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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3072
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dc.contributor.authorNagendra, K. N-
dc.contributor.authorFrisch, H-
dc.contributor.authorFaurobeet-Scholl, M-
dc.contributor.authorPaletou, F-
dc.date.accessioned2008-08-12T08:56:43Z-
dc.date.available2008-08-12T08:56:43Z-
dc.date.issued2000-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 255 - 258en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3072-
dc.description.abstractWe present an application of the PALI (Polarized Approximate Lambda Iteration) method to the resonance scattering in spectral lines formed in the presence of weak magnetic fields. The method is based on an operator perturbation approach, and can efficiently give solutions for oriented vector magnetic fields in the solar atmosphere.en
dc.format.extent108579 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000JApA...21..255Nen
dc.subjectPolarizationen
dc.subjectMagnetic Fieldsen
dc.subjectRadiative Transferen
dc.subjectStars:Atmospheresen
dc.subjectMethods: Numericalen
dc.titleAn Operator Perturbation Method of Polarized Line Transfer V. Diagnosis of Solar Weak Magnetic Fieldsen
dc.typeArticleen
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