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首页> 外文期刊>Tectonophysics: International Journal of Geotectonics and the Geology and Physics of the Interior of the Earth >Correlation between the Palaeozoic structures from West Iberian and Grand Banks margins using inversion of magnetic anomalies
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Correlation between the Palaeozoic structures from West Iberian and Grand Banks margins using inversion of magnetic anomalies

机译:西伊比利亚古大陆构造与格兰德河岸缘的磁异常反演

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摘要

The Ibero-Armorican Arc (IAA) is a huge geological structure of Pre-Cambrian origin, tightened during hercynian times and deeply affected by the opening of the Atlantic Ocean and the Bay of Biscay. Its remnants now lie in Iberia, north-western France and the Canadian Grand Banks margins. The qualitative correlation between these three blocks has been attempted by several authors (e.g. Lefort, J.P., 1980. Un 'Fit' structural de l'Atlantique Nord: arguments geologiques pour correler les marqueurs geophysiques reconnus sur les deux marges. Mar. Geol. 37, 355-369; Lefort, J.P., 1983. A new geophysical criterion to correlate the Acadian and Hercynian orogenies of Western Europe and Eastern America. Mem. Geol. Sec. Am. 158, 3-18; Galdeano, A., Miranda, J.M., Matte, P., Mouge, P., Rossignol, C., 1990. Aeromagnetic data: A tool for studying the Variscan are of Western Europe and its correlation with transatlantic structures. Tectonophysics 177, 293-305) using magnetic anomalies, mainly because they seem to preserve the hercynian zonation, in spite of the strong thermal and mechanical processes that took place during rifting and ocean spreading. In this paper, we present a new contribution to the study of the IAA structure based on the processing of a compilation of magnetic data from Iberia and Grand Banks margins. To interpret the magnetic signature, a Fourier-domain-based inversion technique was applied, considering a layer with a constant thickness of 10 km, and taking into account only the induced field. The digital terrain model was derived from ETOPO5 (ETOPO5, 1986. Relief map of the earth's surface. EOS 67, 121) and TerrainBase (TerrainBase, 1995. In: Row III, L.W., Hastings, D.A., Dunbar, P.K. (Eds.), Worldwide Digital Terrain Data, Documentation Manual, CD-ROM Release 1.0. GEODAS-NGDC Key to Geophysical Records. Documentation N. 30, April) databases. The pseudo-susceptibility distribution obtained was repositioned for the 156.5 Ma epoch, using the Srivastava and Verhoef [Srivastava, S.P., Verhoef, J., 1992. Evolution of Mesozoic sedimentary basins around the North Central Atlantic: a preliminary plate kinematic solution. In: Parnell, J. (Ed.), Basins on the Atlantic Seaboard: Petroleum Geology Sedimentology and Basin Evolution, Geological Society Special Publication No. 62, pp. 397-420] pole. Using this coherent magnetic framework, we can verify that the continuity between adjacent blocks is quite good, in terms of the amplitude, wavenumber and magnetic susceptibility pattern. If we accept that the magnetic properties can be taken as a marker of the hercynian zonation, as was verified in previous studies (Miranda, J.M., Galdeano, A., Rossignol, J.C., Mendes-Victor, L.A., 1989. Aeromagnetic anomalies in mainland Portugal and their tectonic implications. Earth Planet. Sci. Lett. 95, 161-177; Galdeano, A., Miranda, J.M., Matte, P., Mouge, P., Rossignol, C., 1990. Aeromagnetic data: A tool for studying the Variscan are of Western Europe and its correlation with transatlantic structures. Tectonophysics 177, 293-305; Socias, I., 1994. Estudios de los Elementos del Campo Magnetico en la Espana Peninsular a partir de Dates Aeromagmaneticos. Ph.D. thesis, University of Madrid), we can conclude that (1) the characteristic magnetic signature of Ossa Morena Zone is absent on the Iberian Margin and west of it; (2) no eastward continuation of the Collector Anomaly is found in Iberia; (3) only the inner zones of the Variscan Belt can be followed towards NW France; (4) there is a major (left lateral ?) strike-slip fault along the northern Portuguese shoreline that cuts the IAA and significantly displaces the once-contiguous variscan units. (C) 2000 Elsevier Science B.V. All rights reserved. [References: 46]
机译:伊比利亚-阿莫里奇弧(IAA)是前寒武纪起源的巨大地质结构,在海西时期被收紧,并受到大西洋和比斯开湾的开放的深刻影响。现在,它的残余地区位于伊比利亚,法国西北部和加拿大大银行地区。这三个区块之间的定性相关性已经由几位作者进行了尝试(例如,Lefort,JP,1980年。《北大西洋的'适合'的结构:论辩者论证》,《地学研究》,《地学研究》,Mar.Geol。,37年)。 ,355-369; Lefort,JP,1983.与西欧和东欧的阿卡迪亚和海西造山带相关的新地球物理标准,《地质学报》,美国第158卷,第3-18页; Galdeano,A。,米兰达, JM,Matte,P.,Mouge,P.,Rossignol,C.,1990.航空磁数据:研究西欧Variscan的工具及其与跨大西洋结构的关系。构造物理177,293-305),使用了磁异常,主要是因为尽管在裂谷和海洋扩散过程中发生了强烈的热力和机械作用,但它们似乎保留了海西星带。在本文中,我们基于Iberia和Grand Banks边界的磁数据汇编处理,为IAA结构研究提供了新的贡献。为了解释磁性特征,应用了基于傅立叶域的反演技术,考虑了恒定厚度为10 km的层,并且仅考虑了感应场。数字地形模型是从ETOPO5(ETOPO5,1986年。地球表面起伏图,EOS 67、121)和TerrainBase(TerrainBase,1995年)中获得的。资料来源:Row III,LW,Hastings,DA,Dunbar,PK(编辑)。 ,《全球数字地形数据》,文档手册,CD-ROM发行版1.0,GEODAS-NGDC地球物理记录的密钥,文档号:N.30,4月)。使用Srivastava和Verhoef [Srivastava,S.P.,Verhoef,J.,1992。北部中大西洋周围的中生代沉积盆地的演化:初步的板块运动学解决方案,将获得的拟磁化率分布重新定位到156.5 Ma时代。在:Parnell,J.(编辑),《大西洋沿岸盆地:石油地质沉积学和盆地演化》,地质学会特别出版物第62号,第397-420页]中。使用这种相干的磁性框架,我们可以验证相邻块之间在振幅,波数和磁化率模式方面的连续性非常好。如果我们接受磁特性可以作为海西星带的标志,如先前的研究(Miranda,JM,Galdeano,A.,Rossignol,JC,Mendes-Victor,LA,1989年所证实的那样)。葡萄牙及其构造意义,《地球行星》,《科学与通讯》,第95期,第161-177页; Galdeano,A。,米兰达,JM,Matte,体育,Mouge,体育,Rossignol,C.,1990年。研究Variscan是西欧及其与跨大西洋构造的关系,构造物理177,293-305; Socias,I.,1994. Estudios de los Elementos del Campo Magnetico en la Espana Peninsular a Partir de Dates Aeromagmaneticos。Ph.D.马德里大学的论文),我们可以得出以下结论:(1)伊比利亚边缘及其西部不存在Ossa Morena地带的特征性磁特征; (2)在伊比利亚没有发现收集器异常向东延伸; (3)只有瓦里斯卡纳带的内部区域可以追随法国西北部; (4)葡萄牙北部海岸线上有一条主要的(左外侧?)走滑断层,该断层切割了IAA,并大大取代了曾经连续的变扫描单元。 (C)2000 Elsevier Science B.V.保留所有权利。 [参考:46]

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