Using the total radiation belt electron content calculated from Van Allen Probe phase space
density, the time‐dependent and global response of the outer radiation belt during storms is …

A statistical analysis on the radiation belt dropouts is performed based on 4 years of electron
phase space density data from the Van Allen Probes. The μ, K, and L* dependence of …

Abstract We use Van Allen Probes data to investigate the responses of tens of keV to 2 MeV
electrons throughout a broad range of the radiation belts (2.5≤ L≤ 6.0) during 52 …

We study the effect of interplanetary coronal mass ejection (ICME)‐driven sheath regions on
relativistic outer radiation belt electron fluxes. We employ superposed epoch analysis, and …

Determining preferential solar wind conditions leading to efficient radiation belt electron
acceleration is crucial for predicting radiation belt electron dynamics. Using Van Allen …

Using 5‐year of measurements from Van Allen Probes, we present a survey of the statistical
dependence of the Earth's outer radiation belt electron flux dropouts during geomagnetic …

Superposed epoch analyses were performed on 193 significant relativistic electron flux
dropout events, in order to study the roles of different solar wind parameters in driving the …

Dropout events are dramatic decreases in radiation belt electron populations that can occur
in as little as 30 minutes. Loss to magnetopause due to a combination of magnetopause …

Dropouts in electron fluxes at L∼ 4.2 were investigated for a broad range of energies from
120 keV to 10 MeV, using 16 years of electron flux data from Combined X‐ray Dosimeter on …

The outer radiation belt consists of relativistic (> 0.5 MeV) electrons trapped on closed
trajectories around Earth where the magnetic field is nearly dipolar. During increased …