42 lines
1.6 KiB
Plaintext
42 lines
1.6 KiB
Plaintext
The directory contains input data for two test cases.
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The first one is computing a spectrum for a
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Kurucz model, Teff=9750 K, log g = 4, for a short wavelength
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range between 1400 and 1410 A.
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In order to be able to use the script file RSynspec, one needs to
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copy the original Kurucz model file (ap00t9750g40k2.dat), and the
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standard input file (tab.5) to the name with a common core name,
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in this case kurucz9750g40, as it is done in the script file R1.
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The spectrum is computed with atomic lines only.
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Without using the script R1, the same model can be run as:
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ln -s -f $TLUSTY/data data
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ln -s -f data/linelist.test fort.19
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cp ap00t9750g40k2.dat fort.8
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$TLUSTY/synspec/synspec.exe < tab.5 > kurucz9750g40.log
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cp fort.7 kurucz9750g40.spec
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cp fort.17 kurucz9750g40.cont
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cp fort.12 kurucz9750g40.eqws
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One can similarly run a spectrum for a pure continuum (plus
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hydrogen lines), as first copying fort.55.con to fort.55
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cp fort.55.con fort.55
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$TLUSTY/synspec/synspec.exe < tab.5 > tmp.log
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This is mentioned just for completeness, but is not
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a part of the test case.
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The second test is computing a spectrum between 2500 and 7500 A
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for a solar-type star, Teff=5500 K, log g = 4.5, taking into
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account three line lists, all in the binary format: gfATO.bin (atomic),
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gfMOL.bin (diatomic molecules), and gfTiO.bin (TiO).
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The model core name is kur55g45.
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The standard input file, tab.5, is almost identical to cool.5 used
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iun the previous test, but contains the keyword parameter file
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(tab.nst) that sets generating four output files with interesting
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parameters pertaining to the equation of state, fort.51 - 54.
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These files are explained in detail in Paper IV (manual), Sec.3.3.
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