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1.
杨文采  刘晓宇  陈召曦  江金生 《地球科学》2022,47(10):3491-3500
通过分辨率达到0.5°×0.5°×10 km的青藏高原地壳与上地幔三维成像,为研究青藏高原在新生代的动力学作用提供了新的认识.软流圈的波速扰动数据证实,特提斯大洋板块在拆沉后只俯冲到410 km的间断面之上,并不是所有的大洋板块都会俯冲到上地幔底部.这种大洋板块在软流圈拆沉后激发的热流体上涌,造成高原中部大规模的火山喷发,是青藏高原隆升的主要动力来源之一.根据上地幔三维地震层析成像结果定量计算了岩石圈-软流圈界面(LAB)的深度,揭示了软流圈地幔物质的上涌或者岩石圈地块下沉的作用布局,表明青藏高原的东部在新生代动力学作用过程中是一个相对独立的岩石圈地幔块体.   相似文献   

2.
Laboratory and numerical experiments and boundary layer analysis of the entrainment of buoyant asthenosphere by subducting oceanic lithosphere implies that slab entrainment is likely to be relatively inefficient at removing a buoyant and lower viscosity asthenosphere layer. Asthenosphere would instead be mostly removed by accretion into and eventual subduction of the overlying oceanic lithosphere. The lower (hot) side of a subducting slab entrains by the formation of a ∼10–30 km‐thick downdragged layer, whose thickness depends upon the subduction rate and the density contrast and viscosity of the asthenosphere, while the upper (cold) side of the slab may entrain as much by thermal ‘freezing’ onto the slab as by mechanical downdragging. This analysis also implies that proper treatment of slab entrainment in future numerical mantle flow experiments will require the resolution of ∼10–30 km‐thick entrainment boundary layers.  相似文献   

3.
Progress in the Study of Deep Profiles of Tibet and the Himalayas (INDEPTH)   总被引:5,自引:0,他引:5  
This paper introduces 8 major discoveries and new understandings with regard to the deep structure and tectonics of the Himalayas and Tibetan Plateau obtained in Project INDEPTH, They are mainly as follows. (1) The upper crust, lower crust and mantle lithosphere beneath the blocks of the plateau form a "sandwich" structure with a relatively rigid-brittle upper crust, a visco-plastic lower crust and a relatively rigid-ductile mantle lithosphere. This structure is completely different from that of monotonous, cold and more rigid oceanic plates. (2) In the process of north-directed collision-compression of the Indian subcontinent, the upper crust was attached to the foreland in the form of a gigantic foreland accretionary wedge. The interior of the accretionary wedge thickened in such tectonic manners as large-scale thrusting, backthrusting and folding, and magmatic masses and partially molten masses participated in the crustal thickening. Between the upper crust and lower crust lies a large detachment (e.g  相似文献   

4.
大陆下地壳拆沉模式初探   总被引:21,自引:7,他引:21  
下地壳拆沉是人们关注的问题,文中指出下地壳拆沉必须满足至少三个条件:(1)地壳加厚使其下部达到熘辉岩相是拆沉的前提.(2)大规模岩浆活动使大量低密度的中酸性物质移出下地壳,使下地壳密度增加直至超过下伏地幔.由于下地壳榴辉岩石部分熔融所形成的岩浆具有埃达克岩的地球化学特征,因此,大规模魂达克岩的熔出是下地壳拆沉的先决和必要条件.(3)岩石圈地幔转化为软流圈地幔,使下地壳能够进入地幔.陆壳下的岩石圈地幔原先是冷的、刚性的和不易流动的,如果有热和水的加入,可以被软化,使其变成热的、塑性的和易流动的软流圈地幔。因此,岩石圈了幔转化为软流圈地幔是下地壳拆沉的必要条件。作者认为,下地壳不大可能整体拆沉,而很可能是一块一块如飘雪花似地拆沉。如果下地壳的密度降低(低于下伏地幔),如果地幔停止热的供给,如果陆壳底部的软流圈地幔幔又恢复为岩石圈地幔,拆沉即终止。文中讨论了中国东部中生代下地壳拆沉的可能性,探讨了岩石圈减薄的机制,认为下地壳不需要也不可能与岩石圈地幔一道拆况。  相似文献   

5.
青藏高原隆升三阶段模型的数值模拟   总被引:13,自引:0,他引:13  
傅容珊 《地学前缘》2000,7(4):588-596
研究表明 ,青藏高原的隆升不仅是印度板块和欧亚板块碰撞的结果 ,它同时受到高原下部地幔物质运移以及地幔和岩石层之间耦合作用的影响。文中以青藏高原隆升三阶段模式(BCCM )为基本模型 ,对在印度板块向北推移、挤压而导致的高原隆升演化的数值模拟结果进行处理。处理中考虑了与抬升过程相应的剥蚀过程 ,同时还考虑在高原演化的后期大约 8~10Ma时发生的下伏岩石层底部的对流搬离 (convectiveremoval)而导致的隆升作用。结果表明 ,模型描述的青藏高原隆升演化过程和观测资料有较好的吻合 ,同时显示高原下部岩石层的对流搬离可能是最近 8~ 10Ma以来高原整体隆升的主导机制。  相似文献   

6.
Mafic alkalic volcanism was widespread in the Carpathian–Pannonian region (CPR) between 11 and 0.2 Ma. It followed the Miocene continental collision of the Alcapa and Tisia blocks with the European plate, as subduction-related calc-alkaline magmatism was waning. Several groups of mafic alkalic rocks from different regions within the CPR have been distinguished on the basis of ages and/or trace-element compositions. Their trace element and Sr–Nd–Pb isotope systematics are consistent with derivation from complex mantle-source regions, which included both depleted asthenosphere and metasomatized lithosphere. The mixing of DMM-HIMU-EMII mantle components within asthenosphere-derived magmas indicates variable contamination of the shallow asthenosphere and/or thermal boundary layer of the lithosphere by a HIMU-like component prior to and following the introduction of subduction components.Various mantle sources have been identified: Lower lithospheric mantle modified by several ancient asthenospheric enrichments (source A); Young asthenospheric plumes with OIB-like trace element signatures that are either isotopically enriched (source B) or variably depleted (source C); Old upper asthenosphere heterogeneously contaminated by DM-HIMU-EMII-EMI components and slightly influenced by Miocene subduction-related enrichment (source D); Old upper asthenosphere heterogeneously contaminated by DM-HIMU-EMII components and significantly influenced by Miocene subduction-related enrichment (source E). Melt generation was initiated either by: (i) finger-like young asthenospheric plumes rising to and heating up the base of the lithosphere (below the Alcapa block), or (ii) decompressional melting of old asthenosphere upwelling to replace any lower lithosphere or heating and melting former subducted slabs (the Tisia block).  相似文献   

7.
Speculations on the nature and cause of mantle heterogeneity   总被引:8,自引:0,他引:8  
Hotspots and hotspot tracks are on, or start on, preexisting lithospheric features such as fracture zones, transform faults, continental sutures, ridges and former plate boundaries. Volcanism is often associated with these features and with regions of lithospheric extension, thinning, and preexisting thin spots. The lithosphere clearly controls the location of volcanism. The nature of the volcanism and the presence of ‘melting anomalies’ or ‘hotspots’, however, reflect the intrinsic chemical and lithologic heterogeneity of the upper mantle. Melting anomalies—shallow regions of ridges, volcanic chains, flood basalts, radial dike swarms—and continental breakup are frequently attributed to the impingement of deep mantle thermal plumes on the base of the lithosphere. The heat required for volcanism in the plume hypothesis is from the core. Alternatively, mantle fertility and melting point, ponding and focusing, and edge effects, i.e., plate tectonic and near-surface phenomena, may control the volumes and rates of magmatism. The heat required is from the mantle, mainly from internal heating and conduction into recycled fragments. The magnitude of magmatism appears to reflect the fertility, not the absolute temperature, of the asthenosphere. I attribute the chemical heterogeneity of the upper mantle to subduction of young plates, aseismic ridges and seamount chains, and to delamination of the lower continental crust. These heterogeneities eventually warm up past the melting point of eclogite and become buoyant low-velocity diapirs that undergo further adiabatic decompression melting as they encounter thin or spreading regions of the lithosphere. The heat required for the melting of cold subducted and delaminated material is extracted from the essentially infinite heat reservoir of the mantle, not the core. Melting in the upper mantle does not requires the instability of a deep thermal boundary layer or high absolute temperatures. Melts from recycled oceanic crust, and seamounts—and possibly even plateaus—pond beneath the lithosphere, particularly beneath basins and suture zones, with locally thin, weak or young lithosphere. The characteristic scale lengths—150 to 600 km—of variations in bathymetry and magma chemistry, and the variable productivity of volcanic chains, may reflect compositional heterogeneity of the asthenosphere, not the scales of mantle convection or the spacing of hot plumes. High-frequency seismic waves, scattering, coda studies and deep reflection profiles are needed to detect the kind of chemical heterogeneity and small-scale layering predicted from the recycling hypothesis.  相似文献   

8.
Free conductive flows in the asthenosphere, layer C, and subduction zone are considered on the basis of experimental and theoretical simulation. The main forces acting on the oceanic lithospheric plate in the subduction zone are described. The horizontally directed forces arising due to free convection in the asthenosphere and transferring the oceanic lithospheric plate toward subduction zone have been estimated. These are friction force Fa and force of gravitational sliding F rd. Thermogravitational force F tg, which is created because the subducting lithospheric plate has a lower average temperature than the ambient mantle, is estimated. The force created owing to phase transitions in the subducted plate has been estimated as well. The tangential stress at the contact of the subducting plate with the continental lithosphere and underlying upper mantle has been determined. The horizontal force arising due to different lateral temperature gradients in the upper mantle on the left and on the right of the subducting plate has been estimated. The results of experimental modeling of the effect exerted upon subduction by counter free convective flows developing in the asthenosphere are considered. The experiments show that the position of the descending free convective flow and thus of the subduction zone depends on the ratio of the thermal power of astehnospheric countercurrents. The pressure arising near the 670 km boundary gives rise to spreading of the subducting plate over this boundary.  相似文献   

9.
We combine geological and geophysical data to develop a generalized model for the lithospheric evolution of the central Andean plateau between 18° and 20° S from Late Cretaceous to present. By integrating geophysical results of upper mantle structure, crustal thickness, and composition with recently published structural, stratigraphic, and thermochronologic data, we emphasize the importance of both the crust and upper mantle in the evolution of the central Andean plateau. Four key steps in the evolution of the Andean plateau are as follows. 1) Initiation of mountain building by 70 Ma suggested by the associated foreland basin depositional history. 2) Eastward jump of a narrow, early fold–thrust belt at 40 Ma through the eastward propagation of a 200–400-km-long basement thrust sheet. 3) Continued shortening within the Eastern Cordillera from 40 to 15 Ma, which thickened the crust and mantle and established the eastern boundary of the modern central Andean plateau. Removal of excess mantle through lithospheric delamination at the Eastern Cordillera–Altiplano boundary during the early Miocene appears necessary to accommodate underthrusting of the Brazilian shield. Replacement of mantle lithosphere by hot asthenosphere may have provided the heat source for a pulse of mafic volcanism in the Eastern Cordillera and Altiplano at 24–23 Ma, and further volcanism recorded by 12–7 Ma crustal ignimbrites. 4) After 20 Ma, deformation waned in the Eastern Cordillera and Interandean zone and began to be transferred into the Subandean zone. Long-term rates of shortening in the fold–thrust belt indicate that the average shortening rate has remained fairly constant (8–10 mm/year) through time with possible slowing (5–7 mm/year) in the last 15–20 myr. We suggest that Cenozoic deformation within the mantle lithosphere has been focused at the Eastern Cordillera–Altiplano boundary where the mantle most likely continues to be removed through piecemeal delamination.  相似文献   

10.
Based on geological and isotope geochemical data obtained during the past decade, the eastern Sikhote Alin volcanic belt can be considered as a polygenic structure with spatially superimposed magmatic complexes of different geodynamic stages. Only Late Cretaceous intermediate and silicic volcanics enriched in LILE and depleted in HFSE can be interpreted as typical subduction complexes. Cenozoic lavas of mainly basic composition were formed after the termination of active subduction under complex dynamic conditions of the rearrangement of eastern Eurasia owing to the collision with the Indian plate. The eruption of Eocene-Oligocene-early Miocene basalts corresponded to the transform continental margin environment, rupture of an ancient subducted slab, and upwelling of hot depleted oceanic asthenosphere of the Pacific MORB-type into the Asian subcontinental lithosphere with EMII-like isotopic characteristics. The late Miocene-Pliocene magmatic activity of the eastern Sikhote Alin showed an intraplate character, but the composition of erupted magmas was strongly affected by previous tectonomagmatic events: subduction of different ages and opening of the Sea of Japan Basin. The distinct EMI isotopic signature of low-potassium plateau basalts, which is not observed in the lavas of earlier stages of volcanic belt evolution, suggests that the continental asthenosphere contributed to magma formation, and the direction of mantle flows changed owing to the formation of a new subduction zone.  相似文献   

11.
大陆溢流玄武岩的地球化学特征及起源   总被引:9,自引:0,他引:9  
快速上涌的大陆溢流玄武岩(CFB),与大陆裂开存在密切的成因关系。CBF总体岩石及地球化学成分均一,富集同位素及不相容元素,但一些样品含有明显的亏损成分,反映出普遍的地幔不均一性,来自上下地幔边界及软流圈的地幔柱提供了CFB所需的主要物质和能量来源,地壳混染作用对CBF的成分影响不大,而受俯冲带脱水流体以及热地幔柱自身与围岩发生的交代作用影响。交代岩石圈地幔对CBF产生重要影响,很好地解释了CFB所具备的微量元素和同位素特征。  相似文献   

12.
THE TECTONICS OF TIBET  相似文献   

13.
大陆岩石圈研究进展   总被引:5,自引:0,他引:5  
陈凌  朱日祥  王涛 《地学前缘》2007,14(2):58-75
从地震学、地球化学、岩石学等不同学科的角度,对大陆岩石圈研究进展做了简要介绍。不同学科的最新研究成果表明,岩石圈在热状态、化学成分和力学行为等方面具有高度非均匀性。这不仅表现为岩石圈性质和结构随深度的变化,而且还反映在不同时代、大陆与海洋以及克拉通和造山带岩石圈结构特征的显著差异上。性质和结构的差异体现了岩石圈形成和长期演化过程的复杂性。我们认为,不同岩石圈块体之间、岩石圈与深部对流地幔之间普遍存在着相互作用。这种相互作用被认为是稳定克拉通岩石圈遭受改造甚至破坏的深部机制,同时还是地球深、浅部物质交换的重要方式,因而显著影响着地球深部的对流和地表的构造过程。值得注意的是,由于岩石圈本身定义的模糊性及其厚度的不确定性,地震活动与岩石圈强度之间的关系以及大陆岩石圈演化的规律性等问题仍有待于进一步的研究和探索。  相似文献   

14.
Imaging the continental upper mantle using electromagnetic methods   总被引:9,自引:0,他引:9  
Alan G. Jones 《Lithos》1999,48(1-4):57-80
The internal structure of the continental lithosphere holds the key to its creation and development, and this internal structure can be determined using appropriate seismic and electromagnetic methods. These two are complementary in that the seismic parameters usually represent bulk properties of the rock, whereas electrical conductivity is primarily a function of the connectivity of a minor constituent of the rock matrix, such as the presence of a conducting mineral phase, e.g. carbon in graphite form, or of a fluid phase, e.g. partial melt or volatiles. In particular, conductivity is especially sensitive to the top of the asthenosphere, generally considered to be a region of interconnected partial melt. Knowledge of the geometry of the lithosphere/asthenosphere boundary is important as this boundary partially controls the geodynamic processes that create, modify, and destroy the lithosphere. Accordingly, collocated seismic and electromagnetic experiments result in superior knowledge than would be obtained from using each on its own. This paper describes the state of knowledge of the continental upper mantle obtained primarily from the natural-source magnetotelluric technique, and outlines how hypotheses and models regarding the development of cratonic lithosphere can be tested using deep-probing electromagnetic surveying. The resolution properties of the method show the difficulties that can be encountered if there is conducting material in the crust. Examples of data and interpretations from various regions around the globe are discussed to demonstrate the correlation of electromagnetic and seismic observations of the lithosphere–asthenosphere boundary. Also, the observations from laboratory measurements on candidate mineralogies representative of the mantle, such as olivine, are presented.  相似文献   

15.
羌塘西北部松西地区新生代火山岩由安山岩、英安岩和晚期火山颈相流纹斑岩3种岩石类型组成,属于钙碱性-高钾钙碱性岩石系列.岩石富集大离子亲石元素和LREE,相对亏损高场强元素,Nb、Ta、Ti负异常,反映源岩具有壳源特征,基性端员的SiO2含量<53%,表明松西地区玄武安山岩不可能完全由陆壳直接局部熔融产生,应该有少量基性的地幔物质加入.岩浆Eu负异常不明显,说明岩浆来源于加厚陆壳中下部,是印度板块与欧亚板块发生长期碰撞挤压导致青藏高原北部包括羌塘地区的陆壳缩短和加厚、拉萨地块大陆岩石圈的北向俯冲作用以及羌塘陆块之下上涌的软流层物质的底侵作用,引发增厚下地壳发生部分熔融形成的.  相似文献   

16.
Is the westerly rotation of the lithosphere an ephemeral accidental recent phenomenon or is it a stable process of Earth's geodynamics? The reason why the tidal drag has been questioned as the mechanism determining the lithospheric shift relative to the underlying mantle is the apparent too high viscosity of the asthenosphere. However, plate boundaries asymmetries are a robust indication of the ‘westerly’ decoupling of the entire Earth's outer lithospheric shell and new studies support lower viscosities in the low-velocity layer (LVZ) atop the asthenosphere. Since the solid Earth tide oscillation is longer in one side relative to the other due to the contemporaneous Moon's revolution, we demonstrate that a non-linear rheological behavior is expected in the lithosphere mantle interplay. This may provide a sort of ratchet favoring lowering of the LVZ viscosity under shear, allowing decoupling in the LVZ and triggering the westerly motion of the lithosphere relative to the mantle.  相似文献   

17.
Elevations on Earth are dominantly controlled by crustal buoyancy, primarily through variations in crustal thickness: continents ride higher than ocean basins because they are underlain by thicker crust. Mountain building, where crust is magmatically or tectonically thickened, is thus key to making continents. However, most of the continents have long passed their mountain building origins, having since subsided back to near sea level. The elevations of the old, stable continents are lower than that expected for their crustal thicknesses, requiring a subcrustal component of negative buoyancy that develops after mountain building. While initial subsidence is driven by crustal erosion, thermal relaxation through growth of a cold thermal boundary layer provides the negative buoyancy that causes continents to subside further. The maximum thickness of this thermal boundary layer is controlled by the thickness of a chemically and rheologically distinct continental mantle root, formed during large-scale mantle melting billions of years ago. The final resting elevation of a stabilized continent is controlled by the thickness of this thermal boundary layer and the temperature of the Earth’s mantle, such that continents ride higher in a cooler mantle and lower in a hot mantle. Constrained by the thermal history of the Earth, continents are predicted to have been mostly below sea level for most of Earth’s history, with areas of land being confined to narrow strips of active mountain building. Large-scale emergence of stable continents occurred late in Earth’s history (Neoproterozoic) over a 100–300 million year transition, irreversibly altering the surface of the Earth in terms of weathering, climate, biogeochemical cycling and the evolution of life. Climate during the transition would be expected to be unstable, swinging back and forth between icehouse and greenhouse states as higher order fluctuations in mantle dynamics would cause the Earth to fluctuate rapidly between water and terrestrial worlds.  相似文献   

18.
Ramon Carbonell   《Tectonophysics》2004,388(1-4):103
A seismic survey with a receiver spacing of 50 m provided one of the most densely sampled wide-angle seismic reflection images of the lithosphere. This unique data set, recorded by an 18-km-long spread, reveals that at wide-angles the shallow subcrustal mantle features high amplitude reflectivity which contrasts with a lack of reflectivity at latter travel times. This change in the seismic signature is located at approximately 120–150 km depth, which correlates with the depth estimates of the lithosphere–asthenosphere boundary (LAB) of previous DSS studies. This seismic signature can be simulated by two-layer mantle model. Both layers with similar average velocities differ in their degree of heterogeneity. The shallow heterogeneous layer and the deeper and more homogeneous one correlate with the lithosphere and the asthenosphere, respectively. Studies involving surface outcrops of ultramafic massifs and mantle xenoliths infer that the upper mantle is a heterogeneous mixture of ultramafic rocks (lherzolites, harzburgites, pyroxenites, peridotites, dunites, and small amounts of eclogites). Laboratory measurements of physical properties of these mantle rocks indicate that compositional variations alone can account for the wide-angle reflectivity. A temperature increase would homogenize the mixture, decreasing the seismic reflection properties due to melting processes. It is proposed that this would take place below 120–150 km (1200 °C, the LAB).  相似文献   

19.
大陆地震构造系统: 以青藏高原及邻区为例   总被引:1,自引:0,他引:1       下载免费PDF全文
李德威  陈继乐  陈桂凡  梁桑 《地球科学》2014,39(12):1763-1775
青藏高原及邻区三角形发震构造域是全球大陆最显著的地震多发区.脆性活动断层及其弹性回跳模式无法合理解释该区深度集中分布在10~40 km的点状震源.针对发震构造和地震机理不明确这一重大科学问题, 以大陆动力学和地球系统动力学新思想为指导, 对青藏高原及邻区发震构造系统进行域、层、带、点相关研究, 阐明大陆地震构造系统的结构型式, 认为下地壳固态流变及其韧性剪切带是提供地震能量的孕震构造, 中地壳韧-脆性剪切带是累积地震能量的发震构造, 上地壳脆性断裂是释放地震能量的释震构造.在研究青藏高原及邻区地震构造系统及其形成背景的基础上, 进一步论证了大陆地震热流体撞击的形成机理: 地幔墙导致大洋中脊之下的软流圈热流物质层流到大陆特定部位汇聚加厚并底辟上升, 造成大陆下地壳部分熔融和固态流变, 并改变莫霍面的产状, 固态流变物质侧向非均匀流动, 形成大陆盆山体系, 流动的韧性下地壳与脆性上地壳之间具有韧-脆性剪切滑脱性质的中地壳不断积累由下地壳热能转换而来的应变能, 形成发震层, 震源定位于下地壳热流物质富集带("热河")中的固态-半固态流变物质撞击到强弱层块之间的构造边界, 不同热构造环境和撞击角度产生5种不同类型的地震.从而为大陆地震的科学预测奠定了全新的理论基础.   相似文献   

20.
Shaohua Zhou 《地学学报》1996,8(6):514-524
An analytical solution has been derived for the steady-state geotherm of the continental lithosphere, using an empirical thermal conductivity model that incorporates the experimentally observed temperature and pressure effect. Based on recent global compilations of crustal thickness and heat flow data, a standard continental lithosphere is re-defined by a global mean model with total crustal thickness of 40 km and surface heat flow of 55 mWm-2 (within which 28 mWm-2 is assumed to be derived from deep mantle source). The thickness of the continental lithosphere (≅125 km), consistent with previous models, is given by the depth at which the geotherm intersects the potential asthenosphere temperature of 1280°C. It is shown that the new steady-state geotherm is much hotter than that based on the previously adopted model where material thermal conductivity is assumed to be constant (≅3.14 W/m/k) throughout the lithosphere. The consequence of this re-evaluation of pre-extension thermal structure in the lithosphere is that the minimum stretching factor required to cause the onset of dry mantle partial melting can be 15–20% lower than the previous estimate. Also, if minor amounts of water or other volatile element or dry basalt are present in the upper mantle, melting of the subcontirfental mantle is very likely to occur for any geotherms constructed using surface heat flows > 30 mWm-2.  相似文献   

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