ULF Wave-Driven Energization of Plasmaspheric Plume Ions During Multi-Step Geomagnetic Storms

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Yingying Zhao, Hui Zhu, Huicong Chen, Zhijie Qin, Zhenghao She
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Abstract

We report direct observations of the energization of plasmaspheric plume ions by ultralow frequency (ULF) waves during a multi-step geomagnetic storm from 25–29 August 2015. Based on Van Allen Probes observations, we identify multiple plasmaspheric plume regions in the afternoon-dusk sector during the storm, characterized by highly irregular density structures. Concurrently, the cold ( < 100 ${< } 100$ V) ion fluxes exhibit intermittent enhancements within these regions. A detailed analysis reveals that the ion flux variations result from the modulation of the ULF wave-driven E × B $E\times B$ drift. Interestingly, the modulated ion fluxes appear at near 90 ° $90{}^{\circ}$ pitch angles and occur only in high-density plumes; no modulation signatures appear in low-density plasma troughs. These observations strongly support that ULF waves can perpendicularly modulate plasmaspheric plume ions within high-density regions via E × B $E\times B$ effects. The present results provide a deeper understanding of the interactions between ULF waves and plasmaspheric plume ions in the inner magnetosphere.

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多步地磁风暴期间等离子体羽流离子的超低频波驱动能量
我们报告了在2015年8月25日至29日的多步地磁风暴期间,等离子体层羽流离子的超低频(ULF)波的直接观测。根据范艾伦探测器的观测,我们确定了风暴期间下午至黄昏部分的多个等离子体羽流区域,其特征是高度不规则的密度结构。同时,冷(< 100$ {<} 100$ V)离子通量在这些区域内表现出间歇性增强。详细的分析表明,离子通量的变化是由极低频波驱动的E × B$ E\乘以B$漂移调制引起的。有趣的是,调制离子通量出现在90°$90{}^{\circ}$俯角附近,并且只发生在高密度羽流中;在低密度等离子体波谷中没有出现调制特征。这些观测结果有力地支持了极低频波可以通过E × B$ E\ × B$效应垂直调制高密度区域内的等离子体羽流离子。目前的结果提供了对极低频波与内磁层等离子体羽流离子之间相互作用的更深入理解。
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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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