...
【24h】

Tracking deep mantle reservoirs with ultra-low velocity zones

机译:跟踪具有超低速带的地幔深层储层

获取原文
获取原文并翻译 | 示例
           

摘要

Some regions of the Earth's lowermost mantle exhibit anomalous seismic properties within a thin zone, less than tens of kilometers in thickness, that directly overlies the core-mantle boundary (CMB). These regions have been dubbed Ultra-Low Velocity Zones (ULVZs) due to their greater than 10% drop in seismic velocities. High resolution seismic array studies have found small, localized ULVZs (e.g., 10 km thick and 50-100 km wide) with a large increase in ULVZ density (~ 10%) relative to the background mantle. Many studies note that ULVZ material may be chemically distinct, though P-to-S-wave velocity reductions are sometimes consistent with partial melting. The apparent absence of ULVZs in many regions of the CMB is consistent with having a distinct chemical signature, regardless of melt content. However, it is unknown how a small volume of very dense ULVZ material can be locally elevated, particularly in the presence of large-scale compositional reservoirs predicted by seismology, geochemistry, and geodynamics. We perform ultra-high resolution, kilometer-scale, thermochemical convection calculations for an entire mantle system containing three distinct compositional components in order to investigate how a ULVZ interacts with large-scale lower mantle compositional reservoirs. We demonstrate that convection can dynamically support small scale accumulations of dense ULVZ material, consistent with the size and density inferred from seismology. Furthermore, we show that ULVZs preferentially reside at the boundaries of large compositional reservoirs, which periodically break apart and merge together in response to changes in downwelling patterns. As they do, ULVZ material migrates and recollects in a systematic fashion. ULVZ material can become entrained in mantle plumes forming from reservoir boundaries, contributing to isotopic anomalies found in hotspot volcanism. Thus ULVZ detection helps to constrain large-scale mantle convection patterns, the locations of compositional reservoir boundaries, and the evolution of geochemical reservoirs.
机译:地球最下层地幔的某些区域在厚度小于几十公里的薄区域内表现出异常的地震特性,该区域直接覆盖了地幔幔边界(CMB)。这些区域被称为超低速带(ULVZs),因为它们的地震速度下降幅度超过10%。高分辨率地震阵列研究发现,小型的局部ULVZ(例如10 km厚和50-100 km宽)相对于背景地幔而言ULVZ密度有较大增加(〜10%)。许多研究指出,ULVZ材料在化学上可能有所不同,尽管P波到S波的速度降低有时与部分熔化相符。不管熔体含量如何,在CMB的许多区域中明显没有ULVZ,这与具有独特的化学特征相一致。但是,未知如何才能局部升高少量的非常致密的ULVZ材料,特别是在存在通过地震学,地球化学和地球动力学预测的大规模成分储层的情况下。我们对包含三个不同组成成分的整个地幔系统进行超高分辨率,千米规模的热化学对流计算,以研究ULVZ如何与大型下地幔成分储层相互作用。我们证明对流可以动态支持致密ULVZ材料的小规模累积,这与地震学推断的大小和密度是一致的。此外,我们显示ULVZs优先驻留在大型成分储层的边界处,周期性地破裂并合并在一起,以响应井下模式的变化。当他们这样做时,ULVZ材料以系统的方式迁移和回收。 ULVZ材料可能夹带在由储层边界形成的地幔柱中,导致热点火山活动中存在同位素异常。因此,ULVZ检测有助于约束大规模的地幔对流模式,组成储层边界的位置以及地球化学储层的演化。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号