中文

Multigrid Methods for Polarized Radiative Transfer

天体物理学 2008-11-26 v1

摘要

A new iterative method for non-LTE multilevel polarized radiative transfer in hydrogen lines is presented. Iterative methods (such as the Jacobi method) tend to damp out high-frequency components of the error fast, but converges poorly due to slow reduction of low-frequency components. The idea is to use a set of differently coarsed grids to reduce both the short- and long-period errors. This leads to the so-called multigrid (MG) methods. For the grid of NN spatial points, the number of iterations required to solve a non-LTE transfer problem is of the order of O(N). This fact could be of great importance for problems with fine structure and for multi-dimensional models. The efficiency of the so-called standard MG iteration in comparison to Jacobi iteration is shown. The formalism of density matrix is applied to the demonstrative example of 1D, semi-infinite, non-magnetic, 3-principal level hydrogen atmospheric model. The effect of depolarizing collisions with thermal electrons is taken into account as well as general treatment of overlapping profiles.

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引用

@article{arxiv.astro-ph/0611112,
  title  = {Multigrid Methods for Polarized Radiative Transfer},
  author = {Jiri Stepan},
  journal= {arXiv preprint arXiv:astro-ph/0611112},
  year   = {2008}
}

备注

4 pages, 1 figure; will appear in the proceedings of the "4th Solar Polarization Workshop", 2005 September 19-23, Boulder, CO, USA