Rigidity dependence of the cosmic-ray modulation parameter at different epochs of solar cycles

Details Rigidity dependence of the cosmic-ray modulation parameter at different epochs of solar cycles Rigidity dependence of the cosmic-ray modulation parameter at different epochs of solar cycles

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2334b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Energetic Particles, Galactic Cosmic Rays, Solar Activity, Solar Cycles, Stratosphere, Universe

Scientific paper

An analysis was made of temporal variations of the galactic-cosmic-ray modulation parameter with a rigidity of 1-25 GV in solar cycles 19 to 21. It is shown that the solar-activity dependence of these variations can be represented in a power form, where the exponent varies from 0.6-0.8 for solar minimum and from 1.5-1.6 for solar maximum, reflecting variations of the spectrum of magnetic inhomogeneities at different epochs of the solar cycle.

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