Properties of EMIC Waves and EMIC Wave-Driven Electron Precipitation in Subauroral Latitudes Observed at Athabasca, Canada

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Asuka Hirai, Fuminori Tsuchiya, Takahiro Obara, Yoshizumi Miyoshi, Yuto Katoh, Yasumasa Kasaba, Kazuo Shiokawa, Atsushi Kumamoto, Yoshiya Kasahara, Shoya Matsuda, Hiroaki Misawa, Satoshi Kurita, Chae-Woo Jun, Hiroyo Ohya, Martin G. Connors
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Abstract

Electromagnetic ion cyclotron (EMIC) waves are believed to cause the loss of relativistic electrons from the outer radiation belt into the atmosphere due to pitch angle scattering. However, it is still unclear whether all EMIC waves can scatter relativistic electrons or which conditions are favorable for pitch angle scattering by EMIC waves. In this study, we performed a 2-year data analysis of EMIC waves and EMIC wave-driven electron precipitation (EP), from 1 November 2016–31 October 2018. Electromagnetic ion cyclotron waves were observed using a ground-based magnetometer installed at Athabasca (ATH, L = $L=$ 4.3), Canada. Electron precipitation events were identified from very low-frequency radio waves propagated from the transmitters at North Dakota (NDK, L = $L=$ 3.0) and Seattle (NLK, L = $L=$ 2.9) stations in USA to the receiver installed at ATH. The magnetic local time dependence of EMIC waves showed higher occurrence rates in the dawn sector. In contrast, EMIC waves accompanied by EP were localized in the dusk sector and were likely to occur during geomagnetic substorms. We found that EMIC waves accompanied by EP were associated with the main phase of geomagnetic storms and occurred inside the plasmapause. These results suggest that the EMIC waves that cause EP occur in the overlap region between the ring current and dense cold plasma during the main phase of geomagnetic storms. This is consistent with previous studies describing that the electron resonant energy with EMIC waves is lower in regions with high plasma density.

Abstract Image

在加拿大阿萨巴斯卡观测到的亚极光纬度中主波和主波驱动的电子降水的特性
电磁离子回旋波(EMIC)被认为是由于俯仰角散射导致相对论性电子从外层辐射带损失到大气中的原因。然而,是否所有的位波都能散射相对论性电子,以及哪些条件有利于位波的俯仰角散射,目前还不清楚。在这项研究中,我们从2016年11月1日至2018年10月31日对EMIC波和EMIC波驱动的电子沉淀(EP)进行了为期两年的数据分析。电磁离子回旋波采用安装在加拿大阿萨巴斯卡(Athabasca, L=$ L=$ 4.3)的地基磁强计进行观测。电子沉淀事件是从美国北达科他州(NDK, L=$ L=$ 3.0)和西雅图(NLK, L=$ L=$ 2.9)站发射机传播到ATH接收器的极低频无线电波中识别出来的。始位波的磁地方时依赖性在黎明扇区表现出较高的发生率。而伴随EP的地源波则局限于黄昏区,可能发生在地磁亚暴期间。我们发现伴随EP的地磁波与地磁风暴的主相有关,并发生在等离子层顶内部。这些结果表明,在地磁暴的主阶段,引起EP的位源波发生在环电流和致密冷等离子体之间的重叠区域。这与以往的研究结果一致,即在等离子体密度高的区域,带场位波的电子共振能量较低。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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