Effects of two types of solar wind streams on intensity variations of cosmic rays

Details Effects of two types of solar wind streams on intensity variations of cosmic rays Effects of two types of solar wind streams on intensity variations of cosmic rays

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..151..393y&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 151, no. 2, p. 393-396

Physics

9

Coronal Holes, Galactic Cosmic Rays, Solar Activity Effects, Solar Flares, Solar Wind, Forbush Decreases, Neutron Counters, Polarity, Solar Magnetic Field, Solar Terrestrial Interactions

Scientific paper

The influence of two types of high-speed (HS) solar wind streams -- coronal-hole and solar-flare-associated -- on cosmic-ray intensity has been studied using the neutron monitor data of three stations for the period 1972-1984, which includes the year 1980 of solar field reversal. The cosmic-ray depressions associated with the coronal-hole streams are much smaller than the typically Forbush-like depressions. No spectral difference is found in the Forbush-like decreases between the periods before and after the polarity change.

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