supported by the National Natural Science Foundation ofChina (Grant No. 40831061);the National Key Laboratory Special Fund and the Open Research Foundation of Science and Technology on Aerospace Flight Dynamics Laboratory (Grant No. 2012afd1034)
Based on the magnetic field and plasma data obtained by GEOTAIL in 1992-1995 and WIND in1994-2009, the magnetic field and plasma properties in the magnetotail near lunar orbit were studied statistically using the supe...
supported by the National Natural Science Foundation of China (40831061 and 41074117);the Specialized Research Fund for State Key Laboratories
Energetic electrons and ions in the Van Allen radiation belt are the number one space weather threat. Understanding how these energetic particles are accelerated within the Van Allen radiation belt is one of the major...
supported by the Key Project of the National Natural Science Foundation of China (Grant No 40831061)
The Dst index,designed as a proxy of ring current intensity,is known to be also affected by other magnetospheric current systems,e.g.magnetopause current.The pressure-corrected Dst index is obtained by removing the ef...
supported by the KIP Pilot Project of the Chinese Academy of Scineces(KZCX2-YW-123);the National Natural Science Foundation of China (41004072,41031065,41074106,41074117,40974090,40874088 and 40831061);the National Basic Research Program of China(2011CB811405)
It is believed that a southward interplanetary magnetic field (IMF) is mainly responsible for the energy input from solar wind into the magnetosphere.This paper presents an unusual case of strong anti-sunward plasma f...
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 National Natural Science Foundation of China (Grant Nos. 40874076, 40774079, 40925014, 40774078, 40831061);Special Fund for Public Welfare Industry (Meteorology) (Grant No. GYHY200806024);the Construct Program of the Key Discipline in Changsha University of Science and Technology,and the Specialized Research Fund for State Key Laboratories for Space Weather
Interactions between very/extremely low frequency (VLF/ELF) waves and energetic electrons play a fundamental role in dynamics occurring in the inner magnetosphere. Here, we briefly discuss global properties of VLF/ELF...
Supported by the National Natural Science Foundation of China(Grant No.40831061)
One of the most fundamental important issues in the space physics is to understand how solar wind energy transports into the inner magnetosphere.Ultra low frequency(ULF)wave in the magnetosphere and its impact on ener...
Supported by the National Natural Science Foundation of China (Grant No. 40831061)
Interplanetary shock can greatly disturb the Earth's magnetosphere and ionosphere, causing the temporal and spatial changes of the magnetic field and plasmas at the geosynchronous orbit. In this paper, we use the magn...
Supported by the National Natural Science Foundation of China (Grant No. 40831061)
The sources of ultra low frequency (ULF) waves in the magnetosphere are generally believed to be either the external solar wind perturbations or the internal plasma instabilities. When a sudden impulse of the solar wi...