Sa. Kazantsev et Ag. Petrashen, ON THE POLARIZATION ASYMMETRY OF THE H-ALPHA LINE IN EMISSION OF THE SOLAR CHROMOSPHERE, Optics and spectroscopy, 85(2), 1998, pp. 165-167
The process of the proton charge exchange on hydrogen atoms is studied
spectropolarimetrically. Calculation results show that this process m
ay be responsible for the asymmetry in polarization of the H-alpha emi
ssion of the solar chromosphere, which was found out in a series of ex
periments performed at the Crimean Astrophysical Observatory.