Fig. 10From: Dynamics of the terrestrial radiation belts: a review of recent results during the VarSITI (Variability of the Sun and Its Terrestrial Impact) era, 2014–2018Radiation belt response during geomagnetic storms of similar strength. The net flux of energetic electrons may increase, decrease, or stay the same between the main and recovery phase illustrating the important dynamic between energization and loss. Figure is reproduced from Reeves et al. (2013)Back to article page