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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 >Electrical conductivity of hydrous silicate melts: Implications for the bottom-up hydration of Earth's upper mantle
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Electrical conductivity of hydrous silicate melts: Implications for the bottom-up hydration of Earth's upper mantle

机译:含水硅酸盐的电导率熔化:对地球上部地幔的自下而上水合的影响

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The upwelling of the hydrous mantle transition zone triggers dehydration-induced partial melting atop the 410-km discontinuity. Here we investigate the electrical conductivity of hydrous silicate melts in the 200-400 km depth range and explore whether melting at the 410-km depths is responsible for the hydration of the upper mantle. Our experimental electrical conductivity data demonstrate that the mantle at 180-350 km depths is mostly melt free, confirming the H2O under-saturated conditions. However, the residual mantle from partial melting atop the 410-km discontinuity may contain various possible amounts of water according to the initial mantle transition zone and melt concentrations. This residual H2O could contribute to the hydration of the upper mantle either through diffusion or material replacement by upwelling. Our calculations suggest that the diffusion may not be responsible for the hydration of the upper mantle to present H2O concentration of 50-200 ppm wt. Melting of the upwelling mantle transition zone with less than 1500 ppm wt. H2O produces residual peridotites with similar to 200 ppm H2O at the 410-km discontinuity. Continuous upwelling of such hydrous residues would gradually replace the dry upper mantle with depleted residual hydrous peridotites in less than 260 Ma. In this study, we propose a bottom-up hydration mechanism for the Earth's upper mantle driven by dehydration-melting at the 410-km discontinuity. The hydrous partial melting at the top of the asthenosphere appears to be a consequence of H2O saturation in the upwelling residual peridotites. (C) 2019 Elsevier B.V. All rights reserved.
机译:含水套道过渡区的升值触发脱水诱导的偏熔化在410公里的不连续。在这里,我们研究了含水硅酸盐熔体的电导率在200-400公里深度范围内,并探索了410公里深度的熔化是否负责上部地幔的水合。我们的实验导电性数据表明,180-350公里深度的地幔主要熔化,确认H2O饱和条件下。然而,根据初始裂缝过渡区和熔融浓度,来自部分熔点的残留罩可含有各种可能的水量和熔融浓度。这种残留的H2O可以通过升值的扩散或材料替代来促进上部搭腔的水合。我们的计算表明,扩散可能不负责上部地幔的水合,以呈现50-200ppm的H2O浓度为50-200ppm。熔化覆盖的地幔过渡区,少于1500ppm wt。 H2O在410公里的不连续中产生与200ppm H2O相似的残留恒星。连续升值这种含水残留物将逐渐取代干燥的上部搭腔,在少于260mA的情况下用耗尽的残余湿润的岩浆。在这项研究中,我们提出了通过在410公里的不连续的脱水熔化的脱水熔化驱动的地球上部地幔的自下而上的水化机制。在哮喘圈顶部熔化似乎是H2O饱和在升温的残余恒星中的结果。 (c)2019 Elsevier B.v.保留所有权利。

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