Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3197n&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
The results are presented of analyzing the solar energetic particle (SEP) event number and proton fluence as dependent on solar activity. The analysis allows for the random character of the SEP event occurrences, for the threshold effect in determining the small-size events, for the coincidence (overlap) effects of event determination during high solar activity, and for the statistical and methodological errors in experimental data. It is shown, that the main experimental SEP event data (SEP event number, occurrence frequency, and proton fluences) can be explained fully by two mean regular features of SEP events, namely, (1) the mean SEP event occurrence frequency is proportional to sunspot number and (2) the SEP event distribution function normalized to a unified solar activity is independent of (invariant to) solar activity.
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