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1.
The Tsushima Basin is located in the southwestern Japan Sea, which is a back-arc basin in the northwestern Pacific. Although some geophysical surveys had been conducted to investigate the formation process of the Tsushima Basin, it remains unclear. In 2000, to clarify the formation process of the Tsushima Basin, the seismic velocity structure survey with ocean bottom seismometers and airguns was carried out at the southeastern Tsushima Basin and its margin, which are presumed to be the transition zone of the crustal structure of the southwestern Japan Island Arc. The crustal thickness under the southeastern Tsushima Basin is about 17 km including a 5 km thick sedimentary layer, and 20 km including a 1.5 km thick sedimentary layer under its margin. The whole crustal thickness and thickness of the upper part of the crust increase towards the southwestern Japan Island Arc. On the other hand, thickness of the lower part of the crust seems more uniform than that of the upper part. The crust in the southeastern Tsushima Basin has about 6 km/s layer with the large velocity gradient. Shallow structures of the continental bank show that the accumulation of the sediments started from lower Miocene in the southeastern Tsushima Basin. The crustal structure in southeastern Tsushima Basin is not the oceanic crust, which is formed ocean floor spreading or affected by mantle plume, but the rifted/extended island arc crust because magnitudes of the whole crustal and the upper part of the crustal thickening are larger than that of the lower part of the crustal thickening towards the southwestern Japan Island Arc. In the margin of the southeastern Tsushima Basin, high velocity material does not exist in the lowermost crust. For that reason, the margin is inferred to be a non-volcanic rifted margin. The asymmetric structure in the both margins of the southeastern and Korean Peninsula of the Tsushima Basin indicates that the formation process of the Tsushima Basin may be simple shear style rather than pure shear style.  相似文献   

2.
A study has been made about the structural attribute of the NNW-trendingShizikou linear image belt in the head area of the reservoir of the Yangtze River Gorges and theevaluation of its crustal stability. On the basis of regional geological surveys and by making astructural analysis and a multidisciplinary study, it has been ascertained that the segment withthe best displayed image characteristics is marked by a gravity gliding structure with a multilay-er gliding fold type architecture. This paper also analyzes the medium conditions, slope struc-ture and dynamic setting for the formation of the structure system.  相似文献   

3.
Since 1975 several high-resolution seismic-refraction and reflection surveys have been carried out in western Germany to investigate the structure of the Earth's crust and uppermost mantle. The investigation culminated in the seismic-refraction survey along the 825 km long central part of the European Geotraverse (EGT) in 1986. This contribution summarizes the main results of the more recent crustal investigations along and around the EGT. The internal crustal structure throughout the area of the Variscides is very complex and changes laterally considerably. Distinct crustal blocks differing in their internal structure can be assigned to geologically defined units of the Variscan and Caledonian orogeny. In spite of local deviations, in general a more or less transparent and low-velocity upper crust contrasts with a highly reflective lower crust. A subdivision of upper and lower crust by a well-defined boundary (Conrad discontinuity) is not always seen. Towards the Alps the average velocity of the lower crust is as low as 6.2 km s?1, in contrast to the area north of the Swabian Jura where the velocities above Moho vary between 6.8 and 7.2 km s?1. In Northern Germany, the Elbe line separates the lower crust into two regions with 6.4 km s?1 average velocity in the south and 6.9 km s?1 in the north. The total crustal thickness under the Variscan part of Germany is fairly constant between 28 and 30 km, except under the Rhine Graben area with 25–26 km and beneath the central part of the Rhenish Massif where an anomalous crustal thickening to 37 km is observed. Under northern Germany the Moho rises to about 26 km depth and the data indicate at least one fault-like step of 1 km before the crust thickens toward the Ringkobing-Fyn basement high. The synthesis of seismic velocity structure and petrological information from xenolith studies allows us to propose a mafic composition for the deeper levels of the crust and uppermost mantle which may be valid at least for the central part of the Variscan crust along the European Geotraverse in Central Europe.  相似文献   

4.
围绕着长江三峡库处区狮子口ＮＮＷ向线性影像带的构造性及其地壳稳定性评价问题进行了专题研究，以区域地质调查为基础，运用构造解析方法，采用多学科，多手段的综合研究，确认该影像带影像特征最明显的地段乃是一个滑褶型多层式得力滑动构造，本文还分析了该系统形成的介质条件，斜坡构造及动力环境。  相似文献   

5.
The initial coda of teleseismic P‐waves contains considerable information about the crust and upper mantle structure directly beneath a receiver. When this information can be recovered for a dense network of seismographs much can be learned about the structure of the earth. Data from the high quality broadband seismic stations of the SKIPPY and KIMBA projects along with permanent stations are used to investigate the upper crustal structure of Australia. A dataset of 65 shear‐velocity models derived from receiver functions has enabled the sedimentary and upper crustal structure of Australia to be summarised. Regions of thick soft sediment show good agreement with topographical lows. A simple relation between upper‐crustal velocity and magnetisation, as has been suggested by other investigators, has not been observed, but this may be due to the magnetic signal being muted by overlying sediments. A prominent mid‐crustal discontinuity is apparent in the Tasman and New England mega‐elements. This may represent a mid‐crustal décollement that had structural control during accretion.  相似文献   

6.
A report about three seismic projects with their first results in the exploration of the deep subsurface rocks of the Central Europe and the Alps. In addition a summary is given of the crustal and structure of the different continents based on literature about similar work done in other countries and continents. A profile round about the earth shows the crustal structure of America, Europe, and Asia.- -author.  相似文献   

7.
Magnetic observations over the area of the Transantarctic Mountains (TAM) and the Ross Sea have been compiled into a digital database that furnishes a new regional scale view of the magnetic anomaly crustal field in this key sector of the Antarctic continent. This compilation is a component of the ongoing IAGA/SCAR Antarctic Digital Magnetic Anomaly Project (ADMAP). The aeromagnetic surveys total 115 000 line km, and are distributed across the Victoria Land sector of the TAM, the Ross Sea, and Marie Byrd Land. The magnetic campaigns were performed within the framework of the national and international Italian–German–US Antarctic research programs and conducted with differing specifications during nine field seasons from 1971 until 1997. Generally flight line spacing was less than 5 km while survey altitude varied from about 610 to 4000 m above sea level for barometric surveys and was equal to 305 m above topography for the single draped survey. Reprocessing included digitizing the old contour data, improved levelling by means of microlevelling in the frequency domain, and re-reduction to a common reference field based on the DGRF90 model. A multi-frequency grid procedure was then applied to obtain a coherent and merged total intensity magnetic anomaly map. The shaded relief map covers an area of approximately 380 000 km2. This new compilation provides a regional image of the location and spatial extent of the Cenozoic alkaline magmatism related to the TAM–Ross Sea rift, Jurassic tholeiites, and crustal segments of the Early Palaeozoic magmatic arc. A linear, approximately 100-km wide and 600-km long Jurassic rift-like structure is newly identified. Magnetic fabric in the Ross Sea rift often matches seismically imaged Cenozoic fault arrays. Major buried onshore pre-rift fault zones, likely inherited from the Ross Orogen, are also delineated. These faults may have been reactivated as strike-slip belts that segmented the TAM into various crustal blocks.  相似文献   

8.
Abdullh M.S. Al-Amri   《Tectonophysics》1998,290(3-4):271-283
The crustal structure of the western Arabian platform is derived using the spectral analysis of long-period P-wave amplitude ratios. The ratio of the vertical to the horizontal component is used to obtain the crustal transfer function based on thickness variations, crustal velocities, densities and the angle of emergence at the lower crust and upper mantle interface. Eleven well-defined earthquakes recorded at the long-period RYD station during the period from 1985 to 1994 were selected for analysis based on the following criteria: focal depths with a range between 7 and 89 km, body-wave magnitudes greater than 4.7, epicentral distances with a range from 8.8° to 26.5°, and back azimuthal coverage from 196° to 340°. Spectral analysis calculations were based on the comparison of the observed spectral ratios with those computed from theoretical P-wave motion obtained using the Thomson–Haskell matrix formulation for horizontally layered crustal models. The selection of the most suitable model was based on the identification of the theoretical model which exhibits the highest cross-correlation coefficient with the observed transfer function ratio. By comparing the spectral peak positions of the observed and theoretical values, the thickness and velocity can be resolved within 3 km and 1 km/s, respectively, of the observed values. The spectral analysis of long-period P-waves can detect a thin layer near the surface of about 1.6 km thick and a velocity contrast of about 10% with that of the underlying layer. A strong velocity gradient of about 0.05 km/s per km was found in the upper crust and 0.02 km/s per km in the lower crust. The derived crustal model is not unique due to the theoretical assumptions (horizontal layering, constant densities and velocities in each layer), quality of the data and complexities of the crustal structure. The crustal model suggests that the crust consists of five distinct layers. The upper crustal layer has a P-wave velocity of about 5.6 km/s and is about 1.6 km thick. The second layer has a velocity of about 6.2 km/s and is 10.2 km thick. The third layer shows a velocity of 6.6 km/s and is 6.8 km thick. The fourth layer has a velocity of about 6.8 km/s and is 12.3 km thick. The lower crustal layer has a velocity of about 7.5 km/s and is 9.3 km thick. The Mohorovicic discontinuity beneath the western Arabian platform indicates a velocity of 8.2 km/s of the upper mantle and 42 km depth.  相似文献   

9.
When the inversion of vertical load deformation on Earth’s surface using GRACE (Gravity Recovery and Climate Experiment) data, the load Love numbers based on PREM (Preliminary Reference Earth Model) are commonly used. But the crustal structure under China mainland especially under Tibet Plateau is quite different from that given by PREM Earth model. New load Love numbers were calculated based on a modified Earth model which accounted for regional crustal structure in China mainland. And the effect of regional crustal structure in China mainland for estimation of vertical load deformation on Earth’s surface using GRACE RL05 data was investigated in this paper. It is found that the effect of crustal difference is very prominent. The relative difference of load Love numbers for vertical deformation can reach about 11% at degree 90. The extreme value of difference in vertical load deformation below 90 degree of spherical harmonic coefficients located at the southeastern Tibet Plateau and the maximum relative difference reaches 10%. The relative difference of the root mean square is about 4%. It is suggesting that an Earth model with a more realistic crustal structue instead of PREM should be used for the estimation of vertical load deformation in China mainland espacially in Tibet Plateau.  相似文献   

10.
杨晓松  马瑾 《地学前缘》2003,10(Z1):240-247
块体构造理论的发展不断地深化着人们对现今大陆岩石圈运动 ,尤其是大陆强震的孕育和发生规律的认识。块体底部边界的构造性质是块体运动的核心问题之一 ,同时也是块体构造理论研究中的薄弱环节。确定块体底部边界的岩石物理性质是利用地球物理方法探测和识别块体底部边界的前提。文中依据现代实验岩石学、实验岩石物理学、地球物理学、地质学等的研究成果 ,对块体底部边界之成因属性和岩石物理性质进行了分析。将大陆块体划分为两种基本类型———地壳型块体和岩石圈型块体。地壳型块体是由大陆上部地壳所构成的“薄板” ,壳内软弱带的顶面为其底部边界和潜在的解耦带。岩石圈型块体在岩石圈尺度上是力学耦合的 ,以上地幔软流圈的顶面为其底部边界。壳内软弱带具有垂直方向低速和各向异性的基本特征 ,联合多种地震测深方法有望确定块体的底界。在现今构造活动区内 ,地壳型块体的潜在解耦带可能由壳内部分熔融带承担。青藏高原南部—川滇地区 2 0 35km的深度上广泛存在低速带。地热、岩石学、实验岩石学和模拟均显示该地区的低速带具有部分熔融的成因属性。块体沿着该壳内低速层与下伏地壳发生某种程度解耦。  相似文献   

11.
Despite the various opening models of the southwestern part of the East Sea (Japan Sea) between the Korean Peninsula and the Japan Arc, the continental margin of the Korean Peninsula remains unknown in crustal structure. As a result, continental rifting and subsequent seafloor spreading processes to explain the opening of the East Sea have not been adequately addressed. We investigated crustal and sedimentary velocity structures across the Korean margin into the adjacent Ulleung Basin from multichannel seismic (MCS) reflection and ocean bottom seismometer (OBS) data. The Ulleung Basin shows crustal velocity structure typical of oceanic although its crustal thickness of about 10 km is greater than normal. The continental margin documents rapid transition from continental to oceanic crust, exhibiting a remarkable decrease in crustal thickness accompanied by shallowing of Moho over a distance of about 50 km. The crustal model of the margin is characterized by a high-velocity (up to 7.4 km/s) lower crustal (HVLC) layer that is thicker than 10 km under the slope base and pinches out seawards. The HVLC layer is interpreted as magmatic underplating emplaced during continental rifting in response to high upper mantle temperature. The acoustic basement of the slope base shows an igneous stratigraphy developed by massive volcanic eruption. These features suggest that the evolution of the Korean margin can be explained by the processes occurring at volcanic rifted margins. Global earthquake tomography supports our interpretation by defining the abnormally hot upper mantle across the Korean margin and in the Ulleung Basin.  相似文献   

12.
Analyses of bathymetry, gravity and seismic reflection data of the diffusive plate boundary in the central Indian Ocean reveal a new kind of deformed structure besides the well-reported structures of long-wavelength anticlinal basement rises and high-angle reverse faults. The structure (basement trough) has a length of about 150 km and deepens by up to 1 km from its regional trend (northward dipping). The basement trough includes a rise at its center with a height of about 1.5km. The rise is about 10 km wide with rounded upper surface and bounded by vertical faults. A broad freeair gravity low of about 20 mGal and a local high of 8 mGal in its center are associated with the identified basement trough and rise structure respectively. Seismic results reveal that the horizontal crustal compression prevailing in the diffusive plate boundary might have formed the basement trough possibly in early Pliocene time. Differential loading stresses have been generated from unequal crust/sediment thickness on lower crustal and upper mantle rocks. A thin semi-ductile serpentinite layer existing near the base of the crust that is interpreted to have been formed at mid-ocean ridge and become part of the lithosphere, may have responded to the downward loading stresses generated by the sediments and crustal rocks to inject the serpentinites into the overlying strata to form a classic diapiric structure.  相似文献   

13.
We analyzed a total of 206 receiver functions beneath Kottamiya broadband station in northern Egypt to study the crustal structure and any azimuthal variations in the crustal thickness. The computed receiver functions are subdivided according to their azimuth into eight subgroups and analyzed separately using a genetic algorithm. The genetic algorithm is more appropriate than conventional linearized inversion schemes in regions where there is little a priori information about local crustal structures such as northern Egypt because it does not strongly depend on an initial model. The study region is located on the unstable shelf of Egypt in the northeastern corner of Africa. Little information about the deep structure of the crust beneath this region is available. For this reason, we have adopted the genetic algorithm to seismic waveform data recorded by Kottamiya broadband station. The crustal thickness varies slightly from 32 to 34 km with an average of 32.25 km, which is consistent with previous studies in the region. The crustal thickness shows a tendency of decrease toward the east and northeast being consistent with the general tectonic setting of the region including the opening of the Red Sea in the Tertiary times. Nonetheless, more teleseismic receiver functions from earthquakes recorded at denser seismic stations in northern Egypt and the southeastern Mediterranean combined with surface wave dispersion data as well as other geophysical investigations are necessary for more detailed imaging of the crustal structure which will deepen our understanding of the current tectonic and seismic activities of the region.  相似文献   

14.
为了解准噶尔盆地深部构造特征,综合利用“深部探测技术与试验研究(SinoProbe)”项目在准噶尔盆地45°N 88°E处建立的大地电磁标准点实测资料,应用非线性共轭梯度法(NLCG)对该测站两条短剖面进行二维反演,结合新疆准噶尔盆地区域地质资料,对该地区地层电性结构进行了初步分析,发现准噶尔盆地中东部地区地下结构具有很好的电性分层.与现有地质资料相结合,分析发现其电性分层与地壳分层具有较好的对应.根据岩石层电导性推断:研究区域莫霍面埋深在46 km附近,岩石圈厚度在100 km左右.研究结果对准噶尔中东部地区深部地壳结构的认识具有一定的参考价值.   相似文献   

15.
In 1982 a Vibroseis® survey comprising 180 km of reflection profiles was run in northern Switzerland in order to investigate the suitability of the crystalline basement for the deposition of highly radioactive waste. A configuration was chosen with 144 channels, 25 m of geophone spacing, 20 s sweeps ranging from 11 to 61 Hz and stacking of 4 or 8 sweeps of 3 simultaneous vibrators at twice the geophone spacing. The listening time was generally 4 s and at 4 sites it was extended to 11s for the detection of deeper crustal reflectors. This survey unravelled the complicated fault and thrust system beneath the Swiss folded Jura mountains.The stack from 4 s to 11 s reveals clearly a strong sloping reflector between 3.0 and 3.5 s which is strong evidence for a pronounced differentiation in the upper crust. A series of reflections is observed between 5.8 and 7.2 s the top of which can be correlated with the Conrad discontinuity.A strong “layered” signal between 9.0 and 9.5 s is interpreted as reflections from the M-discontinuity. The main features are compatible with results from nearby refraction surveys in the southern Rhinegraben rift system which show a distinct velocity increase of about 0.5 km/s in the lower crust at a depth ranging from 15 to 20 km, followed by an inversion zone or a laminated structure before reaching the Moho at about 27 km depth.The correlation of the field recordings with the first 10 s of the up-sweep only, shows some loss of resolution in the uppermost 3 s because of the lower frequency content of the signal. However, the lower parts of the sections are nearly identical. The fact that the deeper reflectors in the sections can consistently be traced laterally is a strong argument for using this processing technique. Thus high-coverage Vibroseis surveys utilizing up-sweep can be processed for deep crustal reflections even if the recording time is restricted to the standard 4 s, provided the surface static corrections are carried out with high precision.  相似文献   

16.
A number of geodetic techniques exist for measuring instantaneous crustal motions and deformations. Over distances of a few hundred kilometres, conventional terrestrial methods can achieve accuracies of about 1–2 parts in 106 for horizontal positions, but most existing triangulation networks in Australia are of lower accuracies. Geodetic levelling can provide height‐difference measurements with an accuracy of a few mm for points separated by about 100 km, but actual accuracies are often much lower than this. For points separated by longer distances, from a few 100 km to several 1000 km, space techniques can provide precisions of 5–10 cm. Two experiments carried out in Australia confirm that these precisions can be reached. A laser ranging experiment between sites near Canberra and Perth produced a baseline that is precise to better than 10 cm, and a radio‐interferometry experiment between Canberra, Parkes and Sydney produced baselines with precisions of 10 cm. Further evaluation of both systems is required, but the present results indicate that crustal deformations of the order of 10 cm can be measured with repeat surveys.  相似文献   

17.
新—甘地震测深剖面的地壳速度结构及大地构造单元划分   总被引：9，自引：1，他引：9  
根据新—甘地震测深结果,以纵波为主,建立了剖面内地壳速度结构模型,结合横波资料对地壳结构进行了研究。确定出超壳断裂14条;划分出一级构造单元4个;二级构造单元8个。从而,对大地构造和地壳演化提出新的认识,为深入研究区内基础地质具有重要意义。  相似文献   

18.
The Himalaya and Lhasa blocks act as the main belt of convergence and collision between the Indian and Eurasian plates. Their crustal structures can be used to understand the dynamic process of continent–continent collision. Herein, we present a 3D crustal density model beneath these two tectonic blocks constrained by a review of all available active seismic and passive seismological results on the velocity structure of crust and lower lithosphere. From our final crustal density model, we infer that the present subduction-angle of the Indian plate is small, but presents some variations along the west–east extension of the orogenic belt: The dip angle of the Moho interface is about 8–9° in the eastern and western part of the orogenic belt, and about 16° in the central part. Integrating crustal P-wave velocity distribution from wide-angle seismic profiling, geothermal data and our crustal density model, we infer a crustal composition model, which is composed of an upper crust with granite–granodiorite and granite gneiss beneath the Lhasa block; biotite gneiss and phyllite beneath the Himalaya, a middle crust with granulite facies and possible pelitic gneisses, and a lower crust with gabbro–norite–troctolite and mafic granulite beneath the Lhasa block. Our density structure (<3.2 g/cm3) and composition (no fitting to eclogite) in the lower crust do not be favor to the speculation of ecologitized lower crust beneath Himalaya and the southern of Lhasa block.  相似文献   

19.
苏鲁造山带区域地壳山根结构特征   总被引：15，自引：6，他引：15  
徐纪人  赵志新 《岩石学报》2004,20(1):149-156
本利用苏鲁大别造山带及其邻区的三维P波速度资料，详细对比研究了苏鲁与大别超高压变质带莫霍面深度和深部P波速度结构分布特征。结果表明，尽管苏鲁、大别超高压变质带都具有上地壳明显高速且上凸；中地壳增厚；下地壳埋藏较深且下凹等共同的P波速度结构特征，与大别地区相比较，苏鲁超高压变质带还存在着独特的区域性特征。从地貌上看，苏鲁地区山脉已经基本消失。苏鲁超高压变质带的地壳厚度为32～33公里，深于其周围地区2～3公里，但是莫霍面下凹程度远不如大别地区，造山带地壳山根已逐步趋向消失。苏鲁地区上地壳P波速度高于大别，比其周围地区约快1～1．2km/s，有可能显示了该区有更多高速、高密度的超高压变质岩折返到上地壳与地表的岩石物性效果。大别造山带山脉依然存在，莫霍面下凹更明显，沿NWW向串状残留地壳山根最深为37～38公里，深于其周围地区3～4公里。对比研究结果表明，由于区域构造运动的作用，苏鲁大别造山带中的不同地段，在其造山、演化过程中也存在着差别。苏鲁的造山运动起始虽略晚于大别，但结束的更快，比大别更早进入了造山运动的后期。分析促使苏鲁造山运动进程加速的主要构造原因可能有两点，郯庐断裂带的左旋走滑运动以及通过中国华北区域的大范围NW-SE向扩张应力场的影响。大区域构造背景加速了苏鲁造山带地表高山侵蚀过程的同时，随着山根浮力的不断减弱，地壳深部山根逐渐趋向消失。地壳速度结构特征有可能反映了苏鲁造山带的地壳山根随着地表山脉的侵蚀而减弱，趋向消失的过程。  相似文献   

20.
《International Geology Review》2012,54(12):1079-1102
In the past few years, meteoritic and cometary impacts have emerged as a major geological agent in the construction and evolution of planetary surfaces. Formation of complex central ring, peak ring and multiring craters involves excavation and melting of large volumes of crustal material. High-resolution geophysical mapping measuring gravity, magnetics, and topography of the Moon and Mars have recently provided information on the subsurface structure of large basins and aided in identifying buried giant craters. The terrestrial crater record has been significantly erased by tectonic, magmatic, and erosion processes and only a small proportion of impact structures remain. Record of multiring craters is limited to three examples: Vredefort, Sudbury and Chicxulub. Deep geophysical surveys and geochemical and isotopic studies of those craters provide means to evaluate the influence of large impacts on the lithospheric and crustal evolution by providing estimates of excavation depth and volume, amounts of material fragmented, ejected, vaporized and melted, and effects on the crustal stratigraphy and crustal thickness. Analyses on the melt from Vredefort, Sudbury, and Chicxulub indicate andesitic composition derived from lower-crustal material. The melt formed inside the lower transient cavity from lower crustal material that was then redistributed and emplaced in upper-crustal levels, resulting in crustal redistribution. Crystalline basement clasts fragmented and incorporated into the breccias show varying degrees of alteration but no significant thermal effects. Ejecta were deposited locally within the crater region and ballistic material and fine ejecta are globally distributed on the planetary surface. Impacts influence the crust–mantle boundary, with Moho uplift. Material from the mantle was not incorporated into the melt and impact breccias, indicating that the excavation cavities were confined to the lower crust. This is also apparently the case for the giant basins on the Moon, including the 2500 km diameter South Pole-Aitken Basin. Considering the numbers of large multiring basins, possible flux of large impacts, and effects on target surfaces, crustal scale redistribution of material during those large impacts has played a major role in the evolution of planetary surfaces.  相似文献   

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