The computation of radiation transport using Feautrier variables. II - Spectrum line formation in moving media

Details The computation of radiation transport using Feautrier variables. II - Spectrum line formation in moving media The computation of radiation transport using Feautrier variables. II - Spectrum line formation in moving media

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jcoph..64....1m&link_type=abstract

Journal of Computational Physics (ISSN 0021-9991), vol. 64, May 1986, p. 1-26.

Astronomy and Astrophysics

Astrophysics

6

Astronomical Spectroscopy, Astrophysics, Line Spectra, Radiative Transfer, Algorithms, Atomic Spectra, Integral Equations, Particle Motion, Spheres

Scientific paper

The Feautrier symmetric/antisymmetric radiation field averages are presently applied to the solution of line transport problems in moving media. These methods, which have proven to be useful in a variety of astrophysical applications, are suggested to be applicable to other areas of computational physics. Attention is given to algorithms for both observer-frame and comoving-frame approaches, noting their respective advantages and shortcomings.

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