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Exact solution of the standard transfer problem in a stellar atmosphere

L. Chevallier·B. Rutily
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Abstract

We come back to the analytical solution of the standard transfer problem in a stellar atmosphere. It consists in solving the radiative transfer equation in a homogeneous and isothermal plane-parallel atmosphere, with light scattering taken as isotropic and monochromatic. The literature on the subject is reviewed and the existing solution in a finite slab is improved thanks to the introduction of non classical auxiliary functions. Eleven-figure tables of the solution are given for typical values of the input parameters currently met in stellar atmospheres.

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L. Chevallier, B. Rutily. 2005-04-03. Exact solution of the standard transfer problem in a stellar atmosphere. https://doi.org/10.1016/j.jqsrt.2004.05.065

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