南海北部陆缘地壳结构特征及其构造过程

根据“北部湾大陆缘地壳结构ＰＳ转换波测深”等地球物理测量结果,本文研究了南海北部陆缘的地壳结构特征,讨论了其白垩纪以来的构造过程。地球物理测量表明,由陆向海,南海北部陆缘地壳由陆壳、过渡壳变为洋壳,厚度由３４ｋｍ减薄至８ｋｍ左右。垂向上地壳为３层结构模式。陆壳、过渡壳和洋壳的下地壳Ｐ波速度普遍较高。地壳伸展系数的计算表明南海北部陆缘伸展主要发育于陆坡地区。结合区域地质研究,本文认为：南海北部陆缘及     

地球早期大陆地壳的形成与演化

现代地球岩石圈主要由镁铁质上地幔和长英质地壳两个储集层组成,研究大陆地壳的形成和演化对揭示地球早期地质过程和物质循环、厘定板块构造启动时限具有重要意义。冥古宙—始太古代具有更高的地幔潜能温度和地温梯度,岩浆海冷却形成薄的原始地壳;大洋岩石圈表现为韧性,主要构造机制应为停滞盖层模式,有地幔柱参与。太古宙片麻岩中奥长花岗岩—英云闪长岩—花岗闪长岩（TTG）的出现标志着镁铁质原始地壳向长英质陆壳转变的开始。本文总结了地球早期停滞盖层模式到现代板块构造模式下含水玄武岩部分熔融、结晶分异形成大陆地壳的过程,主要包含幔源岩浆停滞盖层（“自下而上”的热管火山岩和“自上而下”的深成侵入岩构造模式）、增厚镁铁质地壳部分熔融、俯冲洋壳、岛弧及洋底高原部分熔融模式;陆壳的破坏和消减主要受陨石撞击、分层沉降、重力不稳导致拆沉控制;板块构造的出现进一步促进了地球内部的热量扩散,俯冲作用加快了洋壳和陆壳之间的物质循环。最后,结合太古宙变质岩、古老克拉通岩石学特征和锆石Hf、O及全岩Nd、Sr、Ar、Ti同位素组成,讨论了陆壳的形成时间和演化过程： 3.0 Ga之前形成了现有陆壳体积的60%~70%,厚度约为20~40 km;3.0~2.5 Ga,地壳改造速率明显增加,陆壳生长和破坏速率达到动态平衡,表明全球性现代板块构造体制逐渐成为控制大陆形成、裂解和陆壳演化的主要因素。     

地球早期大陆地壳的形成与演化

现代地球岩石圈主要由镁铁质上地幔和长英质地壳两个储集层组成,研究大陆地壳的形成和演化对揭示地球早期地质过程和物质循环、厘定板块构造启动时限具有重要意义。冥古宙—始太古代具有更高的地幔潜能温度和地温梯度,岩浆海冷却形成薄的原始地壳;大洋岩石圈表现为韧性,主要构造机制应为停滞盖层模式,有地幔柱参与。太古宙片麻岩中奥长花岗岩—英云闪长岩—花岗闪长岩(TTG)的出现标志着镁铁质原始地壳向长英质陆壳转变的开始。本文总结了地球早期停滞盖层模式到现代板块构造模式下含水玄武岩部分熔融、结晶分异形成大陆地壳的过程,主要包含幔源岩浆停滞盖层(“自下而上”的热管火山岩和“自上而下”的深成侵入岩构造模式)、增厚镁铁质地壳部分熔融、俯冲洋壳、岛弧及洋底高原部分熔融模式;陆壳的破坏和消减主要受陨石撞击、分层沉降、重力不稳导致拆沉控制;板块构造的出现进一步促进了地球内部的热量扩散,俯冲作用加快了洋壳和陆壳之间的物质循环。最后,结合太古宙变质岩、古老克拉通岩石学特征和锆石Hf、O及全岩Nd、Sr、Ar、Ti同位素组成,讨论了陆壳的形成时间和演化过程：3.0 Ga之前形成了现有陆壳体积的60%～70%,厚度约为20～4...     

青藏高原隆升机制新模式

作为创建大陆动力学理论体系的最佳野外实验室的青藏高原, 涉及当代固体地球科学前沿和热点的许多重大科学问题.迄今为止, 包括板块构造在内的众多模式不能合理地解释青藏高原重要的地质和地球物理现象.本文从下地壳与中上地壳、造山带与沉积盆地的耦合作用出发, 对青藏高原及邻区进行分尺度、分层块、分阶段的构造解析, 提出青藏高原隆升的下地壳层流构造模式, 认为青藏高原地壳增厚和构造隆升是晚新生代由于锡瓦利克盆地、塔里木盆地和四川盆地下地壳的热软化岩石大量流向青藏高原造成的.      

地壳早期演化的研究进展

地壳早期演化研究的主题是探讨早期大陆形成、生长和再循环的地质过程及其地球化学和地球物理模式。由于陆上古老岩石分布极为有限,围绕着陆壳生长速率的争论持续了30多年。地球化学家基于陆壳从地幔萃取而成并导致被萃取后的地幔在地球化学上产生亏损的认识,提出了许多重要的大陆形成、生长、再循环模式。近年来发展起来的高精度MC ICPMS分析技术,使单颗粒锆石Lu Hf同位素系统分析为评价早期地壳演化提供了更多的信息和更为可靠的证据。不同大陆早前寒武纪地壳及地幔地球物理和地球化学状态研究表明,陆壳再循环作用、壳—幔以及壳内（如古老的地壳重熔作用及其与相对较新的地壳发生广泛的混合作用）相互作用是早期大陆演化的重要地质过程。     

惠东─连县地学断面的地壳结构及性质研究

本文利用地球物理－地质地球化学相结合的研究方法，分析了惠东─连县地学断面的地球物理特征及其速度密度模型，探讨了断面地壳的物质组成、结构和深部地壳的形成时代，认为该断面地壳的物质组成以长英质为主，断面深部存在太古代地壳，断面的地壳分层主要由变质相相变产生，由麻粒岩相下地壳、高绿片岩相－角闪岩相中地壳，低绿片岩相及沉积盖层组成上地壳的三部分．     

大陆深部地壳研究中的地质──地球化学方法概述

迄今为止，地球物理方法一直是研究深部地壳结构的重要方法，这种方法主要是利用岩石的物理性质来推测深部地壳的物质组成，地壳的分层及分层界面性质。随着近年来研究发现许多依据地球物理资料和地表地质确定的深度超过1500m即定目标都未得到深钻或超深钻的证实（肖庆辉，1993），这种结果在地学界引起很大反响。从另一个意义上，由地球物理方法确定的地壳仅反映其终态，而对复杂的地壳演化方面尚显不足。深钻和超深钻方法近年来已成为探测深部地完结构的一种重要方法，它可以直观的研究深部地壳的岩浆作用、构造作用、成矿作用，也是研究…     

论南沙海槽的地壳性质

根据海上地球物理测量,对四条剖面的重力和地震剖面资料进行联合正反演推算,结合已发表的国内外地质、地球物理资料对南沙海槽的地壳厚度及性质进行了分析。结果表明,南沙海槽的地壳为一个减薄的陆壳,从南沙微陆块向婆罗洲方向厚度减薄,具有类似大陆边缘从陆壳向洋壳过渡部位的地壳构造特征。顺着海槽的走向,地壳厚度变化趋势是从东北向西南变薄。从构造演化的角度分析,南沙海槽是古南海洋陆交界的边缘,由于古南海的闭合及晚白垩世以后婆罗洲逆时针方向旋转,海槽的大部分是陆壳,其西南端可能有残留的洋壳。     

地壳结构的轮廓和形成

M.尤文、F.普瑞斯論述过“大陆和大洋盆地之間的地球物理差异”,J.季陆利述及过“大陆和大洋盆地之間的地貭差异”。P.M.捷麦尼茲卡娅編制过世界地壳結构厚度图,并論証过地壳厚度与地貭年代的关系。柴田勇曾討論过地壳的分层及其发展过程。这些工作对我們认識地壳結构的輪廓及其发展作出了重要的貢献。本文拟在截至目前为止所收得到的地壳地震測深資料及高温高压下岩石物理性貭实驗結果,結合地面地貭构造研究所取得的結果,来进一步討論一下地壳的厚度、分层、物貭組成及其发展过程等有关問題。     

戈壁荒漠覆盖区地质调查中综合地球物理方法与实践

戈壁荒漠覆盖区地质填图是新时期地质调查工作的重点内容之一.覆盖区地质填图的基本目标包括两个方面,一是揭示覆盖层下伏基岩面地质结构,即填绘基岩面地质图;二是揭示覆盖层地质结构,包括地表覆盖层地质结构和覆盖层的三维地质结构.综合利用地球物理方法可以获得覆盖区地下地质结构、岩石属性、沉积物分布与层状结构等信息.而经济有效地选择和组合实施地球物理方法是完成覆盖区地质填图目标任务的重要保障.基于近年在新疆东天山地区开展的覆盖区地质填图工作,提出了针对多覆盖层结构背景下地质填图的综合地球物理方法组合的技术策略.综合地球物理方法以及新技术在巴里坤盆地和哈密盆地的应用展示了其效果,并为在戈壁荒漠覆盖区地质调查过程中如何开展地球物理工作提供了示范和借鉴.      

From oceanic plateaus to allochthonous terranes: Numerical modelling

Large segments of the continental crust are known to have formed through the amalgamation of oceanic plateaus and continental fragments. However, mechanisms responsible for terrane accretion remain poorly understood. We have therefore analysed the interactions of oceanic plateaus with the leading edge of the continental margin using a thermomechanical–petrological model of an oceanic-continental subduction zone with spontaneously moving plates. This model includes partial melting of crustal and mantle lithologies and accounts for complex rheological behaviour including viscous creep and plastic yielding. Our results indicate that oceanic plateaus may either be lost by subduction or accreted onto continental margins. Complete subduction of oceanic plateaus is common in models with old (> 40 Ma) oceanic lithosphere whereas models with younger lithosphere often result in terrane accretion. Three distinct modes of terrane accretion were identified depending on the rheological structure of the lower crust and oceanic cooling age: frontal plateau accretion, basal plateau accretion and underplating plateaus.Complete plateau subduction is associated with a sharp uplift of the forearc region and the formation of a basin further landward, followed by topographic relaxation. All crustal material is lost by subduction and crustal growth is solely attributed to partial melting of the mantle.Frontal plateau accretion leads to crustal thickening and the formation of thrust and fold belts, since oceanic plateaus are docked onto the continental margin. Strong deformation leads to slab break off, which eventually terminates subduction, shortly after the collisional stage has been reached. Crustal parts that have been sheared off during detachment melt at depth and modify the composition of the overlying continental crust.Basal plateau accretion scrapes oceanic plateaus off the downgoing slab, enabling the outward migration of the subduction zone. New incoming oceanic crust underthrusts the fractured terrane and forms a new subduction zone behind the accreted terrane. Subsequently, hot asthenosphere rises into the newly formed subduction zone and allows for extensive partial melting of crustal rocks, located at the slab interface, and only minor parts of the former oceanic plateau remain unmodified.Oceanic plateaus may also underplate the continental crust after being subducted to mantle depth. (U)HP terranes are formed with peak metamorphic temperatures of 400–700 °C prior to slab break off and subsequent exhumation. Rapid and coherent exhumation through the mantle along the former subduction zone at rates comparable to plate tectonic velocities is followed by somewhat slower rates at crustal levels, accompanied by crustal flow, structural reworking and syndeformational partial melting. Exhumation of these large crustal volumes leads to a sharp surface uplift.     

Crustal structure of the continental margin of Korea in the East Sea (Japan Sea) from deep seismic sounding data: evidence for rifting affected by the hotter than normal mantle

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.     

洋脊地质学与成矿学

洋脊分活动型和稳定型两种,柱状地质剖面由未固结沉积物和上、下洋壳三部分构成,横向断裂带发育。岩石蚀变、变质普遍,可与大陆拉斑玄武岩对比。洋脊正在进行两种成矿过程。近20年在洋脊发现的矿床(化)可分为11个类型,其中有的具有工业意义。洋脊研究的深入,将进一步揭示洋壳的奥秘,还将提高对陆壳以及整个地球历史演化进程中的沉积、岩浆、变质、成矿、成岩和构造等作用以及这些作用之间相互促进和制约关系的认识。     

Thin and layered subcontinental crust of the great Basin western north America inherited from Paleozoic marginal ocean basins?

The seismic profile of the crust of the northern part of the Basin and Range province by its thinness and layering is intermediate between typical continental and oceanic crust and resembles that of marginal ocean basins, especially those with thick sedimentary fill. The geologic history of the Great Basin indicates that it was the site of a succession of marginal ocean basins opening and closing behind volcanic arcs during much of Paleozoic time. A long process of sedimentation and deformation followed throughout the Mesozoic modifying, but possibly not completely transforming the originally oceanic crust to continental crust. In the Cenozoic, after at least 40 m.y. of quiescence and stable conditions, substantial crustal and upper-mantle changes are recorded by elevation of the entire region in isostatic equilibrium, crustal extension resulting in Basin and Range faulting, extensive volcanism, high heat flow and a low-velocity mantle. These phenomena, apparently the result of plate tectonics, are superimposed on the inherited subcontinental crust that developed from an oceanic origin in Paleozoic time and possibly retained some of its thin and layered characteristics. The present anomalous crust in the Great Basin represents an accretion of oceanic geosynclinal material to a Precambrian continental nucleus apparently as an intermediate step in the process of conversion of oceanic crust into a stable continental landmass or craton.     

Construction of the granitoid crust of an island arc. Part II: a quantitative petrogenetic model

Results of simple model calculations that integrate cumulate compositions from the Kohistan arc terrain are presented in order to develop a consistent petrogenetic model to explain the Kohistan island arc granitoids. The model allows a quantitative approximation of the possible relative roles of fractional crystallization and assimilation to explain the silica-rich upper crust composition of oceanic arcs. Depending in detail on the parental magma composition hydrous moderate-to-high pressure fractional crystallization in the lower crust/upper mantle is an adequate upper continental crust forming mechanism in terms of volume and compositions. Accordingly, assimilation and partial melting in the lower crust is not per se a necessary process to explain island arc granitoids. However, deriving few percent of melts using low degree of dehydration melting is a crucial process to produce volumetrically important amounts of upper continental crust from silica-poorer parental magmas. Even though the model can explain the silica-rich upper crustal composition of the Kohistan, the fractionation model does not predict the accepted composition of the bulk continental crust. This finding supports the idea that additional crustal refining mechanism (e.g., delamination of lower crustal rocks) and/or non-cogenetic magmatic process were critical to create the bulk continental crust composition.     

The episodic development of intermediate to silicic volcano-plutonic suites in the Archaean West Pilbara, Australia

Four felsic igneous rock suites in the Archaean West Pilbara have been identified based on geochemistry and geochronology. A voluminous TTG suite formed at ca. 3260 Ma, which appears to be from melting of a mafic-subducted oceanic slab and thus represents generation of new continental crust. A tholeiitic to calc-alkaline volcanic assemblage and coeval granitoids formed at ca. 3120 Ma in an extensional environment. Further TTG magmatism occurred at ca. 3000 Ma, generating both large granitoid complexes and small plutons, again adding new continental crust to the West Pilbara. At 2930-Ma crustal reworking, most likely of the 3000-Ma rocks, generated small plutons that are coeval with layered ultramafic-mafic intrusions in the region. The changes from new crustal material to crustal reworking infer changing tectonic regimes, which is important for models of Archaean continental crust generation. The data presented here indicate that crustal generation mechanisms varied and were episodic in the West Pilbara, implying that early crustal evolution was a result of periodic changes in tectonic regime, which is reflected in the geochemistry of the rocks.     

From continental rifting to seafloor spreading: Insight from 3D thermo-mechanical modeling

Continental rifting to seafloor spreading is a continuous process, and rifting history influences the following spreading process. However, the complete process is scarcely simulated. Using 3D thermo-mechanical coupled visco-plastic numerical models, we investigate the complete extension process and the inheritance of continental rifting in oceanic spreading. Our modeling results show that the initial continental lithosphere rheological coupling/decoupling at the Moho affects oceanic spreading in two manners: (1) coupled model (a strong lower crust mechanically couples upper crust and upper mantle lithosphere) generates large lithospheric shear zones and fast rifting, which promotes symmetric oceanic accretion (i.e. oceanic crust growth) and leads to a relatively straight oceanic ridge, while (2) decoupled model (a weak ductile lower crust mechanically decouples upper crust and upper mantle lithosphere) generates separate crustal and mantle shear zones and favors asymmetric oceanic accretion involving development of active detachment faults with 3D features. Complex ridge geometries (e.g. overlapping ridge segments and curved ridges) are generated in the decoupled models. Two types of detachment faults termed continental and oceanic detachment faults are established in the coupled and decoupled models, respectively. Continental detachment faults are generated through rotation of high angle normal faults during rifting, and terminated by magmatism during continental breakup. Oceanic detachment faults form in oceanic crust in the late rifting–early spreading stage, and dominates asymmetric oceanic accretion. The life cycle of oceanic detachment faults has been revealed in this study.     

The building blocks of continental crust: Evidence for a major change in the tectonic setting of continental growth at the end of the Archean

Oceanic arcs are commonly cited as primary building blocks of continents, yet modern oceanic arcs are mostly subducted. Also, lithosphere buoyancy considerations show that oceanic arcs (even those with a felsic component) should readily subduct. With the exception of the Arabian–Nubian orogen, terranes in post-Archean accretionary orogens comprise < 10% of accreted oceanic arcs, whereas continental arcs compose 40–80% of these orogens. Nd and Hf isotopic data suggest that accretionary orogens include 40–65% juvenile crustal components, with most of these (> 50%) produced in continental arcs.Felsic igneous rocks in oceanic arcs are depleted in incompatible elements compared to average continental crust and to felsic igneous rocks from continental arcs. They have lower Th/Yb, Nb/Yb, Sr/Y and La/Yb ratios, reflecting shallow mantle sources in which garnet did not exist in the restite during melting. The bottom line of these geochemical differences is that post-Archean continental crust does not begin life in oceanic arcs. On the other hand, the remarkable similarity of incompatible element distributions in granitoids and felsic volcanics from continental arcs is consistent with continental crust being produced in continental arcs.During the Archean, however, oceanic arcs may have been thicker due to higher degrees of melting in the mantle, and oceanic lithosphere would be more buoyant. These arcs may have accreted to each other and to oceanic plateaus, a process that eventually led to the production of Archean continental crust. After the Archean, oceanic crust was thinner due to cooling of the mantle and less melt production at ocean ridges, hence, oceanic lithosphere is more subductable. Widespread propagation of plate tectonics in the late Archean may have led not only to rapid production of continental crust, but to a change in the primary site of production of continental crust, from accreted oceanic arcs and oceanic plateaus in the Archean to primarily continental arcs thereafter.     

中国东部新生代玄武岩记录古太平洋俯冲带壳幔相互作用

大陆玄武岩通常具有与洋岛玄武岩相似的地球化学成分,其中含有显著的壳源组分.对于洋岛玄武岩来说,虽然其中的壳源组分归咎于深俯冲大洋板片的再循环,但是对板片俯冲过程中的壳幔相互作用缺乏研究.对于大陆玄武岩来说,由于其形成与特定大洋板片在大陆边缘之下的俯冲有关,可以用来确定古大洋板片俯冲的地壳物质再循环.本文总结了我们对中国东部新生代玄武岩所进行的一系列地球化学研究,结果记录了古太平洋板片俯冲析出流体对地幔楔的化学交代作用.这些大陆玄武岩普遍具有与洋岛玄武岩类似的地球化学成分,在微量元素组成上表现为富集LILE和LREE、亏损HREE,但是不亏损HFSE的分布特点,在放射成因同位素组成上表现为亏损至弱富集的Sr-Nd同位素组成.在排除地壳混染效应之后,这些玄武岩的地球化学特征可以由其地幔源区中壳源组分的性质来解释.俯冲大洋地壳部分熔融产生的熔体提供了地幔源区中的壳源组分,其中包括洋壳镁铁质火成岩、海底沉积物和大陆下地壳三种组分.华北和华南新生代大陆玄武岩在Pb同位素组成上存在显著差异,反映它们地幔源区中的壳源组分有所区别.中国东部新生代玄武岩的地幔源区是古太平洋板片于中生代俯冲至亚欧大陆东部之下时,在>200 km的俯冲带深度发生壳幔相互作用的产物.在新生代期间,随着俯冲太平洋板片的回卷引起的中国东部大陆岩石圈拉张和软流圈地幔上涌,那些交代成因的地幔源区发生部分熔融,形成了现今所见的新生代玄武岩.      

造山带橄榄岩记录的大陆俯冲带多期壳幔相互作用

俯冲带是地壳与地幔之间物质交换的主要场所.前人对大洋俯冲带壳幔相互作用进行了大量研究,但是对俯冲带壳幔相互作用的物理化学过程和机理仍缺乏明确认识.在大陆俯冲带出露有造山带橄榄岩,它们来自俯冲板片之上的地幔楔,是解决这个问题的理想样品.通过对大别-苏鲁和柴北缘造山带橄榄岩进行系统的岩石学和地球化学研究,发现地幔楔橄榄岩由于俯冲地壳的交代作用而含有新生锆石和残留锆石,它们能为地壳交代作用时间、交代介质来源、性质和组成提供制约.地幔楔橄榄岩在大陆碰撞过程的不同阶段受到了俯冲大陆地壳衍生的多期不同性质流体的交代作用.地幔楔橄榄岩还受到了陆壳俯冲之前古俯冲洋壳衍生流体的交代作用.深俯冲陆壳衍生熔体与橄榄岩反应形成的石榴辉石岩具有高的水含量,能提供高水含量的地幔源区.