Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3337p&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
The events of the intensity increase of energetic solar particles are analyzed on the basis of data of the 10K-80 spectrometer installed aboard the "Interball-2". The analysis of four solar cosmic ray events based on the comparison of measured solar cosmic ray fluxes and calculated ones allows to make the definite conclusions: 1. The particle propagation model in interplanetary space, which takes into account the impulsive injection in time and their diffusive propagation only along the interplanetary magnetic field lines, describes, on the whole, real events. 2. Considerable generation of turbulence by the solar energetic particles flux and high speed of shock can result in the increasing of magnitude of flow up to arrival of a distubance. 3. At the beginning of the 23 rd solar cycle maximum the total number of the injected particles and their total energy in individual events were N > 1035 particles, E > 1029 erg, respectively.
Petukhov S. I.
Starodubtsev S. A.
Timofeev V. E.
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