重联流出中电子涡的观测与重建

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-01-11 DOI:10.1029/2024JA033473
J. Q. Niu, Z. Wang, H. S. Fu, J. B. Cao, W. D. Fu
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引用次数: 0

摘要

2017年1月27日,在地球磁层顶重联流出中,磁层多尺度观测到由电子K-H不稳定性驱动的一系列电子涡。我们发现涡旋内部的电子涡度可以达到200 s−1以上,这与电子扩散区的强涡度事件相当。利用速度场的一阶泰勒展开法,进一步重建了两个电子涡旋的三维拓扑结构,发现一个涡旋是收敛的,另一个涡旋是发散的。有趣的是,在发散涡旋中观察到电子温度的升高,而在收敛涡旋中没有,这表明电子动力学与涡旋拓扑有关。我们的研究表明,在重联流出中由强烈的电子剪切流形成的电子K-H涡具有不同的拓扑类型,这将有助于我们更好地理解地球磁层顶重联的图景。
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Observation and Reconstruction of Electron Vortex in Reconnection Outflow

On 27 January 2017, Magnetospheric Multi-Scale observed a series of electron vortexes, which are driven by the electron Kelvin-Helmholtz (K-H) instability in the reconnection outflow at terrestrial magnetopause. We find the electron vorticity can reach above 200 s−1 inside the vortexes, which is comparable to the strong vorticity events in the electron diffusion region. Using the First-Order Taylor Expansion for Velocity field method, we further reconstruct the 3D topology of two electron vortexes and find one vortex is converging while another vortex is diverging. Interestingly, enhancement of electron temperature was observed in the diverging vortex but not in the converging vortex, indicating electron dynamics is related to the vortex topology. Our study suggests that electron K-H vortexes formed by the intense electron shear flow in the reconnection outflow have different types of topologies and will help us better understand the reconnection picture at the terrestrial magnetopause.

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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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