the historical code used recombination emissivitities from some papers, and build collisional - radiative models on its own. The stout database now has no way to include these stand-along recombination intensities.
examples are in prt_lines_lv1_li_ne.cpp. two things need to be done.
the fitted emissivites are for very low densities - there must be a correction for collisional suppression.
the emission must be added to the stout model.
very important for, example, C III 977 (Lya for that species)
{
"status": "new",
"changetime": "2019-02-04T13:14:42Z",
"_ts": "1549286082026814",
"description": "the historical code used recombination emissivitities from some papers, and build collisional - radiative models on its own. The stout database now has no way to include these stand-along recombination intensities. \n\nexamples are in prt_lines_lv1_li_ne.cpp. two things need to be done.\n\nthe fitted emissivites are for very low densities - there must be a correction for collisional suppression.\n\nthe emission must be added to the stout model.\n\nvery important for, example, C III 977 (Lya for that species)",
"reporter": "gary",
"cc": "",
"resolution": "",
"time": "2013-11-03T23:03:51Z",
"component": "atomic/molecular data base",
"summary": "recombination add on components in stout data",
"priority": "blocker",
"keywords": "",
"version": "stout",
"milestone": "c19 branch",
"owner": "nobody",
"type": "defect - wrong answer"
}
reported by: @CloudyLex
the historical code used recombination emissivitities from some papers, and build collisional - radiative models on its own. The stout database now has no way to include these stand-along recombination intensities.
examples are in prt_lines_lv1_li_ne.cpp. two things need to be done.
the fitted emissivites are for very low densities - there must be a correction for collisional suppression.
the emission must be added to the stout model.
very important for, example, C III 977 (Lya for that species)
Migrated from https://www.nublado.org/ticket/270