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Structural style of the Okcheon fold-thrust belt in the Taebaeksan Zone, Korea

机译:韩国太白山地区的Okcheon褶皱冲断带的构造样式

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Structural interpretation of the distinct map pattern defined by highly connected thrust traces in the map view of the Taebaeksan Zone provides insight into the structural style of the northeastern Okcheon Belt. The map pattern can generally be explained by either a folded imbricate fan or a hinterland dipping duplex. The same geometry could also be formed by a complex combination of major imbricate thrusts and their connecting splays, having the structural architecture of a typical fold-thrust belt. However, a folded imbricate fan model is not adequate to explain the absence of late Paleozoic to early Mesozoic strata (i.e. the Pyeongan Supergroup) between two major thrusts (viz. the Pyeongchang and Machari thrusts) in this area. This result further suggests that the Yeongwol area, the western part of the Taebaeksan Zone, is a duplex that corresponds to a more internal and deeper hinterland part of the fold-thrust belt, while the imbricate thrusts with low connectivity in the Taebaek area, the eastern part of the Taebaeksan Zone, indicate a more external and shallower foreland portion of the belt. In addition, cross-cutting relations and newly obtained sensitive high-resolution ion microprobe (SHRIMP) U-Pb zircon ages from a cross-cutting dike and syntectonic sedimentary rocks suggest limited thrust reactivation after the early Jurassic and early Tertiary, respectively. In spite of this, the original geometry of the foldthrust wedge in the Taebaeksan Zone remained well preserved. (C) 2015 Elsevier Ltd. All rights reserved.
机译:在太白山地区的地图视图中,由高度连接的逆冲径迹所定义的独特地图模式的结构解释,可让您深入了解东北Okcheon带的结构样式。映射模式通常可以用折叠的扇状扇形或腹地浸染双工来解释。相同的几何形状也可以由主要的波浪状推力及其连接张开的复杂组合形成,具有典型的褶皱-冲断带的结构。但是,折叠的扇状扇状模型不足以解释该地区两个主要逆冲推力(即平昌和马卡里逆冲推力)之间没有晚古生代到早中生代地层(即平安超群)。这个结果进一步表明,太白山带西部的灵越地区是一个双重地层,对应于褶皱冲断带的一个更内部和更深的腹地部分,而在太白山地区的胶结冲断带的连通性较低。太白山带的东部表示该带的外部和较浅的前陆部分。此外,横切关系和新近获得的敏感高分辨离子微探针(SHRIMP)U-Pb锆石年龄来自横切堤和同构造沉积岩,分别表明侏罗纪早期和第三纪早期的逆冲推力作用有限。尽管如此,太白山地区褶皱推力楔的原始几何形状仍然得到了很好的保留。 (C)2015 Elsevier Ltd.保留所有权利。

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