Fig. 7
Left panel: proton flux from AMS02 (Aguilar et al. 2015) and CREAM (Yoon et al. 2011), and a fit of the spectrum between 45 GeV and 200 GeV that we assume here to be the mean Galactic flux. Right panel: data divided by the theoretical mean above 45 GeV, together with conditions ψc/ ⟨ Ψ ⟩ and ψmax/ ⟨ Ψ ⟩ of Fig. 2 (solid for MAX model, dashed for MED, and dotted for MIN).
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