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马尼拉俯冲带北段增生楔前缘构造变形和精细结构
引用本文:高金尉,吴时国,姚永坚,陈传绪,宋陶然,王吉亮,孙金,张汉羽,马本俊,谢杨冰.马尼拉俯冲带北段增生楔前缘构造变形和精细结构[J].地球物理学报,2018,61(7):2845-2858.
作者姓名:高金尉  吴时国  姚永坚  陈传绪  宋陶然  王吉亮  孙金  张汉羽  马本俊  谢杨冰
作者单位:1. 国土资源部海底矿产资源重点实验室, 广州 510075;2. 中国科学院深海科学与工程研究所, 三亚 572000;3. 广州海洋地质调查局, 广州 510760;4. 海南省海底资源与探测技术重点实验室, 三亚 572000
基金项目:国土资源部海底矿产资源重点实验室开放基金(2016GMGS-DK154),国家自然科学基金项目(41476046,41576068,91428204)和中国地质调查局项目(DD20160138,1212011220116)联合资助.
摘    要:马尼拉俯冲带是南海的东部边界,记录了南海形成演化的关键信息,同时也是地震和海啸多发区域.本文利用过马尼拉俯冲带北段的高分辨率多道地震剖面,分析了研究区内海盆和海沟的沉积特征,精细刻画了区内增生楔前缘的构造变形、结构以及岩浆活动特征.研究区内增生楔下陆坡部分由盲冲断层、构造楔和叠瓦逆冲断层构成,逆冲断层归并于一条位于下中新统的滑脱面上,滑脱面向海方向的展布明显受到增生楔之下埋藏海山和基底隆起的影响;上陆坡的反射特征则因变形强烈和岩浆作用而难以识别;岩浆活动开始于晚中新世末期并持续至第四纪.马尼拉俯冲带北段增生楔的形成时间早于16.5 Ma,并通过前展式逆冲向南海方向扩展;马尼拉俯冲带的初始形成时间可能在晚渐新世,而此时南海海盆扩张仍在持续.南海东北缘19°N-21°N区域为南海北部陆坡向海盆的延伸,高度减薄的陆壳的俯冲造成马尼拉海沟北段几何形态明显地向东凹进.

关 键 词:马尼拉俯冲带  增生楔  构造变形  初始俯冲  多道地震  
收稿时间:2017-09-26

Tectonic deformation and fine structure of the frontal accretionary wedge,northern Manila subduction zone
GAO JinWei,WU ShiGuo,YAO YongJian,CHEN ChuanXu,SONG TaoRan,WANG JiLiang,SUN Jin,ZHANG HanYu,MA BenJun,XIE YangBing.Tectonic deformation and fine structure of the frontal accretionary wedge,northern Manila subduction zone[J].Chinese Journal of Geophysics,2018,61(7):2845-2858.
Authors:GAO JinWei  WU ShiGuo  YAO YongJian  CHEN ChuanXu  SONG TaoRan  WANG JiLiang  SUN Jin  ZHANG HanYu  MA BenJun  XIE YangBing
Institution:1. Key Laboratory of Marine Mineral Resources, Ministry of Land and Resources, Guangzhou 510075, China;2. Institute of Deep-sea Science and Engineering, Chinese Academy of Sciences, Sanya 572000, China;3. Guangzhou Marine Geological Survey, Guangzhou 510760, China;4. Key Laboratory of Submarine Resources and Prospecting, Hainan Province, Sanya 572000, China
Abstract:The Manila subduction zone is the eastern boundary of the South China Sea (SCS), which records key information on the evolution of the SCS, also is an area with active earthquakes and tsunamis. Using high resolution multi-channel seismic data across the northern Manila subduction zone, this paper characterizes the tectonic deformation and structure of the frontal accretionary wedge as well as magmatism and sedimentary features of the oceanic basin and trench in the subduction zone. Results show that the lower slope of accretionary wedge consists mainly of imbricated thrusts, structural wedges and blind thrusts that act as frontal faults, whereas the internal architecture of the upper slope is difficult to identify because of intense deformation and magmatism. All the thrust faults merged into a lower Miocene decollement which cuts off the middle Miocene strata and can be traced upward into the Pliocene strata, indicating that the fault is influenced by local buried seamounts and basement uplift below the accretionary wedge. Magmatic activities lasted from late Miocene to Quaternary in the oceanic basin, trench and accretionary wedge in the study area. We suggest that the accretionary wedge of the northern Manila subduction zone begun to thrust before 16.5 Ma and is still propagating to the SCS through piggyback thrusting at present. The Manila subduction zone probably initiated in the late Oligocene when the oceanic basin of the SCS continued to spread. The region of hyper-extended continental crust extends from the continental slope to the oceanic basin between 19°N and 21°N in the northeastern SCS. The subduction of this hyper-extended continental crust resulted in a significant variation in the geometry of the northern Manila trench, which shows a concave eastward pattern to the Luzon Arc.
Keywords:Manila subduction zone  Accretionary wedge  Tectonic deformation  Incipient subduction  Multi-channel seismic
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