Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4159
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dc.contributor.authorPeraiah, A-
dc.contributor.authorRao, D. M-
dc.date.accessioned2008-12-22T15:34:25Z-
dc.date.available2008-12-22T15:34:25Z-
dc.date.issued1981-12-
dc.identifier.citationAstrophysics and Space Science, Vol. 80, No. 2, pp. 437 - 442en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4159-
dc.descriptionOpen Access-
dc.description.abstractWe have obtained a simultaneous solution of the statistical equilibrium equation for a non-LTE two-level atom and the radiative transfer equation in the comoving frames by employing the angle-averaged partial frequency redistribution.R i with isotropic scattering. In the first iteration we have set the population density of the upper level equal to zero and allow it to be populated in the subsequent iterations. The solution converges within two to four iterations. The process of iteration is terminated when the ratios of population densities in two successive iterations at each radial point, attain an accuracy of 1%. The effects of partial frequency redistribution is to increase the population density of the upper level. Radial gas motions do not seem to have significant effects, although in highly extend geometries, velocity gradients change the population densities considerably.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1981Ap%26SS..80..437Pen
dc.relation.urihttp://dx.doi.org/10.1007/BF00652942en
dc.rightsD. Reidel Publishing Co.,-
dc.subjectAtomic Energy Levelsen
dc.subjectDistribution Functionsen
dc.subjectRadiative Transferen
dc.subjectResonance Linesen
dc.subjectStellar Atmospheresen
dc.subjectEquilibrium Equationsen
dc.subjectFrequency Distributionen
dc.subjectGas Dynamicsen
dc.subjectIterative Solutionen
dc.subjectStatistical Analysisen
dc.titleEffects of partial frequency redistribution on the level population densities in a resonance lineen
dc.typeArticleen
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