standard80_sn_kurucz

#This is the standard set of data files created for python81c - collision stength included
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# This first file sets up the basics - abundances and numbers of levels allowed
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data/atomic_extra/elem_ions_ver_80_sn.dat
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# These are the level files used in standard79 - they tend to have very few levels for each state
# partiularly for the upper levels - they are used to compute PI and recomb rates
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data/atomic/topbase_levels_h.dat
data/atomic/topbase_levels_he.dat
data/atomic/topbase_levels_cno.dat
data/atomic/topbase_levels_fe.dat
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# This a new level file - all ions have ten levels - the new levels will add to those in the files above
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data/atomic/topbase_all_levels_10_lev.dat
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# The next file is the levels used to compute line emission
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data/atomic_extra/levels_kur.dat
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# And the next is for the actual lines
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data/atomic_extra/lines_linked_kur.dat
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# And this next is for the collision strength data
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data/atomic/ver_upsilon_linked.dat
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data/atomic/excited.dat
data/atomic/recomb.dat
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# The next set of topbase PI cross sections are those used in atomic79
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data/atomic/topbase_h1_phot_extrap.dat
data/atomic/topbase_he1_phot_extrap.dat
data/atomic/topbase_he2_phot_extrap.dat
data/atomic/topbase_cno_phot_extrap.dat
data/atomic/topbase_fe_phot_extrap.dat
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#Next is VFKY PI cross sections, supplemented with VY data out to 50kev.
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data/atomic/vfky_outershell_tab.dat
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#Next is VY inner shell photoionization cross sections
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data/atomic/vy_innershell_tab.dat
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#Now we have electron yield data from Kaastra and Mewe, matching the inner shells
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data/atomic/kaastra_electron_yield.dat
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#Next is dielectronic recombination data from chianti.
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data/atomic/chianti_dr.dat
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#Next is total radiative recombinaion rate from chianti
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data/atomic/chianti_rr.dat
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#Next is badnell style ground state radiative recombinaion rate
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data/atomic/Badnell_GS_RR.dat
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#Next is gaunt factor data from sutherland (1997)
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data/atomic/gffint.dat
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#Next is direct ionization from dere
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data/atomic/di_dere.dat
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