Relativistic Solar Proton Dynamics in Large GLE of 23rd Solar Cycle

Details Relativistic Solar Proton Dynamics in Large GLE of 23rd Solar Cycle Relativistic Solar Proton Dynamics in Large GLE of 23rd Solar Cycle

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3401v&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

6

Scientific paper

The primary relativistic solar proton (RSP) parameters during the largest ground level enhancements (GLE) of 23 solar cycle: 14 July, 2000 and 15 April, 2001 have been obtained by modeling of the responses of neutron monitors of the worldwide network and comparing them with observations. The modeling comprised an optimization procedure as well as proton trajectory calculations in the up-to-date magnetosphere model Tsyganenko-2002 (T202). The spectra, pitch-angle distributions and anisotropy of RSP obtained for successive moments of time allowed to study the dynamical changes of these parameters during the events.

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