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The hydrogen atom kinetics in flare star chromospheres
Published online by Cambridge University Press: 23 September 2016
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
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- Copyright
- Copyright © Kluwer 1990
References
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