Directional Variation of 5 GeV Muon Flux Observed in the Underground Muon Telescope

Details Directional Variation of 5 GeV Muon Flux Observed in the Underground Muon Telescope Directional Variation of 5 GeV Muon Flux Observed in the Underground Muon Telescope

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3573a&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 small muon telescope is placed in the underground lab oratory. The muon energy threshold is about 5 GeV which corresp onds to primary CR energies above 15 GeV (maximal contribution at 100 GeV). We have observed a number of Forbush Decrease events which made a 1-2 percent fall in observed counting rate. The telescope has 2 degrees directional accuracy. This allows to study the directional variation of muon flux at the disturbance time. We present analysis of directional variation in time with respect to neutron monitor Forbush Decrease registration. The model explanation for observed differences between FD events will be presented. The project of large underground muon detector will be presented.

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