Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1740
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dc.contributor.authorSampoorna, M-
dc.contributor.authorNagendra, K. N-
dc.contributor.authorFrisch, H-
dc.date.accessioned2007-07-26T06:35:41Z-
dc.date.available2007-07-26T06:35:41Z-
dc.date.issued2008-09-
dc.identifier.citationJournal of Quantitative Spectroscopy and Radiative Transfer, Vol. 109, No. 14, pp. 2349 - 2363en
dc.identifier.urihttp://hdl.handle.net/2248/1740-
dc.descriptionRestricted Access-
dc.description.abstractThe polarized approximate lambda iteration (PALI) technique developed for the weak field Hanle effect relies on the decomposition of the Stokes parameters I, Q and U into six cylindrically symmetrical components. It has been applied to complete and partial frequency redistribution with redistribution matrices in which frequency redistribution is decoupled from scattering polarization. For partial frequency redistribution, the decoupling is obtained by an adequate decomposition of the frequency space into several domains. By angle-averaging frequency-dependent terms in the exact weak field Hanle redistribution matrix for a normal Zeeman triplet, we construct a redistribution matrix with coupling between frequency redistribution and polarization and no domain decomposition. The coupling is contained in generalized frequency redistribution functions that depend on the magnetic field. The redistribution matrix is expanded in the Landi Degl’Innocenti spherical tensors for polarimetry View the MathML source and the Stokes parameters are decomposed into cylindrically symmetrical components. A PALI method is set up for the calculation of these components. The Stokes parameters are calculated for different simple atmospheric models. The positive Q direction corresponds to the linear polarization perpendicular to the solar limb. It is shown that the frequency space decomposition may induce large errors on Stokes U in the transition region between line core and line wings but can safely be used for Stokes I and Q, the errors staying less than 1% at all the frequencies.en
dc.format.extent338258 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherElsevieren
dc.relation.urihttp://dx.doi.org/10.1016/j.jqsrt.2008.05.011en
dc.rights© Elsevier Ltd All rights reserved-
dc.subjectLine formationen
dc.subjectPolarizationen
dc.subjectRadiative transferen
dc.subjectScatteringen
dc.subjectNumerical methods-
dc.subjectSun-
dc.subjectAtmosphere-
dc.titleThe Hanle effect with partial frequency redistribution. Construction of a frequency-dependent polarization matrix and numerical solution by a PALI methoden
dc.typeArticleen
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