Intensity increases of cosmic rays prior to recurrent Forbush effects

Details Intensity increases of cosmic rays prior to recurrent Forbush effects Intensity increases of cosmic rays prior to recurrent Forbush effects

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..541k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, July-Aug. 1985, p. 541-544. In Russian.

Computer Science

1

Forbush Decreases, Neutrons, Solar Cosmic Rays, Solar Wind, Solar Flares, Statistical Analysis

Scientific paper

Intensity variations of the neutron component of cosmic rays are examined for the period just before the earth encounters a high-velocity stream (HVS) of the solar wind of nonflare origin. A statistical analysis of data for a number of HVSs during 1973-1974 shows that an increase in cosmic-ray intensity of about 0.4 percent is observed just before the HVS encounters the earth.

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