首页> 外文期刊>Journal of geophysical research. Solid earth: JGR >Nature of the lithosphere across the Variscan orogen of SW Iberia: Dense wide-angle seismic reflection data
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Nature of the lithosphere across the Variscan orogen of SW Iberia: Dense wide-angle seismic reflection data

机译:伊比利亚西南部瓦里斯坎造山带岩石圈的性质:密集的广角地震反射数据

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Two wide-angle seismic transects have been acquired across the SW Iberian Massif, They crossed three major geological zones (South Portuguese Zone, Ossa-Morena Zone, and Central Iberian Zone), with their tectonic contacts and the Pyrite Belt being of greatest interest. A total of 690 digital seismic recording instruments (650 Texans and 40 Reftek 3 component units) from the IRIS-PASSCAL Instrument Pool were used. The transects (A and B) are each approximately 300 km long and consist of 3 and 6 shot points, respectively, with an approximately 60-km shot point interval. The charge sizes range from 1000 kg at the edges to 500 kg at the center. These recently acquired experiments were designed to provide velocity constraints on the lithosphere and to complement the previously acquired normal incidence seismic profile IBERSEIS. Both data sets are part of the SW Iberia project, which was developed within the EUROPROBE program and designed to address fundamental questions about the nature and dynamics of the Variscan lithosphere The acquisition parameters provide closely spaced wide-angle seismic images of the lithosphere beneath SW Iberia. In transect A, the station spacing was on average 400 m, while along transect B, the receiver spacing was approximately 150 m. Because of this close trace spacing, the lateral continuity of the seismic arrivals is greatly improved. Frequency analysis revealed that the recorded events feature relatively low frequencies (6-25 Hz) After processing, the shot records show high-amplitude and well-defined arrivals. The interpreted PmP arrival, located at approximately 11 s (normal incidence traveltime), is characterized by high amplitude and relatively low frequency (6-12 Hz), A well-defined Pn arrival appears at offsets beyond 120 km. At far offsets greater than 180 km, an upper mantle reflection is observed. Furthermore, within the upper crust, the shots records feature a relatively high-velocity arrival, located at 4-5-s normal incidence traveltime The analysis of this arrival indicates that it probably corresponds to the top of the Iberian Reflective Body identified in the IBERSEIS deep seismic profile The velocity models obtained by forward modeling show a complex crust, especially in the middle crust. The velocity models are the most detailed ones that have been produced in the area and contain a large amount of new features that are relevant to the understanding of the composition of the crust and upper mantle beneath the zone. The velocity depth functions derived from the velocity models have higher middle crustal velocities than the average in other continental areas, A comparison between laboratory seismic velocity measurements and the velocities of the models was carried out in order to estimate the crustal and the upper mantle composition. Results indicate that the high middle crust velocities correspond to rocks of a mafic composition. The combined data set reveals new aspects related to the lithospheric evolution of this transpressive orogen and allows us to attempt an interpretative cross section of the upper lithosphere in SW Iberia.
机译:在西南伊比利亚地块上已采集到两个广角地震样带,它们穿越了三个主要地质带(南葡萄牙带,奥萨-莫雷纳带和伊比利亚中部带),它们的构造接触和黄铁矿带引起了人们的极大兴趣。 IRIS-PASSCAL仪器库总共使用了690台数字地震记录仪器(650台德州仪器和40台Reftek 3组件)。样条线(A和B)的长度分别约为300公里,分别由3个和6个射击点组成,间隔约为60公里。装药量从边缘的1000千克到中心的500千克不等。这些最近获得的实验旨在提供对岩石圈的速度限制,并补充先前获得的法向入射地震剖面IBERSEIS。这两个数据集都是SW Iberia项目的一部分,该项目是在EUROPROBE计划中开发的,旨在解决有关Variscan岩石圈的性质和动力学的基本问题。采集参数提供了SW Iberia下方岩石圈的近距离广角地震图像。在样带A中,站间距平均为400 m,而在样带B上,接收器间距约为150 m。由于这种紧密的走线间隔,极大地改善了地震波到达的横向连续性。频率分析显示,所记录的事件具有相对较低的频率(6-25 Hz),经过处理后,镜头记录显示出高振幅和明确的到达。解释的PmP到达时间大约为11 s(垂直入射行进时间),具有高振幅和相对较低的频率(6-12 Hz)的特征。PnP到达的定义清晰,出现在120 km以上的偏移处。在远大于180 km的偏移处,观察到上地幔反射。此外,在上地壳内,射击记录的特征是相对高速到达,位于法线入射传播时间4-5-s。对该到达的分析表明,它可能对应于IBERSEIS中识别的伊比利亚反光体的顶部深层地震剖面通过正演模拟获得的速度模型显示出复杂的地壳,尤其是在中地壳中。速度模型是该区域中最详细的模型,其中包含大量与了解该区域以下地壳和上地幔成分有关的新特征。从速度模型推导出的速度深度函数的中地壳速度要比其他大陆地区的平均值高。为了估计地壳和上地幔的成分,对实验室地震速度测量值和模型速度进行了比较。结果表明,较高的中地壳速度对应于镁铁质成分的岩石。合并后的数据集揭示了与该超压造山带岩石圈演化有关的新方面,并允许我们尝试对伊比利亚西南部岩石圈上部进行解释性的剖析。

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