Electron flux oscillations are often observed in electron energy channels in the range of 10 keV to 100 keV. They are observed in the form of flux fluctuations with periods …
JL Chen, H Zou, YX Hao, YG Ye… - Journal of …, 2024 - Wiley Online Library
Abstract The Van Allen Probes mission contributed to the discovery of the relativistic (∼ 500 keV–2 MeV) and ultra‐relativistic (∼> 2 MeV) electron three‐belt structure in Earth's …
In the past two years, many progresses were made in magnetospheric physics by the data of OMNI, SuperMAG networks, Double Star Program, Cluster, THEMIS, RBSP, DMSP …
The interplanetary (IP) shock with the sudden increase of solar wind dynamic pressure can cause the acceleration and transportation of energetic electrons in the inner …
Z Luo, L Xie, S Fu, Z Pu, Y Xiong, X Zhou… - Geophysical …, 2022 - Wiley Online Library
Microinjection phenomena, characterized by dispersive oscillations of electron fluxes at the Pc5 period and bi‐directional pitch angle anisotropy, are frequently observed by …
H Wu, T Chen, V Kalegaev, S Ye - Journal of Geophysical …, 2023 - Wiley Online Library
Electron flux dropout is an extraordinary phenomenon in the outer radiation belt, which is characterized by a drastic depletion in trapped electron populations over a broad range of …