Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3287
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dc.contributor.authorRangarajan, K. E-
dc.date.accessioned2008-09-01T09:26:30Z-
dc.date.available2008-09-01T09:26:30Z-
dc.date.issued1999-10-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 308, No. 4, pp. 1053 - 1060en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/3287-
dc.description.abstractThe polarized radiative transfer equation is solved when angle-dependent partial redistribution and non-coherent electron scattering are included as line-scattering mechanisms. A static atmosphere with plane parallel symmetry is assumed. Test calculations are used to illustrate the effects of the electron-scattering coefficient, the thermalization parameter and the continuous absorption coefficient on the line polarization. Results of angle-averaged and angle-dependent redistribution functions are compared and it is shown that angle-dependent functions should be used to model the wing polarization of optically thin lines. The lower the continuous absorption compared with the electron scattering, the higher the wing polarization.en
dc.language.isoenen
dc.publisherThe Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999MNRAS.308.1053Ren
dc.subjectElectron scatteringen
dc.subjectPolarizationen
dc.titleThe effect of angle-dependent non-coherent electron scattering and partial redistribution on the polarization of resonance linesen
dc.typeArticleen
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