Perturbation solutions of the equation of radiative transfer in a stellar atmosphere

Details Perturbation solutions of the equation of radiative transfer in a stellar atmosphere Perturbation solutions of the equation of radiative transfer in a stellar atmosphere

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56..401c&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 3, Apr. 1977, p. 401-405. Research supported by the Deutsche Forschungsgemeinschaft an

Astronomy and Astrophysics

Astrophysics

1

Nonequilibrium Plasmas, Perturbation Theory, Radiative Transfer, Stellar Atmospheres, Convergence, Magnetohydrodynamic Flow, Nonuniform Plasmas, Run Time (Computers), Series Expansion

Scientific paper

Of prime importance in the study of gasdynamic phenomena in stellar atmospheres is the ability to solve the radiative transfer equation in a nonequilibrium inhomogeneous moving plasma. This paper describes a flexible and efficient method for solving this type of problem. The method is based on a perturbation-series solution of the transfer equation. The terms in the perturbation series are obtained by repeated solution of a very simple transfer equation; the final solution may be as accurate as the application requires.

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