Background fluxes of 1-MeV protons in interplanetary space in the 21st solar cycle

Details Background fluxes of 1-MeV protons in interplanetary space in the 21st solar cycle Background fluxes of 1-MeV protons in interplanetary space in the 21st solar cycle

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..445z&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 28, May-June 1990, p. 445-450. In Russian.

Physics

Background Radiation, Interplanetary Space, Solar Cycles, Solar Protons, Correlation Coefficients, Interplanetary Magnetic Fields, Shock Wave Propagation, Solar Flares

Scientific paper

The time behavior of proton fluxes in the 0.97-1.85 MeV energy range in interplanetary space during quiet periods from 1975 to 1986 is investigated on the basis of IMP-8 data. An analysis of time variations of these fluxes on different times scales demonstrates the existence of different levels of background fluxes differing in intensity and periodicity and apparently having different sources.

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