Prediction of Solar Proton Event Fluence spectra from their Peak flux spectra | Journal of Space Weather and Space Climate

Open Access

Fig. 15

(a) Cumulative distributions of Peak occurrence in hours after onset at 6 MeV, 26.3 MeV and 115 MeV. (b) Cumulative distributions of Peak occurrence relative to total Event duration at the same energies. Red dashed lines denote the 70% limit.

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