Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7313
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dc.contributor.authorSampoorna, M-
dc.contributor.authorNagendra, K. N-
dc.contributor.authorFrisch, H-
dc.contributor.authorStenflo, J. O-
dc.date.accessioned2020-11-20T13:16:29Z-
dc.date.available2020-11-20T13:16:29Z-
dc.date.issued2019-07-
dc.identifier.citationAstronomical Society of the Pacific Conference Series, Vol. 519, pp. 109-112en_US
dc.identifier.isbn978-1-58381-925-8-
dc.identifier.issn1050-3390-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7313-
dc.descriptionRestricted Access © Astronomical Society of the Pacific http://aspbooks.org/a/volumes/article_details/?paper_id=38880en_US
dc.description.abstractScattering of solar limb darkened radiation field on atoms and molecules produces linearly polarized spectrum of the sun (Second Solar Spectrum). Partial frequency redistribution (PFR) plays a fundamental role in shaping the wings of linearly polarized profiles of strong resonance lines. Here we present the effects of the angle dependent (AD) PFR on resonance polarization both in the presence and absence of magnetic fields. We consider scattering on a two-level atom with unpolarized lower level, and a one dimensional isothermal atmosphere.en_US
dc.language.isoenen_US
dc.publisherAstronomical Society of the Pacificen_US
dc.relation.ispartofseriesAstronomical Society of the Pacific Conference Series;519-
dc.subjectpolarized spectrum of the sunen_US
dc.subjectPartial frequency redistribution (PFR)en_US
dc.subjectpolarizationen_US
dc.titleEffects of angle-dependent partial frequency redistrubtion on polarized line profilesen_US
dc.typeArticleen_US
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