Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2479
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSampoorna, M-
dc.contributor.authorNagendra, K. N-
dc.contributor.authorStenflo, J. O-
dc.date.accessioned2008-06-20T10:33:37Z-
dc.date.available2008-06-20T10:33:37Z-
dc.date.issued2008-05-
dc.identifier.citationAPJ, Vol. 679, No. 1, pp. 889 – 899en
dc.identifier.urihttp://hdl.handle.net/2248/2479-
dc.descriptionRestricted Accessen
dc.description.abstractThe polarized radiative transfer equation is solved numerically, taking into account both the Zeeman absorption matrix and the Hanle-Zeeman redistribution matrix, to obtain line profiles for arbitrary magnetic field strengths, partial frequency redistribution, and scattering-dominated line transitions. The limiting cases of weak-field Hanle scattering and strong-field Zeeman true absorption are retrieved. The intermediate regime, where both Zeeman absorption and scattering effects are important, is studied in some detail. The numerical method is applied to various test cases to illustrate aspects of partial frequency redistribution on line scattering in magnetic fields of arbitrary strength and directionen
dc.format.extent520871 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/587477en
dc.subjectline: formation-magnetic fields-methodsen
dc.subjectnumerical-polarization-radiative transfer-scattering-Sun: atmosphereen
dc.titleHanle-Zeeman Redistribution Matrix. III. Solution of the Polarized Line Formation Problemen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Sampoorna.pdf
  Restricted Access
Restricted Access508.66 kBAdobe PDFView/Open Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.