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Early Permian Pangea 'B' to Late Permian Pangea 'A'

机译:早二叠纪Pangea'B'到晚二叠纪Pangea'A'

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The pre-drift Wegenerian model of Pangea is almost universally accepted, but debate exists on its pre-Jurassic configuration since Ted Irving introduced Pangea 'B' by placing Gondwana farther to the east by ~3000 km with respect to Laurasia on the basis of paleomagnetic data. New paleomagnetic data from radiometrically dated Early Permian volcanic rocks from parts of Adria that are teconically coherent with Africa (Gondwana), integrated with published coeval data from Gondwana and Laurasia, again only from igneous rocks, fully support a Pangea 'B' configuration in the Araly Permian. The use of paleomagnetic data strictly from igneous rocks excludes artifact from sedimentary inclination error as a contributing explanation for Pangea 'B'. The ultimate option to reject Pangea 'B' is to abandon the geocentric axial dipole hypothesis by introducing a significant non-dipole (zonal octupole) component in the Late Paleozoic time-averaged geomagnetic field. We demonstrate, however, by using a dataset consisting entirely of paleomagnetic directions with low inclinations from sampling sites confined to one hemisphere from Gondwana as well as Laurasia that the effects of a zonal octupole field contribution would not explain away the paleomagnetic evidence for Pangea 'B' in the Early Permian. We teherefore regard the paleomagnetic evidence for an Early Permian Pangea "b" as robust. The transformation from Pangea 'B' to Pangea 'A' took place during the Permian because Late Permian paleomagnetic data allow a Pangea 'A' configuration. We therefore review geological evidence from the literrature in support of an intra-Pangea dextral megashear system. The transformation occurred after the cooling of the Variscan mega-suture and lasted ~20 Myr. In this interval, the Neotethys Ocean opened between India/Arabia and the Cimmerian microcontinents in the east, while widespread lithospheric wrenching and magmatism took place in the west around the Adriatic promontory. The general distribution of plate boundaries and resulting adriving forces are qualitatively consistent with a right-lateral shear cou;oe between Gondwana and Laurasia during the Permian. Transcurrent plate boundaries associated with the Pangea transformation reactivated Variscan shear zones and were subsequently exploited by the opening of western Neotethyan seaways in the Jurassic.
机译:Pangea的漂移前Wegenerian模型几乎被普遍接受,但是自从Ted Irving在古地磁的基础上,将Gondwana相对于Laurasia定位在距东至东约3000 km的地方将Gondwana推向更远的东方,从而引入了Pangea'B'以来,就对其侏罗纪前的构造存在争议。数据。来自与非洲(冈瓦纳)在地学上相干的阿德里亚部分地区的放射性二叠纪早期火山岩的新古地磁数据,再加上来自冈瓦纳和劳拉西亚的已发布的同年代数据,同样仅来自火成岩,完全支持了该地区的Pangea'B'构型。阿拉里二叠纪。严格使用来自火成岩的古磁数据,将人为因素排除在沉积倾角误差之外,这是对Pangea'B'的一个解释。拒绝Pangea'B'的最终选择是通过在晚古生代时间平均地磁场中引入显着的非偶极(区域八极)分量来放弃地心轴向偶极子假设。但是,我们通过使用一个完全由古磁方向组成的数据集来证明,该数据集来自冈瓦纳和劳拉西亚的一个局限在半球采样点的低倾斜度,纬向八极磁场贡献的影响并不能解释Pangea'B的古磁证据。在二叠纪初期。因此,我们认为早二叠世Pangea“ b”的古磁证据是可靠的。在二叠纪发生了从Pangea'B'到Pangea'A'的转变,因为晚二叠纪古地磁数据允许Pangea'A'构造。因此,我们从文献学中回顾了地质学证据,以支持庞加内右旋巨剪系统。变形发生在Variscan大型缝线冷却后,持续约20 Myr。在此间隔内,新特提斯海域在印度/阿拉伯和东部的西里米亚微大陆之间开放,而在亚得里亚海角周围的西部则发生了广泛的岩石圈扭动和岩浆作用。板块边界的总体分布和由此产生的推动力在质量上与二叠纪冈瓦纳和劳拉西亚之间的右旋剪切速率一致。与Pangea转换相关的跨流板块边界重新激活了Variscan剪切带,随后被侏罗纪西部新特提斯海道开放所开发。

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