Trapping of Whistler Waves in the Magnetic Hole at a Dipolarization Front

IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY
K. Jiang, S. Y. Huang, X. D. Yu, Z. G. Yuan, Q. Y. Xiong, R. T. Lin, L. Yu
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引用次数: 0

Abstract

Dipolarization fronts (DFs) host plentiful dynamics in the magnetotail. Small-scale magnetic structures and waves are frequently found at and around the DFs. Whistler waves are closely related to DFs, and the flux pileup regions (FPRs) behind DFs are thought to be the source regions of the whistler waves around DFs. Statistically, whistler waves are much more frequently observed in FPRs than at DFs. Here, we present an observation of whistler waves in a magnetic hole at a DF. Theoretical calculations show that the observed whistler waves can be trapped in the magnetic hole. Furthermore, theoretical calculations suggest that whistler waves cannot be trapped at a DF if the DF has no sub-structures. Our results indicate the importance of the magnetic structures on the propagation of whistler waves around the DFs and could explain why whistler waves are rarely observed at the DFs.

Abstract Image

双极化前沿(DFs)在磁尾中承载着大量的动态变化。小尺度磁结构和磁波经常出现在 DFs 及其周围。啸叫波与双极化锋密切相关,双极化锋背后的磁通堆积区(FPR)被认为是双极化锋周围啸叫波的源区。据统计,在 FPRs 中观测到的啸叫波比在 DFs 中观测到的啸叫波要频繁得多。在这里,我们展示了在 DF 磁洞中观测到的啸叫波。理论计算表明,观测到的啸叫波可能被困在磁洞中。此外,理论计算还表明,如果 DF 没有子结构,啸叫波就不可能被困在 DF 中。我们的结果表明了磁结构对啸叫波在 DF 周围传播的重要性,也可以解释为什么在 DF 上很少观测到啸叫波。
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来源期刊
Geophysical Research Letters
Geophysical Research Letters 地学-地球科学综合
CiteScore
9.00
自引率
9.60%
发文量
1588
审稿时长
2.2 months
期刊介绍: Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRLmaintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.
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