Characteristics of Forbush decreases in recurrent high-velocity streams of the solar wind

Details Characteristics of Forbush decreases in recurrent high-velocity streams of the solar wind Characteristics of Forbush decreases in recurrent high-velocity streams of the solar wind

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..884k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Nov.-Dec. 1990, p. 884-886. In Russian.

Physics

1

Forbush Decreases, Galactic Cosmic Rays, Solar Terrestrial Interactions, Solar Wind, Magnetic Disturbances, Solar Activity Effects, Solar Wind Velocity

Scientific paper

Variations of the index of the rigidity spectrum of galactic cosmic rays gamma within high-velocity streams of the solar wind are examined. It is shown that gamma reaches its minimum at the moment of velocity maximum; its value is then restored to that characteristic for quiet conditions. It is concluded that, in high-velocity solar-wind streams, the cosmic-ray flux at a fixed geocentric distance in the ecliptic plane is lower than in the quiet solar wind, and that this difference increases with increasing plasma velocity in the high-velocity streams.

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