Relativistic solar proton dynamics during the 14 July, 2000 GLE

Details Relativistic solar proton dynamics during the 14 July, 2000 GLE Relativistic solar proton dynamics during the 14 July, 2000 GLE

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3379p&link_type=abstract

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

Physics

3

Scientific paper

The primary relativistic solar proton parameters during the 14 July 2000 "Bastille day" GLE have been obtained by a modeling of the ground level enhancement (GLE) effect on the neutron monitor network and comparing it with observed values. The modeling comprised an optimization procedure as well as proton trajectory calculations in the Tsyganenko-89 geomagnetic field model. The spectrum, pitch-angle distribution and anisotropy of relativistic solar protons (RSP) obtained for 6 successive moments of time showed a certain dynamical changes of these parameters during the event. It was shown that during the 14 July 2000 GLE the increase effect on the ground was caused by imposing of two components of relativistic solar protons, fast and delayed one originated probably from various sources on the Sun.

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