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首页> 外文期刊>Chemical geology >Clinopyroxene and titanomagnetite cation redistributions at Mt. Etna volcano (Sicily, Italy): Footprints of the final solidification history of lava fountains and lava flows
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Clinopyroxene and titanomagnetite cation redistributions at Mt. Etna volcano (Sicily, Italy): Footprints of the final solidification history of lava fountains and lava flows

机译:斜山辉石和钛磁铁矿阳离子再分布。埃特纳火山(意大利西西里岛):熔岩喷泉和熔岩流最终凝固历史的足迹

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For a better understanding of the final solidification history of eruptions at Mt. Etna volcano (Sicily, Italy), we have investigated cation redistributions at the interface between sub-millimetre-sized clinopyroxene and titanomagnetite crystal rims and coexisting melts. The studied products were scoria clasts from lava fountains and rock samples from pahoehoe and aa lava flows. Our data indicate that scoria clasts from lava fountaining were rapidly quenched at the contact with the atmosphere, preserving the original crystal textures and compositions inherited during magma dynamics within the plumbing system. Kinetics and energetics of crystallization were instantaneously frozen-in and post-eruptive effects on mineral chemistry were negligible. The near-equilibrium compositions of clinopyroxene and titanomagnetite indicate that lava fountain episodes were supplied by high-temperature, H2O-rich magmas ascending with velocities of 0.01-0.31 m/s. In contrast, magmas feeding lava flow eruptions underwent a more complex solidification history where the final stage of the crystal growth was mostly influenced by volatile loss and heat dissipation at syn- and post-eruptive conditions. Due to kinetic effects associated with magma undercooling, clinopyroxenes and titanomagnetites formed by crystal attachment and agglomeration mechanisms leading to intricate intergrowth textures. The final compositions of these minerals testify to closure temperatures and melt-water concentrations remarkably lower than those estimated for lava fountains. Kinetically-controlled cation redistributions at the crystal-melt interface suggest that the solidification of magma was driven by degassing and cooling processes proceeding from the uppermost part of the volcanic conduit to the surface. (C) 2015 Elsevier B.V. All rights reserved.
机译:为了更好地了解火山最终的凝固历史。埃特纳火山(意大利西西里岛),我们研究了亚毫米大小的斜辉石与钛磁铁矿晶体边缘和共存熔体之间界面的阳离子再分布。研究的产品是来自熔岩喷泉的火山灰碎屑和来自pahoehoe和aa熔岩流的岩石样品。我们的数据表明,熔岩喷泉喷出的碎渣碎屑在与大气层接触后迅速淬灭,保留了管道系统内岩浆动力学过程中继承的原始晶体质地和成分。结晶的动力学和能量被瞬间冻结,而萌发后对矿物化学的影响可以忽略不计。斜辉石和钛磁铁矿的近平衡组成表明,熔岩喷泉事件是由高温,富含H2O的岩浆以0.01-0.31 m / s的速度上升提供的。相反,熔岩流爆发的岩浆经历了更复杂的凝固过程,在结晶过程的最后阶段,结晶生长的最后阶段主要受挥发损失和热耗散的影响。由于与岩浆过冷有关的动力学效应,由晶体附着和团聚机制形成的斜辉石和钛磁铁矿导致复杂的共生纹理。这些矿物的最终成分证明了封闭温度和熔水浓度明显低于熔岩喷泉的估计值。在晶体-熔体界面上动力学控制的阳离子再分布表明,岩浆的凝固是由从火山导管的最上部到地表进行的脱气和冷却过程驱动的。 (C)2015 Elsevier B.V.保留所有权利。

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