Solar flare phenomena forecast: solar proton events

Abstract

The problems of predicting solar flare events, the only source of high-energy protons, both from the process of energy release itself and from the accompanying dynamic phenomena: shock waves and coronal mass ejections propagating from the place of energy release, are considered from modern positions. The possibility of predicting the flare events themselves ensures the interaction of new emerging magnetic fluxes with the magnetic fields of active regions and outside them, but always on the dividing line of polarities. The possibility of the release of solar protons during of a flare event is determined by the characteristics and localization of the flare event, its CME parameters, and the ratio of its energy in different radiation ranges.