极光漩涡和滚动磁毯

IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY
Xiaoyan Zhou, Donald Hampton
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引用次数: 0

摘要

我们报告了2024年1月1日在阿拉斯加的Poker Flat观测到的四个波长的圆柱形极光漩涡的夜侧阵列。在站点的南部,一个已经存在的东西弧形从西部开始,在向东延伸的过程中演变成卷曲,然后是螺旋状,在大约2分钟内开始了亚风暴的扩张。在427.8、557.7、630.0和1100.0 nm的四个波长上都可以看到漩涡,表明一个大约200公里高的圆柱体,跨越100-300公里的高度。涡旋尺寸为~ 30 × 40 km(东西×南北)。估计平均能量和能量通量为4-6 keV和30-40 mW/m2。极光形态表明,一种遥远的剪切力触发了开尔文-亥姆霍兹不稳定性,产生了局部涡旋,像卷地毯一样卷起了磁通量。向上的磁场定向电流(向下的电子)随着滚动的磁毯而弯曲,在电离层产生螺旋形的极光足迹。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The Auroral Vortex and Rolling Magnetic Carpet

The Auroral Vortex and Rolling Magnetic Carpet

The Auroral Vortex and Rolling Magnetic Carpet

The Auroral Vortex and Rolling Magnetic Carpet

We report a nightside array of cylindrical auroral vortices observed at four wavelengths on 1 January 2024 from Poker Flat, Alaska. A pre-existing east–west arc just south of the site began beading from the west, evolving into curls and then spirals while extending eastward, initiating a substorm expansion within ∼2 min. The vortices were seen in all four wavelengths at 427.8, 557.7, 630.0, and 1100.0 nm, indicating a ∼200 km-tall cylinder spanning 100–300 km altitude. Vortex dimensions were ∼30 × 40 km (east–west × north–south). Estimated average energy and energy flux were 4–6 keV and 30–40 mW/m2. The auroral morphology suggests that a remote shear force triggered the Kelvin–Helmholtz instability, generating local vortices that rolled up the magnetic flux like coiling a carpet. Upward field-aligned currents (downward electrons) warped with the rolling magnetic carpet, producing a spiraling auroral footprint in the ionosphere.

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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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