Nonstationary effects in the 11-year variation of the intensity of galactic cosmic rays

Details Nonstationary effects in the 11-year variation of the intensity of galactic cosmic rays Nonstationary effects in the 11-year variation of the intensity of galactic cosmic rays

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2106z&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

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Galactic Cosmic Rays, Solar Activity Effects, Astronomical Models, Computational Astrophysics, Periodic Variations, Radiant Flux Density, Solar Wind, Spatial Distribution, Temporal Distribution

Scientific paper

A numerical simulation is used to analyze the 11-year modulation of galactic cosmic rays (GCRs) and their distribution in interplanetary space in the framework of a model which takes into account the spatial and temporal variations of solar-wind properties. The HL index is taken as the measure of solar activity. It is concluded that in order to construct a consistent model of GCR variations with the solar-activity cycle it is necessary to take into account the actual nonstationary distribution of solar-wind properties.

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