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Intraplate continental deformation: Influence of a heat-producing layer in the lithospheric mantle

机译:板内大陆变形:岩石圈地幔中产热层的影响

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Deformation of the continental lithosphere is traditionally modeled assuming that heat production in the subcontinental lithospheric mantle is negligible. Although this may be appropriate for highly depleted Archean lithosphere, studies of mantle xenoliths and lithospheric-derived mafic rocks suggest that heat productions of up to 0.4 mu W/m(3) may be attained in the mantle of Phanerozoic and Neoproterozoic regions due to modal metasomatism. To investigate the effect of a local enrichment in heat-producing elements within the lithospheric mantle on the continental deformation, we performed a series of 2D thermo-mechanical models simulating the deformation of a lithospheric plate 1000 km long, which contains in its central part a 200 km wide and 20 km-thick mantle layer with a heat production of 0.05-0.25 mu W/m(3) between 40 and 80 km depth, leading to a local enhancement of the surface heat flow by 1-5 mW/m(2). Compression models show that a 20 km-thick layer with a heat production as low as 0.05 mu W/m(3) within the shallow lithospheric mantle leads to strain localization in both the enriched mantle and the overlying crust. Strain localization depends exponentially on the temperature increase in the lithosphere section, which is controlled by the volume of metasomatized mantle and the intensity of the metasomatic enrichment in heat-producing elements. A heat production of 0.25 mu W/m(3) between 60 and 80 km depth results, for instance, in strains within and above the metasomatized mantle 5 times higher than in the surrounding lithosphere. Strain localization also depends on the location of the heat-producing domain and on the plate theological structure; deeper heat-producing domains and weaker plates leading to stronger localization. These results provide an explanation for strain localization in intraplate environments, leading to the formation of orogenic belts situated hundreds to thousands of kilometers away from known plate boundaries, as observed in the Neoproterozoic belts of Gondwana and in the present-day deformation of the Asian plate.
机译:传统上,对大陆岩石圈的变形建模是假设次大陆岩石圈地幔中的热量产生可以忽略不计。尽管这可能适合高度贫瘠的太古代岩石圈,但对地幔异种岩和岩石圈派生的镁铁质岩石的研究表明,由于模态作用,在生代和新元古代地区的地幔中可能产生的热量高达0.4μW / m(3)。交代。为了研究岩石圈地幔中生热元素的局部富集对大陆形变的影响,我们进行了一系列二维热力学模型模拟,模拟了1000 km长的岩石圈板块的变形,其中心部分包​​含: 200 km宽和20 km厚的地幔层,在40至80 km的深度之间产生的热量为0.05-0.25μW / m(3),从而导致表面热量的局部增加1-5 mW / m( 2)。压缩模型表明,在浅层岩石圈地幔中,厚度为20 km的层的热量产生低至0.05μW / m(3),从而导致在富集地幔和上覆地壳中都发生了应变局部化。应变的局域性取决于岩石圈截面的温度升高,这取决于交代化地幔的体积和生热元素交代富集的强度。在深度为60至80公里之间,产生的热量为0.25μW / m(3),例如,交化地幔内部和之上的应变是周围岩石圈的5倍。应变局部化还取决于发热区域的位置和板的神学结构。较深的生热域和较弱的板块导致更强的局部化。这些结果解释了板内环境中的应变局部化,导致形成了距已知板块边界数百至数千公里的造山带,正如在冈瓦纳的新元古代带和当今亚洲板块的变形中所观察到的那样。 。

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