Fig. 10.
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Mean values of the proton peak fluxes (in pfu) at several integral energies (E > 10; >30; >60 and >100 MeV) and their respective standard deviation of the mean, as a function of the mean SXR duration (in minutes) for the solar flares associated with SEP events in the SEP part of the database. Each integral energy is color coded as in Figure 8.
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