Dynamics of the Cosmic Ray Current Behaviour during Large-Scale Solar Wind Disturbances

Details Dynamics of the Cosmic Ray Current Behaviour during Large-Scale Solar Wind Disturbances Dynamics of the Cosmic Ray Current Behaviour during Large-Scale Solar Wind Disturbances

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3613k&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

By using treatment results of world net neutron monitor data by the global survey method, the behaviour of cosmic ray current (anisotropy) during Forbusheffects for the 1965 to 1999 period is analyzed. Peculiarities of the current behaviour before the shock wave arrival are investigated depending on the value of intensity decrease effect and helio coordinates of disturbance sources on the Sun. Data of the Yakutsk underground complex of muon telescopes are also used in the analysis. Possibilities to predict the arrival of large-scale disturbances of interplanetary medium at the Earth by the behaviour of the observed cosmic ray anisotropy are discussed.

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