月表线性构造自动提取新方法研究:以澄海地区月岭为例

月岭作为月球表面上最常见的线性构造之一,可以反映月球区域性的构造特征和应力状态,对研究月球地质演化有着重要意义。前人对线性构造的解译方式通常是以人工目视解译为主,应用遥感影像数据和激光高度计数据等对月表线性构造进行解译和提取。随着数据精度的提高,以及对研究效率的要求,形成一种行之有效的线性构造自动提取方法具有必要性。文中以地形曲率为原理,借鉴前人应用地形曲率提取地表特征线的方法,以“嫦娥一号”CCD2C影像数据和LOLA激光高度计数据和LRO的宽视角影像数据为基础,以澄海为研究区域,进行线性构造的自动提取。研究区试验结果表明,文中提出的基于地形曲率的方法是可行的,并与人工解译的月岭结果进行对比,发现精确度更高,反映地形变化更为明显,为进一步研究构造演化提供基础,提高解译效率和精度。     

基于多尺度数字地形定量分析的月球线性构造自动提取研究

月球表面构造对于理解和重建月球地质构造演化具有重要意义,月岭、月溪等线性构造的形态及分布特征与月球内动力构造运动密切相关。极为有限的样品和难度极高的野外勘察使得遥感成为行星科学研究的最主要手段。中国、美国、日本、印度等国先后发射的多颗新型探月卫星获取了大量高质量数据,尤其是高分辨率的数字地形数据(DTM,Digital Terrain Model)。高分辨率的DTM为月球表面构造特征的自动提取带来了新的机遇与挑战。文中利用多种分辨率的DTM数据,基于多尺度数字地形定量分析方法,识别和提取月球表面的线性构造。使用的地形数据包括500 m分辨率“嫦娥一号”激光高度计数据,100 m分辨率LRO-WAC广角相机数据,60 m分辨率的LRO-LOLA激光测距仪数据以及分辨率高达5 m的LRO-NAC窄视角相机数据。文中使用地形曲率来识别月溪月岭等线性构造,并利用不同滑动窗口大小和阈值进行线性构造的自动提取。对研究区试验结果的定量分析表明,文中提出的基于地形曲率的月表线性构造自动提取方法是有效且可行的,其结果可为月球表面线性构造解译提供重要参考,提高构造解译时效性和精度。     

西南印度洋中脊斜向扩张分段特征及构造成因探讨

斜向扩张是超慢速扩张洋中脊独特的构造特征,其地形分段特征明显区别于经典的快速-慢速端元洋中脊模型,是理解超慢速扩张洋中脊地质过程的重要切入点。基于西南印度洋中脊Indomed-Gallieni和Shaka-DuToit段多波束地形数据,分析了不同斜向扩张角度(α)洋中脊的地形分段样式。其中,46.5°~47.5°E(α=5°)、16°~25°E(α=10°)和48.5°~52°E(α=15°)为近正向扩张段,发育雁列式叠置的中央火山脊;47.5°~48.5°E(α=50°)和16°~25°E(α=60°)为斜向扩张段,仅在洋脊段中部形成中央火山脊。利用有限差分+颗粒法(FD+MIC)数值模拟技术研究了洋中脊应变分布特征对不同α值的响应,结合地形分析,认为斜向扩张角度和温度异常分布共同控制了洋中脊地形分段样式。近正向扩张洋中脊(α＜20°)在温度异常处形成地壳伸展应变的集中区,有利于岩浆汇聚,发育雁列式叠置的中央火山脊,其位置随温度异常分布的变化而改变;斜向扩张洋中脊(α>20°)地壳伸展应变集中区的位置受斜向扩张几何样式控制,在洋脊段中部发育中央火山脊,对温度异常不敏感,形成位置长期固定的岩浆活动中心。     

印度洋构造过程重建与成矿模式：西南印度洋洋中脊的启示EI北大核心CSCD

印度洋经历过复杂的构造演化,其中3次重大的三联点和洋中脊跃迁、板块重组对印度洋现今构造格局的形成具有重要影响。本文基于Gplates板块重建技术和古水深数据,并融合前人热点和年代学研究结果,重点探讨了120 Ma、90 Ma、84 Ma、65 Ma、40 Ma、24 Ma和15 Ma发生在印度洋的重大构造事件,讨论了这些构造事件在西南印度洋超慢速扩张脊构造特征上的关联,探讨了西南印度洋不同演化阶段的两种海底热液成矿模式,即早期热点-洋中脊相互作用相关的热点成矿模式和后期海洋核杂岩相关的湿点成矿模式。     

印度洋构造过程重建与成矿模式:西南印度洋洋中脊的启示

印度洋经历过复杂的构造演化,其中3次重大的三联点和洋中脊跃迁、板块重组对印度洋现今构造格局的形成具有重要影响。本文基于Gplates板块重建技术和古水深数据,并融合前人热点和年代学研究结果,重点探讨了120 Ma、90 Ma、84 Ma、65 Ma、40 Ma、24 Ma和15 Ma发生在印度洋的重大构造事件,讨论了这些构造事件在西南印度洋超慢速扩张脊构造特征上的关联,探讨了西南印度洋不同演化阶段的两种海底热液成矿模式,即早期热点-洋中脊相互作用相关的热点成矿模式和后期海洋核杂岩相关的湿点成矿模式。     

西南印度洋构造地貌与构造过程

本文基于海底水深数据,制定了西南印度洋超慢速扩张脊新的海底构造地貌划分原则,将西南印度洋划分为7级构造地貌单元;并以该洋中脊中段的Discovery II和Gallieni转换断层之间及其邻区的海底构造地貌特征为依据,将其与该区断裂演化、分段性、分段拓展机制、中央裂谷形成过程、脊–柱相互作用和洋中脊跃迁进行综合分析。结果表明,该区洋中脊可以划分为4个三级构造地貌单元(即洋中脊的一级分段),从西向东被Andrew Bain和Prince Edwards、Discovery II以及Gallieni转换断层依次分割,分别反映为强热点–洋中脊相互作用的扩张脊、弱热点–洋中脊相互作用的扩张脊和正常超慢速扩张脊的地貌类型。每个三级分段可进一步划分为3~4个四级分段,本文仅侧重Discovery II和Gallieni转换断层间洋中脊四到七级的4个级别分段划分(即洋中脊的四级构造地貌单元再划分为3级)。其中,第七级构造地貌单元分别为侧列式裂谷(剪切带)、雁列式裂谷、横断层带等构造分割。该段洋中脊先后受Marion、Crozet、Madagascar等热点或海台的影响,经历了3次洋中脊跃迁,时间大致分别为80 Ma,60 Ma和40 Ma,该过程与冈瓦纳大陆裂解以来的大洋演化有关。最后,本文详细分析了20 Ma以来的西南印度洋洋中脊轴部的周期性拉分式断陷、多米诺式箕状断陷、地堑式断陷和海洋核杂岩等构造过程。     

大西洋中脊区线性构造解译及热液成矿关联

基于大西洋最新的高精度水深数据,协同重力、磁力数据,利用地形分割算法、GIS技术等综合解译大西洋洋脊线性构造,并将其与前人研究成果对比、校正、融合、整合、补充,生成大西洋线性构造信息图层。将已查明热液硫化物矿点生成已知矿点图层。将两图层进行空间关联分析,初步得出两者之间关系。     

利用光学遥感数据、GIS及人工神经网络模型分析区域滑坡灾害(英文)

用光学遥感数据和地理信息系统(GIS)分析了马来西亚Selangor地区的滑坡灾害。通过遥感图像解译和野外调查,在研究区内确定出滑坡发生区。通过GIS和图像处理,建立了一个集地形、地质和遥感图像等多种信息的空间数据库。滑坡发生的因素主要为:地形坡度、地形方位、地形曲率及与排水设备距离;岩性及与线性构造距离;TM图像解译得到的植被覆盖情况;Landsat图像解译得到的植被指数;降水量。通过建立人工神经网络模型对这些因素进行分析后得到滑坡灾害图:由反向传播训练方法确定每个因素的权重值,然后用该权重值计算出滑坡灾害指数,最后用GIS工具生成滑坡灾害图。用遥感解译和野外观测确定出的滑坡位置资料验证了滑坡灾害图,准确率为82.92%。结果表明推测的滑坡灾害图与滑坡实际发生区域足够吻合。     

大洋下地壳堆晶岩组成及其对蛇绿岩研究的启示

大洋下地壳是大洋岩石圈和蛇绿岩的重要组成部分,在洋中脊及俯冲带演化以及蛇绿岩成因研究中具有重要的意义。本文总结了不同构造环境形成的大洋下地壳堆晶岩的岩石组合、地球化学组成,以建立起适用于蛇绿岩中堆晶岩的构造环境判别标志。洋中脊和俯冲相关环境堆晶岩在Pearce图解上均区别于对应的熔岩成分,表明蛇绿岩中的堆晶岩无法应用Pearce图解进行构造环境判别。不同构造环境产出的堆晶岩在岩石组合、结晶顺序和地球化学上存在明显差异：(1)绝大多数洋中脊堆晶岩和弧后盆地堆晶岩较为类似,反映其来源于洋中脊玄武岩型母岩浆低压、贫水体系的分离结晶;(2)中大西洋脊DSDP 334的洋中脊堆晶岩较为类似弧前堆晶岩,是海水蚀变难熔橄榄岩重熔或混染的产物;(3)弧前堆晶岩的岩石学、地球化学特征与亏损的富水、富硅的玻安质熔体的低压分离结晶过程相吻合;(4)洋岛堆晶岩的特征与相对贫水、成分富集的洋岛玄武岩高压分离结晶的特征相吻合。最后,本文总结了应用堆晶岩进行蛇绿岩构造环境判别的一系列岩石学、地球化学指标,并结合日喀则蛇绿岩中的堆晶岩体和辉长岩脉的实例论述堆晶岩在蛇绿岩研究中的应用。     

全球中、新生代大地构造特征及其演化框架——《全球中、新生代大地构造图》编图研究进展

全球中、新生代大地构造编图是全球构造理论研究的基础和切入点,本文介绍了该图编制思路与方法、数据来源和大地构造区划,并以地球圈层构造为主线,讨论了全球中生代以来水平构造和全球垂向圈层之间的衔接关系,认为大洋中脊和环太平洋边缘俯冲带通过印度洋、北冰洋、特提斯构造域以及南极洲板块发生构造衔接和转换。南极洲板块周缘被洋中脊环绕,并衔接了全球洋中脊在地球南部的离散运动。结合构造赤道理论,分析了全球不同构造背景下的构造单元之间的关系,认为构造赤道是中生代以来全球构造体制大规模调整的产物。在此基础上,从泛大陆裂解,洋陆关系的角度探讨了中、新生代的全球构造演化。     

What processes at mid-ocean ridges tell us about volcanogenic massive sulfide deposits

Episodic seafloor spreading, ridge topography, and fault movement at ridges find (more extreme) analogs in the arc and back-arc setting where the volcanogenic massive sulfide (VMS) deposits that we mine today were formed. The factors affecting sulfide accumulation efficiency and the extent to which sulfides are concentrated spatially are the same in both settings, however. The processes occurring at mid-ocean ridges therefore provide a useful insight into those producing VMS deposits in arcs and back-arcs. The critical observation investigated here is that all the heat introduced by seafloor spreading at mid-ocean ridges is carried out of the crust within a few hundred meters of the ridge axis by ??350°C hydrothermal fluids. The high-temperature ridge hydrothermal systems are tied to the presence of magma at the ridge axis and greatly reduce the size and control the shape of axial magma intrusions. The amount of heat introduced to each square kilometer of ocean crust during its formation can be calculated, and its removal by high-temperature convection allows calculation of the total base metal endowment of the ocean basins. Using reasonable metal deposition efficiencies, we conclude that the ocean floor is a giant VMS district with metal resources >600 times the total known VMS reserves on land and a copper resource which would last >6,000?years at current production rates.     

Morphotectonics and tectonic processes of the Southwest Indian OceanEI北大核心CSCD

The Southwest Indian mid-ocean ridge (SWIR) is an ultraslow spreading ridge. Based on the submarine bathymetric data, we develop a new division principle on submarine morphotectonics and subdivide the SWIR into the seven-order tectonic geomorphologic units. Taking its submarine morphotectonics in the middle segment and adjacent seafloors of the mid-ocean ridge between Discovery II and Gallieni transform faults as a sample, this paper systematically analyzes its tectonic evolution, segmentation, segmentation and propagation mechanism, the formation of the central rift valley, the ridge-plume interactions, and the ocean ridge jumping. The results showed that the mid-ocean ridges can be divided into four three-order morphotectonics units (i.e., one-order segments of mid-ocean ridge), from west to east, which are separated by the Andrew Bain, the Prince Edwards, the Discovery II, and the Gallieni transform faults, respectively, corresponding to ridge landforms associated with a strongly hotspot-affected ridge, a weakly hotspot-affected ridge, and a normal ultraslow spreading ridge. Each segment can be further subdivided into three or four secondary segments. This paper focuses only on the segmentation and division from fourth-order to seventh-order morphotectonics units between the Discovery II and the Gallieni transform faults (i.e., the fourth-order morphotectonics unit of mid-ocean ridges can be subdivided into other three secondary units). Here the seventh-order morphotectonics unit consists of segments of laterally-aligned rifts (shear zone), en echelon rifts, and other transverse-faulting structures. The mid-ocean ridge segment experienced three oceanic ridge jumping at about 80 Ma, 60 Ma and 40 Ma, respectively, which were affected by the Marion and Crozet hotspots, or the Madagascar Plateau, etc. The oceanic processes of the SWIR are related to the Gondwana breakup, and its tectonic processes has been analyzed in detail as the periodic pull-apart extension, domino-style half-graben, graben subsidence, oceanic core complex, etc. in axial mid-oceanic ridge since 20 Ma. ©, 2015, Science Press. All right reserved.     

The problem of vortical movements in the solid earth and their role in geotectonics

Crustal structural features having a vortical or spiral shape were discovered in the first third of the 20th century. Since then, such features of various ranks, but similar appearance, have been revealed in different geotectonic settings; however, an adequate tectonic interpretation has not been offered. With allowance for the specific character of vortical movement, the evolution of the structural geometry of the North Atlantic basins and different segments of the global system of mid-ocean ridges is considered in this paper. It is shown that vortical movements do take place in the solid Earth during ocean formation and create scale-invariant rifting and spreading systems, where the spreading axis tends to undergo whirling. The size of these systems differs by more than two orders of magnitude. Many geotectonic phenomena that accompany the formation of oceans, including segmentation of the ocean floor and passive continental margins, folding of the sedimentary cover at these margins, and tectonic delamination of the oceanic lithosphere, may be explained by vortical movements of different ranks. In addition, the vortical structures on continents are variable in size and related to lithotectonic complexes of different ages. The vortical structural units of the Mediterranean Belt are considered as an example. Being driven by the same physical mechanism, the vortical movements depend on the dynamics of different geospheres. These movements are realized only in a nonlinear, nonequilibrium medium. Hence, only nonlinear and nonequilibrium thermodynamics will serve as a theoretical basis for a new concept, which is coming currently to take the place of plate tectonics.     

洋中脊热液系统中的锇及其同位素

洋中脊热液系统是将相对富集在深部的Os运移到海底表面的重要媒介,同时该过程也是全球Os循环的重要组成部分.在归纳总结洋中脊热液系统各物源组分和产物中Os的化学形态、含量及其同位素组成特征的基础上,探讨了Os在洋中脊热液活动各阶段中的分布演化规律及物源贡献特征.在缺乏沉积物覆盖的洋中脊区域,热液系统中的Os及其同位素组成特征主要受控于海水和不同构造环境下洋壳组分特征的差异以及这两种物源组分混合比例的不同.经历了海底之下的水岩反应后,围岩会将下渗海水中的部分放射性成因Os固定,而将自身富集的非放射性成因Os释放进入热液流体中.堆积在海底之上的各种热液产物中的Os大多来自海水,而海底之下的热液产物则因为海水下渗深度以及海水与热液流体混合程度的差异而体现出宽泛的Os含量和187Os/188Os比值变化范围.      

Dependence of mid-ocean ridge morphology on spreading rate in numerical 3-D models

The morphology of natural mid-ocean ridges changes significantly with the rate of extension. Full spreading rate on Earth varies over more than one order of magnitude, ranging from less than 10 mm/yr at the Gakkel Ridge in the Arctic Ocean to 170 mm/yr at the East Pacific Rise. The goal of this study is to reproduce and investigate the spreading patterns as they vary with extension rate using 3-D thermomechanical numerical models. The applied finite difference marker-in-cell code incorporates visco-plastic rheology of the lithosphere and a crustal growth algorithm. The evolution of mid-ocean ridges from nucleation to a steady-state is modelled for a wide range of spreading rates. With increasing spreading rate, four different regimes are obtained: (a) stable alternating magmatic and amagmatic sections (≈ 10 mm/yr), (b) transient features in asymmetrically spreading systems (≈ 20 mm/yr), (c) stable orthogonal ridge-transform fault patterns (≈ 40 mm/yr) and (d) stable curved ridges (≥ 60 mm/yr). Modelled ultraslow and slow mid-ocean ridges share key features with natural systems. Abyssal hills and oceanic core complexes are the dominant features on the flanks of natural slow-spreading ridges. Numerically, very similar features are produced, both generated by localised asymmetric plate growth controlled by a spontaneous development of large-offset normal faults (detachment faults). Asymmetric accretion in our models implies a lateral migration of the ridge segment, which might help explaining the very large offsets observed at certain transform faults in nature.     

慢速—超慢速扩张西南印度洋中脊研究进展

西南印度洋中脊具有慢速—超慢速扩张速率和斜向扩张的特征,是全球洋中脊系统研究的热点之一,也是研究海底构造环境、热液活动、地幔深部过程及其动力学机制的重要区域。在前人工作的基础上较为详细地介绍了西南印度洋中脊的研究历史、地形划分、扩张速率及其构造特征,归纳了西南印度洋中脊热液活动及岩石地球化学特征,探讨了超慢速扩张洋脊和超镁铁质岩系热液系统的特殊性,并认为超慢速扩张洋脊广泛暴露的地幔岩及其蛇纹石化作用、超镁铁质岩系热液系统以及热液硫化物成矿作用是西南印度洋中脊今后研究的重要内容。     

Accretion of oceanic crust under conditions of oblique spreading

The accretion of oceanic crust under conditions of oblique spreading is considered. It is shown that deviation of the normal to the strike of mid-ocean ridge from the extension direction results in the formation of echeloned basins and ranges in the rift valley, which are separated by normal and strike-slip faults oriented at an angle to the axis of the mid-ocean ridge. The orientation of spreading ranges is determined by initial breakup and divergence of plates, whereas the within-rift structural elements are local and shallow-seated; they are formed only in the tectonically mobile rift zone. As a rule, the mid-ocean ridges with oblique spreading are not displaced along transform fracture zones, and stresses are relaxed in accommodation zones without rupture of continuity of within-rift structural elements. The structural elements related to oblique spreading can be formed in both rift and megafault zones. At the initial breakup and divergence of continental or oceanic plates with increased crust thickness, the appearance of an extension component along with shear in megafault zones gives rise to the formation of embryonic accretionary structural elements. As opening and extension increase, oblique spreading zones are formed. Various destructive and accretionary structural elements (nearly parallel extension troughs; basin and range systems oriented obliquely relative to the strike of the fault zone and the extension axis; rhomb-shaped extension basins, etc.) can coexist in different segments of the fault zone and replace one another over time. The Andrew Bain Megafault Zone in the South Atlantic started to develop as a strike-slip fault zone that separated the African and Antarctic plates. Under extension in the oceanic domain, this zone was transformed into a system of strike-slip faults divided by accretionary structures. It is suggested that the De Geer Megafault Zone in the North Atlantic, which separated Greenland and Eurasia at the initial stage of extension that followed strike-slip offset, evolved in the same way.     

Deformation of oceanic lithosphere near slow-spreading ridge discontinuities

Transform and non-transform discontinuities that offset slow spreading mid-ocean ridges involve complex thermal and mechanical interactions. The truncation of the ridge axis influences the dynamics of spreading and accretion over a certain distance from the segment-end. Likewise, the spreading system is expected to influence the lithospheric plate adjacent to the ridge-end opposite of the discontinuity. Tectonic effects of the truncated ridge are noticeable in for example the contrast between seafloor topography at inside corners and outside corners, along-axis variations in rift valley depth, style of crustal accretion, and ridge segment retreat and lengthening. Along such slow-spreading discontinuities and their fossil traces, oceanic core complexes or mega-mullion structures are rather common extensional tectonic features. In an attempt to understand deformation of oceanic lithosphere near ridge offsets, the evolution of discontinuities, and conditions that may favor oceanic core complex formation, a three-dimensional thermo-mechanical model has been developed. The numerical approach allows for a more complete assessment of lithosphere deformation and associated stress fields in inside corners than was possible in previous 3-D models. The initial suite of results reported here focuses on deformation when axial properties do not vary along-strike or with time, showing the extent to which plate boundary geometry alone can influence deformation. We find that non-transform discontinuities are represented by a wide, oblique deformation zone that tends to change orientation with time to become more parallel to the ridge segments. This contrasts with predicted deformation near transform discontinuities, where initial orientation is maintained in time. The boundary between the plates is found to be vertical in the center of the offset and curved at depth in the inside corners near the ridge–transform intersection. Ridge–normal tensile stresses concentrate in line with the ridge tip, extending onto the older plate across the discontinuity, and high stress amplitudes are absent in the inside corners during the magmatic accretionary phase simulated by our models. With the tested rheology and boundary conditions, inside corner formation of oceanic core complexes is predicted to be unlikely during magmatic spreading phases. Additional modeling studies are needed for a full understanding of extensional stress release in relatively young oceanic lithosphere.     

天然矿物自然铝的研究进展

综述了国内外自然铝的发现与研究史;自然铝的物理性质和颗粒形态、元素组成及含量、晶体结构参数等特征;自然铝的成因模式。自然铝主要见于老的火山和热液矿石中,或现代和中-新生代的海底活动构造带（如转换断层、中央海隆以及弧后扩张中心）的海洋沉积物中,有地幔碳热还原、海底热液内生和陆地表生置换等3种成因模式。     

热点作用背景下的洋中脊跃迁和扩展作用:印度洋盆地张开过程探讨

在《印度洋底大地构造图》的基础上,分析了印度洋盆构造格局和洋盆演化重大事件序列,并从印度洋盆初始裂解机制、扩张中心跃迁与热点作用、洋中脊扩展作用等方面讨论了印度洋盆的张开过程,提出以下几点认识:(1)现今印度洋洋中脊可分为两个系统:东南印度洋中脊-中印度洋中脊-卡斯伯格洋脊系统(东支)和西南印度洋中脊系统(西支),前者是太平洋洋中脊扩展作用的产物,后者是太平洋-东南印度洋中脊与大西洋中脊之间构造调节的产物;(2)印度洋盆最初裂解受地幔柱垂向挤压-水平伸展作用控制,沿前寒武造山带等地壳薄弱带发育;(3)印度洋盆经历两次扩张中心的跃迁,其趋向性跃迁方向与热点相对板块的运动方向具有一致性,显示两者存在内在联系。(4)大西洋和太平洋洋中脊在印度洋交汇,于古近纪连通,末端伴随陆块持续发生碎裂化、裂解化,可称为鱼尾构造模式,表明印度洋盆衔接和调节了三大洋盆的发育和演化过程,具有全球洋盆枢纽的关键意义。