首页> 外文学位 >Sources of magnetic and gravity anomalies on the Scotian Shelf southeast of Cape Breton Island, Nova Scotia, and onshore-offshore geological correlations using geophysical modeling.
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Sources of magnetic and gravity anomalies on the Scotian Shelf southeast of Cape Breton Island, Nova Scotia, and onshore-offshore geological correlations using geophysical modeling.

机译:利用地球物理模型,在新斯科舍省布雷顿角岛东南部的斯科蒂大陆架上的磁性和重力异常源,以及陆上-海上地质相关性。

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摘要

The Scatarie Ridge Magnetic Anomalies (SRMA) form a prominent northeast-trending belt, 100 km long by 25 km wide, on the Scotian Shelf southeast of Cape Breton Island. Using the second vertical derivative magnetic map, the SRMA has been resolved into a linear anomaly trending east-northeast, and two large magnetic aureoles located north of the central part of the SRMA. Forward potential field models, constrained by seismic and well log data in the offshore and density and susceptibility measurements from onshore and some offshore units indicate that the southern margin of the linear anomaly is the northern margin of the Orpheus Graben. A south-dipping fault separates rocks of the Meguma terrane to the south from rocks of the Avalon terrane to the north of the graben. In the models, the Avalon terrane to a depth of about 15 km consists of five geological units with different magnetic susceptibility and density values. The source of the large linear anomaly is interpreted to be a belt of mafic volcanic rocks at a depth of 6--15 km. The large magnetic aureoles have associated gravity anomalies indicating that they are caused by granite plutons and magnetic rocks in the surrounding contact metamorphic aureoles. In the Gabarus Bay area, similar magnetic aureoles are associated with the Devonian Deep Cove granite and other intrusions. In contrast, two granitic bodies south of the Orpheus Graben in the Meguma terrane have densities and magnetic susceptibilities similar to Devonian plutons onshore in the Meguma terrane. Upper crustal units beneath the Avalon terrane offshore have higher susceptibility and lower density than units beneath the onshore Mira terrane, suggesting that the offshore area is a different part of the Avalon terrane, perhaps equivalent to the Antigonish Highlands or eastern Newfoundland.
机译:Scatarie Ridge磁异常(SRMA)在布雷顿角岛东南部的Scotian大陆架上,形成了一条长100公里,宽25公里的东北向突出带。使用第二个垂直导数磁图,SRMA已分解为东-东北向的线性异常,以及位于SRMA中部北部的两个大型磁极。正向势场模型受海洋中的地震和测井数据以及来自陆上和一些海洋单元的密度和磁化率测量的约束,表明线性异常的南边缘是Orpheus Graben的北边缘。向南倾斜的断层将南部的Meguma地貌的岩石与the石北部的Avalon地貌的岩石分隔开。在模型中,深度约15 km的阿瓦隆地层由五个具有不同磁化率和密度值的地质单元组成。线性大异常的根源被解释为在6--15 km深度的镁铁质火山岩带。大型磁性金闪石具有相关的重力异常,表明它们是由花岗岩接触岩和周围接触变质金闪石中的磁性岩石引起的。在Gabarus湾地区,泥盆纪深湾花岗岩和其他侵入带也伴有类似的磁性极光。相反,在Meguma地貌中Orpheus Graben以南的两个花岗岩体的密度和磁化率与Meguma地貌中陆上的泥盆系云母相似。与陆上米拉(Mira)陆下的单元相比,近海阿瓦隆(Avalon)地表以下的上地壳单元具有更高的敏感性和更低的密度,这表明近海区域是阿瓦隆(Avalon)地表的不同部分,可能等同于安蒂戈尼什高地或纽芬兰东部。

著录项

  • 作者

    Lyon, Sheri Ann.;

  • 作者单位

    Acadia University (Canada).;

  • 授予单位 Acadia University (Canada).;
  • 学科 Geology.;Geophysics.
  • 学位 M.Sc.
  • 年度 2008
  • 页码 170 p.
  • 总页数 170
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地质学;地球物理学;
  • 关键词

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