Some aspects of the solution of vector transfer equation in a magnetized medium

Details Some aspects of the solution of vector transfer equation in a magnetized medium Some aspects of the solution of vector transfer equation in a magnetized medium

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.117..121n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 117, no. 1, Dec. 1985, p. 121-135.

Statistics

Computation

6

Computational Astrophysics, Magnetic Stars, Polarized Radiation, Transfer Functions, Numerical Analysis, Run Time (Computers), Zeeman Effect

Scientific paper

A simplification of the numerical method of solving the vector transfer equation, given earlier by Nagendra and Peraiah (1985), is described for problems which involve only absorption. This makes it possible to attempt to solve under realistic conditions and with reduced computing efforts, the important problems of polarization of light emerging from magnetized stars. For the purpose of illustration, the equations described are used for solving the continuum and Zeeman line transfer problems.

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