Two solar proton fluence models based on ground level enhancement observations | Journal of Space Weather and Space Climate

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

Open Access

Fig. 6

(a) Parameter R₀ as a function of parameter J₀. GLEs are shown in blue and ESP components in red. Results of a linear fit in log-log-scale is shown in black. ESP components as well as GLE 42 are excluded from the fit. (b) Parameter γ₁ as a function of parameter J₀. The formatting is similar to a), but the fit is performed in log-lin-scale.

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