Physics
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2341e&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser
Physics
Galactic Cosmic Rays, Radiant Flux Density, Solar Activity, Solar Cycles, Amplitude Modulation, Heliosphere
Scientific paper
A model is proposed to explain 11-year intensity variations of galactic
cosmic rays. This modulation model explicitly takes into account the
nonstationary character of the modulation and the relationship between
the modulation effects and active processes in long-lasting solar active
regions.
Ermakov S. I.
Kontor N. N.
Liubimov G. P.
Pavlov N. N.
Reizman Ia. S.
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