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  Solution of Multi-dimensional Polarized Radiative Transfer Equation with PFR

Anusha, L. S. (2019). Solution of Multi-dimensional Polarized Radiative Transfer Equation with PFR. Radiative Signature from the Cosmos, 519, 105-108.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0007-0AEB-6 Version Permalink: http://hdl.handle.net/21.11116/0000-0007-0AEC-5
Genre: Journal Article

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 Creators:
Anusha, L. S.1, Author              
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1Max Planck Institute for Solar System Research, Max Planck Society, ou_1125546              

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 Abstract: Solar observations and numerical simulations have proved the existence of enormous inhomogeneous structures in the solar atmosphere. Solving polarized radiative transfer (RT) equation is a powerful means of understanding the effects of these inhomogeneities on the spectrum emerging from the Sun. To take spatial inhomogeneities into account, a solution of the transfer equation in multi-dimensional (multi-D) geometries is necessary. Here we present a summary of the developments we carried out in a series of papers, to solve multidimensional polarized RT equation with partial frequency redistribution (PFR) and the application of these methods to analyze the observations.

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Language(s): eng - English
 Dates: 20182019
 Publication Status: Published in print
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 Rev. Type: Peer
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Title: Radiative Signature from the Cosmos
Source Genre: Proceedings
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Pages: - Volume / Issue: 519 Sequence Number: - Start / End Page: 105 - 108 Identifier: -