Variations of cosmic-ray density and the solar wind

Details Variations of cosmic-ray density and the solar wind Variations of cosmic-ray density and the solar wind

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23.1015c&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, Nov.-Dec. 1983, p. 1015-1017. In Russian.

Physics

2

Cosmic Rays, Particle Flux Density, Solar Activity Effects, Solar Wind, Annual Variations, Density Distribution, Radiation Distribution, Solar Cycles

Scientific paper

The important role of the solar wind in the formation of 11-year variations of cosmic-ray density is confirmed for the example of the 21st solar cycle. An analysis is made of yearly values of cosmic-ray intensity for 1976-1982 according to Iakutsk ionization-chamber data, corrected for Ip, W, the aa-index. The results predict a softer energy spectrum of 11-year variations of cosmic-ray density in the first half of the 21st cycle. Data for 1976-1982 confirm this prediction; beta is equal to 6.3 during this period.

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