Computer Science
Scientific paper
Oct 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kosis..34..464z&link_type=abstract
Kosmicheskie Issledovaniia, Tom 34, No. 5, p. 464 - 468
Computer Science
Cosmic Rays: Solar Modulation, Cosmic Rays: Protons, Cosmic Rays: Variations
Scientific paper
Comparison of variations in the background fluxes of ≡1 MeV protons (the "quiet time" fluxes) with galactic cosmic ray variations is performed. It is shown that these particle fluxes manifested a negative correlation over the entire 1-year cycle as well as over rather short periods (≡1.5 year), such as decreases in cosmic ray intensity caused by the global magnetic structures in the heliosphere. The times of onset and end of these decreases in cosmic ray intensity agreed well with the simultaneous increases in the background fluxes of ≡1 MeV protons during the early phase of the 21st solar cycle (1978 - 1981). Possible reasons for the interrelations between these two particle populations of quite different origins are discussed.
Logachev Yu. I.
Zel'Dovich M. A.
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