naa a22 4500 51073233X CHVBK 20180411082957.0 cr unu---uuuuu 180411e20131001xx s 000 0 eng 10.1134/S1063772913100053 doi (NATIONALLICENCE)springer-10.1134/S1063772913100053 Rachkovskii D. Crimean Astrophysical Observatory, Nauchnyi, Crimea, Ukraine aut A quasi-classical method for deriving the equations of radiative transfer in a magnetic field [Elektronische Daten] [D. Rachkovskii] A new derivation of the matrix equations of radiative transfer in a magnetic field is presented, which is based on the classical approach of M. Born and V.E. Stepanov. Convenient vector relations making it possible to formulate the radiative-transfer equations in an arbitrary coordinate system and choose a convenient system of Stokes parameters are presented. The cases of the solar atmosphere and a stellar atmosphere with a dipolar magnetic field are presented as examples. The use of the radiative-transfer equations written in terms of two main oscillation components (the method of V.E. Stepanov) can lead to crude errors when the complex nature of the absorption coefficients is taken into account. Pleiades Publishing, Ltd., 2013 Astronomy Reports Springer US; http://www.springer-ny.com 57/10(2013-10-01), 766-777 1063-7729 57:10<766 2013 57 11444 https://doi.org/10.1134/S1063772913100053 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1134/S1063772913100053 text/html Onlinezugriff via DOI NATIONALLICENCE 100 1- Rachkovskii D. Crimean Astrophysical Observatory, Nauchnyi, Crimea, Ukraine aut NATIONALLICENCE 773 0- Astronomy Reports Springer US; http://www.springer-ny.com 57/10(2013-10-01), 766-777 1063-7729 57:10<766 2013 57 11444 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer