Fig. 1.

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Proton (left panel) and helium (right panel) local spectra computed for the γ-optimized scenario are plotted against a representative set of data. For each species the spectra as predicted using the Max and Min source spectrum setups are shown. The corresponding lines computed for the Base scenario are not shown since they are almost coincident with those reported here above 10 GeV n−1 (at the Solar System position).
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