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81.
渤海湾地区碰撞型海风锋天气过程的资料诊断分析   总被引:2,自引:0,他引:2  
利用多普勒雷达资料和地面自动站以及再分析资料对近年来7次典型的渤海湾地区碰撞型海风锋天气过程进行了分析。资料分析显示对流系统正面碰撞海风锋时(偏东西向碰撞)得到显著发展,而追赶碰撞海风锋时(偏南北向)则没有明显加强。海风锋移动沿途近地面出现明显的降温和风切变可以帮助判断海风锋的移动位置。高层稳定的偏西风有利于引导对流系统与西进海风锋发生正面碰撞。而低层的风场辐合则有利于碰撞过程中对流运动的发生,同时副高西北侧的水汽输送为降水的形成提供了有利条件。渤海湾地区地形的热力效应形成的低层偏中性层结有利于对流运动的发生,另外,在高空偏西风环境下地形可能对与海风锋碰撞的对流系统的触发或加强有促进作用。  相似文献   
82.
研究了2维平面管网碰撞分析算法,首先通过碰撞预判断,提高算法检测效率,分析了基于矢量积的直线管段相交算法。提出基于ArcEngine的折线管段的碰撞分析算法,并介绍了具体实现流程,利用C#编程技术实现了城市地下管网碰撞分析。  相似文献   
83.
早期碰撞造山带的研究是探索板块构造早期体制的前缘领域。五台山地貌高差巨大(达2437m)、山体雄伟、地质露头连续完整,是我国早前寒武纪地质研究的经典地区和认识大陆克拉通早期地壳演化的窗口,已成为世界早前寒武纪碰撞造山带的典型实例。围绕五台山构造样式的深入研究,对于揭示早期板块构造演化及中浅地壳构造层次具有重要的地质意义。 大量的野外地质调查及构造横剖面研究表明,五台山东冶亚群为华北克拉通的早期沉积盖层,它以开阔复式向形为特征,不整合于造山杂岩及其前陆冲断带和前陆盆地之上。区域变质相的分布及豆村亚群主期褶皱枢纽指示,五台山花岗岩—绿岩区向西南掀斜,出露了新太古代碰撞造山带不同构造单元(造山杂岩及前陆冲断带和前陆盆地)中浅层次上连续而完整的构造剖面。前陆冲断带以沉积岩系大规模平卧褶皱和逆断层、蛇绿岩混杂带和基底构造活化为特征。造山杂岩发育低角度逆断层和复杂叠加褶皱,伴随不同时期花岗岩类的侵位。从浅部层次向深部,绿岩带复式褶皱逐渐被与TTG杂岩构造叠置的表壳岩构造岩片取代,构造面理由陡立趋于平缓。与世界其他花岗岩—绿岩区相比,五台山区完好保留了造山带挤压构造及其前陆盆地沉积,指示早期碰撞造山过程的强烈构造缩短和大规模地壳隆升作用,是研究早期板块碰撞造山过程的重要例证。  相似文献   
84.
新疆塔里木—西昆仑宽频地震观测实验研究   总被引:4,自引:2,他引:4       下载免费PDF全文
利用获取的宽频地震数据,采用接收函数方法,获得了塔里木块体与青藏高原北缘西昆仑山结合部位的地壳及上地幔结构新信息。塔里木块体的地壳结构相对简单,其块体南缘的莫霍界面深度为42km,且向南倾斜,在西昆仑山前深度增加到50km左右。接收函数图象清晰地显示出,塔里木块体南缘和西昆仑山下存在南倾和北倾的构造特征,这些构造特征可以用地壳和上地幔相互穿插和变形的岩石圈碰撞模型来解释。  相似文献   
85.
大理点苍山正片麻岩初步研究   总被引:5,自引:0,他引:5  
沙绍礼  刘宇淳 《云南地质》2001,20(3):260-269
点苍山正片麻岩分为两类:斜长片麻岩和花岗片麻岩。前者属岛孤火山岩,形成于中晚元古代。二者主要化学组分具相关性,花岗片麻岩是由早形成的斜长片麻岩、斜片角闪岩经深熔作用而成。  相似文献   
86.
东秦岭-桐柏-大别山碰撞造山带北部早古生代变质火山岩系具有与大洋拉斑玄武岩相似的岩石学、岩石化学及微量元素特征,与镁铁质、超镁铁质岩块、辉绿岩墙群以及变质的沉积岩断片共同构成蛇绿混杂岩带。它们原来形成在华北断块南部大陆边缘的早古生代边缘海盆地的洋壳上。这个边缘海盆地的产生与华南洋壳海域岩石圈断块在晚前寒武纪时期向北俯冲有关,是震旦纪古边缘海继续扩张的结果。在加里东末期到海西早期,扬子断块与华北断块发生碰撞,边缘海闭合。  相似文献   
87.
The Ontong Java Plateau (OJP) in the western central Pacific is the largest and thickest oceanic plateau and one of a few oceanic plateaus converging on an island arc (Solomon island arc—SIA). To better understand the evolution of the North Solomon trench (NST), active oblique convergence between the OJP and SIA, and late Neogene development of Malaita accretionary prism (MAP), we present 850 km of multichannel seismic reflection data integrated with 7832 km2 of IZANAGI side-scan sonar coverage. We have focussed the study at the transition area between the well-defined northwestern end of the North Solomon trench and a diffusely deformed area where the trench is actively propagating in a northwestward direction. The deeper structure beneath the survey area is discussed by Phinney et al. [Oceanic plateau accretion in the Malaita accretionary prism inferred from multi-channel seismic reflection data, this issue] using deeper penetration, multichannel seismic reflection lines. The serial cross sections provided by multichannel seismic profiling combined with the IZANAGI backscattering imagery provides a time series evolution for the development of the North Solomon trench. The main evolutionary stages include (1) the incipient trench in the northern area marked by a diffuse zone of deformation above a broad arch in the crust. Deeper penetration profiles by Phinney et al. show the bulge is related to a deeper decollement fault that is propagating upward and seaward through the crust. (2) The formation of a continuous thrust front in the central area. Deeper penetration profiles by Phinney et al. show this thrust front is surface expression of the same decollement present at depth to the north. The boundary between the surface trace of the thrust and the diffuse area of deformation in the northern area is inferred as a vertical, high-angle tear fault with left-lateral offset. (3) The formation of a deep, elongate trench which controls gravitationally related slumping and sedimentation around the steep edges of the trench fill basin. The areas to the southeast are those that have undergone convergence for the longest period of time and therefore show better developed trench structures and a reduced width of the MAP. Areas to the northwest have undergone convergence for a shorter period of time and show less developed trench structures and a wide area of the MAP.  相似文献   
88.
The present kinematic and dynamic analysis of large-scale strike-slip faults, which enabled the formation of a collage of Altai terranes as a result of two collisional events. The Late Devonian–Early Carboniferous collision of the Gondwana-derived Altai-Mongolian terrane and the Siberian continent resulted in the formation of the Charysh–Terekta system of dextral strike-slip faults and later the Kurai and Kuznetsk–Teletsk–Bashkauss sinistral strike-slip faults. The Late Carboniferous–Permian collision of the Siberian and Kazakhstan continents resulted in the formation of the Chara, Irtysh and North-East sinistral strike-slip zones. The age of deformation of both collisional events becomes younger toward the inner areas of the Siberian continent. In the same direction the amount of displacement of strike-slip faulting decreases from several thousand to several hundred kilometers. The width of the Late Paleozoic zone of deformation reaches 1500 km. These events deformed the accretion-collision continental margins and their primary paleogeographic pattern.  相似文献   
89.
The Altai-Salair area in southern Siberia is a Caledonian folded area containing fragments of Vendian–Early Cambrian island arcs. In the Vendian–Early Cambrian, an extended system of island arcs existed near the Paleo-Asian Ocean/Siberian continent boundary and was located in an open ocean realm. In the present-day structural pattern of southern Siberia, the fragments of Vendian–Early Cambrian ophiolites, island arcs and paleo-oceanic islands occur in the accretion–collision zones. We recognized that the accretion–collision zones were mainly composed of the rock units, which were formed within an island-arc system or were incorporated in it during the subduction of the Paleo-Asian Ocean under the island arc or the Siberian continent. This system consists of accretionary wedge, fore-arc basin, primitive island arc and normal island arc. The accretionary wedges contain the oceanic island fragments which consist of OIB basalts and siliceous—carbonate cover including top and slope facies sediments. Oceanic islands submerged into the subduction zone and, later were incorporated into an accretionary wedge. Collision of oceanic islands and island arcs in subduction zones resulted in reverse currents in the accretionary wedge and exhumation of high-pressure rocks. Our studies of the Gorny Altai and Salair accretionary wedges showed that the remnants of oceanic crust are mainly oceanic islands and ophiolites. Therefore, it is important to recognize paleo-islands in folded areas. The study of paleo- islands is important for understanding the evolution of accretionary wedges and exhumation of subducted high-pressure rocks.  相似文献   
90.
Numerical sensitivity studies were carried out to investigate the influence of shape variations of colliding ice particles on the collisional behavior. Therefore, two general ice particle shapes were considered: ice plates and ice columns. The changing of the shape of the ice particles was described by the changing of the axis ratio of the particles. Numerical growth calculations with a cloud model were carried out to show the impact of the axis ratio variations on the collectional growth in comparison to calculations with a constant axis ratio. Ice plates show significant differences between the two cases, whereas for ice columns the effect of the axis ratio variations is less important.  相似文献   
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