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Mantle flow and melting beneath young oceanic lithosphere: Seismic studies of the Galápagos Archipelago and the Juan de Fuca Plate

机译:年轻的海洋岩石圈下的地幔流动和融化:加拉帕戈斯群岛和胡安德富卡板块的地震研究

摘要

In this dissertation, I use seismic imaging techniques to constrain the physical state of the upper mantle beneath regions of young oceanic lithosphere. Mantle convection is investigated beneath the Galápagos Archipelago and then beneath the Juan de Fuca (JdF) plate, with a focus on the JdF and Gorda Ridges before turning to the off-axis asthenosphere. In the Galápagos Archipelago, S-to-p receiver functions reveal a discontinuity in seismic velocity that is attributed to the dehydration of the upper mantle. The depth at which dehydration occurs is shown to be consistent with prior constraints on mantle temperature. A comparison between results from receiver functions, seismic tomography and petrology shows that mantle upwelling and melt generation occur shallower than the depth of the discontinuity, despite the expectation of high viscosities in the dehydrated layer. Beneath the JdF and Gorda Ridge, low Vs anomalies are too large to be explained by the cooling of the lithosphere and are attributed to partial melt. The asymmetry, large Vs gradients, and sinuosity of the anomalies beneath the JdF Ridge are consistent with models of buoyancy-driven upwelling. However, deformation zone processes appear to dominate mantle flow over seafloor spreading beneath the Explorer and Gorda diffuse plate boundaries. Finally, S-to-p receiver functions reveal a seismic discontinuity beneath the JdF plate that can only be attributed to seismic anisotropy. Synthesis of the receiver function results with prior SKS splitting results requires heterogeneous anisotropy between the crust and the discontinuity. Models of anisotropy feature increasing anisotropy before the decrease at the discontinuity, but well below the base of the lithosphere, and a clockwise rotation of the fast direction with increasing depth. In these results and even in the SKS splitting results, additional driving mechanisms for mantle flow such as density or pressure anomalies are required.
机译:在本文中,我使用地震成像技术来约束年轻的海洋岩石圈区域下方的上地幔的物理状态。在加拉帕戈斯群岛下方,然后在胡安·德·富卡(JdF)板下方,研究地幔对流,重点是JdF和Gorda Ridges,然后转向离轴软流圈。在加拉帕戈斯群岛,S-to-p接收器功能揭示了地震速度的不连续性,这归因于上地幔的脱水。脱水发生的深度与先前对地幔温度的限制一致。接收器功能,地震层析成像和岩石学的结果之间的比较表明,尽管期望在脱水层中具有高粘度,但地幔上升流和熔体生成的深度要比不连续的深度浅。在JdF和Gorda Ridge下,低Vs异常太大,无法用岩石圈的冷却来解释,并且归因于部分熔融。 JdF山脊下方异常的不对称性,大的Vs梯度和弯曲度与浮力驱动的上升流模型一致。然而,变形区过程似乎主导了在Explorer和Gorda扩散板边界之下扩散的海底上的地幔流。最后,从S到p的接收器功能揭示了JdF板下方的地震不连续性,这只能归因于地震各向异性。接收器功能结果与先前的SKS分裂结果的综合要求地壳和间断面之间存在异质各向异性。各向异性模型的特征在于,各向异性在不连续性减小之前先增大,但远低于岩石圈的底部,并且随着深度的增加,快速方向沿顺时针方向旋转。在这些结果中,甚至在SKS分裂结果中,都需要用于地幔流动的其他驱动机制,例如密度或压力异常。

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    Byrnes Joseph;

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  • 年度 2017
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