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Line formation in spherical media with partial frequency redistribution. I - Solution of the line transfer

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dc.contributor.author Peraiah, A
dc.date.accessioned 2008-12-19T15:02:37Z
dc.date.available 2008-12-19T15:02:37Z
dc.date.issued 1978-09
dc.identifier.citation Astrophysics and Space Science, Vol. 58, No. 1, pp. 189 - 205. en
dc.identifier.issn 1572-946X
dc.identifier.issn 0004-640X
dc.identifier.uri http://hdl.handle.net/2248/4156
dc.description.abstract The solution of line transfer with partial redistribution for an arbitrary (i.e., either stationary or moving) spherical medium is formulated in the framework of discrete space theory. The equation of line transfer for a two-level atom in spherical symmetry is solved for the case of isotropic scattering by using a source function and a line source function together with two angle-dependent and angle-averaged redistribution functions corresponding to zero natural line width and radiation damping with coherence in the atom's rest frame. Two pairs of reflection and transmission coefficients are obtained along with the source vectors, and results are examined for a static medium. It is found that large differences exist between the lines formed by complete and partial redistribution functions and that these differences persist in both spherically symmetric and plane-parallel geometries. en
dc.language.iso en en
dc.publisher Kluwer Academic Publishers en
dc.relation.uri http://adsabs.harvard.edu/abs/1978Ap%26SS..58..189P en
dc.relation.uri http://dx.doi.org/10.1007/BF00645386 en
dc.subject Line Spectra en
dc.subject Radiative Transfer en
dc.subject Stellar Atmospheres en
dc.subject Stellar Spectra en
dc.subject Distribution Functions en
dc.subject Doppler Effect en
dc.subject Optical Thickness en
dc.subject Scattering Functions en
dc.title Line formation in spherical media with partial frequency redistribution. I - Solution of the line transfer en
dc.type Article en


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