Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..559...85s&link_type=abstract
SPECTRAL LINE SHAPES: Volume 11, 15th ICSLS. AIP Conference Proceedings, Volume 559, pp. 85-87 (2001).
Astronomy and Astrophysics
Astrophysics
Plasma Sources, Dielectric Properties, Thermodynamics Of Plasmas
Scientific paper
The Stark broadened profiles of the Lyman, Balmer and Paschen lines of neutral hydrogen have been calculated from the line center to the line wings. The Model Microfield method has been used for both the electron and ion contributions. The no quenching and the dipolar approximations have been used. The plasma is assumed to be composed of electrons and protons. The available data, accessible at the Center de Données de Strasbourg (CDS) together with an interpolating routine, allow each series to be calculated up to the Inglis-Teller limit, for a wide range of density and temperature covering almost all conditions in astrophysical plasmas. .
Hutcheon Richard
Stehlé Chantal
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