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Dynamics of deep submarine silicic explosive eruptions in the Kermadec arc, as reflected in pumice vesicularity textures

机译:Kermedc弧中深海潜硅爆炸的动力学,如浮石泡状纹理所反映的

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摘要

Despite increasing recognition of silicic pumice-bearing deposits in the deep marine environment, the processes involved in explosive silicic submarine eruptions remain in question. Here we present data on bubble sizes and number densities (number of bubbles per unit of melt matrix) for deep submarine-erupted pumices from three volcanoes (Healy, Raoul SW and Havre) along the Kermadec arc (SW Pacific) to investigate the effects of a significant (>~1 km) overlying water column and the associated increased hydrostatic pressure on magma vesiculation and fragmentation. We compare these textural data with those from chemically similar, subaerially erupted pyroclasts from nearby Raoul volcano as well as submarine-erupted ‘Tangaroan’ fragments derived by non-explosive, buoyant detachment of foaming magma from Macauley volcano, also along the Kermadec arc. Deep submarine-erupted pumices are macroscopically similar (colour, density, texture) to subaerial or shallow submarine-erupted pumices, but show contrasting microscopic bubble textures. Deep submarine-erupted pyroclasts have fewer small (<10 ?m diameter) bubbles and narrower bubble size distributions (BSDs) when compared to subaerially erupted pyroclasts from Raoul (35-55 ?m vs. 20-70 ?m range in volume based median bubble size, respectively). Bubble number density (BND) values are consistently lower than subaerial-erupted pyroclasts and do not display the same trends of decreasing BND with increasing vesicularity. We interpret these textural differences to result from deep submarine eruptions entering the water column at higher pressures than subaerial eruptions entering the atmosphere (~10 MPa vs. 0.1 MPa for a vent at 1000 mbsl). The presence of an overlying water column acts to suppress rapid acceleration of magma, as occurs in the upper conduit of subaerial eruptions, therefore suppressing coalescence, permeability development and gas loss, amounting to closed-system degassing conditions. The higher confining pressure environment of deep submarine settings hinders extensive post-fragmentation clast expansion, coalescence of bubbles, and thinning of bubble walls, causing clasts to have similar BND values regardless of their vesicularity. Although deep submarine-erupted pyroclasts are closely similar to their subaerial counterparts on the basis of bulk vesicularities and macroscopic appearance, they differ markedly in their microscopic textures, allowing them to be fingerprinted in modern and ancient pumiceous marine sediments.
机译:尽管在深海海洋环境中对硅质浮石沉积物的认识日益提高,但爆炸性硅质海底火山爆发涉及的过程仍存在疑问。在这里,我们介绍了沿着Kermadec弧(西南太平洋)来自三个火山(Healy,Raoul SW和Havre)的深潜海底火山喷发的气泡尺寸和数量密度(每单位熔融基质的气泡数量)的数据,以研究气泡的影响。显着(>〜1 km)的上水柱,并伴随着对岩浆囊泡化和破碎的静水压力的增加。我们将这些质地数据与附近Raoul火山的化学相似的,从海底喷发的火山碎屑岩以及海底喷发的“ Tangaroan”碎片进行了比较,这些碎片是从Macroley火山以及Kermadec弧的泡沫岩浆非爆炸性,浮力分离而来的。深层海底喷出的脓疱在宏观上类似于海底或浅层海底喷发的脓疱(颜色,密度,质地),但显示出相反的微观气泡纹理。与来自拉乌尔的地下喷发火山成虫相比,深部水下喷发的火山成虫具有更少的小(直径小于10 µm的气泡)和更窄的气泡尺寸分布(BSD)(35-55 µm与20-70 µm的体积基准中值范围相比)气泡大小)。气泡数密度(BND)值始终低于空中喷出的火山碎屑体,并且没有显示出随着水泡度增加而降低BND的相同趋势。我们解释这些结构差异是由于深海喷发在比进入大气的海底喷发更高的压力下进入水柱的结果(〜10 MPa对1000 mbsl的通风口为0.1 MPa)。上方水柱的存在可抑制岩浆的快速加速(如在地下喷发的上导管中发生的情况),从而抑制聚结,渗透性发展和气体损失,相当于封闭系统的除气条件。深海环境中较高的围压环境阻碍了碎片化后的大块膨胀,气泡聚结和气泡壁变薄,从而导致了具有不同BND值的膨胀,无论其囊泡大小如何。尽管在散装水泡和宏观外观的基础上,深部海底火山爆发的火山碎屑体与海底火山爆发的火山体非常相似,但它们的微观结构却有显着差异,从而使它们在现代和古代浮游的海洋沉积物中被指纹识别。

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