High-energy solar cosmic rays

Details High-energy solar cosmic rays High-energy solar cosmic rays

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..353z&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, May-June 1989, p. 353-358. In Russian.

Physics

1

Energetic Particles, Neutron Counters, Radiation Measurement, Solar Cosmic Rays, Energy Spectra, Flux Quantization, Solar Protons, Temporal Distribution

Scientific paper

Five-minute data from the Alma-Ata high-altitude neutron monitor are examined for cases of the detection of high-energy solar cosmic rays (SCRs). Eight cases of intensity increase during solar proton events with amplitudes of 0.4-2.0 percent were found. Time variations of intensity are evaluated for the events of May 7, 1978 and Dec. 7-8, 1982. Integral SCR fluxes are calculated for three cases.

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