Updated Model of the Solar Energetic Proton Environment in Space | Journal of Space Weather and Space Climate

Measurement, Specification and Forecasting of the Solar Energetic Particle Environment and GLEs

Open Access

Fig. 15

Comparison of SAPPHIRE outputs (at confidence levels of 50%, 60%, 70%, 80%, 90%, 95% and 99% - grey lines) for proton cumulative fluence (left) and peak flux (right) at solar maximum with data from ACE/EPAM for 1 year (top panel), 2 years (middle panel) and 7 years (bottom panel).

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