Polarization of the H α emission and proton isotropization in solar flares

Details Polarization of the H α emission and proton isotropization in solar flares Polarization of the H α emission and proton isotropization in solar flares

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008astl...34...52t&link_type=abstract

Astronomy Letters, Volume 34, Issue 1, pp.52-58

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Isotropization mechanisms for a beam of low-energy (10-100 keV) protons in the H α formation region are considered. An increase in the magnetic field strength is shown to have no significant effect on the pitch-angle distribution of the accelerated particles in the solar chromosphere. The excitation of small-scale Alfvén waves by protons can lead to their effective scattering. The results obtained are used to interpret peculiarities of the impact polarization of the H α emission.

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