Solar protons in the 22nd cycle of solar activity

Details Solar protons in the 22nd cycle of solar activity Solar protons in the 22nd cycle of solar activity

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32...23n&link_type=abstract

Geomagnetizm i Aehronomiya (ISSN 0016-7940), vol. 32, no. 5, p. 23-28.

Computer Science

Earth Orbital Environments, Solar Activity Effects, Solar Cycles, Solar Flares, Solar Protons, Solar Terrestrial Interactions, Galactic Cosmic Rays, Solar Cosmic Rays

Scientific paper

The characteristics of solar proton events (SPEs) with a flux in the maximum of not less than 1/sq cm s sr (Ep greater than 10 MeV) in earth orbit have been investigated on the basis of meteor-satellite observations. The characteristics of SPEs and their sources over the last three 11-year cycles are compared. It is concluded that the differences in the flux, spectral, and temporal parameters of SPEs in the 22nd cycle are mainly determined by the characteristics of burst sources of solar cosmic ray protons.

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