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 …
Impact angle control of interplanetary shock geoeffectiveness
DM Oliveira, J Raeder - Journal of Geophysical Research …, 2014 - Wiley Online Library
Abstract We use Open Geospace General Circulation Model global MHD simulations to
study the nightside magnetospheric, magnetotail, and ionospheric responses to …
study the nightside magnetospheric, magnetotail, and ionospheric responses to …
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 …
Geomagnetic and ionospheric responses to the interplanetary shock wave of March 17, 2015
VA Pilipenko, M Bravo, NV Romanova… - Izvestiya, Physics of the …, 2018 - Springer
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 …
from the solar wind through the magnetosheath, magnetosphere, and ionosphere down to …
Effects of nearly frontal and highly inclined interplanetary shocks on high‐latitude field‐aligned currents (FACs)
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 …
(NFSs) and highly inclined shocks (HISs) through a superposed epoch analysis. The FACs …
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 …
Magnetic local time and latitude dependence of amplitude of the main impulse (MI) of geomagnetic sudden commencements and its seasonal variation
A Shinbori, Y Tsuji, T Kikuchi, T Araki… - Journal of …, 2012 - Wiley Online Library
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 …
geomagnetic sudden commencements (SCs) and its seasonal variation have been …
太阳风--磁层相互作用的磁流体力学数值模拟研究
王赤 - 空间科学学报, 2011 - cjss.ac.cn
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 …
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 …
Magnetosphere response to solar wind dynamic pressure change: Vortices, ULF waves, and aurorae
QQ Shi, XC Shen, AM Tian… - Dayside …, 2020 - Wiley Online Library
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 …
wind. One of the most obvious and important perturbations are solar wind dynamic pressure …