Detection of Extensive Equatorial Plasma Depletions After the 2022 Tongan Volcanic Eruption From Multiple Geodetic Satellite Ranging Systems

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Shin-Chan Han, Hyosub Kil, Richard Ray, Frank Lemoine, Colin Waters
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Abstract

We present a number of unique observations of ionospheric anomalies following the Hunga-Tonga Hunga-Ha'apai (HTHH) volcanic eruption on 15 January 2022. All are based on non-dedicated geodetic satellite systems: Global Positioning System tracking of Low Earth Orbit (LEO) CubeSats, intersatellite tracking between two GRACE Follow-On satellites, satellite radar altimeters to the ocean surface, and Doppler radio beacons from ground stations to LEO geodetic satellites. Their observations revealed the development of anomalously large trough-like plasma depletions, along with plasma bubbles, in the equatorial regions of the Pacific and East Asian sectors. Trough-like plasma depletions appeared to be confined within approximately ±20° magnetic latitude, accompanied by density enhancements just outside this latitude range. These plasma depletions and enhancements were aligned with the magnetic equator and occurred across broad longitudes. They were detected in regions where atmospheric waves from the HTHH eruption passed through around the time of the sunset terminator. We interpret these phenomena in terms of the E dynamo electric fields driven by atmospheric waves from the eruption. The uplift of the ionosphere beyond satellite altitudes, followed by subsequent plasma diffusion to higher latitudes along magnetic field lines, results in the formation of trough-like plasma depletions around the magnetic equator and density enhancement at higher latitudes. The detection of plasma bubbles in the Asian sector during the non-bubble season (January) is likely associated with the uplift of the ionosphere at the sunset terminator.

从多个大地测量卫星测距系统探测 2022 年汤加火山爆发后的大范围赤道等离子体损耗
我们介绍了 2022 年 1 月 15 日 Hunga-Tonga Hunga-Ha'apai (HTHH)火山爆发后电离层异常的一些独特观测结果。所有观测均基于非专用大地测量卫星系统:全球定位系统对低地球轨道(LEO)立方体卫星的跟踪、两颗 GRACE 后续卫星之间的卫星间跟踪、对海洋表面的卫星雷达测高仪以及从地面站到低地球轨道大地测量卫星的多普勒无线电信标。他们的观测结果表明,在太平洋和东亚扇区的赤道地区,出现了异常巨大的槽状等离子体耗竭,并伴有等离子体气泡。槽状等离子体损耗似乎局限在大约±20°的磁纬度范围内,而在这一纬度范围之外则伴有密度增强。这些等离子体损耗和增强与磁赤道成一直线,发生在宽广的经度上。它们是在日落终结者前后 HTHH 喷射产生的大气波经过的区域被探测到的。我们用爆发产生的大气波驱动的 E 动力电场来解释这些现象。卫星高度以外的电离层隆起,随后等离子体沿磁场线向高纬度扩散,导致在磁赤道周围形成槽状等离子体耗竭,而在高纬度则形成密度增强。在非气泡季节(1 月)在亚洲地区探测到等离子气泡可能与日落终结点电离层的抬升有关。
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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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