English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Solution of Multi-dimensional Polarized Radiative Transfer Equation with PFR

MPS-Authors
/persons/resource/persons123099

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

External Resource
No external resources are shared
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

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


Cite as: http://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.