Exact solution of the standard transfer problem in a stellar atmosphere

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dc.creatorChevallier, L.
dc.creatorRutily, B.
dc.date2005-04-03
dc.date.accessioned2026-07-07T02:17:22Z
dc.date.available2026-07-07T02:17:22Z
dc.descriptionWe 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.
dc.description23 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0504049
dc.identifierhttp://arxiv.org/abs/astro-ph/0504049
dc.identifierJ.Quant.Spectrosc.Radiat.Trans. 91 (2005) 373-391
dc.identifierdoi:10.1016/j.jqsrt.2004.05.065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9147
dc.subjectAstrophysics
dc.titleExact solution of the standard transfer problem in a stellar atmosphere
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