New progress of Double Star-Cluster joint exploration and study  

作　　者：LIU ZhenXing PU ZuYin CAO JinBin SHEN Chao LU Li ZHANG LingQian 

机构地区：[1]Center for Space Science and Applied Research,Chinese Academy of Sciences,Beijing 100080,China [2]School of Earth and Space Science,Peking University,Beijing 100080,China

出　　处：《Science China(Technological Sciences)》2008年第10期1565-1579,共15页中国科学（技术科学英文版）

基　　金：the National Natural Science Foundation of China: DSP-Cluster six point coordinated exploration and research (Grant No. 40620130094);Multiple temporal-spatial scale physical processes of geospace storms (Grant No. 40390150);Driven process of multiple space regions and muitiple temporal-spatial-scale of geospace Storms (Grant No. 40390151)

摘　　要：The magnetic reconnection of magnetosphere and the magnetospheric space storms (including magnetospheric substorm, magnetic storm, magnetospheric particle storm) has long been one of the most challenging subjects in the so-lar-terrestrial physics. The reconnection mechanism and global triggering process of the magnetospheric space storms are still unclear up to now. Based on the Double Star Program (DSP) and Cluster joint measurements, we have observed the solar wind density hole, the component magnetic field reconnection in the magnetopause, the structures of magnetic storm ring current, global and multi-scale driven and triggering processes of magnetospheric substorm. In this paper we will briefly introduce these results.The magnetic reconnection of magnetosphere and the magnetospheric space storms (including magnetospheric substorm, magnetic storm, magnetospheric particle storm) has long been one of the most challenging subjects in the solar-terrestrial physics. The reconnection mechanism and global triggering process of the magnetospheric space storms are still unclear up to now. Based on the Double Star Program (DSP) and Cluster joint measurements, we have observed the solar wind density hole, the component magnetic field reconnection in the magnetopause, the structures of magnetic storm ring current, global and multi-scale driven and triggering processes of magnetospheric substorm. In this paper we will briefly introduce these results.

关 键 词：solar WIND MAGNETIC RECONNECTION magnetospheric SUBSTORM MAGNETIC STORM 

分 类 号：P353[天文地球—空间物理学]