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首页> 外文期刊>Contributions to Mineralogy and Petrology >Pre- and syn-eruptive degassing and crystallisation processes of the 2010 and 2006 eruptions of Merapi volcano, Indonesia
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Pre- and syn-eruptive degassing and crystallisation processes of the 2010 and 2006 eruptions of Merapi volcano, Indonesia

机译:印度尼西亚默拉皮火山2010年和2006年喷发前和喷发过程中的脱气和结晶过程

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摘要

The 2010 eruption of Merapi (VEI 4) was the volcano's largest since 1872. In contrast to the prolonged and effusive dome-forming eruptions typical of Merapi's recent activity, the 2010 eruption began explosively, before a new dome was rapidly emplaced. This new dome was subsequently destroyed by explosions, generating pyroclastic density currents (PDCs), predominantly consisting of dark coloured, dense blocks of basaltic andesite dome lava. A shift towards open-vent conditions in the later stages of the eruption culminated in multiple explosions and the generation of PDCs with conspicuous grey scoria and white pumice clasts resulting from sub-plinian convective column collapse. This paper presents geochemical data for melt inclusions and their clinopyroxene hosts extracted from dense dome lava, grey scoria and white pumice generated during the peak of the 2010 eruption. These are compared with clinopyroxene-hosted melt inclusions from scoriaceous dome fragments from the prolonged dome-forming 2006 eruption, to elucidate any relationship between pre-emptive degassing and crystallisation processes and eruptive style. Secondary ion mass spectrometry analysis of volatiles (H_2O, CO_2) and light lithophile elements (Li, B, Be) is augmented by electron microprobe analysis of major elements and volatiles (Cl, S, F) in melt inclusions and groundmass glass. Geobarometric analysis shows that the clinopyroxene phenocrysts crystallised at depths of up to 20 km, with the greatest calculated depths associated with phenocrysts from the white pumice. Based on their volatile contents, melt inclusions have re-equilibrated during shallower storage and/or ascent, at depths of -0.6-9.7 km, where the Merapi magma system is interpreted to be highly interconnected and not formed of discrete magma reservoirs. Melt inclusions enriched in Li show uniform "buffered" Cl concentrations, indicating the presence of an exsolved brine phase. Boron-enriched inclusions also support the presence of a brine phase, which helped to stabilise B in the melt. Calculations based on S concentrations in melt inclusions and groundmass glass require a degassing melt volume of 0.36 km~3 in order to produce the mass of SO_2 emitted during the 2010 eruption. This volume is approximately an order of magnitude higher than the erupted magma (DRE) volume. The transition between the contrasting eruptive styles in 2010 and 2006 is linked to changes in mag-matic flux and changes in degassing style, with the explosive activity in 2010 driven by an influx of deep magma, which overwhelmed the shallower magma system and ascended rapidly, accompanied by closed-system degassing.
机译:2010年的默拉皮火山喷发(VEI 4)是自1872年以来火山最大的一次喷发。与默拉皮火山近期活动中典型的长时间喷发的圆顶形成喷发形成鲜明对比,2010年的喷发开始爆发,随后迅速建立了新的圆顶。这个新的圆顶后来被爆炸破坏,产生了火山碎屑密度流(PDC),主要由玄武岩安山岩圆顶熔岩的深色致密块组成。喷发后期向开孔条件的转变最终导致了多次爆炸,并产生了次平流对流柱塌陷导致明显的灰渣和白色浮渣产生的PDC。本文介绍了从2010年喷发高峰期产生的致密圆顶熔岩,灰色氧化渣和白色浮石中提取的熔体包裹体及其斜辉石基质的地球化学数据。将这些与来自2006年长时间形成的穹顶喷发的孢子状穹顶碎片中的含辉石的熔体包裹体进行了比较,以阐明先发性脱气和结晶过程与喷发样式之间的任何关系。通过电子微探针分析熔体夹杂物和磨碎玻璃中的主要元素和挥发物(Cl,S,F),可增强对挥发性有机物(H_2O,CO_2)和轻亲石元素(Li,B,Be)的二次离子质谱分析。地质气压分析表明,斜辉石的隐晶石在长达20 km的深度结晶,最大的计算深度与白色浮石的隐晶石有关。根据挥发物含量,熔体包裹体在-0.6-9.7 km深度处的较浅的储存和/或上升过程中已重新平衡,其中默拉皮岩浆系统被解释为高度互连,而不是由离散的岩浆储集层形成。富含锂的熔体夹杂物显示出均匀的“缓冲” Cl浓度,表明存在溶解的盐水相。富含硼的夹杂物还支持盐水相的存在,这有助于稳定熔体中的B。根据熔体夹杂物和毛玻璃中的S浓度进行计算,需要产生0.36 km〜3的脱气熔体体积,以产生2010年喷发期间排放的SO_2量。该体积比喷发岩浆(DRE)体积高大约一个数量级。在2010年和2006年形成鲜明对比的喷发形式之间的过渡与岩浆通量的变化和脱气形式的变化有关,2010年的爆炸性活动是由深部岩浆涌入驱动的,淹没了较浅的岩浆系统并迅速上升,伴随着密闭系统的脱气。

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