Solution of Multi-dimensional Polarized Radiative Transfer Equation with PFR

Anusha, L. S.

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Solution of Multi-dimensional Polarized Radiative Transfer Equation with PFR

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Anusha, L. S.
Max Planck Institute for Solar System Research, Max Planck Society;

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

Cite as: https://hdl.handle.net/21.11116/0000-0007-0AEB-6

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.