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Measurements of He isotopic ratio in cosmic rays in the 100 MeV – 1 GeV range with the PAMELA experiment

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Figure

Fig. 2. Energy loss in tracker (mean in all planes hit) vs trackerrigidity for positively charged particles
Fig. 5.3He/4He ratio R as a function of kinetic energy per nu-cleon (top) and rigidity (bottom)
Table 1. GALPROP parameters for the models considered as described in Ptuskin et al. (2006)

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