地球准垂直弓形激波电子动力学熵生成的统计研究

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-01-10 DOI:10.1029/2024JA033049
M. Lindberg, A. Wallner, S. Berglund, A. Vaivads
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摘要

我们利用磁层多尺度任务研究了地球准垂直弓形激波的电子动力学熵。我们对电子熵的变化如何取决于与无碰撞冲击交叉相关的不同等离子体参数进行了统计研究。电子熵的变化与上游电子等离子体β、alfv马赫数和电子热马赫数有很强的相关性。我们通过将激波中电子熵的变化与激波过渡层中不同区域内不同频率间隔测量的电场和磁场波能强度相关联来研究熵产生的来源。在较低混合频率和电子回旋频率之间,观察到激波坡道和激波脚内较高的电场波功率时,电子熵变化更大,这表明静电波对地球准垂直弓形激波的电子动力学熵产生很重要。在本研究中没有考虑到任何最终的交叉冲击电位对电子熵产生的贡献。
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Statistical Study of Electron Kinetic Entropy Generation at Earth's Quasi-Perpendicular Bow Shock

We use the Magnetospheric Multiscale mission to study electron kinetic entropy across Earth's quasi-perpendicular bow shock. We perform a statistical study of how the change in electron entropy depends on the different plasma parameters associated with a collisionless shock crossing. The change in electron entropy exhibits strong correlations with upstream electron plasma beta, Alfvén Mach number, and electron thermal Mach number. We investigate the source of entropy generation by correlating the change in electron entropy across the shock to the measured electric and magnetic field wave power strengths for different frequency intervals within different regions in the shock transition layer. The electron entropy change is observed to be greater for higher electric field wave power within the shock ramp and shock foot for frequencies between the lower hybrid frequency and electron cyclotron frequency, suggesting electrostatic waves are important for electron kinetic entropy generation at Earth's quasi-perpendicular bow shock. Any eventual cross-shock potential contribution to the electron entropy generation has not been considered in this study.

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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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