Asymmetry of the cosmic-ray modulation region

Details Asymmetry of the cosmic-ray modulation region Asymmetry of the cosmic-ray modulation region

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..925s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Sept.-Oct. 1991, p. 925-927. In Russian.

Physics

1

Coronal Holes, Galactic Cosmic Rays, Interplanetary Magnetic Fields, Polar Regions, Solar Wind Velocity, Density Distribution, Forbush Decreases, Shock Waves, Solar Terrestrial Interactions

Scientific paper

The behavior of the galactic-cosmic-ray (GCR) intensity at the boundary of the IMF sectors in 1974 is analyzed. The results obtained are explained by assuming the existence of a significant north-south GCR density gradient during this period associated with an observed latitudinal asymmetry in the velocity of the solar wind from polar coronal holes. The annual variations of the intensity in 1976 confirm this finding.

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