Resonance line formation in arbitrary moving envelopes

Details Resonance line formation in arbitrary moving envelopes Resonance line formation in arbitrary moving envelopes

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233..486b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 2, July 1990, p. 486-496.

Statistics

Computation

7

Computational Astrophysics, Nonequilibrium Thermodynamics, Operators (Mathematics), Radiative Transfer, Resonance Lines, Stellar Atmospheres, Algorithms, Line Spectra, Linear Operators, Transfer Functions

Scientific paper

A numerical method for solving the radiative transfer problem in an arbitrary moving atmosphere is described. The method involves the construction of transformation operators which relate functions of spatial position to optical path length and vice versa. Numerical results are presented for several one-dimensional examples with different velocity fields.

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