双极化前沿背后的扩展能量转换和电子加速

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2024-07-11 DOI:10.1029/2024JA032810
X. N. Xing, C. M. Liu, Y. Y. Liu, B. N. Zhao
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引用次数: 0

摘要

地球磁尾的能量转移和传输主要是由嵌入等离子体射流内部的双极化前沿(DFs)驱动的。迄今为止,人们一直认为双极化前沿驱动的能量转移发生在前沿局部。与传统认识不同的是,我们在这里首次观测到了延伸到 DF 后方很远的持续能量转换。持续的能量转换由能量负载主导,主要由电子流贡献,在湍流、衰减的通量堆积区(FPR)内发展,位于 DF 后方近 10 dDF(DF 的厚度)处。能量传递链可能由离子流和环境等离子体之间的相互作用启动,并由电子动力学关闭,从而导致垂直于磁场的电子加速。这些结果突出表明,湍流 FPRs 中的电子物理学在行星磁层的能量传输中起着至关重要的作用。
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Extended Energy Conversion and Electron Acceleration Behind Dipolarization Front

Energy transfer and transport in the terrestrial magnetotails are primarily driven by dipolarization fronts (DFs) embedded inside plasma jets. The DF-driven energy transfer has hitherto been believed to occur locally at the fronts. Different from the traditional knowledge, here we present the first observation of persistent energy conversion extended far behind a DF. The persistent energy conversion, which was dominated by energy loads and mainly contributed by electron currents, developed inside a turbulent, decaying flux pileup region (FPR), nearly 10 dDF (DF’s thickness) behind the DF. The energy transfer chain may be initiated by interaction between the ion flow and ambient plasmas and closed by electron dynamics, leading to electron acceleration perpendicular to magnetic field. These results highlight that electron physics in turbulent FPRs plays a crucial role in the energy transport in the planetary magnetospheres.

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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
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