Distribution of cosmic rays connected with high-velocity streams of the solar wind

Details Distribution of cosmic rays connected with high-velocity streams of the solar wind Distribution of cosmic rays connected with high-velocity streams of the solar wind

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2149k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Cosmic Rays, Magnetohydrodynamic Flow, Solar Wind, Space Plasmas, Correlation Coefficients, Diurnal Variations, Interplanetary Magnetic Fields, Neutron Counters, Root-Mean-Square Errors

Scientific paper

Data from a ring of neutron-monitor stations are used to analyze the cosmic-ray anisotropy in the transition region where the leading edge of high-velocity streams of the solar wind interacts with the quiet solar wind. The events of December 6-9, 1970, May 6-10, 1973, and May 14-25, 1973 were investigated. An increase in cosmic-ray intensity due an anisotropic stream observed in the 135-deg E direction was found to occur before the earth encountered the high-velocity stream. It is shown that the high-velocity streams have a more regular magnetic field than the quiet wind.

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