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近地磁尾重联中哨声波和Hall磁场的Cluster观测
引用本文:魏新华,周国成,曹晋滨,O.Santolik,H.Reme,N.Cornilleau,Andre Balogh.近地磁尾重联中哨声波和Hall磁场的Cluster观测[J].地球物理学报,2007,50(3):662-671.
作者姓名:魏新华  周国成  曹晋滨  O.Santolik  H.Reme  N.Cornilleau  Andre Balogh
作者单位:1.中国科学院空间科学与应用研究中心空间天气学国家重点实验室,北京 100080 2 中国科学院研究生院,北京 100049 3 Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic 4 Centre d'Etude Spatiale des Rayonnements, 31028, Toulouse, France 5 CETP/UVSQ, Velizy, France 6 The Blachett
基金项目:国家自然科学基金项目(40523006,40574061,40574067),中国科学院国际合作创新团队资助,中国科学院百人计划资助,国家重点基础研究发展计划(2006CB806305)资助
摘    要:在2001~2003年Cluster飞船通过近地磁尾期间,共探测到14次重联事件,在这些事件中同时还观测到等离子体波活动.本文把14次事件分为三大类,其中:第I类包含了8次事件,它们是在等离子体片内先于重联事件观测到波活动,并且还同时观测到Hall磁场.经过分析判断,这类事件中观测到的波是右旋偏振的哨声波.第II类包含了2次事件,这类事件也观测到了Hall磁场和右旋偏振的哨声波.第Ⅲ类也包含了2次事件,这类事件只是普通的重联事件,没有观测到Hall磁场,但是波活动明显先于重联事件.在我们观测的14次事件中,比较强烈的哨声波和Hall 磁场是一一对应的,因此哨声波可能主要是在Hall磁场的四极结构区激发的.

关 键 词:磁尾  无碰撞重联  哨声波  Cluster飞船  Hall磁场  
文章编号:0001-5733(2007)03-0662-10
收稿时间:2006-7-6
修稿时间:2006-07-06

Whistle and Hall magnetic field associated with near-Earth magnetotail reconnection observed by Cluster
WEI Xin-Hua,ZHOU Guo-Cheng,CAO Jin-Bin,O.Santolik,H.Reme,N.Cornilleau,Andre Balogh.Whistle and Hall magnetic field associated with near-Earth magnetotail reconnection observed by Cluster[J].Chinese Journal of Geophysics,2007,50(3):662-671.
Authors:WEI Xin-Hua  ZHOU Guo-Cheng  CAO Jin-Bin  OSantolik  HReme  NCornilleau  Andre Balogh
Institution:1.Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080, China 2 Graduate University of the Chinese Academy of Sciences, Beijing 100049, China 3 Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic 4 Centre d'Etude Spatiale des Rayonnements, 31028, Toulouse, France 5 CETP/UVSQ, Velizy, France 6 The Blachett Laboratory, Imperial College, London, U.K
Abstract:During 2001 - 2003, the Cluster spacecraft passed through the near-Earth magnetotail, and observed 14 magnetotail reconnection events. Simuhaneously, Cluster observed electromagnetic wave associated with reconnection events. There are three kinds of reconnection events in these 14 events. There are 8 events in the first kind of reconnection event, in this kind of reconnection events wave activity were observed prior to the reconnection event and simultaneously Hall magnetic field was observed. The wave activity included right hand polarized Whistler. The second kind of reconnection events had two events. Whistler waves and Hall magnetic field were observed in this kind of events, but the wave activity was not prior to reconnection events. The third kind of events had two events. The Whistler waves and Hall magnetic were not observed in this kind of reconnection event. In these 14 events, the strong Whistler waves corresponded to Hall magnetic field. Whistler waves may mainly be excited in Hall magnetic field regions.
Keywords:Magnetotail  Collisionless reconnection  Whistler wave  Cluster spacecraft  Hall magnetic field
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