Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3847k&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
Scientific paper
Recently the conclusion has been made that in the behaviour of the galactic cosmic rays some effects characteristic of the maximum phase of a solar cycle could be isolated: (1) the sudden decreases (the Gnevyshev Gaps) in the modulation and variability and (2) the change in the energy dependence of the cosmic ray modulation from that characteristic of the ascending phase of a solar cycle. In this paper we discuss the definition of the maximum phase in the solar and cosmic ray characteristics and consider the neutron monitor and balloon data during the last four full solar cycles in order to check the chronological order of the mentioned cosmic ray effects. Then the drawn conclusions are checked against the development of the current solar cycle 23.
Bazilevskaya Galina A.
Krainev M. B.
Makhmutov Vladimir S.
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