arguments
/// * `freq` - Frequency (Hz)
/// * `_id` - Depth index (unused in this implementation)
/// * `t` - Temperature (K)
/// * `ane` - Electron density
///
/// # Returns
/// Broadening factor
pub fn feautr_lyman(freq: f64, _id: usize, _t: f64, _ane: f64) -> f64 {
// Tabulated wavelength offsets (Å from line center)
const DL: [f64; 20] = [
-150.0, -120.0, -90.0, -60.0, -40.0, -20.0, -10.0, -8.0, -4.0, -2.0,
2.0, 4.0, 8.0, 10.0, 20.0, 40.0, 60.0, 90.0, 120.0, 150.0,
];
// Tabulated profiles at different electron densities
const F05: [f64; 20] = [
0.0537, 0.0964, 0.1330, 0.3105, 0.4585, 0.6772, 0.8229, 0.8556, 0.9250, 0.9618,
0.9733, 1.1076, 1.0644, 1.0525, 0.8841, 0.8282, 0.7541, 0.7091, 0.7164, 0.7672,
];
const F10: [f64; 20] = [
0.1986, 0.2764, 0.3959, 0.5740, 0.7385, 0.9448, 1.0292, 1.0317, 0.9947, 0.8679,
0.8648, 0.9815, 1.0660, 1.0793, 1.0699, 1.0357, 0.9245, 0.8603, 0.8195, 0.7928,
];
const F20: [f64; 20] = [
0.4843, 0.5821, 0.7003, 0.8411, 0.9405, 1.0300, 1.0029, 0.9753, 0.8478, 0.6851,
0.6861, 0.8554, 0.9916, 1.0264, 1.0592, 1.0817, 1.0575, 1.0152, 0.9761, 0.9451,
];
const F40: [f64; 20] = [
0.7862, 0.8566, 0.9290, 0.9915, 1.0066, 0.9878, 0.8983, 0.8513, 0.6881, 0.5277,
0.5302, 0.6920, 0.8607, 0.9111, 0.9651, 1.0793, 1.1108, 1.1156, 1.1003, 1.0839,
];
let dlam = 2.997925e18 / freq - 1215.685;
// Find interval
let mut i = 20;
for k in 1..20 {
if dlam <= DL[k] {
i = k;
break;
}
}
let j = i - 1;
let c = DL[j] - DL[i];
let a = (dlam - DL[i]) / c;
let b = (DL[j] - dlam) / c;
// Interpolate profiles
let mut x = [0.0; 4];
x[0] = F05[j] * a + F05[i] * b;
x[1] = F10[j] * a + F10[i] * b;
x[2] = F20[j] * a + F20[i] * b;
x[3] = F40[j] * a + F40[i] * b;
// Temperature interpolation (simplified - using average)
// In full implementation, would use JT, TI0, TI1, TI2 arrays
let y = (x[0] + x[1] + x[2] + x[3]) / 4.0;
0.5 * (y + 1.0)
}
#[cfg(test)]
mod tests {
use super::*;
#[test]
fn test_lymlin_basic() {
let params = LymlinParams {
id: 0,
freq: 2.466e15, // Near Lyman alpha
pop_h: 1.0e16,
pop_excited: [1.0e10, 1.0e9, 1.0e8, 1.0e7],
t: 6000.0,
ane: 1.0e13,
iath: 1,
iophli: 1,
wn_hint: [1.0, 1.0, 1.0, 1.0, 1.0],
};
let result = lymlin(&params);
assert!(result.ably.is_finite());
assert!(result.emly.is_finite());
assert!(result.scly.is_finite());
assert!(result.ably >= 0.0);
}
#[test]
fn test_lymlin_far_from_line() {
// Far from Lyman lines, opacity should be small
let params = LymlinParams {
id: 0,
freq: 1.0e15, // Far from Lyman alpha
pop_h: 1.0e16,
pop_excited: [1.0e10, 1.0e9, 1.0e8, 1.0e7],
t: 6000.0,
ane: 1.0e13,
iath: 1,
iophli: 1,
wn_hint: [1.0, 1.0, 1.0, 1.0, 1.0],
};
let result = lymlin(&params);
assert!(result.ably < 1e10); // Should be relatively small
}
#[test]
fn test_lymlin_no_hydrogen() {
// Without hydrogen, opacity should be zero
let params = LymlinParams {
id: 0,
freq: 2.466e15,
pop_h: 1.0e16,
pop_excited: [1.0e10, 1.0e9, 1.0e8, 1.0e7],
t: 6000.0,
ane: 1.0e13,
iath: 0, // No hydrogen
iophli: 1,
wn_hint: [1.0, 1.0, 1.0, 1.0, 1.0],
};
let result = lymlin(&params);
assert_eq!(result.ably, 0.0);
assert_eq!(result.emly, 0.0);
assert_eq!(result.scly, 0.0);
}
#[test]
fn test_feautr_lyman_basic() {
let result = feautr_lyman(2.466e15, 0, 6000.0, 1.0e13);
assert!(result.is_finite());
assert!(result > 0.0);
}
}
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//! 矩阵求逆(高斯-约旦消元法)。
//!
//! 重构自 SYNSPEC `matinv.f`
//!
//! 使用高斯-约旦消元法就地求逆矩阵。
/// 矩阵求逆(就地操作)。
///
/// 使用高斯-约旦消元法对 N×N 矩阵 A 求逆。
/// 矩阵以行优先存储,最大维度为 NR×NR,实际使用 N×N。
/// 求逆结果直接写回 A。
///
/// # 参数
///
/// * `a` - 输入矩阵(行优先存储),求逆后被替换为逆矩阵
/// * `n` - 矩阵实际维数
/// * `nr` - 矩阵最大维数(行优先存储的列数)
pub fn matinv(a: &mut [f64], n: usize, nr: usize) {
if n == 0 {
return;
}
// 1x1 矩阵的特殊情况
if n == 1 {
a[0] = 1.0 / a[0];
return;
}
// 创建增广矩阵 [A | I],使用 n×2n 的工作空间
let n2 = 2 * n;
let mut aug = vec![0.0; n * n2];
for i in 0..n {
for j in 0..n {
aug[i * n2 + j] = a[i * nr + j];
}
aug[i * n2 + n + i] = 1.0;
}
// 前向消元(带部分选主元)
for col in 0..n {
// 选主元
let mut max_val = aug[col * n2 + col].abs();
let mut max_row = col;
for row in (col + 1)..n {
let val = aug[row * n2 + col].abs();
if val > max_val {
max_val = val;
max_row = row;
}
}
// 交换行
if max_row != col {
for j in 0..n2 {
aug.swap(col * n2 + j, max_row * n2 + j);
}
}
// 缩放主行
let pivot = aug[col * n2 + col];
if pivot.abs() < 1e-30 {
return; // 奇异矩阵
}
for j in 0..n2 {
aug[col * n2 + j] /= pivot;
}
// 消元
for row in 0..n {
if row != col {
let factor = aug[row * n2 + col];
for j in 0..n2 {
aug[row * n2 + j] -= factor * aug[col * n2 + j];
}
}
}
}
// 提取逆矩阵
for i in 0..n {
for j in 0..n {
a[i * nr + j] = aug[i * n2 + n + j];
}
}
}
#[cfg(test)]
mod tests {
use super::*;
use approx::assert_relative_eq;
#[test]
fn test_matinv_1x1() {
let mut a = vec![4.0];
matinv(&mut a, 1, 1);
assert_relative_eq!(a[0], 0.25, epsilon = 1e-12);
}
#[test]
fn test_matinv_2x2() {
// [1 2]
// [3 4]
// det = 1*4 - 2*3 = -2
// 逆矩阵: [-2 1]
// [1.5 -0.5]
let mut a = vec![1.0, 2.0, 3.0, 4.0];
matinv(&mut a, 2, 2);
assert_relative_eq!(a[0], -2.0, epsilon = 1e-10);
assert_relative_eq!(a[1], 1.0, epsilon = 1e-10);
assert_relative_eq!(a[2], 1.5, epsilon = 1e-10);
assert_relative_eq!(a[3], -0.5, epsilon = 1e-10);
}
#[test]
fn test_matinv_identity() {
// 单位矩阵的逆是自身
let mut a = vec![1.0, 0.0, 0.0, 0.0, 1.0, 0.0, 0.0, 0.0, 1.0];
matinv(&mut a, 3, 3);
assert_relative_eq!(a[0], 1.0, epsilon = 1e-12);
assert_relative_eq!(a[4], 1.0, epsilon = 1e-12);
assert_relative_eq!(a[8], 1.0, epsilon = 1e-12);
assert_relative_eq!(a[1], 0.0, epsilon = 1e-12);
assert_relative_eq!(a[2], 0.0, epsilon = 1e-12);
}
#[test]
fn test_matinv_roundtrip() {
// A * A^{-1} 应该接近单位矩阵
let orig = vec![2.0, 1.0, 0.0, 1.0, 3.0, 1.0, 0.0, 1.0, 2.0];
let mut a = orig.clone();
matinv(&mut a, 3, 3);
// 计算 orig * a(应该接近单位矩阵)
let mut product = vec![0.0; 9];
for i in 0..3 {
for j in 0..3 {
for k in 0..3 {
product[i * 3 + j] += orig[i * 3 + k] * a[k * 3 + j];
}
}
}
// 检查对角线接近 1
assert_relative_eq!(product[0], 1.0, epsilon = 1e-10);
assert_relative_eq!(product[4], 1.0, epsilon = 1e-10);
assert_relative_eq!(product[8], 1.0, epsilon = 1e-10);
// 检查非对角线接近 0
assert_relative_eq!(product[1], 0.0, epsilon = 1e-10);
assert_relative_eq!(product[2], 0.0, epsilon = 1e-10);
}
}

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