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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Multipoint observations of substorm pre-onset flows and time sequence in the ionosphere and magnetosphere
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Multipoint observations of substorm pre-onset flows and time sequence in the ionosphere and magnetosphere

机译:多点的观察亚暴pre-onset流和电离层和时间序列磁气圈

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In this paper, we use a rare and close longitudinal conjunction of the THEMIS spacecraft with the Sondrestrom radar to present multipoint observations of important features of the time sequence of substorm pre-onset plasma flows in the ionosphere and magnetotail on March 5, 2008. We found that the onset was preceded sequentially by enhanced polar cap flows heading equatorward near the polar cap boundary, and then by tail fast flows from the mid-tail to the near-Earth region. We also observed in situ fluctuations in short-period Pi2 band (~30-50 s) in both the magnetic field and plasma pressure during the initial couple of min of the fast flows, occurring nearly simultaneously with the dipolarization and the fast flows and propagating earthward. Our results suggest that these fluctuations may be triggered by the fast flows, and may play an important role in the substorm onset process. Our event suggests that localized tail reconnection may be triggered by the enhanced polar cap flows, though the reconnection location cannot be unambiguously determined. Earthward fast flows are generated as a result of the tail reconnection and reach the inner magnetosphere to initiate the substorm onset. The presented case is consistent with that predicted by the Nishimura et al. (2010a) scenario.
机译:在本文中,我们使用一个罕见的和关闭纵向THEMIS计划的结合多点Sondrestrom雷达的礼物观测的重要特征序列的亚暴pre-onset等离子体流于2008年3月5日,电离层、磁尾。我们发现按顺序出现以前通过增强的极冠航向朝赤道方向流动附近的极冠边界,然后尾巴快从mid-tail近地流动地区。短周期Pi2乐队(~ 30 - 50 s)的在磁场和等离子体的压力最初几分钟的快速流动,几乎同时发生dipolarization和快速流动和传播向地面。波动可能引发的快速流动,亚暴,可能发挥重要作用发病过程。尾巴重新连接可能引发的增强的极冠流,虽然重新连接位置不能明确确定。向地球的快速流动产生的结果尾巴重新连接,达到内部磁层亚暴开始启动。提出了预测是一致的西村et al。(2010)的场景。

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