Inner Magnetospheric Oxygen Torus Induced by Electromagnetic Ion Cyclotron Waves

IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Geophysical Research Letters Pub Date : 2025-02-28 DOI:10.1029/2024GL113798
Zhiyong Wu, Zhenpeng Su, Huinan Zheng, Yuming Wang
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Abstract

Cold oxygen ions escaping from the ionosphere and temporarily trapped near the plasmapause form the oxygen torus. Mass-loading by these oxygen ions significantly affects magnetospheric plasma processes. However, due to the technical challenges in measuring cold oxygen ions and the limited spatial and temporal coverage of space missions within the magnetosphere-ionosphere coupling system, the generation mechanism of oxygen torus remains unclear. Here, we propose a novel approach to determine the ion abundances from the observable polarization and propagation characteristics of electromagnetic ion cyclotron (EMIC) waves and identify a narrow oxygen torus near the noonside plasmapause during a geomagnetically quiet period. Our data and theoretical calculations suggest that the formation of this oxygen torus involved excitation of EMIC waves by ring current protons, wave-driven Landau heating of plasmaspheric electrons, heat conduction from the magnetosphere to the ionosphere, and upwelling of ionospheric oxygen ions into the magnetosphere.

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电磁离子回旋波诱导的内磁层氧环
从电离层逸出的冷氧离子暂时被困在等离子体顶附近,形成氧环。这些氧离子的质量负荷显著影响磁层等离子体过程。然而,由于测量冷氧离子的技术挑战和空间任务在磁层-电离层耦合系统内的有限时空覆盖,氧环的产生机制尚不清楚。在这里,我们提出了一种新的方法来确定离子丰度,从可观察到的极化和电磁离子回旋波(EMIC)的传播特性,并确定一个狭窄的氧环附近正午等离子体顶在一个地磁安静期。我们的数据和理论计算表明,这个氧环的形成涉及到环电流质子激发场波,等离子体电子的波驱动朗道加热,从磁层到电离层的热传导,以及电离层氧离子上涌到磁层。
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来源期刊
Geophysical Research Letters
Geophysical Research Letters 地学-地球科学综合
CiteScore
9.00
自引率
9.60%
发文量
1588
审稿时长
2.2 months
期刊介绍: Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRLmaintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.
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