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Polarized Line Formation in Multi-dimensional Media. IV. A Fourier Decomposition Technique to Formulate the Transfer Equation with Angle-dependent Partial Frequency Redistribution

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dc.contributor.author Anusha, L. S
dc.contributor.author Nagendra, K. N
dc.date.accessioned 2011-09-21T10:08:16Z
dc.date.available 2011-09-21T10:08:16Z
dc.date.issued 2011-09-20
dc.identifier.citation The Astrophysical Journal, Vol. 739, No. 1, 40 en
dc.identifier.uri http://hdl.handle.net/2248/5571
dc.description Open Access en
dc.description.abstract To explain the linear polarization observed in spatially resolved structures in the solar atmosphere, the solution of polarized radiative transfer (RT) equation in multi-dimensional (multi-D) geometries is essential. For strong resonance lines, partial frequency redistribution (PRD) effects also become important. In a series of papers, we have been investigating the nature of Stokes profiles formed in multi-D media including PRD in line scattering. For numerical simplicity, so far we have restricted our attention to the particular case of PRD functions which are averaged over all the incident and scattered directions. In this paper, we formulate the polarized RT equation in multi-D media that takes into account the Hanle effect with angle-dependent PRD functions. We generalize here to the multi-D case the method for Fourier series expansion of angle-dependent PRD functions originally developed for RT in one-dimensional geometry. en
dc.language.iso en en
dc.publisher IOP Publishing en
dc.relation.uri http://iopscience.iop.org/0004-637X/739/1/40/ en
dc.rights © IOP Publishing en
dc.subject Line: formation en
dc.subject Magnetic fields en
dc.subject Polarization en
dc.subject Radiative transfer en
dc.subject Scattering en
dc.subject Sun: atmosphere en
dc.title Polarized Line Formation in Multi-dimensional Media. IV. A Fourier Decomposition Technique to Formulate the Transfer Equation with Angle-dependent Partial Frequency Redistribution en
dc.type Article en


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