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Solar-Cycle Variations of South-Atlantic Anomaly Proton Intensities Measured With The PAMELA Mission
A. Bruno, M. Martucci, F. S. Cafagna +50
We present a study of the solar-cycle variations of >80 MeV proton flux intensities in the lower edge of the inner radiation belt, based on the measurements of the Payload for Anti…
Empirical Model of 10-130 MeV Solar Energetic Particle Spectra at 1 AU Based on Coronal Mass Ejection Speed and Direction
Alessandro Bruno, Ian G. Richardson
We present a new empirical model to predict solar energetic particle (SEP) event-integrated and peak intensity spectra between 10 and 130 MeV at 1 AU, based on multi-point spacecra…
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…
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…