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Solar energetic particle events observed by the PAMELA mission
A. Bruno, G. A. Bazilevskaya, M. Boezio +55
Despite the significant progress achieved in recent years, the physical mechanisms underlying the origin of solar energetic particles (SEPs) are still a matter of debate. The compl…
Time dependence of the e^- flux measured by PAMELA during the July 2006 - December 2009 solar minimum
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +58
Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy not accessible…
PAMELA's Measurements of Magnetospheric Effects on High Energy Solar Particles
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +64
The nature of particle acceleration at the Sun, whether through flare reconnection processes or through shocks driven by coronal mass ejections (CMEs), is still under scrutiny desp…
Observations of the December 13 and 14, 2006, Solar Particle Events in the 80 MeV/n - 3 GeV/n range from space with PAMELA detector
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +61
We present the space spectrometer PAMELA observations of proton and helium fluxes during the December 13 and 14, 2006 solar particle events. This is the first direct measurement of…