下二叠世至中新世伊比利亚的视极漂移路径及其与运动演化的关系。

J. Schott
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引用次数: 4

摘要

对伊比利亚板块在二叠纪至中新世范围内可靠的古磁极进行了评述。在剔除属于移位或变形区域或代表重磁化的数据后,选择11个磁极。利用该数据库,构造了视极漂移路径(APW)。使用了两种方法。第一种是改进的滑动窗口方法。第二种是最近在APW建模中发展起来的小电路拟合。该方法仅适用于下二叠统-下侏罗统径迹。最后,验证了该方法与已知伊比利亚飞机运动模型的一致性。粗略地说,有两种模型描述伊比利亚相对于欧洲的进化:单一旋转模型和左移模型。结果,对于下二叠统-下侏罗统,这两种模式在欧洲和伊比利亚的APW之间得出了统计上等效的拟合结果。因此,这清楚地表明,目前缺乏palcommagnetic数据阻止了我们对伊比利亚的动力学演化给出严密的约束。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Lower Permian to Miocene apparent polar wander path for Iberia and its bearings on kinematic evolution.
A review of the reliable paleomagnetic poles for the Iberian plate is given in the range Permian to Miocene. After rejection of data belonging to displaced of deformed areas, or representing remagnetizations, 11 poles are selected. Using this data base, an Apparent Polar Wander Path (APW) is constructed. Two methods are used. The first one is a refined sliding window method. Ihe second one is the small circie fitting recently developped in APW modelling. This method is appropiate for the lower Perrnian-lower Jurassic track only. Finaily, the consistency of the APW with known kinematic models for Iberia is tested. There are, roughly speaking, two kinds of models describing the evolution of Iberia relative to Europe: single rotation models and left-lateral shift models. As a result, both models lead to statistically equivalent fits between the European and iberian APW’s, for the lower Permian-lower Jurassic track. Thus, it is clearly shown that the current lack of palcomagnetic data prevents us from giving close constraints to the kinernatic evolution of Iberia.
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