Statistical analysis of solar proton events in different energy channels

Details Statistical analysis of solar proton events in different energy channels Statistical analysis of solar proton events in different energy channels

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3465b&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

A new catalogue of the solar proton events in the energy channels >10 MeV, >30 MeV, >60 MeV and >100 MeV and GLE for the period 1976-2000 was created. Solar proton events (SPEs) for three complete 11-year solar cycles (1976-2000) have been studied. Longitudinal distribution of the 168 identified Hα solar flares and peak size distributions of all 200 events with proton energy >10 MeV and peak intensity >10 pfu (particle cm-2 s-1 sr-1 ) observed at 1 AU were obtained. In addition, to examine the energy dependence of the proton event frequency we have constructed the peak size distributions for three energy thresholds of protons >30 MeV, >60 MeV and >100 MeV for the time interval 05.1987÷10.1995.

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