Spectra of solar energetic protons derived from statistical analysis of experimental data on a large set of events

Details Spectra of solar energetic protons derived from statistical analysis of experimental data on a large set of events Spectra of solar energetic protons derived from statistical analysis of experimental data on a large set of events

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3185m&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

The presented analysis of the energy spectra of solar energetic protons differs from the earlier analyses in that not only a broader energy range is analyzed, but also the method of simultaneous statistical analysis of a large data set is used. The SEP events supported by the proton peak flux data in a broad energy range (METEOR, IMP8, GOES, balloons, and groundbased neutron monitors) are analyzed. The proton energy for the analyzed events turns out to range from 4 MeV to 11 GeV. The analysis has shown that the ≥30 MeV proton energy spectra in SEP events can most adequately be described by power-law functions of rigidity.

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