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Seismic and aseismic slip on the Central Peru megathrust

机译:秘鲁中部特大推力上的地震和地震

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Slip on a subduction megathrust can be seismic or aseismic, with the two modes of slip complementing each other in time and space to accommodate the long-term plate motions. Although slip is almost purely aseismic at depths greater than about 40 km, heterogeneous surface strain suggests that both modes of slip occur at shallower depths, with aseismic slip resulting from steady or transient creep in the interseismic and postseismic periods. Thus, active faults seem to comprise areas that slip mostly during earthquakes, and areas that mostly slip aseismically. The size, location and frequency of earthquakes that a megathrust can generate thus depend on where and when aseismic creep is taking place, and what fraction of the long-term slip rate it accounts for. Here we address this issue by focusing on the central Peru megathrust. We show that the Pisco earthquake, with moment magnitude M_w = 8.0, ruptured two asperities within a patch that had remained locked in the interseismic period, and triggered aseismic frictional afterslip on two adjacent patches. The most prominent patch of afterslip coincides with the subducting Nazca ridge, an area also characterized by low interseismic coupling, which seems to have repeatedly acted as a barrier to seismic rupture propagation in the past. The seismogenic portion of the megathrust thus appears to be composed of interfingering rate-weakening and rate-strengthening patches. The rate-strengthening patches contribute to a high proportion of aseismic slip, and determine the extent and frequency of large interplate earthquakes. Aseismic slip accounts for as much as 50-70% of the slip budget on the seismogenic portion of the megathrust in central Peru, and the return period of earthquakes with M_w = 8.0 in the Pisco area is estimated to be 250 years.
机译:俯冲超大推力上的滑动可以是地震的也可以是地震的,两种滑动模式在时间和空间上相互补充,以适应板块的长期运动。尽管在大于约40 km的深度处滑移几乎完全是抗震的,但非均质的表面应变表明这两种滑模都发生在较浅的深度,而抗震滑移是由于地震之间和地震后的稳定或瞬态蠕变引起的。因此,活动断层似乎包括在地震过程中主要滑动的区域,以及大部分由于地震而滑动的区域。因此,特大推力可能产生的地震的规模,位置和频率取决于地震发生在何处,何时发生,以及占长期滑移率的比例。在这里,我们将重点放在秘鲁中部的大推力上来解决这个问题。我们显示,Misco震级为M_w = 8.0的Pisco地震破坏了一个在地震间隔期间保持锁定状态的斑块中的两个凹凸,并在两个相邻的斑块上引发了地震摩擦后滑。滑移最突出的地块与俯冲的纳斯卡海脊相吻合,纳斯卡海脊也以低地震耦合为特征,过去似乎一再成为阻碍地震破裂传播的障碍。因此,超大推力的震源部分似乎由指间减弱速率和加强速率的斑块组成。加强速度的板块引起了很大比例的地震滑移,并确定了大板块间地震的程度和频率。秘鲁中部特大推力的发震部分,抗震滑移占滑移预算的50%至70%,而皮斯科地区M_w = 8.0的地震的重现期估计为250年。

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  • 来源
    《Nature》 |2010年第7294期|p.78-81|共4页
  • 作者单位

    Institut de Recherche pour le Developpement, 44 Boulevard de Dunkerque, 13572 Marseille cedex 02, France lnstituto Geofisico del Peru, Calle Badajos 169, Urb. Mayorazgo, Ate, Lima, Peru Laboratoire de Geophysique Interne et Tectonophysique, Universite Joseph Fourier/CNRS/IRD/LCPC, Observatoire des Sciences de I'Univers de Grenoble, BP 53, 38041 Grenoble cedex 9, France Laboratoire des Mecanismes de Transfert en Geologie, Universite Paul Sabatier/CNRS/IRD, Observatoire Midi-Pyrenees, 14 Avenue Edouard Belin, 31400 Toulouse, France;

    rnTectonics Observatory, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA;

    rnlnstituto Geofisico del Peru, Calle Badajos 169, Urb. Mayorazgo, Ate, Lima, Peru;

    rnTectonics Observatory, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA Ashima Research, Pasadena, 600 S. Lake Ave., Pasadena, California 91106, USA;

    rnGeoAzur, 250 Rue Albert Einstein, 06560 Valbonne, France;

    rnInstitut de Recherche pour le Developpement, 44 Boulevard de Dunkerque, 13572 Marseille cedex 02, France lnstituto Geofisico del Peru, Calle Badajos 169, Urb. Mayorazgo, Ate, Lima, Peru Laboratoire de Geophysique Interne et Tectonophysique, Universite Joseph Fourier/CNRS/IRD/LCPC, Observatoire des Sciences de I'Univers de Grenoble, BP 53, 38041 Grenoble cedex 9, France;

    rnInstitut de Recherche pour le Developpement, 44 Boulevard de Dunkerque, 13572 Marseille cedex 02, France GeoAzur, 250 Rue Albert Einstein, 06560 Valbonne, France;

    rnTectonics Observatory, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA;

    rnInstitut de Recherche pour le Developpement, 44 Boulevard de Dunkerque, 13572 Marseille cedex 02, France lnstituto Geofisico del Peru, Calle Badajos 169, Urb. Mayorazgo, Ate, Lima, Peru Laboratoire des Mecanismes de Transfert en Geologie, Universite Paul Sabatier/CNRS/IRD, Observatoire Midi-Pyrenees, 14 Avenue Edouard Belin, 31400 Toulouse, France;

    rnDepartment of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, California 95064, USA Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94550, USA;

    rnInstitut de Recherche pour le Developpement, 44 Boulevard de Dunkerque, 13572 Marseille cedex 02, France;

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