Flare activity and the proton fluxes in the near and distant heliosphere in solar cycle 21

Details Flare activity and the proton fluxes in the near and distant heliosphere in solar cycle 21 Flare activity and the proton fluxes in the near and distant heliosphere in solar cycle 21

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990baicz..41..251k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 41, no. 4, July 1990, p. 251, 252.

Astronomy and Astrophysics

Astronomy

3

Heliosphere, Proton Flux Density, Solar Flares, Solar Protons, Sunspot Cycle, Annual Variations, Sunspots

Scientific paper

The occurrence of solar proton events in the course of the sunspot cycles shows a regularity: the first maximum is located near the maximum of R; this is followed by a decrease. The second maximum occurred 2-3 years after the maximum of R. Annual mean values of proton fluxes of about 1 MeV near the earth, or at large distances in the heliosphere, demonstrate the same change.

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