English

Coronal Polarization

Solar and Stellar Astrophysics 2011-04-05 v1

Abstract

We present an overview of the physical mechanisms responsible for the coronal polarization at different wavelength regimes. We also review different techniques using coronal polarization to determine various quantities necessary for understanding the thermodynamic properties of the solar coronal plasma. This includes the coronal magnetic field, electronic densities, temperatures, velocities, etc. The future needs to acquire better information on the solar corona using polarization will be outlined.

Keywords

Cite

@article{arxiv.1104.0598,
  title  = {Coronal Polarization},
  author = {N. -E. Raouafi},
  journal= {arXiv preprint arXiv:1104.0598},
  year   = {2011}
}

Comments

8 pages, 5 figures, 6th Solar Polarization Workshop

R2 v1 2026-06-21T17:49:10.908Z