Half-range moment methods for radiative transfer in spherical geometry. V - Line formation in a static atmosphere

Details Half-range moment methods for radiative transfer in spherical geometry. V - Line formation in a static atmosphere Half-range moment methods for radiative transfer in spherical geometry. V - Line formation in a static atmosphere

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...286..659r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 15, 1984, p. 659-665. Research supported by the Smithsonian Astro

Statistics

Computation

4

Computational Astrophysics, Line Spectra, Method Of Moments, Radiative Transfer, Stellar Atmospheres, Gas Expansion, Integral Equations, Optical Thickness

Scientific paper

The author describes a fast, accurate numerical technique for solving
the problem of line formation in a static spherical atmosphere. Two
numerical examples provide a comparison of this method with two other
independent calculations. The method of solution can accommodate the
effects of atmospheric expansion and frequency redistribution.

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