Database of episode-integrated solar energetic proton fluences | Journal of Space Weather and Space Climate

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

Open Access

Fig. 2

This figure shows the spectra fitting process of the Band, Weibull, and Ellison-Ramaty functions for the April 18, 2014 episode. The top panel shows the Band Function fit, which had a χ² value of 2.02. The middle panel uses the Ellison-Ramaty model to fit the episode and the fit had a χ² value of 0.9839. The bottom panel shows the Weibull function and had a χ² value of 1.214. The Ellison-Ramaty model was chosen to fit this episode.

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