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

dc.contributor.author	Nagendra, K. N
dc.contributor.author	Peraiah, A
dc.date.accessioned	2007-07-27T05:02:23Z
dc.date.available	2007-07-27T05:02:23Z
dc.date.issued	1985-12
dc.identifier.citation	Astrophysics & Space Science, Vol. 117, pp. 121-135	en
dc.identifier.uri	http://hdl.handle.net/2248/1744
dc.description.abstract	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	en
dc.format.extent	1096360 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1985Ap%26SS.117..121N	en
dc.subject	Magnetic stars	en
dc.subject	Numerical analysis	en
dc.title	Some aspects of the solution of vector transfer equation in a magnetized medium	en
dc.type	Article	en