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What drives and resists plate sinking through the transition zone?

是什么驱动和阻止板块通过过渡区下沉？

基本信息

批准号：
NE/J008028/1
负责人：
Jeroen Van Hunen
金额：
$ 25.51万
依托单位：
Durham University
依托单位国家：
英国
项目类别：
Research Grant
财政年份：
2013
资助国家：
英国
起止时间：
2013 至无数据
项目状态：
已结题

来源：
https://gtr.ukri.org/projects?ref=NE%2FJ008028%2F1
关键词：
What drives resists plate sinking

项目摘要

Mantle circulation is largely driven by the sinking ('subduction') of cold and dense tectonic plates. When these cold slabs reach the transition zone between the upper and lower mantle (from 400 to 800 km depth), their progress is hampered by rapid increases in mantle density and viscosity, as mantle minerals change phase. X-ray type images of the interior of the Earth made using earthquake waves ('seismic tomography') reveal that this zone only forms a barrier for some slabs, while others seem to pass through unhindered. Furthermore, when the seismic images are compared with plate motions through time, it becomes clear that slabs penetrated the lower mantle in the past, where shallower parts of the plate are trapped in the transition zone today. This, as well as evidence of fast and slow subduction phases in plate motions (Goes et al., Nature 2008) indicate that this is a time dependent process, where plate material may pond until a critical mass of material has accumulated, and then flush rapidly into the lower mantle.It is important to understand this fundamental part of mantle circulation as it controls how efficiently the Earth cools and how well heterogeneities like sediments, crust, fluids and CO2 are mixed into it, or brought back up. Furthermore, sudden slab flushing events into the lower mantle have been linked to periods of continental crust formation, changes to the early atmosphere and reorganisations of plate motions. We will investigate slab behaviour in the transition zone using 3D dynamic models of subduction, and evaluate which of the modelled mechanisms are consistent with observational data from the Pacific. Previous numerical models have investigated how individual factors like slab strength, slab density, coupling to the upper plate, and mantle phase transitions affect whether a slab goes straight through the transition zone or stalls there. However, none of these individual parameters can explain the observed variations of plate-transition zone interaction. Nor is it clear for how long slabs may be stalled, and hence on which time scales the upper and lower mantle mix, and on which time scales plate motions and accompanying surface deformation vary. As single properties do not explain the variability of slab-transition-zone interaction, the interplay between mantle, downgoing and upper-plate properties must be crucial. Studying the interaction between these different factors requires 3D dynamic models that let plate motions and slab morphology develop freely, something that is numerically challenging. In recent years, our groups developed such dynamic models and elucidated how combinations of plate density, strength and width control upper-mantle slab morphology. The newest generation of these dynamic models, developed by the group of the PI at Durham, are now capable of modelling all potentially relevant plate and mantle parameters. With these models, we will explore a wide range of parameters to determine which combinations lead to slab ponding and penetration. Next we will compare modelled conditions for stalling and release with those that can be inferred for major subduction zones throughout the last 100-200 million years of Earth history from seismic tomography, plate motion histories and earthquakes in downgoing slab. This will be done using the expertise in model-data comparison in the group of the Co-I at Imperial, in collaboration with partners Prof. Spakman and Prof. Torsvik, leading experts in seismic imaging and plate motion reconstructions, respectively. With these new models and this interdisciplinary team, we will be able to answer the fundamental question of how the transition zone traps and releases subducting slabs, a process that plays a pivotal role in the Earth's internal and plate-tectonic evolution.

地幔环流在很大程度上是由冷而致密的构造板块的下沉（俯冲）驱动的。当这些冷板块到达上地幔和下地幔之间的过渡区（深度从400到800公里）时，它们的进展受到地幔密度和粘度迅速增加的阻碍，因为地幔矿物改变了相位。使用地震波（“地震层析成像”）拍摄的地球内部X射线图像显示，该区域仅对某些板块形成障碍，而其他板块似乎可以不受阻碍地穿过。此外，当地震图像与板块运动进行比较时，很明显，板块在过去穿透了下地幔，而今天板块的较浅部分被困在过渡带中。这一点，以及板块运动中快速和缓慢俯冲阶段的证据（Goes等人，自然2008）表明这是一个时间依赖性的过程，板块物质可能会汇集，直到物质积累到临界质量，然后迅速涌入下地幔。重要的是要了解地幔循环的这一基本部分，因为它控制着地球冷却的效率，以及沉积物，地壳，流体和CO2等非均匀性如何混合到其中，或带回来。此外，突然进入下地幔的板块冲刷事件与大陆地壳形成、早期大气变化和板块运动重组有关。我们将使用俯冲的三维动态模型研究过渡区的板块行为，并评估哪些建模机制与太平洋的观测数据一致。以前的数值模型已经研究了单个因素，如板片强度，板片密度，耦合到上板，地幔相变影响板片是否直接通过过渡区或失速。然而，这些参数都不能解释观察到的变化的板过渡区相互作用。也不清楚板块可能停滞多久，因此，上地幔和下地幔在哪个时间尺度上混合，以及板块运动和伴随的地表变形在哪个时间尺度上变化。由于单一的属性不能解释板块过渡带相互作用的变化，地幔，下行和上板块属性之间的相互作用必须是至关重要的。研究这些不同因素之间的相互作用需要3D动态模型，让板块运动和板块形态自由发展，这在数值上是具有挑战性的。近年来，我们的团队开发了这样的动力学模型，并阐明了板块密度，强度和宽度的组合如何控制上地幔板块形态。由达勒姆的PI小组开发的最新一代动态模型现在能够模拟所有可能相关的板块和地幔参数。有了这些模型，我们将探索各种参数，以确定哪些组合导致板积水和渗透。接下来，我们将比较模型化的条件停滞和释放与那些可以推断的主要俯冲带在过去的1亿至2亿年的地球历史，地震层析成像，板块运动的历史和地震下行板。这将利用帝国理工学院Co-I小组在模型数据比较方面的专业知识，与合作伙伴Spakman教授和Torsvik教授合作，他们分别是地震成像和板块运动重建方面的领先专家。有了这些新模型和这个跨学科的团队，我们将能够回答过渡带如何捕获和释放俯冲板块的基本问题，这一过程在地球内部和板块构造演化中起着关键作用。