Hydrogen stark profiles for astrophysics

Details Hydrogen stark profiles for astrophysics Hydrogen stark profiles for astrophysics

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..216..607s&link_type=abstract

Spectral line shapes. AIP Conference Proceedings, Volume 216, pp. 607-608 (1990).

Physics

1

Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Zeeman And Stark Effects

Scientific paper

A large number of hydrogen line profiles are calculated in the framework
of the model microfield method with specific modification for electronic
contributions. Profiles of the Lyman, Balmer and Paschen series have
been obtained from the center to the Holtsmark wings of the lines. (AIP)

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