Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/403
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dc.contributor.authorPeraiah, A-
dc.date.accessioned2005-05-18T09:55:29Z-
dc.date.available2005-05-18T09:55:29Z-
dc.date.issued1986-05-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 5, No. 2, pp. 113-140en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/403-
dc.description.abstractWe present details of a new technique of obtaining a numerical solution of the radiative transfer equation in spherical symmetry in a polychromatic system. We employed the integral operators together with an interpolation formula of the specific intensity defined on radius-angle-frequency grid. We found that the method is quite stable and employs a large stepsize in all the variables on the grid. We employed complete redistribution in calculating the linesen
dc.format.extent1047293 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectSpectral linesen
dc.subjectRadiative transfer equation in spherical symmetryen
dc.titleIntegral Operator Technique of Line Transferen
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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