Cosmic-ray variations due to the 22-year magnetic solar cycle

Details Cosmic-ray variations due to the 22-year magnetic solar cycle Cosmic-ray variations due to the 22-year magnetic solar cycle

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1809s&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1809-1811. In Russian.

Physics

Annual Variations, Cosmic Rays, Magnetic Effects, Solar Cycles, Flux Quantization, Long Term Effects, Stratosphere

Scientific paper

It is shown that the time period 1972-1979 was characterized not only by the presence of anomalous helium in circumsolar space but also by the appearance of an additional particle flux in the 100-500 MeV per nucleon energy range. This period was also characterized by the additional modulation of a flux of 2-15 GV particles and large and temporally stable divergences between readings of several neutron monitors. It is difficult to explain this combination of phenomena by modulation theory with allowance for particle drift owing to the fact that an increase in the low-energy cosmic-ray flux was observed at the same time as a decrease in the flux of particles of relatively high energy.

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