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Hydrogen isotope analysis of rehydrated silicic lavas: implications for eruption mechanisms

机译:复水硅质熔岩的氢同位素分析:对喷发机理的启示

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Bulk and step-heating hydrogen isotope measurements of glassy and vesicular samples from three young rhyolite lavas demonstrate for the first time that magmatic H_2O can be distinguished from meteoric H_2O added during rehydration. Step-heat extractions of gases obtained at five temperatures show that most meteoric H_2O is released at around 400 ℃, while magmatic H_2O comes off during the fusion step at 1100-1200 ℃. Magmatic H_2O contents from vertically-arrayed lava samples show a downward increase consistent with the equilibrium pressure-dependence of H_2O solubility. These gradients imply that volatile concentrations high enough to generate pyroclastic flows during front collapse may be found in the upper portions of silicic domes produced by relatively high eruption rates.
机译:对来自三个年轻流纹岩熔岩的玻璃状和囊状样品的大体积和逐步加热的氢同位素测量结果首次证明,岩浆水H_2O可以与水化过程中添加的陨石H_2O区分开。在五个温度下对气体进行的分步加热萃取表明,在1100-1200℃的聚变步骤中,大多数的H_2O释放在400℃左右,而岩浆H_2O则在燃烧过程中释放出来。垂直排列的熔岩样品中岩浆中H_2O的含量呈下降趋势,与H_2O溶解度的平衡压力相关。这些梯度表明,在相对较高的喷发速率产生的硅质穹顶的上部,可能会发现足够高的挥发物浓度,足以在前塌陷过程中产生火山碎屑流。

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