The interaction of ultra-low-frequency pc3-5 waves with charged particles in Earth's magnetosphere
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 …
transfer energy from the solar wind to energetic particle populations in Earth's inner …
Dayside transient phenomena and their impact on the magnetosphere and ionosphere
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 …
transfer events, and surface waves, are frequently observed upstream from the bow shock …
Global propagation of magnetospheric Pc5 ULF waves driven by foreshock transients
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 …
with particles and transferring energy in the coupled magnetospheric and ionospheric …
Solar wind pressure pulse‐driven magnetospheric vortices and their global consequences
QQ Shi, MD Hartinger, V Angelopoulos… - Journal of …, 2014 - Wiley Online Library
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 …
pressure enhancement in the nightside plasma sheet using multipoint measurements from …
Immediate impact of solar wind dynamic pressure pulses on whistler‐mode chorus waves in the inner magnetosphere
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 …
been increasing reports of solar wind dynamic pressure pulses influencing the whistler …
Magnetohydrodynamics (MHD) numerical simulations on the interaction of the solar wind with the magnetosphere: A review
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 …
wind with the magnetosphere is the key element of the space weather cause-and-effect …
Disappearance of plasmaspheric hiss following interplanetary shock
Plasmaspheric hiss is one of the important plasma waves controlling radiation belt
dynamics. Its spatiotemporal distribution and generation mechanism are presently the object …
dynamics. Its spatiotemporal distribution and generation mechanism are presently the object …
Magnetospheric vortices and their global effect after a solar wind dynamic pressure decrease
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 …
Substorms (THEMIS) satellites, we report a magnetospheric flow vortex driven by a negative …
Joint responses of geosynchronous magnetic field and relativistic electrons to external changes in solar wind dynamic pressure and interplanetary magnetic field
LY Li, JB Cao, JY Yang, YX Dong - Journal of Geophysical …, 2013 - Wiley Online Library
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 …
MeV) electrons at geosynchronous orbit to 201 interplanetary perturbations during 6 years …
The chain response of the magnetospheric and ground magnetic field to interplanetary shocks
TR Sun, C Wang, JJ Zhang… - Journal of …, 2015 - Wiley Online Library
In response to interplanetary (IP) shocks, magnetic field may decrease/increase
(negative/positive response) in nightside magnetosphere, while at high latitudes on the …
(negative/positive response) in nightside magnetosphere, while at high latitudes on the …