Features of cosmic ray anisotropy behavior during periods of Forbush decreases

Details Features of cosmic ray anisotropy behavior during periods of Forbush decreases Features of cosmic ray anisotropy behavior during periods of Forbush decreases

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1954a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Physics

Cosmic Rays, Forbush Decreases, Magnetic Storms, Anisotropy, Vector Spaces

Scientific paper

The behavior of the anisotropy vector of cosmic rays in periods before, during, and after Forbush decreases is investigated. Several events in which the anisotropy vector experienced one or two rotations during the Forbush decrease period were detected. Events both with and without rotation of the cosmic ray anisotropy vector are described within the framework of cosmic ray anisotropy diffusion theory.

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