Twenty-seven-day variations of Galactic cosmic rays in 1976

Details Twenty-seven-day variations of Galactic cosmic rays in 1976 Twenty-seven-day variations of Galactic cosmic rays in 1976

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..341s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Mar.-Apr. 1991, p. 341-343. In Russian.

Physics

Galactic Cosmic Rays, Periodic Variations, Solar Activity, Solar Cycles, Helium Ions, Interplanetary Magnetic Fields, Spatial Distribution

Scientific paper

Consideration is given to the 27-day intensity wave of Galactic cosmic rays observed in 1976 during a solar minimum period. The variation amplitude is about 1.5-2 percent. The same type of variation, but of a much greater amplitude, is experienced by the flux of He-4 nuclei as evidenced by IMP-8 measurements. It is suggested that the observed phenomenon is due to the spatial asymmetry of the region of the cosmic-ray modulation.

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