Solution of non-coherent spectral line transfer problem for finite atmosphere by the Fn-method

Details Solution of non-coherent spectral line transfer problem for finite atmosphere by the Fn-method Solution of non-coherent spectral line transfer problem for finite atmosphere by the Fn-method

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146..311r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 2, July 1988, p. 311-319.

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Computation

Computational Astrophysics, Stellar Atmospheres, Stellar Interiors, Transfer Functions, Absorptivity, Integral Equations, Light Scattering, Optical Thickness

Scientific paper

A semianalytic solution of the transfer equation for the line transfer problem involving no absorption in the continuum has been obtained. Application of the orthogonality and normalization integrals of McCormick and Siewert (1970) has made possible the derivation of a set of singular integral equations for the noncoherent spectral line formation problem in finite media. Fn equations for exit distributions are employed to obtain algebraic equations with suitable recursion relations.

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