Long-Term Variation of Small Energy Proton Intensity According to Satellite Data and Hysteresis between Cosmic Rays and Solar Activity

Details Long-Term Variation of Small Energy Proton Intensity According to Satellite Data and Hysteresis between Cosmic Rays and Solar Activity Long-Term Variation of Small Energy Proton Intensity According to Satellite Data and Hysteresis between Cosmic Rays and Solar Activity

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.4111d&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

For investigation of the hysteresis effect for small energies of galactic CR we analyzed satellite 5-min data on proton fluxes with energies > 1 MeV, > 2 MeV, > 5 MeV, > 10 MeV, > 30 MeV, > 50 MeV, > 60 MeV, > 100 MeV, and in intervals 10-30 MeV, 30-60 MeV, and 60-100 MeV during January 1986-31 December 1999. The analysis of the hysteresis effect is made according to procedure described in [1]; corrections on drift effects are based on paper [2]. This research is partly supported by INTAS grant No. 00810.

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