Primary and secondary effects in cosmic-ray variations at solar proton events
Bulletin of the Russian Academy of Sciences: Physics(2009)
Abstract
The variations of the cosmic-ray rigidity spectrum in the energy range from 0.8 MeV to several dozen GeV at solar proton events in January 2005 and December 2006 have been analyzed. A comparison of the observed and model spectra revealed the power range of direct detection of solar cosmic rays and moments of their observations.
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Key words
Energy Range,Model Spectrum,Solar Wind Plasma,Solar Proton Event,Solar Origin
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