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Hanle-Zeeman Redistribution Matrix. II. Comparison of Classical and Quantum Electrodynamic Approaches

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dc.contributor.author Sampoorna, M
dc.contributor.author Nagendra, K. N
dc.contributor.author Stenflo, J. O
dc.date.accessioned 2008-03-04T06:11:04Z
dc.date.available 2008-03-04T06:11:04Z
dc.date.issued 2007-12
dc.identifier.citation The Astrophysical Journal, Vol. 670, pp. 1485 – 1503 en
dc.identifier.uri http://hdl.handle.net/2248/2111
dc.description.abstract The Hanle-Zeeman redistribution matrix accounts for the intricately coupled correlations in frequency, angle, and polarization between the incoming and outgoing radiation and embodies the physics of the scattering process. We show explicitly for a scattering transition the equivalence between the Hanle-Zeeman redistribution matrix that is derived through quantum electrodynamics and the one derived through classical, time-dependent oscillator theory. This equivalence holds for all strengths and directions of the magnetic field. Several aspects of the Hanle-Zeeman redistribution matrix are illustrated, and explicit algebraic expressions are given, which are of practical use for the polarized line transfer computations. While the efficiency of the Hanle effect is usually confined to the line core, we show how elastic collisions can produce a “wing Hanle effect” as well under favorable conditions in the solar atmosphere. en
dc.format.extent 985670 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher University of Chicago Press en
dc.relation.uri http://www.journals.uchicago.edu/doi/abs/10.1086/522562 en
dc.subject atomic processes—line en
dc.subject formation—polarization—radiative transfer en
dc.title Hanle-Zeeman Redistribution Matrix. II. Comparison of Classical and Quantum Electrodynamic Approaches en
dc.type Article en


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