Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jphb...17.1477s&link_type=abstract
Journal of Physics B - Atomic and Molecular Physics (ISSN 0022-3700), vol. 17, April 28, 1984, p. 1477-1489.
Astronomy and Astrophysics
Astrophysics
18
H Alpha Line, Spectral Line Width, Stark Effect, Astrophysics, Low Density Research, Molecular Relaxation, Perturbation Theory, Quantum Electronics
Scientific paper
Stark profiles of the H-alpha lines of hydrogen are computed at densities from (1 to 1000) x 10 to the 10th/cu cm in the 'impact' theory. By a comparison with quantal results it is shown that a simple semiclassical perturbational approach with appropriate cutoffs is sufficient to give accurate profiles in the line center. Neglecting the natural broadening and the fine-structure effects, it is proved that the electronic broadening is negligible and that the profile has a Lorentzian shape; and an analytical expression of the half width is obtained.
Feautrier N.
Stehlé Chantal
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