地表下:压力引起的行星尺度波、火山闪电和由Hunga Tonga-Hunga Ha'apai火山海底喷发引起的气体云

David A. Yuen , Melissa A. Scruggs , Frank J. Spera , Yingcai Zheng , Hao Hu , Stephen R. McNutt , Glenn Thompson , Kyle Mandli , Barry R. Keller , Songqiao Shawn Wei , Zhigang Peng , Zili Zhou , Francesco Mulargia , Yuichiro Tanioka
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引用次数: 81

摘要

本文通过综合火山爆发后最初几周内可获得的各种初步地震、火山学、声波和闪电数据,叙述了2022年1月15日亨加汤加-亨加哈帕火山灾难性喷发的最终爆发事件。火山爆发的第一个小时产生了快速传播的海啸波、长周期地震波、响亮的声波、次声波、异常强烈的火山闪电和不稳定的火山羽流,这些火山羽流短暂地到达了58公里高的地球中间层。在世界范围内记录了强烈的地震信号,全球叠加地震图显示了在最强烈的潜水活动期间的间歇性地震事件,它们与斐济记录的次声压波形具有良好的相关性。引力波信号的强度足以在最初的几个小时内在整个地球上观测到,其中一些信号随后环绕地球多次。这些大振幅、长波长的大气扰动来自于地球大气层,它是在2022年1月15日UTC时间0402±1-1800的不稳定但准连续的喷发所释放的岩浆混合物(火山灰、熔体和气体)的强迫下产生的。大气强迫持续的时间比现代仪器记录的大地震破裂的时间要长得多,它产生了一种冲击波,这种冲击波源于压缩空气和周围(波浪状)海面之间的相互作用。这种情况不同于地震滑坡、山体滑坡或火山口崩塌产生的海啸波的传统观点,因为与热的、富含挥发物的潜水柱相关的挥发物的超临界性质导致了巨大的(~ 1000倍)体积变化。烟羽高度的时间序列可以转化为体积流量和质量流量。喷发持续时间约为12小时,喷发体积和质量估计分别为1.9 km3和约2 900 Tg,对应于该事件的VEI为5-6。岩浆-海水相互作用产生细灰,伴随高单位质量电荷和高喷发前溶解挥发物浓度,增强了闪电的高频率和强度。对闪电频率的分析提供了羽流活动和喷发强度的快速度量。这次喷发的许多方面有待多学科团队的进一步研究。它为高能火山喷发及其伴随现象的复杂、非线性行为的基础研究提供了一个独特的机会,对减轻灾害、火山预测和未来灾害的第一反应工作具有重要意义。
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Under the surface: Pressure-induced planetary-scale waves, volcanic lightning, and gaseous clouds caused by the submarine eruption of Hunga Tonga-Hunga Ha'apai volcano

We present a narrative of the eruptive events culminating in the cataclysmic January 15, 2022 eruption of Hunga Tonga-Hunga Ha'apai Volcano by synthesizing diverse preliminary seismic, volcanological, sound wave, and lightning data available within the first few weeks after the eruption occurred. The first hour of eruptive activity produced fast-propagating tsunami waves, long-period seismic waves, loud audible sound waves, infrasonic waves, exceptionally intense volcanic lightning and an unsteady volcanic plume that transiently reached—at 58 ​km—the Earth's mesosphere. Energetic seismic signals were recorded worldwide and the globally stacked seismogram showed episodic seismic events within the most intense periods of phreatoplinian activity, and they correlated well with the infrasound pressure waveform recorded in Fiji. Gravity wave signals were strong enough to be observed over the entire planet in just the first few hours, with some circling the Earth multiple times subsequently. These large-amplitude, long-wavelength atmospheric disturbances come from the Earth's atmosphere being forced by the magmatic mixture of tephra, melt and gasses emitted by the unsteady but quasi-continuous eruption from 0402±1–1800 UTC on January 15, 2022. Atmospheric forcing lasted much longer than rupturing from large earthquakes recorded on modern instruments, producing a type of shock wave that originated from the interaction between compressed air and ambient (wavy) sea surface. This scenario differs from conventional ideas of earthquake slip, landslides, or caldera collapse-generated tsunami waves because of the enormous (∼1000x) volumetric change due to the supercritical nature of volatiles associated with the hot, volatile-rich phreatoplinian plume. The time series of plume altitude can be translated to volumetric discharge and mass flow rate. For an eruption duration of ∼12 ​h, the eruptive volume and mass are estimated at 1.9 ​km3 and ∼2 900 ​Tg, respectively, corresponding to a VEI of 5–6 for this event. The high frequency and intensity of lightning was enhanced by the production of fine ash due to magma—seawater interaction with concomitant high charge per unit mass and the high pre-eruptive concentration of dissolved volatiles. Analysis of lightning flash frequencies provides a rapid metric for plume activity and eruption magnitude. Many aspects of this eruption await further investigation by multidisciplinary teams. It represents a unique opportunity for fundamental research regarding the complex, non-linear behavior of high energetic volcanic eruptions and attendant phenomena, with critical implications for hazard mitigation, volcano forecasting, and first-response efforts in future disasters.

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