supported by Major Project of Chinese National Programs for Fundamental Research and Development(Grant No.2021YFA0718600);China Space Agency Project(Grant No.D020301);the National Natural Science Foundation of China(Grant No.42011530080);financial support from the Canadian Space Agency and NSERC;partially supported by National Science Foundation(Grant No.AGS-1352669)。
We present evidence of geomagnetic storms in Mercury’s magnetosphere based on MESSENGER magnetic field observations made just before the probe impacted the planet.Our findings answer the question of whether geomagnet...
supported by the National Natural Science Foundation of China (Grant Nos. 41574154 and 41431071)
In this paper, we study the characteristic of large-scale convection electric field in the inner magnetosphere, using magnetospheric multiscale(MMS) observations between L=5 and L=8 over the period from September 1, 2...
supported by the Italian Space Agency in the framework of the“Accordo Attuativo n.2016-16-H0 Progetto Limadou Fase E/Scienza”(CUP F12F1600011005)
CSES(China Seismo-Electromagnetic Satellite) is a mission developed by CNSA(Chinese National Space Administration) and ASI(Italian Space Agency), to investigate the near-Earth electromagnetic, plasma and particle envi...
supported by the National Natural Science Foundation of China(Grant Nos.41374167,41074117&41374166)
The variation of the flux of energetic electrons in the magnetosphere has been proven to be strongly related to the solar wind speed. Observations of GEO orbit show that the flux of low-energy electrons is not only mo...
supported by the National Natural Science Foundation of China (Grant Nos. 40931056, 40874089);the National Basic Research Program of China ("973" Project) (Grant Nos. 2008CB425704)
The energy budget of the magnetosphere-ionosphere (MI) system during 1998-2008 was examined by using Akasofu's epsilon function. The results showed that 1) the yearly average rate of solar wind energy input into the M...
supported by the National Natural Science Foundation of China(Grant No.40704032)
Based on the magnetospheric kinetic theory, a model is developed to specify the flux of energetic electrons in the inner and middle magnetosphere. Under the assumption of adiabatic motion and isotropic particle distri...
supported by the key project of National Natural Science Foundation of China (Grant No. 40831061);the Specialized Research Fund for State Key Laboratories of China
The ultra low frequency (ULF) wave in magnetosphere can act as an important means for solar wind energy inward transmission.This paper quantitatively analyzes the propagation process of the ULF wave triggered by the i...
Supported by the Ministry of Science and Technology of China(Grant No.2006CB806305);the National Natural Science Foundation of China(Grant Nos.40621003,40620130094,40674094and40731054);the Hundred Talents Program of the CAS,and the Specialized Research Fund for State Key Laboratories
By analyzing hot ion and electron parameters together with magnetic field measurements from Cluster, an event of magnetopause crossing of the spacecraft has been investigated. At the latitude of about 40° and magneti...
the National Natural Science Foundation of China (Grant Nos. 40621003, 40728005,40674094, and 40390150);Ministry of Science and Technology of China (Grant No. 2006CB806305);Hundred Talents Program of the CAS
The equatorial and polar satellites of the Double Star Project (DSP) were launched successfully on December 29, 2003 and July 25, 2004, respectively, and both of them are operating smoothly. The DSP provides a good op...
the Ministry of Science and Technology of China (Grant No. 2006CB806305);the National Natural Science Foundation of China (Grant Nos. 40621003, 40674094);the Hundred Talents Program of the CAS
An event of Cluster-Double Star conjunction observations of magnetic reconnec-tion at high latitude magnetopause nightside of both cusps and solar wind trans-port into magnetosphere caused by such reconnection process...