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

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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


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