Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4284
Full metadata record
DC FieldValueLanguage
dc.contributor.authorPeraiah, A-
dc.contributor.authorVarghese, B. A-
dc.date.accessioned2009-01-23T16:41:06Z-
dc.date.available2009-01-23T16:41:06Z-
dc.date.issued1984-12-
dc.identifier.citationAstrophysics and Space Science, Vol. 107, No. 1, pp. 177 - 190en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4284-
dc.description.abstractThe equation of radiative transfer in spherically symmetric shells with arbitrary internal sources is solved. The equation of transfer is integrated on a discrete grid of angle and radius. The size in angle coordinates is determined by the roots of a quadrature formula, while the size in radial coordinates is determined by the non negativity of the reflection and transmission operators. Two cases of variation of the Planck formula are considered: (1) constant throughout the medium and (2) varying as 1/r-squared. It is found that in the inner shells the radiation directed toward the center of the sphere is greater than that directed away from the center. In the outer shells the converse is true.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1984Ap%26SS.107..177Pen
dc.relation.urihttp://dx.doi.org/10.1007/BF00649623en
dc.subjectRadiation Distributionen
dc.subjectRadiative Transferen
dc.subjectScattering Functionsen
dc.subjectSpherical Shellsen
dc.subjectAngular Distributionen
dc.subjectComputational Gridsen
dc.subjectPlanck’s constanten
dc.subjectRun Time (Computers)en
dc.subjectSpheresen
dc.titleRadiative transfer equation in spherically-symmetric non-scattering mediaen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Radiative transfer equation705.64 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.