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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Structure and dynamics of the nightside poleward boundary: Sounding rocket and ground-based observations of auroral electron precipitation in a rayed curtain
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Structure and dynamics of the nightside poleward boundary: Sounding rocket and ground-based observations of auroral electron precipitation in a rayed curtain

机译:夜间极地边界的结构和动力学:探测窗帘中极光电子沉淀的探空火箭和地面观测

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摘要

The Cascades2 auroral sounding rocket provides a case study for comparing multipoint in situ ionospheric observations of a nightside auroral poleward boundary intensification with ground-based optical observations of the same event. Cascades2 was launched northward from Poker Flat Alaska on 20 March 2009 at 11:04 UT. The 13 min flight reached an apogee of 564 km over the northern coast of Alaska. The experiment included a five-payload array of in situ instrumentation, ground cameras at three different points under the trajectory, multiple ground magnetometers, the Poker Flat Incoherent Scatter Radar (PFISR) radar, and the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft in the magnetotail. The rays of the poleward boundary intensification (PBI) curtain have along-arc motions of 8.5 km/s and along-arc spacings of 16 km. Modulated maximum energy envelopes and energy fluxes of the associated electron precipitation correspond to this spatial structure of the visible rays. The electron precipitation is additionally modulated at a higher frequency, and velocity dispersion analysis of these 8 Hz signatures implies Alfvénic wave-particle acceleration of an ambient ionospheric electron source occurring a few hundred km above the observation point. These observations parameterize the curtain of Alfvénic activity above the PBI event, both in the dispersive ionosphere and in the magnetotail reconnection region. The along-arc variations in brightness correspond to variations in precipitating electron energy flux interpreted as an along-arc modulation of the maximum energy of the Alfvénic wave-particle acceleration process; this is a new interpretation of the formation of rayed structures in auroral curtains. We consider the various possible magnetospheric and ionospheric drivers for the control of the observed along-arc structuring and motions.
机译:Cascades2极光探测火箭提供了一个案例研究,用于将夜间极光极向边界强化的多点原位电离层观测与同一事件的地面光学观测进行比较。 Cascades2于2009年3月20日(美国时间)UT从阿拉斯加扑克之星向北推出。 13分钟的飞行达到了阿拉斯加北部海岸564公里的最高点。实验包括五个有效载荷的现场仪器阵列,在轨迹下三个不同点的地面摄像头,多个地面磁力计,扑克平面非相干散射雷达(PFISR)雷达以及亚暴期间事件的时间历史和宏观尺度的相互作用( THEMIS)太空船在磁尾中。极向边界增强(PBI)幕帘的射线具有8.5 km / s的沿弧运动和16 km的沿弧间距。相关电子沉淀的调制最大能量包络线和能量通量与可见光的这种空间结构相对应。另外,还以更高的频率调制电子沉淀,并且对这8 Hz信号的速度色散分析表明,周围电离层电子源的Alfvénic波粒加速度发生在观测点上方几百公里处。这些观察参数化了在分散电离层和磁尾重连区域中,PBI事件上方的Alfvénic活动的帷幕。亮度沿电弧的变化对应于析出的电子能通量的变化,这被解释为阿尔夫涅克波粒子加速过程的最大能量的沿电弧调制。这是对极光幕帘中射线结构形成的新解释。我们考虑使用各种可能的磁层和电离层驱动器来控制观测到的弧线构造和运动。

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