Origin of Electron Boomerang Stripes: Statistical Study
编号:175 稿件编号:997 访问权限:仅限参会人 更新:2021-06-14 09:03:50 浏览:750次 口头报告

报告开始:2021年07月10日 18:05 (Asia/Shanghai)

报告时间:15min

所在会议:[S9B] 9B、行星科学与空间物理 » [S9B-1] 9B、行星科学与空间物理-1

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摘要
In the outer radiation belt, localized ultralow frequency (ULF) waves can interact with energetic electrons by drift resonance, leading to quasiperiodic oscillations. The oscillations in the pitch angle spectrum can be characterized by either boomerang‐shaped or straight stripes. Previous studies have shown that boomerang‐shaped stripes evolve from straight ones when electrons drift away from the localized wave interaction region. Based on the time‐of‐flight technique on the pitch angle‐dependent drift velocity, the origin can be remotely identified from the pitch angle dispersion. We report 27 straight stripe events and 86 boomerang‐shaped events observed by Van Allen Probes from January 1, 2013, to December 31, 2017. Statistical study shows a good coincidence between the locations of straight ones and traceback regions from boomerang‐shaped ones. These locations, mainly located in noon‐to‐dusk region, coincide well with the plasmaspheric plumes. Thus, localized ULF waves trapped in the plume may result in the preference of localized ULF wave‐electron interactions at noon‐to‐dusk region.
关键字
Drift Resonace,Localized ULF waves,Boomerang-shaped Stripes
报告人
赵兴鑫
北京大学

稿件作者
赵兴鑫 北京大学
郝以鑫 北京大学
宗秋刚 北京大学
周煦之 北京大学
乐超 北京大学
陈兴燃 北京大学
刘鹰 北京大学空间物理与应用技术研究所
刘志扬 北京大学
BlakeJ.B. Space Science Applications Laboratory , The Aerospace Corporation, E1 Segundo, California, USA.
ClaudepierreS. G. Space Science Applications Laboratory , The Aerospace Corporation, E1 Segundo, California, USA.
ReevesG. D. Los Alamos National Laboratory, Los Alamos, New Mexico, USA
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