Particle Concentrations and Sizes for the Onset of Settling-Driven Gravitational Instabilities: Experimental Validation and Application to Volcanic Ash Clouds

IF 3.9 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Allan Fries, Jonathan Lemus, Paul A. Jarvis, Amanda B. Clarke, Jeremy C. Phillips, Irene Manzella, Costanza Bonadonna
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Abstract

Settling-driven gravitational instabilities (SDGIs) can form at the base of buoyant particle-laden suspensions, modulating particle sedimentation in various settings such as meteorological and volcanic clouds, fluvial plumes, magma chambers, submarine hydrothermal plumes, or industrial emissions. These instabilities result in the formation of rapidly descending currents called ‘fingers’ within which fine particles settle faster collectively than individually. This study investigates SDGI triggering conditions underneath volcanic ash clouds through analogue experiments considering sedimentation from aqueous particle suspensions. We confirm that the conditions for which SDGIs develop are controlled by two dimensionless numbers: Bf (ratio of the characteristic finger velocity to the individual particle settling velocity); and Bi (ratio of timescale for individual particle settling to that for collective settling controlled by inertial drag). SDGIs are triggered for values of Bf and Bi > 1 for which particles are fully coupled with the flow within fingers. Using these parameters, we produce a regime diagram for the 2010 eruption of Eyjafjallajökull (Iceland) that describes particle settling as a function of particle concentration and size. More studies are needed to produce a general regime diagram accounting for the evolution of SDGIs properties with eruption and atmospheric parameters. Nonetheless, our study confirms that fingers affect sedimentation from volcanic clouds with high ash volume fractions above 10−6 vol.%. Our validation of criteria predicting the onset of fingers due to SDGIs constitutes a step forward toward the incorporation of these collective settling processes in volcanic ash transport and dispersion models.

Abstract Image

沉降驱动的重力不稳定性开始时的颗粒浓度和大小:火山灰云的实验验证与应用
沉降驱动的重力不稳定性(SDGIs)可在充满浮力的颗粒悬浮物底部形成,在气象和火山云、河流羽流、岩浆室、海底热液羽流或工业排放等各种环境中调节颗粒沉降。这些不稳定性导致形成被称为 "手指 "的快速下降气流,在这些气流中,细颗粒的集体沉降速度要快于个体沉降速度。本研究通过考虑水性颗粒悬浮物沉降的模拟实验,研究火山灰云下的 SDGI 触发条件。我们证实,SDGI 的形成条件受两个无量纲数控制:Bf(特征指速度与单个颗粒沉降速度之比);以及 Bi(单个颗粒沉降时标与受惯性阻力控制的集体沉降时标之比)。当 Bf 和 Bi 的值为 1 时,SDGIs 将被触发,此时颗粒与手指内的气流完全耦合。利用这些参数,我们绘制出了 2010 年冰岛埃亚菲亚德拉角火山喷发的态势图,该态势图描述了颗粒沉降与颗粒浓度和大小的函数关系。还需要进行更多的研究,才能绘制出一个通用的状态图,以说明随着喷发和大气参数的变化,SDGIs 的特性也会发生变化。尽管如此,我们的研究证实了手指会影响火山灰体积分数超过 10-6 vol.% 的火山云的沉降。我们对 SDGIs 引起的指状沉降的预测标准进行了验证,这为将这些集体沉降过程纳入火山灰迁移和扩散模型迈出了一步。
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来源期刊
Journal of Geophysical Research: Solid Earth
Journal of Geophysical Research: Solid Earth Earth and Planetary Sciences-Geophysics
CiteScore
7.50
自引率
15.40%
发文量
559
期刊介绍: The Journal of Geophysical Research: Solid Earth serves as the premier publication for the breadth of solid Earth geophysics including (in alphabetical order): electromagnetic methods; exploration geophysics; geodesy and gravity; geodynamics, rheology, and plate kinematics; geomagnetism and paleomagnetism; hydrogeophysics; Instruments, techniques, and models; solid Earth interactions with the cryosphere, atmosphere, oceans, and climate; marine geology and geophysics; natural and anthropogenic hazards; near surface geophysics; petrology, geochemistry, and mineralogy; planet Earth physics and chemistry; rock mechanics and deformation; seismology; tectonophysics; and volcanology. JGR: Solid Earth has long distinguished itself as the venue for publication of Research Articles backed solidly by data and as well as presenting theoretical and numerical developments with broad applications. Research Articles published in JGR: Solid Earth have had long-term impacts in their fields. JGR: Solid Earth provides a venue for special issues and special themes based on conferences, workshops, and community initiatives. JGR: Solid Earth also publishes Commentaries on research and emerging trends in the field; these are commissioned by the editors, and suggestion are welcome.
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