TAIL RECONNECTION AND PLASMA SHEET FAST FLOWS

机译：尾部重新连接和等离子板快速流动

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The present state of understanding the process of tail reconnectionrnand plasma sheet fast flows obtained fromrnCluster measurements is reviewed. Being a constellationrnof four identical spacecraft, Cluster allows discriminationrnof spatial and temporal variations in magnetic field andrnplasma parameters. Thus it is ideal to study the structurernand dynamics of plasma and fields relevant to reconnection,rnwhich is a highly dynamic system. Observations ofrncurrent sheet crossings near the X-line obtained the geometryrnof reconnection region and confirmed the effectsrnof unmagnetized ions including the Hall-current and itsrnclosure currents. Cluster multi-point observations identifiedrnthree dimensional structures and dynamics of thernfast flows in the plasma sheet, which could be ascribed tornthe localized and/or temporal features of the reconnectionrnregion.

机译：综述了从群测量获得的了解尾部重新连接和血浆片快速流动过程的当前状态。作为星座的四个相同的航天器，星团允许辨别磁场和等离子体参数的时空变化。因此，理想的是研究等离子体的结构和动力学以及与重连接有关的场，这是一个高度动态的系统。观察X线附近的电流片交叉，获得了几何重新连接区域，并确认了未磁化离子的影响，包括霍尔电流及其闭合电流。集群多点观测确定了等离子体片中快速流动的三维结构和动力学，这可以归因于重新连接区域的局部和/或时间特征。

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来源
《Cluster and double star symposium》|2005年|1-6|共6页
会议地点 Noordwijk(NL);Noordwijk(NL)
作者
Rumi Nakamura; Wolfgang Baumjohann; Andrei Runov; Yoshihiro Asano;
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作者单位

Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, A–8042 Graz, Austria,rnEmail: rumi.nakamura@oeaw.ac.at;

Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, A–8042 Graz, Austria;

Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, A–8042 Graz, Austria;

Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, A–8042 Graz, Austria;

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会议组织
原文格式 PDF
正文语种 eng
中图分类
关键词
Cluster; reconnection; magnetosphere; rnplasma sheet;

机译：簇;重新连接；磁层;质膜;

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专利

1. Numerical studies on three-dimensional earthward fast plasma flows in the near-Earth plasma sheet by the spontaneous fast reconnection model [J] . K. Kondoh, M. Ugai Journal of Geophysical Research, A. Space Physics: JGR . 2008,第a3期

机译：自发快速重连接模型对近地等离子体片中三维向地快速等离子体流动的数值研究
2. Tail reconnection region versus auroral activity inferred from conjugate ARTEMIS plasma sheet flow and auroral observations [J] . Nishimura Y., Lyons L.R., Xing X., Journal of Geophysical Research, A. Space Physics: JGR . 2013,第9期

机译：从共轭ARTEMIS血浆片流和极光观测结果推断，尾巴重新连接区与极光活动的关系
3. Tail reconnection region versus auroral activity inferred from conjugate ARTEMIS plasma sheet flow and auroral observations [J] . Nishimura Y., Lyons L.R., Xing X., Journal of Geophysical Research, A. Space Physics: JGR . 2013,第9期

机译：从共轭ARTEMIS血浆片流和极光观测结果推断，尾巴重新连接区与极光活动的关系
4. TAIL RECONNECTION AND PLASMA SHEET FAST FLOWS [C] . Rumi Nakamura, Wolfgang Baumjohann, Andrei Runov, Cluster and Double Star Symposium . 2005

机译：尾部重新连接和等离子板快速流动
5. Anisotropic equilibrium and ballooning mode analysis in the tail plasma sheet. [D] . Lee, Dae-Young. 1993

机译：尾等离子体板的各向异性平衡和膨胀模式分析。
6. THEMIS two‐point measurements of the cross‐tail current density: A thick bifurcated current sheet in the near‐Earth plasma sheet [O] . Miho Saito -1

机译：THEMIS交叉尾电流密度的两点测量：近地等离子体板中的厚分叉电流板
7. MHD study of three-dimensional spontaneous fast magnetic reconnection for cross-tail plasma inflows in magnetotail [O] . 2016

机译：磁尾中横尾等离子流入的三维自发快速磁重连接的MHD研究
8. Nonlinear m = 1 mode and fast reconnection in collisional plasmas [R] . Aydemir, A. Y. 1997

机译：非线性m = 1模式和碰撞等离子体中的快速重新连接

TAIL RECONNECTION AND PLASMA SHEET FAST FLOWS

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