High-power solar proton events at the beginning of the 22nd cycle

Details High-power solar proton events at the beginning of the 22nd cycle High-power solar proton events at the beginning of the 22nd cycle

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1881a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Physics

Energy Spectra, Proton Energy, Solar Cosmic Rays, Solar Protons, Particle Flux Density, Radiant Flux Density, Solar Flares, Temporal Distribution

Scientific paper

Fluxes and energy spectra of protons with energies greater than 150 MeV, which were measured using radiosondes and earth-based facilities in 1988-1989, are presented. The beginning of the 22nd solar cycle differs in the high concentration of proton events with a rigid energy spectrum, prominent among which is the flare of September 29, 1989, which yielded particles with energies greater than 20 GeV. A preliminary analysis of the temporal variations of the proton intensity for this event is presented.

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