Variation of the High-Energy Cosmic Ray Anisotropy with a Solar Activity Cycle

Details Variation of the High-Energy Cosmic Ray Anisotropy with a Solar Activity Cycle Variation of the High-Energy Cosmic Ray Anisotropy with a Solar Activity Cycle

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3985k&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The observation of cosmic ray anisotropy in Yakutsk for many years and
their comparison with a theoretical model are given. It is shown that
the cosmic ray anisotropy depends on a degree of curvature of neutral
surface and the polarity sign of interplanetary magnetic field.

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