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Mesozoic plate tectonic reconstruction of the Carpathian region

机译:喀尔巴阡地区中生代板块构造重建

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摘要

Palaeomagnetic, palaeobiogeographic and structural comparisons of different parts of the Alpine–Carpathian region suggest that four terranes comprise this area: the Alcapa, Tisza, Dacia and Adria terranes. These terranes are composed of different Mesozoic continental and oceanic fragments that were each assembled during a complex Late Jurassic–Cretaceous–Palaeogene history. Palaeomagnetic and tectonic data suggest that the Carpathians are built up by two major oroclinal bends. The Alcapa bend has the Meliata oceanic unit, correlated with the Dinaric Vardar ophiolite, in its core. It is composed of the Western Carpathians, Eastern Alps and Southern Alcapa units (Transdanubian Range, Bükk). This terrane finds its continuation in the High Karst margin of the Dinarides. Further elements of the Alcapa terrane are thought to be derived from collided microcontinents: Czorsztyn in the N and a carbonate unit (Tisza?) in the SE. The Tisza–Dacia bend has the Vardar oceanic unit in its core. It is composed of the Bihor and Getic microcontinents. This terrane finds its continuation in the Serbo–Macedonian Massif of the Balkans. The Bihor–Getic microcontinent originally laid east of the Western Carpathians and filled the present Carpathian embayment in the Late Palaeozoic–Early Mesozoic. The Vardar ocean occupied an intermediate position between the Western Carpathian–Austroalpine–Transdanubian–High Karst margin and the Bihor–Getic–Serbo–Macedonian microcontinent. The Vardar and Pindos oceans were opened in the heart of the Mediterranean–Adriatic microcontinent in the Late Permian–Middle Triassic. Vardar subducted by the end of Jurassic, causing the Bihor–Getic–Serbo–Macedonian microcontinent to collide with the internal Dinaric–Western Carpathian margin. An external Penninic–Váhic ocean tract began opening in the Early Jurassic, separating the Austroalpine–Western Carpathian microcontinent (and its fauna) from the European shelf. Further east, the Severin–Ceahlau–Magura also began opening in the Early Jurassic, but final separation of the Bihor–Getic ribbon (and its fauna) from the European shelf did not take place until the late Middle Jurassic. The Alcapa and the Tisza–Dacia were bending during the Albian–Maastrichtian. The two oroclinal bends were finally opposed and pushed into the gates of the Carpathian embayment during the Palaeogene and Neogene. At that time, the main N–S shortening in distant Alpine and Hellenic sectors was linked by a broader right-lateral shear zone along the former Vardar suture.
机译:高山-喀尔巴阡地区不同部分的古地磁,古生物地理和结构比较表明,该地区包括四个地层:阿尔卡帕,蒂萨,达契亚和亚德里亚。这些地层由不同的中生代大陆和海洋碎片组成,每个碎片都是在侏罗纪-白垩纪-古近纪的复杂历史中组装而成的。古地磁和构造数据表明,喀尔巴阡山脉是由两个主要的口斜弯曲形成的。 Alcapa弯道的核心有Meliata海洋单元,与Dinaric Vardar蛇绿岩相关。它由西喀尔巴阡山脉,东阿尔卑斯山和南阿尔卡帕山脉(Transdanubian Range,Bükk)组成。该地貌在第纳里德斯的高喀斯特边缘发现了它的延续。 Alcapa地层的其他元素被认为是由碰撞的微大陆衍生而来的:N处的Czorsztyn和SE处的碳酸盐单元(Tisza?)。 Tisza–Dacia弯道的核心是Vardar海洋单元。它由Bihor和Getic微大陆组成。在巴尔干地区的塞尔维亚-马其顿地块中发现了这种地层。 Bihor-Getic微大陆最初位于西喀尔巴阡山脉以东,填补了目前的喀尔巴阡山脉在古生代晚期至中生代晚期的禁区。瓦尔达尔海洋在西喀尔巴阡—奥索阿平—Transdanubian—高喀斯特边缘与比霍尔—吉特—塞尔博—马其顿微大陆之间处于中间位置。 Vardar和Pindos海洋在二叠纪中三叠世晚期的地中海-亚得里亚海微大陆的心脏地带开放。 Vardar在侏罗纪末期俯冲,使Bihor–Getic–Serbo–Macedonian微大陆与内部Dinaric–Western喀尔巴阡边缘碰撞。外部的Penninic–Váhic海洋道在侏罗纪早期开始开放,将奥古拉山—西喀尔巴阡山脉的微大陆(及其动物群)与欧洲大陆架分开。再往东,Severin-Ceahlau-Magura也开始在侏罗纪早期开放,但是直到欧洲中侏罗纪晚期,Bihor-Getic丝带(及其动物群)才与欧洲大陆架最终分离。 Alcapa和Tisza–Dacia在Albian–Maastrichtian期间弯曲。在古近纪和新近纪期间,最后两个对口折弯被对向并推入喀尔巴阡河口的大门。当时,在远处的阿尔卑斯和希腊地区,主要的南北向缩短是由沿着前瓦尔达尔缝合线的较宽的右向剪切带联系在一起的。

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