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通过涡轮电泳和烧结在管道内捕获亚微米级火山灰颗粒。

In-conduit capture of sub-micron volcanic ash particles via turbophoresis and sintering.

作者信息

Farquharson Jamie I, Tuffen Hugh, Wadsworth Fabian B, Castro Jonathan M, Unwin Holly, Schipper C Ian

机构信息

Institut Terre et Environnement de Strasbourg, UMR 7063, Université de Strasbourg, Strasbourg, France.

Lancaster Environment Centre, Lancaster University, Lancaster, LA1 4YQ, UK.

出版信息

Nat Commun. 2022 Aug 11;13(1):4713. doi: 10.1038/s41467-022-32522-7.

Abstract

Ash emission in explosive silicic eruptions can have widespread impacts for human health, agriculture, infrastructure, and aviation. Estimates of the total grainsize distribution (TGSD) generated during explosive magma fragmentation underpins eruption models and ash dispersal forecasts. Conventionally, the TGSD constrained via erupted deposits is assumed to match the TGSD produced at explosive fragmentation. Here we present observations from within the vent of a recent rhyolitic eruption (Cordón Caulle, Chile, 2011-2012), demonstrating that fine (<63 μm diameter) and ultra-fine (<2.5 μm diameter) ash particles are captured and sintered to fracture surfaces, and thus sequestered in the shallow subsurface, rather than emitted. We establish a conceptual model-uniquely contextualised through a combination of syn-eruptive observations and detailed post-eruption field investigation-in which turbophoresis (particle migration towards zones of lower turbulence) and rapid sintering create an inverse relationship between particle size and the probability of its subsurface capture. Such size-dependent capture efficiency preferentially removes submicron-diameter ash from the erupted componentry, decoupling the erupted size distribution from magmatic source conditions and potentially playing an important role in modulating eruption dynamics.

摘要

爆发性硅质火山喷发中的火山灰排放会对人类健康、农业、基础设施和航空产生广泛影响。爆炸性岩浆破碎过程中产生的总粒度分布(TGSD)估算为火山喷发模型和火山灰扩散预测提供了支撑。传统上,通过喷发沉积物约束的TGSD被认为与爆炸性破碎时产生的TGSD相匹配。在此,我们展示了对近期一次流纹岩喷发(智利科多恩·考耶火山,2011 - 2012年)火山口内部的观测结果,表明细颗粒(直径<63μm)和超细颗粒(直径<2.5μm)火山灰颗粒被捕获并烧结到断裂面上,从而被隔离在浅地表以下,而非排放到大气中。我们通过喷发期间的观测和详细的喷发后野外调查相结合,建立了一个概念模型,其中,旋流电泳(颗粒向低湍流区域迁移)和快速烧结导致颗粒大小与其被地表以下捕获概率之间呈反比关系。这种与颗粒大小相关的捕获效率优先从喷发物质中去除亚微米级直径的火山灰,使喷发粒度分布与岩浆源条件脱钩,并可能在调节火山喷发动力学方面发挥重要作用。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/9276/9372141/94ebd6e9c4f7/41467_2022_32522_Fig1_HTML.jpg

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