Multi-spacecraft observations of the decay phase of solar energetic particle events

Open Access

Fig. 11.

Decay-time constant against $I_{p, 25}^{\max}$ $I_{p,25}^{\mathrm{max}}$ , the maximum proton ∼ 25 MeV SEP peak flux over all spacecraft within |Δϕ|< 35°. The correlation coefficient for τ vs the logarithm of $I_{p, 25}^{\max}$ $I_{p,25}^{\mathrm{max}}$ is CC = 0.62, with a p value = 0.03.

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