The effects of magnetospheric processes on relativistic electron dynamics in the Earth's outer radiation belt

Using the electron phase space density (PSD) data measured by Van Allen Probe A from January 2013 to April 2015, we investigate the effects of magnetospheric processes on relativistic electron dynamics in the Earth's outer radiation belt during 50 geomagnetic storms. A statistical study shows that the maximum electron PSDs for various μ(μ =630, 1096, 2290, and 3311 MeV/G) at L*~4.0 after the storm peak have good correlations with storm intensity (cc~0.70). This suggests that the occurrence and magnitude of geomagnetic storms are necessary for relativistic electron enhancements at the inner edge of the outer radiation belt (L* =4.0). For moderate or weak storm events (SYM‐Hmin> ~−100 nT) with weak substorm activity (AEmax< 800 nT) and strong storm events (SYM‐Hmin≤ ~−100 nT) with intense substorms (AEmax≥ 800 nT) during the recovery phase, the maximum electron PSDs for various μat different L*values (L* =4.0, 4.5, and 5.0) are well correlated with storm intensity (cc >0.77). For storm events with intense substorms after the storm peak, relativistic electron enhancements at L* =4.5 and 5.0 are observed. This shows that intense substorms during the storm recovery phase are crucial to relativistic electron enhancements in the heart of the outer radiation belt. Our statistics study suggests that magnetospheric processes during geomagnetic storms have a significant effect on relativistic electron dynamics. The occurrence and magnitude of geomagnetic storms are necessary for relativistic electron enhancements at the inner edge of the outer radiation beltIntense substorms after the storm peak are crucial to relativistic electron enhancements in the heart of the outer radiation beltMagnetospheric processes during geomagnetic storms have a significant effect on relativistic electron dynamics