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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…
Lithium and Beryllium isotopes with the PAMELA experiment
W. Menn, E. A. Bogomolov, M. Simon +56
The cosmic-ray lithium and beryllium (Li, Li, Be, Be, Be) isotopic composition has been measured with the satellite-borne experiment PAMELA, which wa…
Evidence of energy and charge sign dependence of the recovery time for the December 2006 Forbush event measured by the PAMELA experiment
R. Munini, M. Boezio, A. Bruno +55
New results on the short-term galactic cosmic ray (GCR) intensity variation (Forbush decrease) in December 2006 measured by the PAMELA instrument are presented. Forbush decreases a…
Ten Years of PAMELA in Space
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +50
The PAMELA cosmic ray detector was launched on June 15th 2006 on board the Russian Resurs-DK1 satellite, and during ten years of nearly continuous data-taking it has observed new i…
Unexpected cyclic behavior in cosmic ray protons observed by PAMELA at 1 AU
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +50
Protons detected by the PAMELA experiment in the period 2006-2014 have been analyzed in the energy range between 0.40-50 GV to explore possible periodicities besides the well known…
Proton fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for the 24th solar cycle
M. Martucci, R. Munini, M. Boezio +51
Precise measurements of the time-dependent intensity of the low energy ( GeV) galactic cosmic rays are fundamental to test and improve the models which describe their propagat…