On Detection of Super Equatorial Plasma Bubbles in the American Sector During the 10–11 October 2024 Geomagnetic Storm

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Irina Zakharenkova, Iurii Cherniak, Andrzej Krankowski, Cesar E. Valladares, Cesar De la Jara Sanchez
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Abstract

Multi-instrument analysis of ground-based and satellite observations (GNSS, ionosondes, magnetometers, Swarm, GOLD) revealed the formation of giant equatorial plasma bubbles (super-EPBs) in the American sector during the 10–11 October 2024 geomagnetic storm. Development of spectacular depletions, stretching between 30°N and 50°S (∼40°MLAT) across American continents with estimated apex altitudes of ∼3,500–4,000 km, was linked to storm-induced prompt penetration electric fields. Sudden southward turning of interplanetary magnetic field Bz component occurred at ∼22:40 UT, 10 October 2024, when the dusk sector reached western South America. Following a strong uplift of the ionosphere over Jicamarca/Peru by more than 400 km, the super-EPBs developed in this region, rapidly reaching midlatitudes. In the equatorial region, super-EPBs were confined to 65°–75°W longitudes. This fortunate localization gives a rare chance to trace super-EPB evolution near-entirely, from equatorial to middle latitudes in both hemispheres, due to extensive ground-based GNSS coverage. This allows us to unveil the complexity of super-EPB evolution with storm's progress: (a) Initial formation of post-sunset super-EPBs as field-oriented, inverted C-shape structures near 65°–75°W, (b) westward drift of outmost parts of these structures across midlatitudes from their original location, (c) formation of fresh post-midnight EPBs over the same locations as post-sunset EPBs, persisting until early morning. Ionosondes in North America midlatitudes (∼42°MLAT) registered rare observations of Spread-F associated with storm-induced EPBs. Strong amplitude scintillations were observed from sunset to sunrise. Super-EPBs bringing ionospheric irregularities and scintillations to unexpectedly high latitudes represent a perplexing phenomenon connecting physical processes across equatorial, middle and high latitudes during geomagnetic disturbances.

2024年10月10-11日地磁风暴期间美国区域超级赤道等离子体气泡探测
对地面和卫星观测(GNSS、电离层探空仪、磁力计、Swarm、GOLD)的多仪器分析显示,在2024年10月10日至11日的地磁风暴期间,美国地区形成了巨大的赤道等离子体气泡(super-EPBs)。在横跨美洲大陆的30°N和50°S(~ 40°MLAT)之间,估计顶点高度为~ 3500 - 4000公里的壮观耗尽的发展与风暴引起的快速穿透电场有关。行星际磁场Bz分量的突然南转发生在2024年10月10日22:40 UT,当黄昏扇区到达南美洲西部时。随着秘鲁Jicamarca上空电离层的强烈抬升超过400公里,超级epb在该地区发展,并迅速到达中纬度地区。在赤道地区,超级epb被限制在经度65°-75°W。由于地面GNSS的广泛覆盖,这种幸运的定位提供了一个难得的机会,几乎完全追踪超级epb的演变,从赤道到中纬度,在两个半球。这使我们能够揭示超级epb随着风暴进展演变的复杂性:(a)日落后超级epb在65°-75°W附近的初始形成为场取向的倒c形结构,(b)这些结构的最外侧部分从其原始位置向西漂移,穿过中纬度地区,(c)午夜后新的epb在与日落后epb相同的位置形成,持续到清晨。在北美中纬度地区(~ 42°MLAT),电离层探测仪记录到了与风暴诱发的epb相关的罕见的Spread-F观测。从日落到日出,观测到强烈的振幅闪烁。超级epb将电离层不规则和闪烁带到意想不到的高纬度地区,这代表了一种令人困惑的现象,它将地磁扰动期间赤道、中高纬度的物理过程联系在一起。
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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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