Scintillations of cosmic-ray intensity - Activity waves

Details Scintillations of cosmic-ray intensity - Activity waves Scintillations of cosmic-ray intensity - Activity waves

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..897k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Nov.-Dec. 1990, p. 897-900. In Russian.

Physics

4

Galactic Cosmic Rays, Neutron Counters, Periodic Variations, Scintillation, Solar Wind, Forbush Decreases, Interplanetary Magnetic Fields, Magnetic Clouds, Shock Waves

Scientific paper

Recurrent variations of the scintillation index of galactic cosmic rays were revealed on the basis of five-minute data from the Tiksi and Apatity neutron monitors. Recurrent amplifications of the scintillation intensity of galactic cosmic rays with characteristic periods of 13-27 days and 3-6 days (activity waves) are observed which are close to periods observed in IMF and solar-wind fluctuations.

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