The anisotropy of cosmic rays connected with the high-velocity solar-wind flux of May 5-13, 1973

Details The anisotropy of cosmic rays connected with the high-velocity solar-wind flux of May 5-13, 1973 The anisotropy of cosmic rays connected with the high-velocity solar-wind flux of May 5-13, 1973

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..908m&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Nov.-Dec. 1982, p. 908-911. In Russian.

Physics

4

Solar Cosmic Rays, Solar Flux, Solar Wind Velocity, Anisotropy, Interplanetary Magnetic Fields, Solar Activity Effects, Solar Physics

Scientific paper

An examination of solar-wind data from May 5-13, 1973 shows that a sunward-directed anisotropy of cosmic rays arises in the region of interaction between fast and slow fluxes of the solar wind. The direction of anisotropy coincides with the direction of the force lines of the interplanetary magnetic field. It is concluded that data on cosmic-ray anisotropy prior to decreases of cosmic-ray intensity can be used to establish the nature of subsequent intensity decreases.

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