Change in the period of variations of the solar-rotation-related variation of cosmic rays

Details Change in the period of variations of the solar-rotation-related variation of cosmic rays Change in the period of variations of the solar-rotation-related variation of cosmic rays

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..552b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, July-Aug. 1984, p. 552-556. In Russian.

Physics

Galactic Cosmic Rays, Solar Rotation, Amplitudes, Interplanetary Magnetic Fields, Long Term Effects, Periodic Variations, Polarity

Scientific paper

The pattern of solar-rotation-related variations of the intensity of galactic cosmic rays (GCRs) and of various modulating factors is evaluated on the basis of Deep River neutron-monitor data for 1958-1981 in an effort to clarify the cause of GCR variations with a period of 26-30 days. Variations with periods of about 27 and 29 days were observed during 1958-1968, while only variations with a period of 28.3 days were observed during 1971-1979. An analysis of different solar-activity indexes and polarity during these time periods did not yield analogous results.

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