Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2479
Title: Hanle-Zeeman Redistribution Matrix. III. Solution of the Polarized Line Formation Problem
Authors: Sampoorna, M
Nagendra, K. N
Stenflo, J. O
Keywords: line: formation-magnetic fields-methods
numerical-polarization-radiative transfer-scattering-Sun: atmosphere
Issue Date: May-2008
Publisher: The American Astronomical Society
Citation: APJ, Vol. 679, No. 1, pp. 889 – 899
Abstract: The 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 direction
Description: Restricted Access
URI: http://hdl.handle.net/2248/2479
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.