This review describes the infrastructure and capabilities of the expanded and upgraded
Canadian Array for Realtime InvestigationS of Magnetic Activity (CARISMA) magnetometer …

We study electron behavior in the outer radiation belts during the 16 July 2017 storm sudden
commencement (SSC), in which prompt intensification of ultrarelativistic electron fluxes was …

In this paper, in terms of an axisymmetric model of the magnetosphere, we formulate the
criteria for which the Alfvén waves in the magnetosphere can be toroidally and poloidally …

Poloidal ultralow frequency (ULF) waves between 5 and 10 mHz were observed by multiple
satellites and three high‐latitude Super Dual Auroral Radar Network radars during the …

Abstract The Van Allen Probes spacecraft have provided detailed observations of the
energetic particles and fields environment for coronal mass ejection (CME)‐shock‐driven …

A compressional Pc5 wave associated with localized hot proton injection was observed by
the five THEMIS (Time History of Events and Macroscale Interactions during Substorms) …

■ Abstract Electromagnetic ion cyclotron (EMIC) waves are believed to be important for
influencing the dynamics of energetic particles in the inner magnetosphere, especially in …

Geomagnetic storms are frequently associated with the formation of multiple bands of
energetic electrons inside the inner radiation belt at L= 1.1–1.9 and with prominent energy …

The substorm process releases large amounts of energy into the magnetospheric system,
although where the energy is transferred to and how it is partitioned remains an open …

In this paper we examine the hypothesis that MeV energy radiation belt electrons can be
energized by ULF waves, the ULF waves themselves being excited by drift‐bounce …