SpectraRust/tlusty/extracted/rtecf1.f
2026-03-19 14:05:33 +08:00

452 lines
12 KiB
Fortran

SUBROUTINE RTECF1(IJ)
C =====================
C
C Solution of the radiative transfer equation with Compton scattering
C for one frequency (assuming the radiation intensity in i
C other frequencies is given
C solution is done for individual angles, and new Eddington factors
C are determined
C
INCLUDE 'IMPLIC.FOR'
INCLUDE 'BASICS.FOR'
INCLUDE 'MODELQ.FOR'
INCLUDE 'ALIPAR.FOR'
INCLUDE 'ITERAT.FOR'
PARAMETER (SIXTH=UN/6.D0,
* THIRD=UN/3.D0,
* TWOTHR=TWO/3.D0)
COMMON/OPTDPT/DT(MDEPTH)
COMMON/SURFEX/EXTJ(MFREQ),EXTH(MFREQ)
COMMON/EXTINT/WANGLE,EXTIN(MFREQ)
COMMON/AUXRTE/
* COMA(MDEPTH),COMB(MDEPTH),COMC(MDEPTH),VL(MDEPTH),
* COME(MDEPTH),U(MDEPTH),V(MDEPTH),BS(MDEPTH),
* AL(MDEPTH),BE(MDEPTH),GA(MDEPTH)
common/comgfs/gfm(mfreq,mdeptc),gfp(mfreq,mdeptc)
DIMENSION RI(MDEPTH),RDH(MDEPTH),RDK(MDEPTH),RDN(MDEPTH),
* DTAU(MDEPTH),ST0(MDEPTH),RDWN(MMUC),
* ali(mdepth)
DIMENSION AANU(MDEPTH),DDD(MDEPTH),FKK(MDEPTH),ali0(mdepth),
* SS0(MDEPTH),
* AAA(MDEPTH),BBB(MDEPTH),CCC(MDEPTH),EEE(MDEPTH),
* ZZZ(MDEPTH),ALRH(MDEPTH),ALRM(MDEPTH),ALRP(MDEPTH),
* ss0c(mdepth)
C
IF(IJ.EQ.1) THEN
if(icompt.gt.0.and.icombc.gt.0) then
IJE=IJEX(IJ)
DO ID=1,ND
rad1(id)=rad(nfreq,id)
fak1(id)=0.333333
ali1(id)=0.
if(ije.gt.0) then
RADEX(IJE,ID)=rad1(id)
FAKEX(IJE,ID)=fak1(id)
END IF
END DO
return
end if
END IF
C
WW=W(IJ)
IJI=NFREQ-KIJ(IJ)+1
FR=FREQ(IJ)
CALL RTECF0(IJ)
c
do id=1,nd
rad1(id)=0.
ali1(id)=0.
rdh(id)=0.
rdk(id)=0.
rdn(id)=0.
st0(id)=vl(id)+(comb(id)+bs(id))*rad(iji,id)
ss0(id)=0.
end do
rdh1=0.
rdhd=0.
c
if(iji.gt.1) then
do id=1,nd
st0(id)=st0(id)+coma(id)*rad(iji-1,id)
end do
end if
if(iji.lt.nfreq) then
do id=1,nd
st0(id)=st0(id)+comc(id)*rad(iji+1,id)
end do
end if
c
if(idisk.eq.0.or.ifz0.lt.0) then
FR15=FR*1.D-15
BNU=BN*FR15*FR15*FR15
PLAND=BNU/(EXP(HK*FR/TEMP(ND))-UN)*RRDIL
DPLAN=BNU/(EXP(HK*FR/TEMP(ND-1))-UN)*RRDIL
IF(TEMPBD.GT.0.) THEN
PLAND=BNU/(EXP(HK*FR/TEMPBD)-UN)*RRDIL
DPLAN=BNU/(EXP(HK*FR/TEMPBD)-UN)*RRDIL
ENDIF
DPLAN=(PLAND-DPLAN)/DT(ND-1)
end if
c
if(icomrt.eq.0) then
c
c ========================================================
c Formal angle-dependent solution done by Feautrier scheme
c ========================================================
c
c loop over angles points
c
do i=1,nmu
do id=1,nd-1
dtau(id)=dt(id)/amu(i)
end do
c
c boundary conditions
c
rup=0.
rdown=0.
rup=extint(ij,i)
if(idisk.eq.0.or.ifz0.lt.0) rdown=pland+amu(i)*dplan
c
c solution of the transfer equation
c
call rtefe2(dtau,st0,rup,rdown,ri)
ttau=0.
do id=1,nd
riid=wtmu(i)*ri(id)
rad1(id)=rad1(id)+riid
rdk(id)=rdk(id)+amu(i)*amu(i)*riid
end do
rdh1=rdh1+amu(i)*wtmu(i)*ri(1)
rdhd=rdhd+amu(i)*wtmu(i)*ri(nd)
end do
rdh1=rdh1-half*hextrd(ij)
c
c ----------------------
c end of the loop over angle points
c
c ===========================================
c Formal angle-dependent solution done by DFE
c ===========================================
c
else
c
c loop over angle points
c ----------------------
c
do i=1,nmuc
do id=1,nd-1
dtau(id)=dt(id)/abs(amuc(i))
end do
c
c boundary conditions
c
rup=0.
rdown=0.
if(amuc(i).lt.0.) rup=extint(ij,i)
C
C diffusion approximation for semi-infinite atmospheres
C
if(idisk.eq.0.or.ifz0.lt.0) rdown=pland+amuc(i)*dplan
c
c the case of finite slab - irradiation of the back side
c
if(amuc(i).gt.0.) rdown=rdwn(nmuc-i+1)
c
c solution of the transfer equation
c
call rtesol(dtau,st0,rup,rdown,amuc(i),ri,ali)
ttau=0.
do id=1,nd
riid=ri(id)*half
rad1(id)=rad1(id)+wtmuc(i)*riid
ali1(id)=ali1(id)+wtmuc(i)*ali(id)
rdh(id)=rdh(id)+amuc1(i)*riid
rdk(id)=rdk(id)+amuc2(i)*riid
rdn(id)=rdn(id)+amuc3(i)*riid
end do
rdwn(i)=ri(nd)
if(amuc(i).gt.0.) rdh1=rdh1+amuc1(i)*ri(1)*half
rdhd=rdhd+abs(amuc1(i))*ri(nd)*half
end do
c
c ----------------------
c end of the loop over angle points
c
end if
c
do id=1,nd
fak1(id)=fak(ij,id)
radk(ij,id)=rdk(id)
if(icomve .gt. 0) then
fkk(id)=rdk(id)/rad1(id)
else
fkk(id)=fak(ij,id)
endif
ss0(id)=0.
end do
if(icomve.gt.0) then
do id=1,nd
fak(ij,id)=rdk(id)/rad1(id)
fak1(id)=fak(ij,id)
fkk(id)=fak(ij,id)
end do
end if
if(rad1(1).gt.0.) then
flux(ij)=rdh1
fhd(ij)=rdhd/rad1(nd)
end if
c
ah=rdh1
if(iwinbl.lt.0) ah=ah+half*hextrd(ij)
aj=rad1(1)
fh(ij)=ah/aj
C
C ********************
C
C Again solution of the transfer equation, now with Eddington
C FKK and FH determined above, to insure strict consistency of the
C radiation field and Eddington factors
C
C Upper boundary condition
C
U0=0.
QQ0=0.
US0=0.
TAUMIN=ABSO1(1)*DEDM1
NMU=3
DO I=1,NMU
IF(IWINBL.EQ.0.AND.WANGLE.EQ.0.) THEN
C
C allowance for non-zero optical depth at the first depth point
C
TAMM=TAUMIN/AMU(I)
EX=EXP(-TAMM)
P0=UN-EX
QQ0=QQ0+P0*AMU(I)*WTMU(I)
U0=U0+EX*WTMU(I)
if(tamm.gt.0.) US0=US0+P0/TAMM*WTMU(I)
END IF
END DO
ID=1
DTP1=DT(ID)
IF(MOD(ISPLIN,3).EQ.0) THEN
B=DTP1*HALF
C=0.
ELSE
B=DTP1*THIRD
C=B*HALF
END IF
BQ=UN/(B+QQ0)
CQ=C*BQ
BBB(ID)=(FKK(ID)/DTP1+FH(IJ)+B)*BQ+SS0(ID)
CCC(ID)=(FKK(ID+1)/DTP1)*BQ-CQ*(UN+SS0(ID+1))
ZZZ(ID)=UN/BBB(ID)
VLL=ST0(ID)+CQ*ST0(ID+1)
c IF(IWINBL.LT.0) VLL=VLL+TWO*HEXTRD(IJ)/DTP1
AANU(ID)=VLL*ZZZ(ID)
DDD(ID)=CCC(ID)*ZZZ(ID)
IF(ISPLIN.GT.2) FFF=BBB(ID)/CCC(ID)-UN
C
C Normal depth point
C
DO ID=2,ND-1
DTM1=DTP1
DTP1=DT(ID)
DT0=TWO/(DTP1+DTM1)
ALP=UN/DTM1*DT0
GAM=UN/DTP1*DT0
IF(MOD(ISPLIN,3).EQ.0) THEN
A=0.
C=0.
ELSE IF(ISPLIN.EQ.1) THEN
A=DTM1*DT0*SIXTH
C=DTP1*DT0*SIXTH
ELSE
A=(UN-HALF*DTP1*DTP1*ALP)*SIXTH
C=(UN-HALF*DTM1*DTM1*GAM)*SIXTH
END IF
AAA(ID)=ALP*FKK(ID-1)-A*(UN+SS0(ID-1))
CCC(ID)=GAM*FKK(ID+1)-C*(UN+SS0(ID+1))
BBB(ID)=(ALP+GAM)*FKK(ID)+(UN-A-C)*(UN+SS0(ID))
VLL=A*ST0(ID-1)+C*ST0(ID+1)+(UN-A-C)*ST0(ID)
AANU(ID)=VLL+AAA(ID)*AANU(ID-1)
IF(ISPLIN.LE.2) THEN
ZZZ(ID)=UN/(BBB(ID)-AAA(ID)*DDD(ID-1))
DDD(ID)=CCC(ID)*ZZZ(ID)
AANU(ID)=AANU(ID)*ZZZ(ID)
ELSE
SUM=-AAA(ID)+BBB(ID)-CCC(ID)
FFF=(SUM+AAA(ID)*FFF*DDD(ID-1))/CCC(ID)
DDD(ID)=UN/(UN+FFF)
AANU(ID)=AANU(ID)*DDD(ID)/CCC(ID)
ENDIF
END DO
C
C Lower boundary condition
C
ID=ND
c
c stellar atmospheric
c
IF(IDISK.EQ.0.OR.IFZ0.LT.0) then
IF(IBC.EQ.0) THEN
BBB(ID)=FKK(ID)/DTP1+HALF
AAA(ID)=FKK(ID-1)/DTP1
VLL=HALF*PLAND+THIRD*DPLAN
ELSE IF(IBC.LT.4) THEN
B=UN/DTP1
A=TWO*B*B
BBB(ID)=UN+SS0(ID)+B*TWO*FHD(IJ)+A*FKK(ID)
AAA(ID)=A*FKK(ID-1)
VLL=ST0(ID)+B*(PLAND+TWOTHR*DPLAN)
ELSE
B=UN/DTP1
A=TWO*B*B
BBB(ID)=B+A*FKK(ID)
AAA(ID)=A*FKK(ID-1)
VLL=B*(PLAND+TWOTHR*DPLAN)
END IF
c
c accretion disk - symmetric boundary
c
ELSE
B=TWO/DTP1
BBB(ID)=FKK(ID)/DTP1*B+UN+SS0(ND)
AAA(ID)=FKK(ID-1)/DTP1*B
VLL=ST0(ID)
END IF
C
EEE(ND)=AAA(ID)/BBB(ID)
ZZZ(ID)=UN/(BBB(ID)-AAA(ID)*DDD(ID-1))
RAD1(ID)=(VLL+AAA(ID)*AANU(ID-1))*ZZZ(ID)
FAK1(ID)=FKK(ND)
ALRH(ID)=ZZZ(ID)
frd=bbb(nd)*rad1(nd)-aaa(nd)*rad1(nd-1)
frd1=(bbb(nd)-un)*rad1(nd)-aaa(nd)*rad1(nd-1)
C
C Backsolution
C
DO ID=ND-1,1,-1
EEE(ID)=AAA(ID)/(BBB(ID)-CCC(ID)*EEE(ID+1))
RAD1(ID)=AANU(ID)+DDD(ID)*RAD1(ID+1)
FAK1(ID)=FKK(ID)
C write(42,642),ij,id,rad1(id),st0(id),fak1(id)
ALRH(ID)=ZZZ(ID)/(UN-DDD(ID)*EEE(ID+1))
ALRM(ID)=0
ALRP(ID)=0
END DO
c
C evaluate approximate Lambda operator
C
C a) Rybicki-Hummer Lambda^star operator (diagonal)
C (for JALI = 1)
C
DO ID=1,ND
ALIM1(ID)=0.
ALIP1(ID)=0.
END DO
IF(JALI.EQ.1) THEN
DO ID=1,ND
ALI1(ID)=ALRH(ID)
END DO
c
IF(IBC.EQ.0) THEN
ali1(nd-1)=rad1(nd-1)/st0(nd-1)
ali1(nd)=rad1(nd)/st0(nd)
END IF
C
C for IFALI>5:
C tridiagonal Rybicki-Hummer operator (off-diagonal terms)
C
IF(IFALI.GE.6) THEN
ALIP1(1)=ALRH(2)*DDD(1)
DO ID=2,ND-1
ALIM1(ID)=ALRH(ID-1)*EEE(ID)
ALIP1(ID)=ALRH(ID+1)*DDD(ID)
END DO
ALIM1(ND)=ALRH(ND-1)*EEE(ND)
IF(IBC.EQ.0) THEN
ALIM1(nd)=0.
ALIM1(nd-1)=0.
ALIP1(nd)=0.
ALIP1(nd-1)=0.
END IF
END IF
c
C b) diagonal Olson-Kunasz Lambda^star operator,
C (for JALI = 2)
C
ELSE IF(JALI.EQ.2) THEN
DO ID=1,ND-1
ALI0(ID)=0.
DO I=1,NMU
DIV=DT(ID)/AMU(I)
ALI0(ID)=ALI0(ID)+(UN-EXP(-DIV))/DIV*WTMU(I)
END DO
END DO
DO ID=2,ND-1
ALI1(ID)=UN-HALF*(ALI0(ID)+ALI0(ID-1))
END DO
ALI1(1)=UN-HALF*(ALI0(1)+US0)
ALI1(ND)=UN-ALI0(ND-1)
ali1(nd-1)=rad1(nd-1)/st0(nd-1)
ali1(nd)=rad1(nd)/st0(nd)
END IF
C
C correction of Lambda^star for scattering
C
IF(ILMCOR.EQ.1) THEN
DO ID=1,ND
ALI1(ID)=ALI1(ID)*(UN+SS0(ID))
ALIM1(ID)=ALIM1(ID)*(UN+SS0(ID))
ALIP1(ID)=ALIP1(ID)*(UN+SS0(ID))
END DO
ELSE IF(ILMCOR.EQ.3) THEN
DO ID=1,ND
ALI1(ID)=ALI1(ID)/(UN+SS0C(ID)*ALI1(ID))
ALIM1(ID)=ALIM1(ID)/(UN+SS0C(ID)*ALIM1(ID))
ALIP1(ID)=ALIP1(ID)/(UN+SS0C(ID)*ALIP1(ID))
END DO
END IF
C
DO ID=1,ND
radcm(iji,id)=rad1(id)
END DO
C
C radiation pressure
C
if(.not.lskip(1,IJ))
* PRD0=PRD0+ABSO1(1)*WW*(RAD1(1)*FH(IJ)-HEXTRD(IJ))
DO ID=1,ND
if(.not.lskip(ID,IJ))
* PRADT(ID)=PRADT(ID)+RAD1(ID)*FAK1(ID)*WW
PRADA(ID)=PRADA(ID)+RAD1(ID)*FAK1(ID)*WW
END DO
c
if(chmax.ge.1.91e-3.and.chmax.le.2.03e-3) then
tauij=taumin
do id=1,nd
if(id.gt.1) tauij=tauij+dt(id-1)
write(97,697) ij,id,tauij,rad1(id),st0(id)/(un+ss0(id)),
* st0(id),un+ss0(id),ali1(id)
end do
697 format(2i4,1p6e12.4)
end if
c
do id=1,nd
fak(ij,id)=fak1(id)
end do
C
C store quantities for explicit (linearized) frequencies
C
IF(IJEX(IJ).LE.0) RETURN
IJE=IJEX(IJ)
DO ID=1,ND
RADEX(IJE,ID)=RAD1(ID)
FAKEX(IJE,ID)=FAK1(ID)
END DO
c
RETURN
END