地球磁尾中强烈能量转换事件的观测

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-04-23 DOI:10.1029/2024JA033416
Y. T. Tang, S. Y. Huang, Z. G. Yuan, K. Jiang, Z. Wang, Q. Y. Xiong, R. T. Lin, L. Yu, H. Bai
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引用次数: 0

摘要

利用磁层多尺度任务的高分辨率数据,我们对地球磁尾中的强烈能量转换事件(IECEs)进行了统计分析。结果表明,离子激振效应的平均持续时间为0.14 s, 95%以上的离子激振效应的空间尺度小于一个离子惯性长度。强烈的能量转换事件不仅发生在等离子体片的磁链、磁孔、双极化锋和磁重联区,而且发生在等离子体片边界层。强烈的能量转换事件倾向于发生在黄昏面和北半球,表现出明显的黎明-黄昏不对称。当行星际磁场呈准南向时,IECEs的发生率要高得多。我们的研究结果可以加深我们对行星磁尾的能量转换和动力学过程的理解。
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Observations of Intense Energy Conversion Events in the Earth's Magnetotail

Using the high-resolution data from the Magnetospheric Multiscale mission, we performed a statistical analysis on intense energy conversion events (IECEs) in the Earth's magnetotail. The results show that the average duration of IECEs is 0.14 s, and the spatial scale of more than 95% of IECEs is smaller than one ion inertial length. Intense energy conversion events can occur not only in flux ropes, magnetic holes, dipolarization fronts and magnetic reconnection region in the plasma sheet, but also in the plasma sheet boundary layer. Intense energy conversion events prefer to occur in the duskside and the northern hemisphere, showing obvious dawn-dusk asymmetry. The occurrence rate of IECEs is much higher when the interplanetary magnetic field is quasi-southward. Our results can deepen our understanding of energy conversion and dynamic processes in the planetary magnetotail.

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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
期刊最新文献
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