Physics
Scientific paper
Mar 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..569v&link_type=abstract
(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest
Physics
Atmospheric Boundary Layer, Solar Protons, Stratosphere, Interplanetary Magnetic Fields, Lines Of Force, Proton Energy, Solar Corona
Scientific paper
Events of solar proton increases in the stratosphere and in the atmospheric boundary layer, observed from 1966 through 1974, are analyzed, using data on the solar magnetic fields. It is shown that in the case where the base point of the line of force that ties the earth to the sun is located in the same unipolar region as the flare, the coronal propagation effects associated with the propagation of solar protons are insignificant, and the time-dependences of the intensities and spectra can be described in terms of interplanetary diffusion. The interface of magnetic polarities in the corona constitutes an appreciable barrier for the longitudinal propagation of even high-energy protons. If the base point of the line of force is located beyond the unipolar magnetic region in which the flare is situated, the behavior of solar particles can no longer be described by diffusion.
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