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Importance of Cross-redistribution in Scattering Polarization of Spectral Lines: The Cases of 3P−3S Triplets of Mg i and Ca i

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dc.contributor.author Sampoorna, M
dc.contributor.author Nagendra, K. N
dc.date.accessioned 2020-11-17T14:03:53Z
dc.date.available 2020-11-17T14:03:53Z
dc.date.issued 2017-04-01
dc.identifier.citation The Astrophysical Journal, Vol. 838, No. 2, 95 en_US
dc.identifier.issn 0004-637X
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7107
dc.description Restricted Access © The American Astronomical Society https://doi.org/10.3847/1538-4357/aa662c en_US
dc.description.abstract Scattering on a multi-level atomic system has dominant contributions from resonance and Raman scattering. While initial and final levels are the same for resonance scattering, they are different for Raman scattering. The frequency redistribution for resonance scattering is described by the usual partial frequency redistribution functions of Hummer, while that for Raman scattering is described by cross-redistribution (XRD) function. In the present paper, we investigate the importance of XRD on linear polarization profiles of 3P−3S triplets of Mg i and Ca i formed in an isothermal one-dimensional atmosphere. We show that XRD produces significant effects on the linear polarization profiles when the wavelength separations between the line components of the multiplet are small, like in the cases of Mg i b and Ca i triplets. en_US
dc.language.iso en en_US
dc.publisher IOP Publishing en_US
dc.subject Radiative transfer en_US
dc.subject Scattering en_US
dc.subject Sun: atmosphere en_US
dc.title Importance of Cross-redistribution in Scattering Polarization of Spectral Lines: The Cases of 3P−3S Triplets of Mg i and Ca i en_US
dc.type Article en_US


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