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首页> 外文期刊>Geophysical Research Letters >MESSENGER observations of magnetospheric substorm activity in Mercury's near magnetotail
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MESSENGER observations of magnetospheric substorm activity in Mercury's near magnetotail

机译:水星附近磁尾的磁层亚暴活动的MESSENGER观测

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MErcury Surface, Space ENviroment, GEochemistry, and Ranging (MESSENGER) magnetic field and plasma measurements taken during crossings of Mercury's magnetotail from 2011 to 2014 have been examined for evidence of substorms. A total of 26 events were found during which an Earth-like growth phase was followed by clear near-tail expansion phase signatures. During the growth phase, just as at Earth, the thinning of the plasma sheet and the increase of the magnetic field intensity in the lobe are observed, but the fractional increase in field intensity could be approximate to 3 to 5 times that at Earth. The average timescale of the growth phase is approximate to 1min. The dipolarization that marks the initiation of the substorm expansion phase is only a few seconds in duration. During the expansion phase, lasting approximate to 1min, the plasma sheet is observed to thicken and engulf the spacecraft. The duration of the substorm observed in this paper is consistent with previous observations of Mercury's Dungey cycle. The reconfiguration of the magnetotail during Mercury's substorm is very similar to that at Earth despite its very compressed timescale.
机译:我们检查了水星的表面,空间环境,地球化学和测距(MESSENGER)磁场和等离子水星在2011年至2014年穿越磁尾的过程中的测量结果,以发现亚暴风雨的迹象。总共发现了26个事件,在此期间,出现了类似地球的生长阶段,之后是明显的近尾膨胀阶段。在生长阶段,与地球一样,可以观察到等离子薄片的变薄和波瓣中磁场强度的增加,但是场强的增加幅度大约是地球的3至5倍。生长阶段的平均时间尺度约为1分钟。标记亚暴扩张阶段开始的双极化持续时间只有几秒钟。在膨胀阶段,持续约1分钟,观察到等离子体片使航天器变厚并吞没了航天器。本文中观察到的亚暴持续时间与先前对水星的“地牢”循环的观察一致。尽管水星压缩了很长时间,但在水星亚暴期间磁尾的重配置与地球的重磁非常相似。

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