南海西南海盆壳幔结构重力反演与热模拟分析

壳幔结构及扩张期后的岩浆活动是研究南海西南海盆形成演化的关键.本文针对NH973-1剖面开展壳幔密度结构重力反演,并依据重力反演的壳幔模型,定量模拟海底扩张期后的壳幔热结构与热演化过程.重力反演表明:西南海盆中央残余扩张脊之下存在一个较深的凹陷带,其下Moho面比两侧略深,呈现扩张期后的热沉降特点.热模拟发现:海盆扩张...     

南海西南海盆构造演化的热模拟研究

南海西南海盆的张裂和海底扩张是白垩纪末至中始新世南海形成过程中最重要的构造事件.本文采用三维有限单元法对该区的热演化过程进行了模拟计算.通过对变形、温度结构的计算,研究了西南海盆张裂变形、海底扩张持续时间、地幔物质上升、地壳岩墙沿扩张中心的挤入扩张活力、岩浆活动等.计算结果表明：由于其深部动力学条件不足,海盆一次扩张持续时间在10～15Ma之间,其后地幔物质的上升活动逐渐停止,地壳失去扩张动力,使得扩张中心成为残留扩张中心的死亡裂谷,而未构成中脊或中隆带.虽然该处地幔物质上升的潜力不足,但伴随局部的断裂,尤其是盆、缘边界的拆离拉张,仍能产生相当强烈的岩浆喷溢活动,导致此区海盆成型之后的海山崛起.     

南海海盆三维重力约束反演莫霍面深度及其特征

利用南海海盆及周边最新的重力,经过海底地形、沉积层的重力效应改正,并采用岩石圈减薄模型的温度场公式,校正了从张裂边缘到扩张海盆的热扰动重力效应.通过研究区的地震剖面和少量声呐数据得到的莫霍面深度点作为约束,采用基于"起伏界面初始模型"的深度修正量反演迭代公式,反演、计算了研究区的莫霍面深度及地壳厚度.结果表明,海盆区莫霍面深度在8~14 km之间,地壳厚度在3~9 km之间;东部海盆和西南海盆残留扩张中心沿NNE向展布向西南延伸至112°E,莫霍面深度超过12 km,地壳厚度在6 km以上,而西北海盆没有明显的增厚扩张中心;在西南海盆北缘的中沙地块南侧,存在一个近EW向地壳减薄带,地壳厚度在9~10 km;莫霍面深度14 km的等深线和地壳厚度9 km的等值线可指示洋陆边界位置.     

南海西南次海盆NH973-1测线地震解释

针对973项目“南海大陆边缘动力学与油气资源潜力”2009年新采集的多道地震剖面NH973-1测线进行了研究分析,获得以下初步认识:(1)西南次海盆深海平原南端下伏巨厚沉积体,表明陆坡坡脚不是洋陆边界的位置,深海平原南端为陆壳分布区,也可解释为洋陆过渡带.这种情况在南海的洋陆边界确定过程中应加以考虑.(2)西南次海盆洋...     

南海西北次海盆的磁条带重追踪及洋中脊分段性

由于缺少有效钻孔资料,对于南海扩张的时间一直存在较大的疑问.在南海三大海盆中,西北次海盆面积最小、磁条带特征不明显,因此对其扩张年代的争议最大.最新采集的高密度(小于10 km测线间距)船测地磁资料清晰地显示了西北次海盆磁条带的存在.在OBS和多道地震资料的约束下,利用船测地磁资料,本文对西北次海盆的地壳年龄进行了重追踪.根据定量的比较,西北次海盆的主体扩张始于35.8 Ma(C16n,2n),在34.7 Ma(C15)时其西南部开始扩张,扩张最终同时终止于33.2 Ma(C13n),整体的全扩张速率在40~50 mm/a之间.这表明南海的扩张可能首先起源于西北次海盆,在其结束扩张后,东部次海盆才开始打开(约30 Ma).得益于数据精度和密度的提高,利用化极后的磁力异常以及反演的磁化强度可以对西北次海盆进行二级中脊段的划分.我们共划分出六个中脊段和一个明确的转换断层.中脊的分段性与OBS反演的地壳厚度的变化相一致.转换断层东侧,中脊主体分为四个中脊段,每个中脊段长度均在30 km左右.转换断层西侧,存在一个长约50 km的中脊段和一个不确切的中脊段.中脊段上磁化强度的变化幅值和中脊段长度在整体上成正比.每个中脊段中央的磁化强度弱于中脊段两端的磁化强度,这与扩张速率相近的大西洋中脊的磁化强度特征一致.     

南海西南次海盆北缘海底地震仪测线深部地壳结构研究

基于2009年和2011年采集的海底地震仪数据,辅以多道地震数据,对南海西南次海盆北缘的地壳结构进行了探索.利用二维射线追踪的反演方法建立测线上的模型.利用声学基底面的反射波,下地壳顶界面的反射波和莫霍面的反射波走时的反演勾绘了地层中的不连续界面,利用自声学基底面下的折射波和来自上地幔的首波来反演整条测线的P波速度结构...     

南海西南次海盆岩石圈结构及其地质意义

南海地区岩石圈资料稀少,阻碍了其形成演化过程的研究.为此,本次研究结合大地热流、空间重力异常、高程、大地水准面和地震数据,在南海西南次海盆反演了两条2.5维岩石圈剖面.本次计算基于三种假设：岩石圈地幔的密度取决于岩石温度;研究区岩石圈处于热稳定状态;研究区处于重力均衡状态.在剖面A-E中,岩石圈底界面从珠江口盆地的105 km迅速抬升到西沙海槽处的50 km,在西沙海槽、西沙-中沙群岛和西南次海盆变化不大,为50~60 km.在剖面F-I中,岩石圈底界面从西沙群岛-中建地块处的88 km向海盆逐渐抬升,在西南次海盆处为46~50 km,到郑和隆起再逐渐变深至64 km.我们比较了西南次海盆岩石圈的冷却模型和热稳定模型,根据冷却模型由水深和热流数据所推断的西南次海盆年龄比实际年龄差很多,说明冷却模型不适用于西南次海盆.通过对比剖面A-E和剖面F-I,说明了剖面A-E经历了更长时间的拉伸,证明南海西南次海盆在形成演化过程中是从北东向南西逐步打开的渐进式扩张.最后,我们综合分析西南次海盆及其大陆边缘的岩石圈结构、减薄陆壳区范围、碳酸盐台地的分布、下地壳韧性流动、流变结构和沉积层特征等多方面资料,认为西南次海盆在形成演化过程中岩石圈地幔首先破裂而地壳后破裂,属于type Ⅱ型非火山型大陆边缘.

     

南海共轭大陆边缘构造属性的综合地球物理研究

利用南海最新的重磁资料,在岩石物性分析和全海域分带变倾角化极磁异常反演磁性基底分布的基础上,选择6条典型剖面拟合反演其密度与磁性结构,在此基础上进行了深部结构的对比分析.反演中尽可能以海底地震仪探测数据(OBS)、多道地震等结果作为约束,其中FF'剖面层速度分析是利用“南海大陆边缘动力学及油气资源潜力”973项目200...     

南海新生代海底扩张的构造演化模式:来自高分辨率地球物理数据的新认识

根据高分辨率重、磁测网数据的分析,结合多波束海底地貌的构造解释,南海海盆新生代经历了两期不同动力特征的海底扩张,25 Ma的沉积-构造事件是其重要分界.早期扩张从约33.5 Ma开始至25 Ma停止,在东部海盆南、北两侧和西北海盆形成了具有近E-W向或NEE向磁条带的老洋壳,是近NNW-SSE向扩张的产物;晚期扩张从2...     

The deep thermal structure of the lithosphere in the northwestern South China Sea and its control on the shallow tectonics

The northwestern sub-basin of South China Sea(SCS) is a unique tectonic unit formed in the early spreading of the SCS. The northwestern Sub-basin has a series of complex geological structures such as seamounts and fault zones surrounded by the Xisha Trough, the Zhongsha Massif, and the Pearl River Valley. These extensional structures and magmatic activity in the northwestern sub-basin are closely related to the lithospheric structure and its deformation. However, details of the deep lithosphere structure are still poorly known. Here, we obtained detailed data of water and Moho depth using sonar buoys,Extended Spread Profiles(ESP), Ocean Bottom Seismometer(OBS), both Multi-beam and land-sea joint seismic surveys in the northwestern sub-basin and its surrounding areas. Then we adopted a thermal isostasy method to calculate the depth of the Lithosphere-Asthenosphere Boundary(LAB) in the northwestern sub-basin of the SCS and its surrounding regions. Results show that the range of LAB depth is ～25–110 km. The shallowest burial depth is 25–60 km occurring in the ocean basin. The depth increases to 60–110 km toward the continental margin. The lithospheric structure on the north and south sides of the Xisha Trough is symmetrical and shows the deep structure and thermal features of aborted rifts. The LAB depth in the Zhongsha Trough and the Zhongsha Massif increased from 60 to 70 km southwestwards, consistent with the trend of surface morphology.The LAB depth to the west side of the Pearl River Valley is 60–80 km, and the thinning of the lithosphere is related to the distribution of faults, depressions and the magmatic activity. The LAB depth in the northwestern sub-basin and the eastern subbasin is less than 60 km with the thinnest part being less than 46 km. Combining ocean drilling, seismic investigation, and seafloor topography, we show that the ocean basin of the northwestern sub-basin of the SCS locates within the 46 km isobath of the LAB. The formation of the rifted valleys and discrete blocks surrounding the ocean basins is both controlled by the regional tectonic movement and the deep thermal state, where their lithospheric structures show strong heterogeneity.     

南海及邻近地区面波层析成像和S波速度结构

本文介绍由面波层析成像得到的南海和邻近地区地壳上地幔三维S波速度结构.研究区域介于100°E～130°E和0°～30°N之间,南海位于区域中心,其北、西、南三面通过大陆架和陆坡分别与华南、印支和巽它地块相连,东面邻接台湾—菲律宾岛弧和西菲律宾海盆.由面波层析成像得到的速度结构横向变化与研究区内构造单元的划分基本相符,给...     

Mantle process beneath Philippine Sea back-arc spreading ridges: A synthesis of peridotite petrology and tectonics

Abstract In order to obtain a general view of the mantle process beneath a back‐arc basin spreading ridge, the diversity of peridotite petrology and tectonic occurrences in two back‐arc basin spreading ridges from the Philippine Sea were examined: the Parece Vela Rift and the Mariana Trough. The Parece Vela Basin spreading ridge (Parece Vela Rift) was a physically fast/intermediate‐spreading ridge, although many tectono‐magmatic features resemble those of slow‐ to ultraslow‐spreading ridges. Two unusual features of the Parece Vela Rift further demonstrate the uniqueness of the ridge: full‐axial development of oceanic core complexes and exposure of mantle peridotite at segment midpoints. The Parece Vela Rift yields a lithological assemblage of residual but still fertile lherzolite/harzburgite, plagioclase‐bearing harzburgite and dunite; similar assemblages are reported from the equatorial Mid‐Atlantic Ridge at the Romanche Fracture Zone and the ultraslow‐spreading ridges from the Indian and Arctic Oceans. The tectono‐magmatic characteristics of the Parece Vela Rift suggest that diffuse porous melt flow and pervasive melt–mantle interaction were the important mantle processes there. Globally, this ‘porous melt flow‐type’ mantle process is likely to occur beneath a segment midpoint of the ridge having a thick lithosphere, typically an ultraslow‐spreading ridge. In contrast, the Mariana Trough is a typical slow‐spreading ridge, exposing mantle peridotite at segment ends. The Mariana Trough yields a lithological assemblage of residual harzburgite and veined harzburgite, a common assemblage among the global abyssal peridotite suite. The tectono‐magmatic characteristics of the Mariana Trough suggest that channeled melt/fluid flow and limited melt–mantle interaction are the important mantle processes there, because of the colder wall‐rock peridotite in the segment end. This ‘channeled melt flow‐type’ mantle process is likely to occur in the shallow lithospheric mantle at the segment ends of any spreading ridges.     

南海大陆边缘动力学:科学实验与研究进展

国家重点基础研究发展计划(973)项目(2007CB411700)首次在南海南部大陆边缘及西南次海盆开展长排列大震源多道地震、海底地震仪(OBS)折射/反射地震等的综合地球物理探测,结合地质构造、地球化学、动力模拟等的综合研究,形成如下重要认识:南海海盆新生代发生了早、晚两期海底扩张.早期扩张发生于33.5～25 Ma...     

穿越东沙隆起和潮汕坳陷的OBS广角地震剖面

为了探明南海中北部陆缘深部地壳结构,使用2D射线追踪正演和反演方法,拟合了一条南海中北部陆缘的OBS广角地震剖面(OBS2006-3).该剖面穿越东沙隆起和潮汕坳陷,长319 km,NNW-SSE走向,共投放海底地震仪14台.速度结构模型表明:潮汕坳陷存在巨厚的中生代沉积,最大厚度达到8 km,速度从顶部的4.4 km...     

穿越南沙礼乐滩的海底地震仪广角地震试验

本文对穿越礼乐滩东北部向西北方向延伸进入中央海盆长369 km的广角地震剖面OBS973-2进行了反演研究,以期了解南海南部陆缘的地壳结构,同时探讨南、北陆缘的共轭问题.结果表明OBS973-2剖面的速度模型中三个沉积层的速度分别为1.8～2.0 km/s、2.0～2.7 km/s和3.5～4.0 km/s;沿剖面沉积...     

由高密度磁异常测量数据分析南海海盆的扩张年龄与扩张模式

南海是西太平洋最大的边缘海,地处欧亚板块、太平洋板块和印度洋板块的交汇处.过去通过磁异常条带对比分析南海扩张年龄的研究很多,但是所依赖的资料有限.本文对南海海盆高密度大批量磁异常测量数据进行了系统分析,实现了平面2D磁异常数据的带通滤波处理,消除了短波长噪音和由深部下地壳和上地幔顶部磁源体引起的长波长背景信息,因此突出了海底扩张所引起的磁异常条带.利用CK95地磁倒转模型和Talwani磁异常正演方法,对南海东部和西南次海盆内的重点磁异常测线进行了正演分析.通过对不同测线之间、不同海盆之间以及同一条测线中的正演磁异常与实测磁异常之间进行对比分析,进一步验证了南海东部次海盆的扩张年龄为32～16.5 Ma;西南次海盆可能的扩张年龄仍具有较大不确定性,可能为42～33 Ma或者24～16 Ma.不同的时间模型所依赖的扩张速率的变化情况不同,全扩张速率随时间变化明显,但主要在40～80 km/Ma之间.单纯根据目前的磁异常资料很难确定西南次海盆与东部次海盆之间的扩张次序.单期次扩张模式很难解释中南断裂两侧的构造物理差异,这种差异可能主要受控于其基底岩石成分、岩石磁化率、岩浆活动、扩张速率以及深部物质冷却磁化的影响,基底深度的变化也对观测磁异常的强度有所影响.相对地,大部分扩张后玄武岩海山的存在对观测的磁异常的影响不明显,针对目前磁异常解释中不可避免的多解性问题,需要运用其他不同的手段和方法,譬如大洋钻探和深拖高分辨率磁异常测量等,来实现对南海不同次海盆扩张年龄的精确估计.我们目前的工作是通向对深拖高分辨率磁异常、船测和航测磁异常、以及卫星磁异常综合解释的第一步.     

A Cretaceous to Paleocene-Eocene South China sea basin origin for the Zambales Ophiolite Complex,Luzon, Philippines?

Abstract The Eocene Zambales Ophiolite Complex that exhibits transitional mid-ocean ridge basalt-island arc tholeiite (MORB-IAT) characteristics was formed in a subduction-related marginal basin. The different surrounding marginal basins of the Philippines, namely, the South China Sea, Sulu Sea Basin, Celebes Basin and the West Philippine Basin have all been modeled to be of probable provenance of this ophiolite complex. Certain information (e.g. age, rock geochemistry, paleomagnetic rotations) and limitations, nevertheless, are inconsistent with the ophiolite complex being generated in these regions. Recent geophysical evidence suggests that the southwest sub-basin of the South China Sea Basin is probably Cretaceous to Paleocene-Eocene in age. This makes it possible to speculate that the Zambales Ophiolite Complex could have come from this sub-basin. The present day rifting of the southern Izu-Mariana arc can be taken as a modern day analog of this type of ophiolite generation.     

Development of basins in the Inner Moray Firth and the North Sea by crustal extension and dextral displacement of the Great Glen Fault

Reflection seismic data provide evidence that Mesozoic dextral movements along the Great Glen Fault line have had an important influence on the development of the Inner Moray Firth Basin. Geophysical evidence further indicates that deep structure beneath the inner basin is dissimilar to that beneath the outer part and Viking and Central Grabens in the North Sea. Tectonic development of the inner basin can nevertheless be fitted into a pattern of North Sea extensional movements which led to the formation of the graben system with which the major North Sea hydrocarbon resources are associated.     

南海西南次海盆的地热流特征与分析

为系统地了解南海西南次海盆的地热流特征,本文通过对研究区及邻域地热流数据的补充采集、收集整理和统计分析,获得了87个有效的地热流数据、一批热导率和生热率的地热参数资料,地热流测点在空间上覆盖了整个区域.研究区的地热流数据分布结果表明,西南次海盆热流密度的平均值为98.1±14.8 mW·m^-2,洋陆过渡带为103.6±19.4 mW·m^-2,南沙岛礁区和西部陆缘分别为79.0±15.5 mW·m^-2和78.3±15.6 mW·m^-2.研究区表层沉积物热导率的平均值0.86±0.06 W·mK^-1,生热率的平均值1.11±0.17 μW·m^-3,海底温度的平均值为2.43±0.01℃.综合海底地形地貌、地质与地球物理资料,认为研究区的热流特征在空间上具有一定的分布规律,表现为：（1）洋盆区测点的热流密度平均值高于两侧陆缘;（2）东南缘洋陆过渡带上测点的地热流密度值高于邻近海盆和南沙岛礁区的测点,而西北缘这种特征不明显;（3）西北翼的热流密度值总体比东南翼高;（4）沿着古扩张中心方向,西南次海盆热流值具有自东北向西南端方向逐步增大的趋势,表明海盆区同时存在着洋中脊与大陆裂谷两种不同的热状态,西南段裂谷热流值比东北段洋中脊高.对西南次海盆沉积物的热导率和生热率值参数的测量及数据空间分析可见,这两种热参数的空间分布无明显规律性,可能与海盆形成之后复杂的沉积环境相关.根据热流-洋壳年龄之间的关系,在西南次海盆东北段26个测站数据中,发现靠近古扩张中心的数据与理论值呈负偏移,而远离古扩张中心的数据呈正偏移,此现象是海盆内地热流数据受不同类型的地下流体影响所致.

     

Summary of electromagnetic investigations in the western part of the Black Sea

Two geoelectric models of the transition zone between the continent and the Black Sea basin were constructed from a variety of independent exploratory methods using natural electromagnetic fields. The models presented characterize some important features of the deep structure of the sea-shore transition zone. In particular, geoelectric properties of the lithosphere beneath the Black Sea basin are found to be approximately oceanic.