Solution of radiative transfer equation in spherically symmetric media with spherical harmonic approximation

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5027

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DC Field	Value	Language
dc.contributor.author	Peraiah, A	-
dc.date.accessioned	2010-02-23T10:16:52Z	-
dc.date.available	2010-02-23T10:16:52Z	-
dc.date.issued	1979-11	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp. 230–239	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/5027	-
dc.description.abstract	A numerical method for obtaining solution of radiative transfer equation in spherically symmetric media with spherical harmonic approximation is presented. The angle derivative is approximated by an orthonormal polynomial and this is represented by a matrix, for a given beam of rays. An error analysis of the curvature matrix and results using the solution for few representative cases has been presented.	en
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.rights	© Indian Institute of Astrophysics	en
dc.subject	Spherically Symmetry	en
dc.subject	Radiative Transfer Equation	en
dc.subject	Spherical Harmonic Approximation	en
dc.title	Solution of radiative transfer equation in spherically symmetric media with spherical harmonic approximation	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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