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首页> 外文期刊>Tectonics >Imaging the crustal structure of the Central Iberian Zone (Variscan Belt): The ALCUDIA deep seismic reflection transect
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Imaging the crustal structure of the Central Iberian Zone (Variscan Belt): The ALCUDIA deep seismic reflection transect

机译:成像伊比利亚中部地区(瓦里斯坎地带)的地壳结构:ALCUDIA深地震反射剖面

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摘要

ALCUDIA is a 230 km long, vertical incidence deep seismic reflection transect acquired in spring 2007 across the southern Central Iberian Zone (part of the pre-Mesozoic Gondwana paleocontinent) of the Variscan Orogen of Spain. The carefully designed acquisition parameters resulted in a 20 s TWTT deep, 60-90 fold, high-resolution seismic reflection transect. The processed image shows a weakly reflective upper crust (the scarce reflectivity matching structures identified at surface), a thick, highly reflective and laminated lower crust, and a flat Moho located at 10 s TWTT (~30 km depth). The transect can be divided into three segments with different structural styles in the lower crust. In the central segment, the lower crust is imaged by regular, horizontal and parallel reflectors, whereas in the northern and southern segments it displays oblique reflectors interpreted as an important thrust (north) and tectonic wedging involving the mantle (south). The ALCUDIA seismic image shows that in an intracontinental orogenic crust, far from the suture zones, the upper and lower crust may react differently to shortening in different sectors, which is taken as evidence for decoupling. The interpreted structures, as deduced from surface geology and the seismic image, show that deformation was distributed homogeneously in the upper crust, whereas it was concentrated in wedge/thrust structures at specific sectors in the lower crust. The seismic image also shows the location of late Variscan faults in spatial association with the lower crustal thickened areas.
机译:ALCUDIA是一条长230公里的垂直入射深地震反射样带,于2007年春季在西班牙瓦里斯卡造山带的南部伊比利亚中部南部地区(中生代冈瓦纳前古大陆的一部分)获得。精心设计的采集参数产生了20 s TWTT深度,60-90倍的高分辨率地震反射样条。处理后的图像显示出反射较弱的上地壳(在表面识别出稀疏的反射率匹配结构),厚的,反射率高且层压的下地壳以及位于TWTT(约30 km深度)处的平坦莫霍面。下地壳中的断面可分为三段,每段具有不同的结构样式。在中央部分,下部地壳由规则的,水平的和平行的反射器成像,而在北部和南部的部分中,则显示倾斜的反射器,这被解释为重要的推力(北)和涉及地幔的构造楔(南)。 ALCUDIA地震图像显示,在距离缝合线区域较远的大陆造山地壳中,上,下地壳对不同区域的缩短可能有不同的反应,这被认为是解耦的证据。从地表地质和地震图像推算出的解释结构表明,变形在上地壳中均匀分布,而变形集中在下地壳中特定区域的楔/推力结构中。地震图像还显示了晚期瓦里斯坎断层的位置,与下地壳增厚区域在空间上相关。

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  • 来源
    《Tectonics 》 |2012年第3期| p.tc3017.1-tc3017.21| 共21页
  • 作者单位

    Departamento de Geodinamica, Facultad de Ciencias, Universidad de Granada, E-18071 Granada, Spain;

    Instituto de Ciencias de la Tierra 'Jaume Almera,' CSIC, Barcelona,Spain;

    Instituto de Ciencias de la Tierra 'Jaume Almera,' CSIC, Barcelona,Spain,Department of Earth Science, Rice University, Houston, Texas, USA;

    Departamento de Geodinamica, Facultad de Ciencias, Universidad de Granada, Granada, Spain;

    Departamento de Geologia, Universidad de Salamanca, Salamanca,Spain;

    Instituto de Ciencias de la Tierra 'Jaume Almera,' CSIC, Barcelona,Spain;

    Departamento de Geodinamica, Facultad de Ciencias, Universidad de Granada, Granada, Spain;

    Departamento de Geodinamica, Facultad de Ciencias, Universidad de Granada, Granada, Spain;

    Instituto Geologico y Minero de Espafia, Madrid, Spain;

    Departamento de Geodinamica, Universidad Complutense de Madrid,Madrid, Spain;

    Instituto Geologico y Minero de Espafia, Madrid, Spain;

    Instituto Geologico y Minero de Espafia, Madrid, Spain;

    Departamento de Geodinamica, Facultad de Ciencias, Universidad de Granada, Granada, Spain;

    Instituto de Ciencias de la Tierra 'Jaume Almera,' CSIC, Barcelona,Spain;

    Instituto Geologico y Minero de Espafia, Madrid, Spain;

    Escuela Politecnica Universitaria de Almaden, Universidad de Castilla-La Mancha, Almaden, Spain;

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