Effects of high-velocity solar-wind streams in cosmic rays during May 14-25, 1973

Details Effects of high-velocity solar-wind streams in cosmic rays during May 14-25, 1973 Effects of high-velocity solar-wind streams in cosmic rays during May 14-25, 1973

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..491d&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, May-June 1984, p. 491-493. In Russian.

Physics

1

Cosmic Ray Showers, Solar Activity Effects, Solar Cosmic Rays, Solar Terrestrial Interactions, Solar Wind Velocity, Anisotropy, Coronal Holes, Interplanetary Magnetic Fields, Particle Flux Density, Solar Flares

Scientific paper

Differences in the anisotropies of flare-related (FR) and coronal-hole-related (CHR) streams are examined on the basis of data for the gigantic high-velocity solar-wind streams of May 14-25, 1973. It is shown that CHR streams are characterized by an anisotropy which arises before the stream arrives at the earth, and by a dominant direction of the anisotropic stream which is toward the sun along the IMF lines. FR streams are characterized by an anisotropy which arises after the stream arrives at the earth.

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