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1.
超越板块构造——我国构造地质学要做些什么? 总被引：25，自引：1，他引：24
对近十年来全球构造学和构造地质学的重要进展进行了简要评述.30年前建立的全球构造理论改变了人们对地球及其演化的认识.作为固体地球统一理论的板块构造主要涉及刚性板块边界之间的变形、地震活动和火山作用.至今还没有完整理论阐明板块运动的驱动力和地幔对流机制.板块边界和板内变形等许多问题仍然无法回答.大陆岩石圈和大洋岩石圈在成分、厚度和力学强度方面有明显的差别, 因此现有板块构造不完全适合于大陆构造.大陆地壳和地幔流变学的综合研究是认识大陆构造和超越板块构造的最佳途径.流变学是大陆造山带几何学和动力学的桥梁.大陆岩石圈对构造作用、重力作用和热作用的响应在很大程度上取决于其流变强度.岩石圈流变性质是岩石圈分层和塑性流动的主导因素.大量透入性变形和巨型大陆造山带内部构造显示非刚性特征.大陆构造和力学行为主要由地壳强度而不是地幔强度所控制.从大陆岩石圈多层性和力学强度不均匀性表征看, 现在是抛弃传统“三明治”构造模式的时候了.面对地球系统科学和地球动力学新思维发展趋势, 多学科综合研究大陆构造(造山带)和加速高水平构造地质学人才的培养是我国构造地质学发展的最紧迫任务 相似文献
2.
The reason for obduction, or tectonic transport of oceanic lithosphere onto continents, is investigated by two‐dimensional thermo‐mechanical numerical modelling based on the geology of the Anatolia–Lesser Caucasus ophiolites. Heating of the oceanic domain and extension induced by far‐field plate kinematics appear to be essential for the obduction of ~80‐Ma‐old oceanic crust over distances exceeding 200 km. Heating of the oceanic lithosphere by mantle upwelling is evidenced by a thick alkaline volcanic series emplaced on top of the oceanic crust 10–20 Ma before obduction, at the onset of Africa–Eurasia convergence. Regional heating reduced the negative buoyancy and strength of the magmatically old lithosphere. Extension facilitated the propagation of obduction by reducing the mantle lithosphere thickness, which led to the exhumation of eclogite‐free continental crust previously underthrusted beneath the ophiolites. This extensional event is ascribed to far‐field plate kinematics resulting from renewed Neotethys oceanic subduction beneath Eurasia. 相似文献
3.
中国西部大陆岩石圈的有效弹性厚度研究 总被引：8，自引：0，他引：8
中国西部是地球上陆地隆升最显著的地区, 有世界上新构造运动最强烈的青藏高原、规模巨大的左行走滑位移的阿尔金断裂系和中亚地区最大的板块内部造山带———天山褶皱造山带.作为印度板块与欧亚板块相互碰撞的会聚带, 本区是研究岩石圈动力学的有利场所.主要运用重力资料和地形资料来研究中国西部地区显著上地壳结构和其上地幔变形之间的关系.依据岩石圈流变学的理论, 在空间域采用垂直和水平受力的多个变刚度的三维有限差分方法来计算弹性板的有效弹性厚度.模拟结果显示中国西部地区的岩石圈有效弹性厚度存在明显的横向不均匀性, 从6~10 km的造山带区域的有效弹性厚度变到大于60 km的古陆区域的有效弹性厚度.青藏高原地区的岩石圈有效弹性厚度平均为30 km, 塔里木盆地的有效弹性厚度为40~50 km, 南、北天山的岩石圈有效弹性厚度分别为10~15 km和30 km左右, 阿尔金断裂在东经90°以西部分的岩石圈有效弹性厚度要小于90°以东部分. 相似文献
4.
A number of authors have modelled the flexure of the lithosphere at an oceanic trench using a thin elastic plate with a hydrostatic restoring force. In some cases good agreement with observed topography is obtained but in other cases the slope of the lithosphere within the trench is greater than that predicted by the elastic theory. In this paper the bending of a thin plate is considered using an elastic-perfectly plastic rheology. It is found that the lithosphere behaves elastically seaward of the trench, but that plasticity decreases the radius of curvature within the trench. The results are compared with a number of observed trench profiles. The elastic-perfectly plastic profiles are in excellent agreement with those profiles that deviate from elastic behavior. 相似文献
5.
超高压榴辉岩流变学研究 总被引：2，自引：0，他引：2
大陆岩石圈和大洋岩石圈在成分、厚度和力学强度方面有明显的差别。因此,现有板块构造不完全适合于大陆构造。大陆地壳和上地幔流变学的综合研究是认识大陆构造最佳途径之一。流变学研究是大陆造山带几何学、运动学和动力学的桥梁。大陆岩石圈对构造作用、重力不稳定性和热结构的响应在很大程度上取决于岩石流变强度。岩石圈流变性质是岩石圈分层、构造复杂性和塑性流动的主导控制因素。超高压榴辉岩在地幔对流、壳-幔物质循环和俯冲带动力学起着重要作用。榴辉岩的流变性质和变形机制对于阐明大陆造山带和大陆深俯冲的动力学过程具有十分重要的意义。本文主要内容包括以下4个方面：（1）岩石流变学研究在地球动力学中地位和重要性;（2）回顾池际尚先生对岩石流变学实验的贡献;（3）近几年来超高压榴辉岩流变学研究成果;（4）国外岩石流变学实验研究发展态势和启示。 相似文献
6.
中国东部燕山期和四川期岩石圈构造滑脱与岩浆起源深度 总被引：9，自引：0，他引：9
较确切地研究岩石圈内部构造滑脱面在地质历史时期形成的时间和部位是当前大地构造学研究的一个重要课题。通过大量收集中国东部燕山期(205~135Ma)和四川期(135~52Ma)岩浆起源深度资料来判断岩石圈内部和底部是否存在局部的构造滑脱界面,是否发生层圈相互作用,是否发生部分的解耦现象,是一种可行的研究方法。研究表明,中国东部燕山期和四川期岩石圈板块的构造滑脱、圈层的解耦作用及相互作用主要集中在中地壳、莫霍面与区域性主干断层的交线附近,而岩石圈板块的底面却并不存在大幅度的滑移。中国东部燕山期和四川期岩浆活动比较发育的地区基本上都位于大兴安岭—山西西部—武陵山—十万大山一线以东地区,而在此线以西地区岩浆活动相当微弱。笔者认为,在侏罗—白垩纪时期,该线以西缺少岩浆活动的地区可能就是当时的大陆型岩石圈,而该线以东岩浆活动剧烈的地区可能就属于海陆过渡型岩石圈。中国东部岩石圈的转型和"变薄",不太可能是深部地幔羽、去根作用、深部地幔热物质上涌或大陆伸展作用的结果,也不太可能与太平洋板块的俯冲作用有直接联系。 相似文献
7.
《Gondwana Research》2016,29(4):1329-1343
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. 相似文献
8.
Numerical modeling is used to investigate the interaction between mantle plume and continental lithosphere, especially the effect of the continental lithosphere structure, the scale and position of mantle plume on the rate of continental drift. Numerical results show that, under the effect of mantle plume, the existence of a thick root of the continental lithosphere affects the rate of continental drift. Moreover, under identical scale of mantle plume, the drift rate decreases with increasing thickness of the root. Besides, the velocity and distance of a continental plate drift are negatively correlated in scale of the continental lithosphere, but correlated with the scale of the mantle plume. For the model without lithospheric root, the mantle plume has a more appreciable impact on the plate drift rate when it comes closer to edge of the continental plate. Our models show that mantle plume can accelerate the continental drift by more than 10 cm/a. The modelling results can provide significant dynamical constraint and geological enlightenment. © 2018, Science Press. All right reserved. 相似文献
9.
Shun-Ichiro Karato 《Tectonophysics》1984,104(1-2)
The physical processes that govern the grain size of rocks in the upper mantle are examined. The analysis is based on the experimental data on creep, recrystallization, and grain growth in dunites and on a theoretical model for the thermomechanical structure of the cooling moving lithosphere. The grain size of rocks is shown to be determined by the in situ stress only at the deeper part where the temperature is high enough to allow significant strain rate. Above this depth, the microstructures record the thermomechanical history of rocks rather than the in situ stress.In the case of the oceanic lithosphere where the thermomechanical history is best known, the following features of grain-size distribution are found. At the uppermost mantle, where the amount of grain growth is limited, the grain size is determined by the initial value and the growth rate, and, where the effect of grain growth dominates, it increases with depth. When the amount of grain growth becomes large and the grain size reaches the steady state size corresponding to the ambient stress while the rock is hot enough to deform, the grain size is then determined by the applied stress. This grain size is, however, frozen, when the rock gets cool and the strain rate becomes too small to induce any further dynamic recrystallization. Thus, at the intermediate depth region, the grain size records the fossil (frozen) stress at which the microstructures of rock have been frozen. Since the frozen stress increases with age, the grain size in this depth interval decreases with depth. Finally, the grain size below this level reflects the in situ stress, and increases with depth, its extent being dependent on the nature of return flow in the deep mantle.Thus the grain size versus depth relation may show a sigmoid curve. The qualitative features of this curve may be similar also in the case of the continental lithosphere, if a similar thermal event (i.e., the intrusion of hot material and subsequent cooling) occurs. The results are quite consistent with the observed depth variation of olivine grain size in peridotite nodules (Avé Lallemant et al., 1980). The present model suggests that the depth of minimum grain size (65 and 150 km at the continental rift zone and the shield region respectively) corresponds to that where the mechanical properties of the upper mantle change from elastic to ductile at tectonic stress levels (~ 1 MPa) and in the geological time scale. This result leads to a new definition of the thickness of lithosphere in terms of its rheological properties. This thickness is about twice as large as that inferred from the flexure of lithosphere but approximately equal to seismic thickness. The model suggests the importance of grain growth as well as dynamic recrystallization and plastic flow in determining the texture of upper mantle rocks and therefore seismic anisotropy. 相似文献
10.
Initiation of Subduction Zones as a Consequence of Lateral Compositional Buoyancy Contrast within the Lithosphere: a Petrological Perspective 总被引：12，自引：1，他引：12
Tonga and Mariana fore-arc peridotites, inferred to representtheir respective sub-arc mantle lithospheres, are compositionallyhighly depleted (low Fe/Mg) and thus physically buoyant relativeto abyssal peridotites representing normal oceanic lithosphere(high Fe/Mg) formed at ocean ridges. The observation that thedepletion of these fore-arc lithospheres is unrelated to, andpre-dates, the inception of present-day western Pacific subductionzones demonstrates the pre-existence of compositional buoyancycontrast at the sites of these subduction zones. These observationsallow us to suggest that lateral compositional buoyancy contrastwithin the oceanic lithosphere creates the favoured and necessarycondition for subduction initiation. Edges of buoyant oceanicplateaux, for example, mark a compositional buoyancy contrastwithin the oceanic lithosphere. These edges under deviatoriccompression (e.g. ridge push) could develop reverse faults withcombined forces in excess of the oceanic lithosphere strength,allowing the dense normal oceanic lithosphere to sink into theasthenosphere beneath the buoyant overriding oceanic plateaux,i.e. the initiation of subduction zones. We term this conceptthe ‘oceanic plateau model’. This model explainsmany other observations and offers testable hypotheses on importantgeodynamic problems on a global scale. These include (1) theorigin of the 43 Ma bend along the Hawaii–Emperor SeamountChain in the Pacific, (2) mechanisms of ophiolite emplacement,(3) continental accretion, etc. Subduction initiation is notunique to oceanic plateaux, but the plateau model well illustratesthe importance of the compositional buoyancy contrast withinthe lithosphere for subduction initiation. Most portions ofpassive continental margins, such as in the Atlantic where largecompositional buoyancy contrast exists, are the loci of futuresubduction zones. KEY WORDS: subduction initiation; compositional buoyancy contrast; oceanic lithosphere; plate tectonics; mantle plumes; hotspots; oceanic plateaux; passive continental margins; continental accretion; mantle peridotites; ophiolites 相似文献
11.
12.
借鉴国内外已有的盆地研究成果,在盆地分析的基础上,从岩石圈板块作用、岩石圈深部作用和岩石圈表生作用3个方面,兼顾系统性、科学性和应用性,确立了盆地新的分类原则,由此深入研究了盆地形成与演化的动力学类型,并进一步阐述了盆地形成与演化的地球动力学机制。研究结果表明:在盆地分类中,首先主要根据盆地形成的地球动力学环境如岩石圈板块作用环境、深部作用环境以及表生作用环境来划分大类;再根据盆地形成与演化的各种地质作用及其动力学过程如构造作用(伸展、挤压或剪切过程)、热力作用及重力作用进行主要类型划分;再根据盆地的基底性质和地壳类型(如陆壳、洋壳或过渡壳)以及盆地的沉积充填史和构造古地理等(如海相盆地、陆相盆地或过渡相盆地)细分亚类。盆地形成与演化的动力学类型主要包括:单一构造或热体制下盆地演化时的原型盆地类型、单一重力体制下盆地演化的原型盆地类型、多种构造-热体制下盆地演化的叠合盆地类型以及多种构造-热体制下盆地演化的残留盆地类型。在单一构造或热体制下,从板块作用或壳幔作用角度原型盆地动力学类型主要划分为:伸展盆地(陆内伸展盆地、陆间伸展盆地、大洋伸展盆地和弧后伸展盆地),挠曲盆地(弧后挠曲盆地、周缘挠曲盆地、陆内挠曲盆地),走滑盆地(走滑伸展盆地、走滑挠曲盆地)以及克拉通盆地(克拉通退缩盆地、克拉通扩展盆地和克拉通迁移盆地);单一重力体制下原型盆地动力学类型有负载盆地和撞击盆地;多种构造-热体制下的叠合盆地动力学类型有叠加盆地和复合盆地;多种构造-热体制下盆地演化的残留盆地动力学类型有伸展隆起下局部沉降引起的残留盆地、推覆褶皱隆起引起的残留盆地、俯冲至局部碰撞引起的残留盆地及周边抬升隆起引起的残留盆地。关于盆地形成与演化的地球动力学机制包括:岩石圈的板块作用机制,岩石圈的深部作用机制以及岩石圈的表生作用机制。岩石圈的板块作用机制包括板块伸展、挤压和剪切作用;岩石圈的深部作用机制包括软流圈与超级地幔柱对岩石圈的作用,尤其是壳幔作用;岩石圈的表生作用机制也很重要,包括盆地的重力作用、大气作用、海洋作用和生物作用。通过本文的研究,可以为研究整个岩石圈演化、壳幔作用、地球动力学过程以及成藏成矿机制奠定重要理论基础;同时,对于沉积盆地矿产资源、能源资源、水资源勘探和开发,以及灾害防治和环境保护也具有重要应用价值。 相似文献
13.
蛇绿岩型金刚石和铬铁矿深部成因 总被引：5，自引：0，他引：5
地球上的原生金刚石主要有3种产出类型,分别来自大陆克拉通下的深部地幔金伯利岩型金刚石、板块边界深俯冲变质岩中超高压变质型金刚石,和陨石坑中的陨石撞击型金刚石。在全球5个造山带的10处蛇绿岩的地幔橄榄岩或铬铁矿中均发现金刚石和其他超高压矿物的基础上,我们提出地球上一种新的天然金刚石产出类型,命名为蛇绿岩型金刚石。认为蛇绿岩型金刚石普遍存在于大洋岩石圈的地幔橄榄岩中,并提出蛇绿岩型金刚石和铬铁矿的深部成因模式。认为早期俯冲的地壳物质到达地幔过渡带(410~660 km深度)后被肢解,加入到周围的强还原流体和熔体中,当熔融物质向上运移到地幔过渡带顶部,铬铁矿和周围的地幔岩石以及流体中的金刚石等深部矿物一并结晶,之后,携带金刚石的铬铁矿和地幔岩石被上涌的地幔柱带至浅部,经历了洋盆的拉张和俯冲阶段,最终在板块边缘就位。 相似文献
14.
湖北郧县王家庄有两期脉体 ,早期为纤维状石英脉 ,总体呈北北东向分布 ,平行脉壁有一中间面使其对称分布 ,显示张性裂隙持续发育过程 ;与之垂直的横向压性裂隙将它“错开”。形貌上酷似板块构造的大洋中脊和转换断层。晚期云母脉叠置在上述两组裂隙之上 ,并使原来裂隙性质发生变化。这些特征与区域应力场分布 ,特别是与两郧断裂的演化息息相关。根据分形理论 ,将王家庄石英云母脉与板块构造进行对比 ,一方面从微观的角度证实了板块构造一些基本观点的合理性。同时从微观信息得到深入研究板块构造的一些新启示 :对板块形成机制不要局限于软流圈对流 ,而应从更深层次研究地幔物质运动规律 ;要将大陆和大洋作为一个整体研究全球应力场分布规律与构造演化历史 ,其中转换断层是联系大陆和大洋的纽带 ;加强RRR型三联点研究 ,它是研究深部 (地幔 )物质运动和上部 (地壳、岩石圈 )构造应力场相互关系的重要窗口 相似文献
15.
Jean H.Bédard 《地学前缘(英文版)》2018,(1)
The lower plate is the dominant agent in modern convergent margins characterized by active subduction,as negatively buoyant oceanic lithosphere sinks into the asthenosphere under its own weight.This is a strong plate-driving force because the slab-pull force is transmitted through the stiff sub-oceanic lithospheric mantle.As geological and geochemical data seem inconsistent with the existence of modernstyle ridges and arcs in the Archaean,a periodically-destabilized stagnant-lid crust system is proposed instead.Stagnant-lid intervals may correspond to periods of layered mantle convection where efficient cooling was restricted to the upper mantle,perturbing Earth's heat generation/loss balance,eventually triggering mantle overturns.Archaean basalts were derived from fertile mantle in overturn upwelling zones(OUZOs),which were larger and longer-lived than post-Archaean plumes.Early cratons/continents probably formed above OUZOs as large volumes of basalt and komatiite were delivered for protracted periods,allowing basal crustal cannibalism,garnetiferous crustal restite delamination,and coupled development of continental crust and sub-continental lithospheric mantle.Periodic mixing and rehomogenization during overturns retarded development of isotopically depleted MORB(mid-ocean ridge basalt)mantle.Only after the start of true subduction did sequestration of subducted slabs at the coremantle boundary lead to the development of the depleted MORB mantle source.During Archaean mantle overturns,pre-existing continents located above OUZOs would be strongly reworked;whereas OUZOdistal continents would drift in response to mantle currents.The leading edge of drifting Archaean continents would be convergent margins characterized by terrane accretion,imbrication,subcretion and anatexis of unsubductable oceanic lithosphere.As Earth cooled and the background oceanic lithosphere became denser and stiffer,there would be an increasing probability that oceanic crustal segments could founder in an organized way,producing a gradual evolution of pre-subduction convergent margins into modern-style active subduction systems around 2.5 Ga.Plate tectonics today is constituted of:(1)a continental drift system that started in the Early Archaean,driven by deep mantle currents pressing against the Archaean-age sub-continental lithospheric mantle keels that underlie Archaean cratons;(2)a subduction-driven system that started near the end of the Archaean. 相似文献
16.
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. 相似文献
17.
《Journal of Asian Earth Sciences》2007,29(1):160-176
Magmatism in the Kirka–Afyon–Isparta (KAI) region, southwestern Turkey, shows a temporal progression from calc-alkaline to ultrapotassic affinity. Magmatic activity is associated with the geodynamic evolution of the ‘Isparta Angle’ and is typical of a collision-affected convergent plate margin, most magmas being enriched in potassium and other large-ion lithophile elements (LILE) and depleted in high-field strength elements (HFSE) such as Ti, Zr, Nb, Ta, and Hf. However, Late Pliocene ultrapotassic lamproites in the south of ‘Isparta Angle’ show HFSE-rich incompatible element distributions, similar to those of ‘non-orogenic’ intraplate leucite basalts (ILB) and oceanic island basalts (OIB). Their association with HFSE-depleted ‘orogenic’ magmas suggests that ultrapotassic character reflects primarily crustal contamination of their mantle sources, rather than magma-wallrock reaction effects. Their relatively high content of Fe and Ti (for equivalent Mg content), and SiO2-undersaturated character suggest that they segregated at relatively high pressures (>ca. 2.0 GPa) from fertile sources. In contrast, the older SiO2-saturated, Afyon (orogenic) magmas which, for equivalent Mg content, show lower contents of Fe and Ti, are better explained as partial melts segregating at ca. 1.0–1.5 GPa from refractory (basalt-depleted) sources, similar to those of basalt-borne xenoliths tapping the lithospheric mantle. The notion of variably fertile contaminated mantle sources is compelling, but needs to be constrained in terms of the dynamic interaction between the lithosphere and asthenosphere and their respective contamination histories. Given the unlikelihood of in situ partial melting of the continental lithosphere mantle, we propose that both orogenic and non-orogenic magmas are generated at different pressures from sources within the convecting asthenosphere, contaminated by both lithospheric mantle and crustal components. This model rests on two testable conjectures: firstly, the interpretation that the continental lithospheric mantle is residual from partial melting at an earlier stage of its history and, secondly, that such material is incorporated into the asthenospheric flow field during and following subduction. The first of these is supported by the ambient compositions of continental basalt-borne xenoliths, while the second is contingent on the prediction that lithospheric mantle may be rheologically transformed during subduction-related hydration prior to its incorporation. The proximity of the Bucak lamproites to the Menderes Massif, a suspected Archean cratonic fragment, highlights the resemblance of these unusual rocks to intra-plate leucite-bearing lamproites elsewhere, whose genesis has been linked to mantle ‘wedge convection’ triggered beneath cratonic and circumcratonic lithosphere domain boundaries. 相似文献
18.
A. M. Petrishchevsky 《Geotectonics》2013,47(6):465-484
Structural forms of emplacement of crustal and mantle rigid sheets in collision zones of lithospheric plates in northeastern Asia are analyzed using formalized gravity models reflecting the rheological properties of geological media. Splitting of the lithosphere of moving plates into crustal and mantle constituents is the main feature of collision zones, which is repeated in the structural units irrespective of their location, rank, and age. Formal signs of crustal sheet thrusting over convergent plate boundaries and subduction of the lithospheric mantle beneath these boundaries have been revealed. The deep boundaries and thickness of lithospheric plates and asthenospheric lenses have been traced. A similarity in the deep structure of collision zones of second-order marginal-sea buffer plates differing in age is displayed at the boundaries with the Eurasian, North American, and Pacific plates of the first order. Collision of oceanic crustal segments with the Mesozoic continental margin in the Sikhote-Alin is characterized, as well as collision of the oceanic lithosphere with the Kamchatka composite island arc. A spatiotemporal series of deep-seated Middle Mesozoic, Late Mesosoic, and Cenozoic collision tectonic units having similar structure is displayed in the transitional zone from the Asian continent to the Pacific plate. 相似文献
19.
《Gondwana Research》2014,25(2):494-508
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. 相似文献
20.
Fluid-mobile trace element constraints on the role of slab melting and implications for Archaean crustal growth models 总被引：11，自引：0，他引：11
Balz S. Kamber Anthony Ewart Kenneth D. Collerson Michael C. Bruce Graeme D. McDonald 《Contributions to Mineralogy and Petrology》2002,144(1):38-56
We use published and new trace element data to identify element ratios which discriminate between arc magmas from the supra-subduction zone mantle wedge and those formed by direct melting of subducted crust (i.e. adakites). The clearest distinction is obtained with those element ratios which are strongly fractionated during refertilisation of the depleted mantle wedge, ultimately reflecting slab dehydration. Hence, adakites have significantly lower Pb/Nd and B/Be but higher Nb/Ta than typical arc magmas and continental crust as a whole. Although Li and Be are also overenriched in continental crust, behaviour of Li/Yb and Be/Nd is more complex and these ratios do not provide unique signatures of slab melting. Archaean tonalite-trondhjemite-granodiorites (TTGs) strongly resemble ordinary mantle wedge-derived arc magmas in terms of fluid-mobile trace element content, implying that they did not form by slab melting but that they originated from mantle which was hydrated and enriched in elements lost from slabs during prograde dehydration. We suggest that Archaean TTGs formed by extensive fractional crystallisation from a mafic precursor. It is widely claimed that the time between the creation and subduction of oceanic lithosphere was significantly shorter in the Archaean (i.e. 20 Ma) than it is today. This difference was seen as an attractive explanation for the presumed preponderance of adakitic magmas during the first half of Earth's history. However, when we consider the effects of a higher potential mantle temperature on the thickness of oceanic crust, it follows that the mean age of oceanic lithosphere has remained virtually constant. Formation of adakites has therefore always depended on local plate geometry and not on potential mantle temperature. 相似文献