Hydrogen atom kinetics in solar and late star atmospheres

Details Hydrogen atom kinetics in solar and late star atmospheres Hydrogen atom kinetics in solar and late star atmospheres

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70.1054b&link_type=abstract

Astronomicheskij Zhurnal, vol. 70, p. 1054

Astronomy and Astrophysics

Astronomy

1

Solar Atmosphere, Late Stars, Stellar Atmospheres, Hydrogen Atoms, H Lines, Radiative Transfer, Electron Density Profiles, Chromosphere

Scientific paper

Sobolev's method for moving media is extended to the case of an optically thick stationary medium. The probabilities of photon escape from a medium are calculated with allowance for the multiplicity of photon scattering and assuming an absorption coefficient that is due to the combined Stark and Doppler effects. Results of calculations for conditions typical of the chromosphere and low-temperature condensation, formed during flares, are discussed as an example. These results can be used for the quantitative interpretation of Balmer line decrements in solar and late star atmospheres.

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