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

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DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

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