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Supercomputer Simulation of Continental Collisions in Precambrian: The Effect of Lithosphere Thickness

机译:前寒武纪大陆碰撞的超级计算机模拟:岩石圈厚度的影响

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摘要

Many aspects of Precambrian tectonics are still unclear due to the undetermined influence of several key physical parameters (the temperature of the mantle, the thickness of the lithosphere, etc.) on the geo-dynamic processes. The values of these parameters in the Precambrian are known to have been significantly different from current conditions. This work presents the results of two-dimensional (2D) numerical petrological-thermomechanical experiments that simulate the process of plate convergence at a velocity of 5 cm/year depending on the thickness of the continental lithosphere. The model continental-lithosphere thickness ranged from 100 to 200 km, the modern mantle temperature exceeded 150℃, while radiogenic heat generation in the continental crust was 1.5 times higher then that at present. The numerical simulations showed that if the lithosphere is 100-160 km thick, the subduction process (closure of an ocean) is terminated by detachment of the oceanic plate from the continental plate (slab break-off) followed by the formation of a large igneous province (an oceanic plateau) between the continents instead of orogeny. The thinner the lithosphere is, the earlier and closer to the surface the slab break-off occurs. Thus, for a model with a continental lithosphere thickness of 150 km, the slab was detached in 10.3 Ma at a depth of 150 km, whereas for a lithosphere of 100 km thick it occurred in just 5.1 Ma almost at the surface. In the latter case, the magma generation area becomes much larger due to the formation of igneous provinces on both sides of the oceanic slab instead of one side, as is proposed in other models. Collision of continents with a very thick lithosphere (200 km or more) is not accompanied by slab break-off and significant volcanic activity. Thus, the results of our modeling show that the SLAB PULL mechanism in a subduction zone contributes to the processes at a plate convergent boundary.
机译:由于几个关键物理参数(地幔温度,岩石圈厚度等)对地球动力学过程的不确定性影响,前寒武纪构造的许多方面仍不清楚。已知前寒武纪中这些参数的值与当前条件有很大不同。这项工作提出了二维(2D)岩石岩石热力学数值实验的结果,该实验模拟了以5 cm / year的速度取决于大陆岩石圈厚度的板块收敛过程。模式大陆-岩石圈的厚度范围为100至200 km,现代地幔温度超过150℃,而大陆地壳的放射生热是目前的1.5倍。数值模拟表明,如果岩石圈的厚度为100-160 km,则俯冲过程(大洋的封闭)会通过将大洋板块从大陆板块剥离(平板破裂)而终止,然后形成大的火成岩。大陆之间的省(海洋高原)而不是造山运动。岩石圈越薄,平板破裂的时间越早,越接近表面。因此,对于大陆岩石圈厚度为150 km的模型,平板在10.3 Ma深度为150 km处发生分离,而对于100 km厚度的岩石圈,其厚度仅在5.1 Ma处接近表层。在后一种情况下,岩浆生成区域变得更大,这是由于在大洋板的两侧而不是一侧形成了火成岩省,这是其他模型所建议的。岩石圈非常厚(200 km或更长)的大陆碰撞没有伴有平板破裂和明显的火山活动。因此,我们的建模结果表明,俯冲带中的SLAB PULL机制有助于板块收敛边界处的过程。

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