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Progress in Earth and Planetary Science
Fig. 11 | Progress in Earth and Planetary Science

Fig. 11

From: A review of the SCOSTEP’s 5-year scientific program VarSITI—Variability of the Sun and Its Terrestrial Impact

Fig. 11

A multi-energy view of flux as a function of L shell (distance from the Earth in unit of Earth radius) and time from the Van Allen Probes mission for 2013. a–d Background-corrected electron fluxes measured by MagEIS, e electron fluxes measured by HOPE, f solar wind speed, g IMF Bz, and g Dst index. Clear differences can be seen in radiation belt electron behavior at different energies and from event to event (taken from Reeves et al. 2016)

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