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Thinning of the Magnetotail Current Sheet Inferred From Low-Altitude Observations of Energetic Electrons

机译:从低空高能电子观测中推断出磁尾电流片的变薄

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The magnetospheric substorm is a key mode of flux and energy transport throughout the magnetosphere associated with distinct and repeatable magnetotail dynamical processes and plasma injections. The substorm growth phase is characterized by current sheet thinning and magnetic field reconfiguration around the equatorial plane. The global characteristics of current sheet thinning are important for understanding of magnetotail state right before the onset of magnetic reconnection and of the key substorm expansion phase. In this paper, we investigate this thinning at different radial distances using plasma sheet (PS) energetic (>50 keV) electrons that reach from the equator to low altitudes during their fast (~1 s) travel along magnetic field lines. We perform a multi-case study and a statistical analysis of 34 events with near-equatorial observations of the current sheet thinning by equatorial missions and concurrent, latitudinal crossings of the ionospheric projection of the magnetotail by the low-altitude Electron Losses and Fields Investigation (ELFIN) CubeSats at approximately the same local time sector. Energetic electron fluxes thus collected by ELFIN provide near-instantaneous (<5 min duration) radial snapshots of magnetotail fluxes. Main findings of this study confirm the previously proposed concepts with low-altitude energetic electron measurements: (a) Energy distributions of low-altitude fluxes are quantitatively close to the near-equatorial distributions, which justifies the investigation of the magnetotail current sheet reconfiguration using low-altitude measurements. (b) The magnetic field reconfiguration during the current sheet thinning (which lasts ≥ an hour) results in a rapid shrinking of the low-altitude projection of the entire PS (from near-Earth, ~10RE, to the lunar orbit ~60RE) to 1–2° of magnetic latitude in the ionosphere. (c) The current sheet dipolarization, common during the substorm onset, is associated with a very quick (~10 min) chang
机译:通量的磁层亚暴是一个关键的模式在磁气圈和能源运输与截然不同的和可重复的磁尾的动力学过程和等离子体注射。特点是电流片变薄周围的磁场重新配置赤道平面。电流片变薄是重要的了解磁尾状态之前磁场重联的发病的关键亚暴扩张阶段。研究这个问题在不同径向变薄距离使用等离子板(PS)精力充沛(> 50凯文)电子从赤道到低海拔在他们快(~ 1 s)沿着磁场线。34事件的研究和统计分析一片观察出现的电流表由赤道任务和稀释并发,纬度的口岸电离层磁尾的投影低空电子损失和字段调查(矮)立方体卫星约当地时间相同的部门。收集的通量因此矮可以几乎瞬时径向(< 5分钟时间)磁尾通量的快照。这项研究证实了以前提出的概念与低空高能电子测量:(a)的能量分布低空通量定量接近的近赤道分布证明了磁尾的调查使用低空电流片重新配置测量。重新配置在当前表变薄(持续≥1小时)导致快速低空投影的萎缩整个PS(从近地,~ 10,月球轨道~ 60 re) 1 - 2°的磁纬度电离层。常见的亚暴发病期间,是相关的常很快(~ 10分钟)

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