On spectral line Stark broadening parameters needed for stellar and laboratory plasma investigations.

Details On spectral line Stark broadening parameters needed for stellar and laboratory plasma investigations. On spectral line Stark broadening parameters needed for stellar and laboratory plasma investigations.

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pobeo..48..127d&link_type=abstract

Publications de l'Observatoire Astronomique de Beograd, No. 48, p. 127 - 138

Astronomy and Astrophysics

Astrophysics

Line Broadening: Stark Effect

Scientific paper

This paper presents a review of semiclassical calculations of Stark broadening parameters and a comparison of different semiclassical procedures is discussed, as well as the agreement with critically selected experimental data and more sophisticated, close coupling calculations. Approximate methods for the calculation of Stark broadening parameters, useful especially in such astrophysical problems where large scale calculations and analyses must be performed and where a good average accuracy is expected, have also been discussed. The beginning and development of line shapes investigations in Yugoslavia has been described as well.

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