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 …

Abstract We use Open Geospace General Circulation Model global MHD simulations to
study the nightside magnetospheric, magnetotail, and ionospheric responses to …

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 …

The propagation of perturbation caused by the interplanetary shock wave of March 17, 2015
from the solar wind through the magnetosheath, magnetosphere, and ionosphere down to …

We present high‐latitude field‐aligned current (FAC) response to nearly frontal shocks
(NFSs) and highly inclined shocks (HISs) through a superposed epoch analysis. The FACs …

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 …

The magnetic local time and latitude dependence of amplitude of the main impulse (MI) of
geomagnetic sudden commencements (SCs) and its seasonal variation have been …

磁层位于地球空间的最外层, 太阳风与磁层的相互作用是空间天气变化因果链中承上启下的关键
环节, 是揭示地球空间天气基本规律的关键科学课题. 地球空间由于时变, 多成分 …

The near‐Earth space environment is greatly affected by transient perturbations in the solar
wind. One of the most obvious and important perturbations are solar wind dynamic pressure …