One of the most important issues in space physics is to identify the dominant processes that
transfer energy from the solar wind to energetic particle populations in Earth's inner …

Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

Abstract Pc5 (2–7 mHz) ultralow frequency (ULF) waves play a significant role in resonating
with particles and transferring energy in the coupled magnetospheric and ionospheric …

We report the in situ observation of a plasma vortex induced by a solar wind dynamic
pressure enhancement in the nightside plasma sheet using multipoint measurements from …

Solar wind‐magnetosphere coupling is a key link of the space weather chain. There have
been increasing reports of solar wind dynamic pressure pulses influencing the whistler …

The magnetosphere is the outermost layer of the geospace, and the interaction of the solar
wind with the magnetosphere is the key element of the space weather cause-and-effect …

Plasmaspheric hiss is one of the important plasma waves controlling radiation belt
dynamics. Its spatiotemporal distribution and generation mechanism are presently the object …

Using multipoint data from three Time History of Events and Macroscale Interactions during
Substorms (THEMIS) satellites, we report a magnetospheric flow vortex driven by a negative …

This paper studied statistically the joint responses of magnetic field and relativistic (> 0.5
MeV) electrons at geosynchronous orbit to 201 interplanetary perturbations during 6 years …

In response to interplanetary (IP) shocks, magnetic field may decrease/increase
(negative/positive response) in nightside magnetosphere, while at high latitudes on the …