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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Link between premidnight second harmonic poloidal waves and auroral undulations: Conjugate observations with a Van Allen Probe spacecraft and a THEMIS all-sky imager
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Link between premidnight second harmonic poloidal waves and auroral undulations: Conjugate observations with a Van Allen Probe spacecraft and a THEMIS all-sky imager

机译:午夜二次谐波极谱波与极光波动之间的联系:使用Van Allen Probe航天器和THEMIS全天空成像仪将观测结果共轭

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We report, for the first time, an auroral undulation event on 1 May 2013 observed by the Time History of Events and Macroscale Interactions During Substorms (THEMIS) all-sky imager (ASI) at Athabasca (L = 4.6), Canada, for which in situ field and particle measurements in the conjugate magnetosphere were available from a Van Allen Probe spacecraft. The ASI observed a train of auroral undulation structures emerging spontaneously in the premidnight subauroral ionosphere during the growth phase of a substorm. The undulations had an azimuthal wavelength of ~180km and propagated westward at a speed of 3–4kms~(-1). The successive passage over an observing point yielded quasiperiodic oscillations in diffuse auroral emissions with a period of ~40 s. The azimuthal wave number m of the auroral luminosity oscillations was found to be m~-103. During the event, the spacecraft-being on tailward stretched field lines ~0.5 R_E outside the plasmapause that mapped into the ionosphere conjugate to the auroral undulations-encountered intense poloidal ULF oscillations in the magnetic and electric fields. We identify the field oscillations to be the second harmonic mode along the magnetic field line through comparisons of the observed wave properties with theoretical predictions. The field oscillations were accompanied by oscillations in proton and electron fluxes. Most interestingly, both field and particle oscillations at the spacecraft had one-to-one association with the auroral luminosity oscillations around its footprint. Our findings strongly suggest that this auroral undulation event is closely linked to the generation of second harmonic poloidal waves.
机译:我们首次报告了加拿大阿萨巴斯卡(L = 4.6)的亚暴期间事件和宏观相互作用的时间历史(THEMIS)全天候成像仪(ASI)观测到的2013年5月1日的一次极光起伏事件,为此共轭磁层中的原位场和粒子测量可从Van Allen Probe航天器获得。 ASI观测到在次暴雨的生长阶段,在午夜前的电离层中自发出现了一系列极光起伏结构。起伏的方位角波长约为180km,并以3-4kms〜(-1)的速度向西传播。连续经过一个观测点会产生约40 s的弥散极光发射中的准周期性振荡。发现极光光度振荡的方位波数m为-103。在活动期间,航天器位于等离子暂停之外的向后拉伸的磁力线上〜0.5 R_E,该等离子暂停映射到电离层中,与极光起伏共轭,在磁场和电场中遇到了强烈的极向性ULF振荡。通过将观测到的波特性与理论预测值进行比较,我们将磁场振荡确定为沿磁场线的二次谐波模式。场振荡伴随着质子和电子通量的振荡。最有趣的是,航天器的场振荡和粒子振荡都与其足迹周围的极光亮度振荡一一对应。我们的发现强烈表明,这种极光起伏事件与二次谐波极向波的产生紧密相关。

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