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Helium fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for solar cycle 24
N. Marcelli, M. Boezio, A. Lenni +53
Time-dependent energy spectra of galactic cosmic rays (GCRs) carry fundamental information regarding their origin and propagation. When observed at the Earth, these spectra are sig…
Time dependence of the flux of helium nuclei in cosmic rays measured by the PAMELA experiment between July 2006 and December 2009
N. Marcelli, M. Boezio, A. Lenni +53
Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles through the heliosphere. T…
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…
Secondary positrons and electrons measured by PAMELA experiment
V. V. Mikhailov, O. Adriani, G. Barbarino +55
We present a measurements of electron and positron fluxes below the geomagnetic cutoff rigidity in wide energy range from 50 MeV to several GeV by the PAMELA magnetic spectrometer.…