Polarization of the hydrogen H alpha line in solar flares - Contribution of the local polarized radiation field and effect of the spectral index of the proton energy distribution
E. Vogt et al., Polarization of the hydrogen H alpha line in solar flares - Contribution of the local polarized radiation field and effect of the spectral index of the proton energy distribution, ASTRON ASTR, 374(3), 2001, pp. 1127-1134
Linear polarization of the hydrogen H alpha line was observed during solar
flares. The polarization vector is directed towards disk center and its deg
ree is of the order of 5%. The best explanation for this polarization is an
isotropic collisional excitation of the n = 3 level of hydrogen by vertical
beams of protons with an energy greater than a few keV. However, previous
calculations gave an expected polarization degree of 2.5% or less, a factor
of two below the observations. In this paper, the theoretical model for th
e formation of the line polarization has been refined, including the effect
of polarization in the local radiation field that is created by hydrogen p
roton anisotropic excitation. We have also increased the spectral index of
the proton energy distribution from 4 to 5, giving more weight to the low e
nergy protons which are the most efficient for impact polarization, without
ionizing the atmosphere too much. It is found that the inclusion of the po
larization of the local radiation field does not increase the H alpha polar
ization very significantly; however, going from a spectral index of 4 to 5
results in an expected polarization degree of 4.5%, compatible with the obs
ervations.