Background proton fluxes of about 1 MeV in interplanetary space and their relationship with solar activity

Details Background proton fluxes of about 1 MeV in interplanetary space and their relationship with solar activity Background proton fluxes of about 1 MeV in interplanetary space and their relationship with solar activity

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1957z&link_type=abstract

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

Physics

Interplanetary Space, Proton Flux Density, Solar Activity, Solar Protons, Cross Correlation, Explorer 50 Satellite, Solar Cycles, Vega Project

Scientific paper

Temporal variations of the intensity of proton fluxes with energy of
about 1 MeV are studied on the basis of IMP8 and Vega-1 and -2 data
during the calm (flareless) period of solar activity during the 21st
cycle. The results point to the solar origin of low-energy background
proton fluxes during the greater part of the solar cycle.

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