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The hydrogen atom kinetics in flare star chromospheres

Published online by Cambridge University Press:  23 September 2016

E. A. Bruevich  and
M.A. Livshits
E. A. Bruevich
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation USSR Academy of Sciences, Troitsk, Moscow Region, 142092, USSR
M.A. Livshits
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation USSR Academy of Sciences, Troitsk, Moscow Region, 142092, USSR

Abstract

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The solution of steady-state equations for hydrogen is carried out. The diffuse radiation field was taken into account in these equations the value βs≡NRB - the escape probability of photons from the medium. This value is calculated for a layer of motionless plasma with finite optical depth. Our results are compared with analogical ones using Sobolev's method.

Type
IV Theoretical Problems and Interpretation of Observations
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 317 - 319
Copyright
Copyright © Kluwer 1990 

References

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