Yield and Response Functions of the Baksan EAS-Array Andyrchy for Single Component

Details Yield and Response Functions of the Baksan EAS-Array Andyrchy for Single Component Yield and Response Functions of the Baksan EAS-Array Andyrchy for Single Component

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3457k&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 significant increases (>3 st.dev.) were recorded at two Baksan EAS-arrays Andyrchy and Carp et in 6 events from 10 Ground Level Enhancements (GLE), which were registered in current cycle of solar activity. It signifies, that the Solar Cosmic Rays (SCR) of high energy are observed approximately in 50% of GLE. It is necessary to take into account a difference of the response functions of EASarrays and neutron monitors to prolong the SCR spectra up to 5.8 GeV (Baksan geomagnetic cut-off ). With this purpose the account of the yield and response functions was executed for single component of the Andyrchy.

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