Almost 40 years ago the concept of the substorm current wedge was developed to explain
the magnetic signatures observed on the ground and in geosynchronous orbit during …

In this paper, the particle acceleration processes around magnetotail dipolarization fronts
(DFs) were reviewed. We summarize the spacecraft observations (including Cluster …

Dipolarization front (DF)—a sharp boundary with scale of ion inertial length (c/ωpi) in the
Earth's magnetotail—can also have fine structures at electron scale (c/ωpe). Such electron …

We review the range of applications and use of the curlometer, initially developed to analyze
Cluster multi‐spacecraft magnetic field data; but more recently adapted to other arrays of …

Using MMS high‐resolution measurements, we present the first observation of fast electron
jet (V e~ 2,000 km/s) at a dipolarization front (DF) in the magnetotail plasma sheet. This jet …

Using the high‐resolution measurements from magnetospheric multiscale mission, here we
present the observational evidence of kinetic interchange instabilities (ICIs) at dipolarization …

Dipolarization fronts (DFs) are believed to play important roles in transferring plasmas,
magnetic fluxes, and energies in the magnetotail. Using the Cluster observations in 2003 …

Understanding how a substorm current wedge (SCW) is formed is crucial to comprehending
the substorm phenomenon. One SCW formation scenario suggests that the substorm time …

Meso-scale auroral forms, such as poleward boundary intensifications, streamers, omega
bands, beads and giant undulations, are manifestations of dynamic processes in the …

We perform a statistical study of flux ropes and reconnection fronts based on MErcury
Surface, Space ENviroment, GEochemistry, and Ranging (MESSENGER) magnetic field and …