Fig. 10From: The extremely high-energy electron experiment (XEP) onboard the Arase (ERG) satelliteTime and spatial variations of energetic electron fluxes during the 14-day interval after April 1, 2017, for 0.9 MeV (top panel) and 2.5 MeV (second panel) observed by XEP. The Dst index (third panel), solar wind speed (fourth panel) and IMF Bz (bottom panel) are also shownBack to article page