Consistency of the average flux of solar energetic particles over timescales of years to megayears

Open Access

Fig. D.1.

Distributions of Weibull parameters λ and k vs. χ² and parameter correlation plot for F₃₀ fit obtained using GOES SC 24 and terrestrial CI proxy data. Red stars correspond to the best-fit parameter values (), and blue dots have χ² ≤ + 2.30, as shown with the dashed red line.

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