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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Short residence times for alkaline Vesuvius magmas in a multi-depth supply system: Evidence from geochemical and textural studies
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Short residence times for alkaline Vesuvius magmas in a multi-depth supply system: Evidence from geochemical and textural studies

机译:碱性维苏威火山岩浆在多深度供应系统中的停留时间短:来自地球化学和质地研究的证据

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It is crucial to understand magma chamber chemico-physical conditions and residence times for high-risk volcanoes because these factors control the occurrence and size of future eruptions. In order to define magmatic pressure-temperature conditions and residence times at the Somma-Vesuvius volcano, we studied the geochemistry and texture of selected past eruptions that are representative of the entire volcanic history.Our petrological model indicates a multi-depth magma chamber composed of a deeper tephritic (350-400. Mpa) magma layer, which fed Strombolian and effusive eruptions during open-conduit activity, and an upper (200-250. Mpa) phonolitic level, which supplied the high explosive events that followed closed-conduit repose time. This upper reservoir matches the inferred transition between sedimentary sequences and metamorphic basement. At this level, the presence of a structural and lithological discontinuity favors magma storage during closed-conduit periods.The prevalent differentiation process was fractional crystallization during the magma cooling associated with upward migration of less dense, evolved liquids. Our results indicate that major steam exolution occurred during the late crystallization stage of phonolites, which accounts for the high Volcanic Explosivity Index (VEI) of eruptions supplied by these melts. Moreover, our phenocryst CSD data reveal the rapid crystallization and differentiation (decades to centuries) of alkaline Somma-Vesuvius magmas. This implies that the 400km~2 partial melting zone detected by tomography studies at 8-10km depth beneath Vesuvius should consist of differentiated magma that is already capable of generating a large-scale (plinian) explosive event if renewed activity develops out of the present closed-conduit state. Additionally, because our microlite CSD data indicate rapid magma migration from the chamber toward the surface, precursory activity could appear only short time before a major eruption.
机译:了解高风险火山的岩浆室化学物理条件和停留时间至关重要,因为这些因素控制着未来喷发的发生和规模。为了确定索马-维苏威火山的岩浆压力-温度条件和停留时间,我们研究了代表整个火山历史的部分过去喷发的地球化学和质地。我们的岩石学模型表明,一个多深度的岩浆室由较深的三叠纪(350-400。Mpa)岩浆层,在开导管活动期间充实了斯特伦伯利亚喷发性喷发,而较高的(200-250。Mpa)胶质水平则提供了封闭导管休止后的高爆炸性事件时间。该上部储层与沉积层序和变质基底之间的推断过渡相匹配。在这个水平上,结构和岩性间断的存在有利于岩浆在封闭导管时期的储存。普遍的分化过程是岩浆冷却过程中的部分结晶,伴随着密度较小,演化的液体的向上迁移。我们的结果表明,主要的蒸汽渗出发生在方沸石的结晶后期,这解释了这些熔体提供的火山爆发的高火山爆炸指数(VEI)。此外,我们的隐晶CSD数据揭示了碱性Somma-Vesuvius岩浆的快速结晶和分化(数十个世纪)。这意味着通过层析成像研究在维苏威火山以下8-10km深度处检测到的400km〜2部分融化带应该由分化的岩浆组成,如果在目前封闭的环境中恢复活动,则该岩浆已经能够产生大规模(p系)爆炸事件。 -导管状态。此外,由于我们的微岩CSD数据表明岩浆从暗室向地表快速迁移,因此前兆活动可能仅在一次大喷发之前很短的时间出现。

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