Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3321m&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
A problem of the upper energy limit for solar cosmic rays (SCR) is studied. Formerly, this limit has been estimated mostly by the data of world network of standard detectors of cosmic rays — neutron monitors, muon telescopes and ionization chambers. Recently, it became possible to use for this purpose also the data of some large non-standard detectors (Baksan Underground Scintillation telescope BUST, Extensive Air Shower (EAS) Arrays like Carp et and Andyrchy, project GRAND Array and others). Even though those detectors have been designed for resolving quite different nuclear and astrophysical problems, nevertheless, they proved to be sensible to the effects caused by powerful sporadic manifestations of the solar activity. These observations allow to advance into the energy range above 100 GeV and understand more distinctly the extreme potentialities of solar accelerators.
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