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The effect of angle-dependent non-coherent electron scattering and partial redistribution on the polarization of resonance lines

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dc.contributor.author Rangarajan, K. E
dc.date.accessioned 2008-09-01T09:26:30Z
dc.date.available 2008-09-01T09:26:30Z
dc.date.issued 1999-10
dc.identifier.citation Monthly Notices of the Royal Astronomical Society, Vol. 308, No. 4, pp. 1053 - 1060 en
dc.identifier.issn 0035-8711
dc.identifier.uri http://hdl.handle.net/2248/3287
dc.description.abstract The 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.iso en en
dc.publisher The Royal Astronomical Society en
dc.relation.uri http://adsabs.harvard.edu/abs/1999MNRAS.308.1053R en
dc.subject Electron scattering en
dc.subject Polarization en
dc.title The effect of angle-dependent non-coherent electron scattering and partial redistribution on the polarization of resonance lines en
dc.type Article en


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