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Radiative transfer equation in spherically-symmetric non-scattering media

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dc.contributor.author Peraiah, A
dc.contributor.author Varghese, B. A
dc.date.accessioned 2009-01-23T16:41:06Z
dc.date.available 2009-01-23T16:41:06Z
dc.date.issued 1984-12
dc.identifier.citation Astrophysics and Space Science, Vol. 107, No. 1, pp. 177 - 190 en
dc.identifier.issn 0004-640X
dc.identifier.uri http://hdl.handle.net/2248/4284
dc.description.abstract The 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.iso en en
dc.publisher D. Reidel Publishing Co. en
dc.relation.uri http://adsabs.harvard.edu/abs/1984Ap%26SS.107..177P en
dc.relation.uri http://dx.doi.org/10.1007/BF00649623 en
dc.subject Radiation Distribution en
dc.subject Radiative Transfer en
dc.subject Scattering Functions en
dc.subject Spherical Shells en
dc.subject Angular Distribution en
dc.subject Computational Grids en
dc.subject Planck’s constant en
dc.subject Run Time (Computers) en
dc.subject Spheres en
dc.title Radiative transfer equation in spherically-symmetric non-scattering media en
dc.type Article en


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