supported by National Natural Science Foundation of China (Grant Nos.40931054, 40704028 and 40523006);National Basic Research Program of China (Grant No.2006CB8062305);Specialized Research Fund for State Key Laboratories
We here study the occurrence rate,probability function of velocity and duration of earthward bursty bulk flows(BBFs) in the Inner Plasma Sheet(IPS,β>0.5) using the data of Cluster in 2001 and 2002.The occurrence r...
Supported by the National Natural Science Foundation of China (Grant No. 40874077, 40621003, 40874091, 40536029, 40523006 and 40604019);the National Basic Research Program of China ("973" Project) (Grant No. 2006CB806304);the Specialized Research Fund for State Key Laboratorie
An asynchronous and parallel time-marching method for three-dimensional (3D) time-dependent magnetohydrodynamic (MHD) simulation is used for large-scale solar wind simulation. It uses different local time steps in the...
Supported by the National Natural Science Foundation of China (Grant Nos. 40621003, 40804046, 40536029, 40674084 and 40523006);the National Basic Re-search Program of China ("973" Project) (Grant No. 4902006CB806304);the Spe-cialized Research Fund for State Key Laboratories;the Open Research Program of the State Key Laboratory of Space Weather, Chinese Academy of Sciences
In this paper,we report two MC events observed by WIND spacecraft with good examples of fieldaligned residual flow inside the MC structure. For both events,the co-moving frames are determined through the deHoffman-Tel...
the National Natural Science Foundation of China(40390153,40523006);973 Program(2006CB806305)
The brief report presents a part of the research results of the magnetospheric physics researches in China during the period of 2006—2008.During the past two years,China-ESA co-operation DSP(Double Star Program) sate...
the National Natural Science Foundation of China (Grant Nos. 40536029, 40621003, 40504020 and 40523006);the National Basic Research Program of China ("973") (Grant No. 2006CB806304);the CAS International Partnership Program for Creative Research Teams
We present the solar-terrestrial transit process of three successive coronal mass ejections (CMEs) of November 4―5, 1998 originating from active region 8375 by using a time-dependent three-dimensional magnetohydrodyn...
the National Natural Science Foundation of China (Grant Nos. 40621003, 40523006, 40704028, 40604018);973 Program of China (Grant No. 2006CB806305);the Specialized Research Fund for State Key Laboratories of China.
Using the data of LFEW/TC-2, we studied the dawn side chorus around substorm onsets during a strong geomagnetic storm in November 2004. During this storm, LFEW/TC-2 observed 14 dawnside chorus events. Nine of them wer...
the National Natural Science Foundation of China (Grant Nos. 40604018, 40523006);CSSAR (Grant No. O72114AA4S);Scientific Research Start-up Foundation for President Prize of CAS, 973 Program of China (Grant No. 2006CB806305);the Specialized Research Fund for State Key Laboratories
During the interval 06:14―07:30 UT on August 24, 2005, since the Earth’s magneto- pause was suddenly compressed by the persistent high-speed solar wind stream with the southward component of the interplanetary magne...
the National Natural Science Foundation of China (40390150,40523006);973 Program 2006CB806305
This paper presents the status of two satellites of Double Star Program,and a part of scientific results based on the data of Double Star Program obtained during the period of 2006-2008.Other scientific results in the...