The RAMESSES experiment—V. Crustal accretion at axial volcanic ridge segments—a gravity study at 57°45'N on the slow spreading Reykjanes Ridge     

Christine Peirce  Debbie A. Navin 《Geophysical Journal International》2002,149(1):76-94

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浙江省地壳构造综合研究   总被引：1，自引：0，他引：1  

杨文采  何良军  江金生  钟庆华  陈勐韬 《地质学报》2022,96(1):95-103

浙江地区基岩为大面积的中生代火山岩覆盖，对了解地壳深部的组成结构造成困难。本文通过对布格重力异常和航磁异常数据进行小波多尺度分解，深入地了解浙江省不同深度的地壳结构，结合地震和大地电磁资料，取得地壳构造的三维信息。根据浙江地区位场的多尺度分解结果，可以将浙江省上地壳细分为六个构造单元：下扬子南部浙北陆沿带、江山- 绍兴古陆块碰撞拼合带、古华夏陆块北沿带、丽水- 余姚早古生代陆缘俯冲带、浙东侏罗纪白垩纪火山岩带和杭嘉地块。在上地壳的六个构造单元中，江山- 绍兴古陆块碰撞拼合带、浙东火山岩带和杭嘉地块具有高密度强磁性的属性；而下扬子南部浙北陆沿带、古华夏陆块北沿带和丽水- 余姚早古生代陆缘俯冲带具有低密度的属性，与它们在古生代受安第斯型大洋俯冲作用有关。浙江省下地壳只有西—西南部低密度区、中部杭州- 嵊州- 苍南中密度带和杭嘉- 舟山群岛- 滨海高密度带三个构造区。东部的中生代陆缘火山弧和杭嘉地块在中下地壳连为一体；江山- 绍兴古陆块碰撞拼合带和古华夏陆块北沿带也连为一体。浙江省中下地壳的格局主要受西太平洋俯冲带向东后撤的影响。  相似文献   

根据重力数据研究黄海周边断裂带在海区的延伸   总被引：43，自引：10，他引：43       下载免费PDF全文

郝天珧  Suh Mancheol  王谦身  CHOI Suckwon  江为为  宋海斌  阎晓蔚  刘建华  姚长利 《地球物理学报》2002,45(3):385-397

根据黄海及周边地区的布格重力资料,通过解析延拓、目标场提取、任意水平方向导数计算、离散小波变换等处理,得到各种有关断裂的信息.经过与地质资料综合分析,选择123°E经线为典型剖面,以地震资料建立初始模型,对该剖面进行重力正反演迭代拟合,最终得到各模块的密度参数及分布,并在此基础上分析了研究区主要断裂的地质地球物理特征,给出了研究区的断裂带、块体结合带分布图.重点对朝鲜半岛西缘断裂带和五莲-青岛-荣城断裂带进行了讨论,提出五莲-青岛-荣城断裂带并未进入朝鲜半岛与临津江断裂带相连.认为朝鲜半岛西缘断裂带西侧属于扬子块体的部分曾受北向应力作用向北发生了平移.由五莲-青岛-荣城断裂带和南黄海北部断裂带、朝鲜半岛西缘断裂带及济州岛南缘断裂带共同组成的断裂带应该是中朝与扬子块体之间的结合带.  相似文献   

云南三江造山带近东西向构造特征及其研究意义   总被引：4，自引：0，他引：4  

管烨  王安建  曹殿华  秦德厚 《地质学报》2004,78(4):494-499

对地球物理位场进行处理分析的结果表明 ,在云南三江造山带近南—北向为主的构造框架背景中 ,存在有多处与之相互正交或斜交的近东—西向构造 ,这些近东西方向展布的构造呈现出隐伏或深部构造特点。在布格重力异常影像中表现为大波长、幅值低的深部构造带特征 ;地质上表现为一系列近东—西向出现的断裂、岩体和矿床的成带分布 ;遥感解译结果则表现出在三江造山带内有多条平行展布的浅埋深东西向隐伏构造带。本文结合地质、地球物理地震波速信息等资料 ,对该区近东西向构造特征及分布规律进行探讨后提出三江地区存在的近东西—向展布的近东西向构造可能是青藏高原主碰撞造山后 ,各块体物质向东南挤出的深部物质流变构造的反映 ,也可能是在三江造山带挤压碰撞及走滑拉张环境下的伸展构造或老构造的再活化。它的形成机制可能类似于青藏高原南部南—北向伸展构造 (裂谷 )。近东—西向构造的深入研究和成因再认识对于深入分析云南三江地区复杂的地质构造 ,区域地壳演化历史 ,特别对是重新认识区域成矿规律、指导找矿具有重要意义  相似文献   

Magmatic underplating beneath the Rajmahal Traps: Gravity signature and derived 3-D configuration     

A. P. Singh  Niraj Kumar  Bijendra Singh 《Journal of Earth System Science》2004,113(4):759-769

The early Cretaceous thermal perturbation beneath the eastern continental margin of the Indian shield resulted in the eruption of the Rajmahal Traps. To understand the impact of the magmatic process that originated in the deep mantle on the lower crustal level of the eastern Indian shield and adjoining Bengal basin the conspicuous gravity anomalies observed over the region have been modelled integrating with available geophysical information. The 3-D gravity modelling has delineated 10–15 km thick high-density (ρ = 3.02 g/cm³) accreted igneous layer at the base of the crust beneath the Rajmahal Traps. Thickness of this layer varies from 16 km to the west of the Rajmahal towards north to about 12 km near Kharagpur towards south and about 18 km to the east of the Raniganj in the central part of the region. The greater thickness of the magmatic body beneath the central part of the region presents itself as the locus of the potential feeder channel for the Rajmahal Traps. It is suggested that the crustal accretion is the imprint of the mantle thermal perturbation, over which the eastern margin of the eastern Indian shield opened around 117 Ma ago. The nosing of the crustal accretion in the down south suggests the possible imprint of the subsequent magmatic intrusion along the plume path.  相似文献   

Wavelet and multitaper coherence methods for assessing the elastic thickness of the Irish Atlantic margin     

E. Daly  C. Brown  C. P. Stark  C. J. Ebinger 《Geophysical Journal International》2004,159(2):445-459

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New views of the spherical Bouguer gravity anomaly   总被引：7，自引：0，他引：7  

P. Vaní&#;ek  R. Tenzer  L. E. Sjöberg  Z. Martinec  W. E. Featherstone 《Geophysical Journal International》2004,159(2):460-472

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Mean Free-Air Gravity Anomalies in the Mountains     

J. Janák  P. Vaníček 《Studia Geophysica et Geodaetica》2005,49(1):31-42

Mean free-air gravity anomalies are often needed in geodesy for gravity field modelling. Two possible ways of compiling the mean free-air gravity anomalies are discussed. One way is via simple Bouguer gravity anomalies and the second and more time consuming way is via refined Bouguer gravity anomalies. In flat areas the differences between using any of the two ways should not be significant. In the mountains however, every effect introducing a high dependency, such as e.g. terrain effect, can negatively affect the interpolation process. In fact, a numerical experiment conducted in one part of Rocky Mountains revealed large and systematic differences. The effect of these differences on the geoid model is more then two meters in the test area. Our investigation shows that this bias is caused by the location of gravity measurement points, chosen mostly on hill-tops. At such points, the terrain correction to gravity is systematically larger than the mean value of the correction. Therefore, it is not possible to prevent the mean free-air gravity anomalies obtained from simple Bouguer gravity anomalies from having a systematic bias. One can see this bias as a result of the aliasing effect because the simple Bouguer gravity anomalies in the mountains contain a higher frequency signal (terrain effect) that is, according to sampling theorem, impossible to reconstruct by sparse measured gravity data, see e.g. (Goos et al., 2003). Therefore, the more rigorous way of computing the mean free-air gravity anomalies is via refined Bouguer gravity anomalies.  相似文献   

Deep structure and evolution of the Harz Mountains: results of three-dimensional gravity and finite-element modeling   总被引：1，自引：0，他引：1  

G. Gabriel  T. Jahr  G. Jentzsch  J. Melzer 《Tectonophysics》1997,270(3-4):279-299

A new Bouguer anomaly map is presented for the region of the entire Harz Mountains based on more than 60,000 gravity values. The various gravity anomalies are discussed and interpretation is carried out by high-resolution 3-D gravity modeling. One of the main subjects of interest in the investigation is the northern boundary fault zone of the Harz Mountains, separating the Mesozoic sediments in the north from the Palaeozoic rocks of the Harz in the south. Dip and vertical displacement are determined for this fault zone; mean values are 3400 m and 70°, respectively. Gravity modeling shows that the Brocken and the Ramberg Granites are distinctly different. The Brocken Granite is shallow, whereas the Ramberg Granite has a maximum depth of 8.5 km and a N---S dimension of 37 km. The prominent Benneckenstein Gravity High is explained by two different models, one based on a granodioritic intrusion (2900 kg/m³) with a center-depth of 14 km and the other based on phyllites (2740 kg/m³) on a depth of 3–4 km.

Studies on the geodynamic evolution of the Harz Mountains are carried out using the finite-element method. On the basis of a 3-D model, vertical displacements that can be related to horizontal forces are computed. For the period of the Variscan Orogeny an uplift of 600 m in the Harz area is calculated, for Late Cretaceous and Tertiary 400 m are determined. The total amount of 1000 m is about 1/2 of the vertical displacement of the northern boundary fault zone of the Harz Mountains shown by the gravity modeling. These results do not contradict geological ideas.  相似文献   

青海省区域地壳稳定性初探     

王臣 《高原地震》1993,(2)

本文主要应用地球物理指标B(布格重力异常梯度值,单位毫伽/公里)值,结合深断裂、地壳结构、布格重力异常特征、莫霍面形态和历史地震分布,对省内区域地壳划分了四个不稳定区;两个次不稳定区;三个基本稳定区和一个稳定区。  相似文献