Cowan Code and Stark Broadening of Spectral Lines of S II, S III and S IV

Details Cowan Code and Stark Broadening of Spectral Lines of S II, S III and S IV Cowan Code and Stark Broadening of Spectral Lines of S II, S III and S IV

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..938..258m&link_type=abstract

SPECTRAL LINE SHAPES IN ASTROPHYSICS: VI Serbian Conference on Spectral Line Shapes in Astrophysics (VI SCSLSA). AIP Conference

Astronomy and Astrophysics

Astrophysics

2

Atomic And Molecular Data, Spectra, And Spectral Parameters, Ab Initio Calculations, Zeeman And Stark Effects, Atomic Spectra

Scientific paper

We present Stark broadening parameters (widths) of 5 multiplets of S II, 3 multiplets of S III and 2 spectral lines of S IV calculated using modified semi-empirical approach (MSE). Needed atomic data (energy levels) have been calculated ab initio using Cowan code. Comparison of energy levels of S II, S III and S IV calculated by Cowan code and energy levels taken from NIST atomic spectra database is given.

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