Solutions for radiative transfer in magnetic atmospheres

Details Solutions for radiative transfer in magnetic atmospheres Solutions for radiative transfer in magnetic atmospheres

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.189..883m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 189, Dec. 1979, p. 883-895. Research supported by the Australian Resear

Astronomy and Astrophysics

Astrophysics

31

Astrophysics, Integral Transformations, Magnetic Effects, Radiative Transfer, Stellar Atmospheres, Zeeman Effect, Differential Equations, Runge-Kutta Method

Scientific paper

An analytical solution method for integrating radiative transfer equations is presented for the problem of radiative transfer in the presence of a magnetic field and absorbing lines. A comparison is made between this method and other solution methods currently in use to solve the radiative transfer problem for polarized light, in terms of their accuracy, computational speed, and convenience. The usefulness and limitations of the different methods are discussed.

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