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Elastic properties of silicate melts: Implications for low velocity zones at the lithosphere-asthenosphere boundary

机译:硅酸盐熔体的弹性特性:对岩石圈-软流圈边界低速带的影响

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摘要

Low seismic velocity regions in the mantle and crust are commonly attributed to the presence of silicate melts. Determining melt volume and geometric distribution is fundamental to understanding planetary dynamics. We present a new model for seismic velocity reductions that accounts for the anomalous compressibility of silicate melt, rendering compressional wave velocities more sensitive to melt fraction and distribution than previous estimates. Forward modeling predicts comparable velocity reductions for compressional and shear waves for partially molten mantle, and for low velocity regions associated with the lithosphere-asthenosphere boundary (LAB), melt present at <5% distributed in near-textural equilibrium. These findings reconcile seismic observations for the LAB regionally and locally and favor models of strong coupling across the LAB rather than melt channeling due to shear deformation.
机译:地幔和地壳中地震速度较低的区域通常归因于硅酸盐熔体的存在。确定熔体体积和几何分布是理解行星动力学的基础。我们提出了一种地震速度降低的新模型,该模型解释了硅酸盐熔体的异常可压缩性,从而使压缩波速度对熔体分数和分布的敏感性比以前的估计高。正演模型预测了部分熔融地幔的压缩波和剪切波的相对速度降低,以及与岩石圈-软流圈边界(LAB)相关的低速区域,熔体以<5%的速率分布在近纹理平衡中。这些发现与区域性和局部性的LAB地震观测值相吻合,并且有利于整个LAB的强耦合模型,而不是由于剪切变形而引起的融化通道。

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