Auroral streamers implication for the substorm progression on September 14, 2004

著录项

• 来源
  《Planetary and space science》 |2012年第1期|p.119-124|共6页
• 作者

  X. Cao; Z.Y. Pu; A.M. Du; S. Tian; X.G. Wang; C.J. Xiao; H.U. Frey; M.V. Kubyshkina; V.M. Mishin; S.Y. Fu; L. Xie; Q.G. Zong;

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• 作者单位

  Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China;

  School of Earth and Space Sciences, Peking University, Beijing, China;

  Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China;

  School of Earth and Space Sciences, Peking University, Beijing, China;

  School of Physics, Peking University, Beijing, China;

  School of Physics, Peking University, Beijing, China;

  Space Science Laboratory, University of California, Berkeley, CA, USA;

  Institute of Physics, University of St. Petersburg. Ulyanovskaya, Russia;

  Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Irkusk, Russia;

  School of Earth and Space Sciences, Peking University, Beijing, China;

  School of Earth and Space Sciences, Peking University, Beijing, China;

  School of Earth and Space Sciences, Peking University, Beijing, China;

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• 收录信息
• 原文格式 PDF
• 正文语种 eng
• 中图分类
• 关键词

  substorm; aurora streamer; reconnection;

  机译：亚暴极光流光;重新连接;