南海打开模式:右行走滑拉分与古南海俯冲拖曳

南海作为东亚大陆边缘最大的边缘海,位于太平洋、印澳和欧亚三个板块的夹持之下,处于特提斯构造域和太平洋构造域的联合作用部位,是揭示新生代两大动力学体系交接转换特征的良好场所。南海海盆为菱形洋盆,包括西北次海盆、东部次海盆和西南次海盆,均在古近纪—中中新世形成,同时伴随着南海北部、西部和南部盆地群发育,盆地边缘油气资源丰富,被称为第二个"波斯湾"。本文搜集了前人对南海洋盆深部形态、磁条带、转换断层等成果,以及南海周边盆地群的沉积体系、沉积相、不整合面相关资料,综合对比了南海北部、西部和南部盆地群的沉积序列、沉积相、沉积厚度,厘定了盆地群断裂体系、断裂组合特征,揭示了南海北部、南部盆地群及西部盆地群中的中建南和万安盆地都是在右行右阶走滑拉分背景下形成的。北部盆地群新生代古近系西厚东薄,新近系东厚西薄,NNE—NE向断裂体系活动早期西强东弱,而晚期东强西弱,从西向东依次停止。同时指出,南海是在NNE向断裂体系右行右阶走滑拉分和古南海俯冲拖曳的联合作用下打开:于34~32 Ma西北次海盆和东部次海盆受控于NNE向断裂的右行右阶走滑拉分作用,沿着NNE-SSW方向开启;32~23 Ma,NNE向走滑断裂活动自西向东逐步停止;于23 Ma左右,"消失"的南海以西的NNE向走滑断裂完全停止活动,同时由于婆罗洲地块逆时针旋转,古南海的俯冲带走向由近E-W向变为NE向,俯冲板块拖曳力也转变为NW-SE向并且占据主导地位,在拖曳力作用下礼乐—巴拉望地块后缘陆壳伸展,导致西南次海盆打开,东部次海盆的扩张方向由NNE-SSW转变为NW-SE向。于15Ma,礼乐—巴拉望地块与婆罗洲地块碰撞,南海停止扩张。     

Thrust front segmentation induced by differential slab retreat in the Apennines (Italy)

New seismic reflection data reveal that the south‐eastward prolongation of the Apennine thrust front in the central Adriatic Sea is most likely located in a more external position with respect to the traditional interpretation. In this new interpretation, the Apennine thrust front shows a segmented geometry in correspondence to the Tremiti lithospheric transfer zone. The available data suggest that the north‐eastward flexural retreat of the subducting Adriatic lithosphere and the related frontal accretion of the Apennine accretionary prism have acted during the last 5 Ma and may be considered still lively in both the Po plain and in the Central Adriatic domain, north of the Tremiti lineament. By analysing the tectonic evolution of the Apulo‐Adriatic areas, it may be argued that the differential slab retreat between the central and southern sectors of the subducting Adriatic plate has been able to induce the segmentation of the Apennine thrust front.     

Trace element and isotopic variations from Mt. Vulture to Campanian volcanoes: constraints for slab detachment and mantle inflow beneath southern Italy

New Sr–Nd–Pb isotopic ratios and trace element data for volcanic mafic rocks outcropping along a E–W transect in southern Italy, from Mt. Vulture to Neapolitan volcanoes, are reported. The variation of LILE/HFSE, HFSE/HFSE and radiogenic isotopes along this transect indicates that all of these volcanoes contain both intra-plate and subduction-related signatures, with the former decreasing from Mt. Vulture to Campanian volcanoes. New data are also reported for the Paleocene alkaline rocks from Pietre Nere (Apulia foreland), which show isotopic ratios mostly overlapping the values for Mediterranean intra-plate volcanoes as well as the Eocene–Oligocene alkaline mafic lavas from the northern Adria plate. Pietre Nere provides evidence for an OIB mantle composition of FOZO-type, free of subduction influences, that is present beneath the Adria plate (Africa) before its collision with Europe. After this collision, and formation of the southern Apennines, westward inflow of mantle from the Adria plate to the Campanian area occurred, as a consequence of slab break off. Interaction of subduction components with inflowing Adria mantle generated hybrid sources beneath the Vulture–Campania area, which can explain the compositional features of both Mt. Vulture and the Campanian mafic rocks. Therefore, mafic magmas from these volcanoes represent variable degrees of mixing between different mantle components.     

Rainfall-induced shallow landslides: a model for the triggering mechanism of some case studies in Northern Italy

The article relates the main findings of a recent investigation aimed at modeling the triggering of shallow landslides. A simplified model for assessing the safety factor of potentially unstable slopes, directly related with rainfall trends, was developed. Based on the geometric characteristics of the slope, the geotechnical properties, and strength parameters of the soil, the model makes it possible to define a safety factor of a slope as a function of time. The model is based on the limit equilibrium method and takes into account the seepage of underground water. The safety factor is, in turn, related to the seasonal rainfall. The model was applied on a local scale to some historical cases which had occurred recently in Northern Italy. The paper shows how the results of the application of the model on a local scale achieve a good agreement between the instability condition and the real date of each considered event.     

Thinning of the Thickened Lithosphere and Its Geodynamic Consequence: Application for Tibetan Plateau

THINNING OF THE THICKENED LITHOSPHERE AND ITS GEODYNAMIC CONSEQUENCE: APPLICATION FOR TIBETAN PLATEAU1　ParsonsB ,McKenzieD .Mantleconvectionandthethermalstructureoftheplates[J] .JGeophysRes,1978,83;4 4 85～4 4 96 . 2　HousemanGA ,McKenzieDP ,MolnarP .Convectiveinstabilityofathickenedboundarylayeranditsrelevanceforthethermalevolutionofcontinentalconvergentbelts[J] .JGeophysRes 1981,86 :6 115～ 6 132 . 3　OwensTJ,ZandtG ,Theimplicationsofc…     

Potential evidence for slab detachment from the flexural backstripping of a foredeep: Insight on the evolution of the Pescara basin (Italy)

The discrepancy between the size of the Apenninic chain and the depth of the Adriatic foredeep is investigated using 2D flexural backstripping on well‐constrained depth‐converted cross‐sections in the Pescara basin (Central Italy). The procedure consisted of removal, uplift, unfolding and unfaulting of the Pliocene–Pleistocene foreland deposits to produce a palaeogeographic map of the basin at the end of the Messinian and to constrain sedimentary rates since the Miocene. Results are found to support the contribution of an external load to the foreland evolution together with the Apenninic chain load. The interplay of the two types of loads resulted in spatial and temporal variations of the foredeep evolution that are quantified by palaeogeographic maps and sedimentation rates obtained through backstripping. Results are interpreted as representing the effects of a southward‐migrating wave linked to slab detachment beneath the Adriatic foredeep. This procedure can be useful to investigate similar problems on other chains worldwide.     

华北中—新生代大陆岩石圈转型的研究现状与方向 ——兼评“岩石圈减薄”和“克拉通破坏”

对我国大陆岩石圈的持续热点研究领域——华北中-新生代大陆岩石圈巨厚减薄研究中所涉及的问题再次进行了评述,特别是将对问题认识过程与克拉通陆内造山研究相联系。综述了岩石地球化学、地球物理、构造地质等不同学科对中生代华北大陆岩石圈演化特征研究的最新进展,以及对大陆岩石圈诸多学科不同定义内涵及由此产生的讨论。在分述了国际大陆岩石圈研究背景,岩石圈转型的空间特征及时间特征,新技术方法的应用,地表构造体系转折的再认识,以及几种可能的转型机制基础上,再次建议以大陆岩石圈全面转型,即一系列大陆岩石圈地质、物理及化学参量的系统变化,来描述这一大尺度东亚地球动力学过程,并提出目前以“克拉通破坏”作为大陆岩石圈改造研究的提法应予修正。呼吁大力鼓励及进行多学科交叉综合研究,重视各学科新技术新方法的引进及应用。在相关研究中高度重视地球深部圈层相互作用,将中生代全球深部地幔事件对中国东部岩石圈地幔全面转型的影响作为今后研究重点。     

Lithosphere development in the Slave craton: a linked crustal and mantle perspective

The late tectonic evolution of the Slave craton involves extensive magmatism, deformation, and high temperature-low pressure (HT-LP) metamorphism. We argue that the nature of these tectonic events is difficult to reconcile with early, pre-2.7 Ga development and preservation of a thick tectosphere, and suggest that crust–mantle coupling and stabilization occurred only late in the orogenic development of the craton. The extent and repetitiveness of the tectonic reworking documented within the Mesoarchean basement complex of the western Slave, together with the development of large-volume, extensional mafic magmatism at 2.7 Ga within the basement complex argue against preservation of a widespread, thick, cool Mesoarchean tectosphere beneath the western Slave craton prior to Neoarchean tectonism. Broad-scale geological and geophysical features of the Slave craton, including orientation of an early F1 fold belt, distribution of ca. 2.63–2.62 Ga plutonic rocks, and the distribution of geochemical, petrological and geophysical domains within the mantle lithosphere collectively highlight the importance of an NE–SW structural grain to the craton. These trends are oblique to the earlier, ca. 2.7 Ga north–south trending boundary between Mesoarchean and Neoarchean crustal domains, and are interpreted to represent a younger structural feature imposed during northwest or southeast-vergent tectonism at ca. 2.64–2.61 Ga. Extensive plutonism, in part mantle-derived, crustal melting and associated HT-LP metamorphism argue for widespread mantle heat input to the crust, a feature most consistent with thin (<100 km) lithosphere at that time. We propose that the mantle lithosphere developed by tectonic imbrication of one or more slabs subducted beneath the craton at the time of development of the D1 structural grain, producing the early 2.63–2.62 Ga arc-like plutonic rocks. Subsequent collision (external to the present craton boundaries) possibly accompanied by partial delamination of some of the underthrust lithosphere, produced widespread deformation (D2) and granite plutonism throughout the province at 2.6–2.58 Ga. An implication of this model is that diamond formation in the Slave should be Neoarchean in age.     

地球深部探测国际发展与我国现状综述

探测人类居住的地球内部的结构和组成是地质学家和地球物理学家共同的奋斗目标。本文介绍了上世纪70年代以来世界主要国家的国际地球探测计划的主要内容,包括美国大陆反射地震探测计划(COCORP)、地球透镜计划(EarthScope),欧洲地球探测计划(EUROPROBE)、德国大陆反射地震计划(DEKORP)、英国反射地震计划(BIRPS)、意大利地壳探测计划(CROP)、瑞士地壳探测计划(NRP20),俄罗斯深部探测计划,加拿大岩石圈探测计划(LITHOPROBE),澳大利亚四维地球动力学计划(AGCRC)、澳大利亚玻璃地球计划(Glass-Earth)和澳大利亚地球探测计划(AuScope),简要概括了国际地球探测计划的成果,回顾了我国地球深部探测的历史与工作基础,简要论述了我国开展地壳探测计划的必要性,并介绍了近期启动的国家科学专项"深部探测技术与实验研究"的目标与"两网、两区、四带、多点"的工作部署,展望了我国地球深部探测发展的未来。     

“三江”古特提斯地幔热柱——洋中脊玄武岩证据

“三江”特提斯巨型造山带由４条板块缝合带和夹于其间的微陆块和弧地体构成。在古特提斯洋闭合而成的澜沧江和金沙江缝合带内，均发育典型的蛇绿岩－蛇绿混杂岩和洋岛玄武岩（ＯＩＢ）组合。ＯＩＢ集中产出于大洋的特定区段（２２０－２４０Ｎ──澜沧江洋；２４０－２７０Ｎ──金沙江洋），形成于洋壳（ＭＯＲＢ）顶部，并被浅水碳酸盐岩覆盖，ＯＩＢ主要岩石类型为苦橄玄武岩、夏威夷岩和钾质粗面玄武岩，三者具特定的空间配置与时间演变规律。根据三江地区ＯＩＢ时空展布规律、岩石组合特点、岩石地球化学特征、源岩化学估算及热幔柱实验成果，提出早古生代时期的澜沧江洋和金沙江洋岩石围下方分别出现地幔热拉，其直径约２００－２５０ｋｍ，具特定的不同于周围地幔的热－化学结构。地幔热柱的尾柱区高热物质熔融，产生苦橄质或苦橄玄武质熔浆，地幔热拉上涌，其冠形头部与周围地幔“混杂”而具化学分带，该区物质熔融，产生富Ｎａ和富Ｋ质ＯＩＢ。     

Mantle Xenoliths from the Southeastern Slave Craton: Evidence for Chemical Zonation in a Thick, Cold Lithosphere

We present the first data on the petrology of the mantle lithosphereof the Southeastern (SE) Slave craton, Canada. These are basedon petrographic, mineralogical and geochemical studies of mantlexenoliths in Pipe 5034 of the Cambrian Gahcho Kué kimberlitecluster. Major types of mantle xenoliths include altered eclogite,coarse garnet or spinel peridotite, and deformed garnet peridotite.The peridotites belong to the low-temperature suite and formedat T=600–1300°C and P= 25–80 kbar in a thick(at least 220–250 km), cool lithosphere. The SE Slavemantle is cooler than the mantle of other Archaean cratons andthat below other terranes of the Slave craton. The thick lithosphereand the relatively cool thermal regime provide favourable conditionsfor formation and preservation of diamonds beneath the SE Slaveterrane. Similar to average Archaean mantle worldwide, the SESlave peridotite is depleted in magmaphile major elements andcontains olivine with forsterite content of 91–93·5.With respect to olivine composition and mode, all terranes ofthe Slave mantle show broadly similar compositions and are relativelyorthopyroxene-poor compared with those of the Kaapvaal and Siberiancratons. The SE Slave spinel peridotite is poorer in Al, Caand Fe, and richer in Mg than deeper garnet peridotite. Thegreater chemical depletion of the shallow upper mantle is typicalof all terranes of the Slave craton and may be common for thesubcontinental lithospheric peridotitic mantle in general. Peridotiticxenoliths of the SE Slave craton were impregnated by kimberliticfluids that caused late-stage recrystallization of primary clinopyroxene,spinel, olivine and spinel-facies orthopyroxene, and formationof interstitial clinopyroxene. This kimberlite-related recrystallizationdepleted primary pyroxenes and spinel in Al. The kimberliticfluid was oxidizing, Ti-, Fe- and K-rich, and Na-poor, and introducedserpentine, chlorite, phlogopite and spinel into peridotitesat P < 35 kbar. KEY WORDS: kimberlite xenolith; lithosphere; mantle terrane; chemical zoning; thermobarometry; Slave craton     

辐流式二沉池中异重流的计算流体力学模型研究

异重流的形成是影响活性污泥系统二沉池水力学性能的主要因素,形成异重流的主要原因包括沉淀池内不均匀的污泥分布和温度分布。采用多相流欧拉模型、标准k-ε湍流模型和Boussinesq假设研究了二沉池中活性污泥和表面散热引起的异重流。表面散热的计算采用经验方程,数值计算结果同实验结果作了比较,结果表明模型能较好地预测辐流式二沉池的流场、温度场和污泥分布。研究还表明,Fr_p2Gr/Re2表示了不均匀温度分布引起的浮升力与不均匀污泥分布引起的作用力的比值,用它可以判断两种作用力在异重流的形成当中的相对大小。     

华北中部岩石圈电性结构——应县—商河剖面大地电磁测深研究

20 0 1年, 沿着山西应县到山东商河, 重新布置大地电磁测深剖面进行研究.采用现代先进的大地电磁数据处理技术和快速松弛二维反演方法获得该剖面二维电性结构模型, 从而充分展示了华北地区岩石圈电性结构的特点.从电性特征上讲, 华北岩石圈以太行山前断裂为界划分为东、西两区, 东区为低阻区, 西区为高阻区.在东区, 上地壳电性结构基本与华北裂谷系的隆、坳构造格局相对应, 岩石圈的电导最高达3× 104 S, 远远大于强烈活动的安第斯山岩浆弧区和西藏高原岩石圈的电导.这里, 在构造连接部位的地壳中有不连续的高导体存在, 电导率大约0.1~ 0.8S/m.在西区, 太行山和恒山的岩石圈为高阻块体, 表现出稳定大陆区岩石圈导电性结构的特点.但恒山高阻块体之下发现一组向西缓倾的高导层, 其电导率为0.0 4~0.2 5S/m, 顶面在2 0km深处, 底面深度大约40km.      

Multi-layer Tectonic Model for Intraplate Deformation and Plastic-Flow Network in the Asian Continental Lithosphere

In a large area of the east—central Asian continent there is a unified seismic network system composed of two families of large—seismic belts that intersect conjugately. Such a seismic network in the middle—upper crust is actually a response to the plastic flow network in the lower lithosphere including the lower crust and lithospheric mantle. The existence of the unified plastic flow system confirms that the driving force for intraplate tectonic deformation results mainly from the compression of the India plate, while the long-range transmission of the force is carried out chiefly by means of plastic flow. The plastic flow network has a control over the intraplate tectonic deformation.     

Origin of paired high pressure–ultrahigh-temperature orogens: a ridge subduction and slab window model

Ultrahigh-temperature (UHT) and high pressure (HP) metamorphic rocks generated at different times in Earth history form paired suites within the same tectonic belts in several regions. We evaluate the thermal regimes and fluid circulation patters in different plate tectonic settings and propose a new model involving ridge subduction where the slab window places hot asthenosphere against the base of the overlying plate and provides an ideal setting for the supply of heat and CO₂-rich fluids at relatively shallow domains, which can explain the formation and preservation of UHT metamorphic rocks in the roots of the arc and forearc. The plate geometry below the slab window would inhibit the normal cooling induced by the slab, and a temporary deprivation of slab-derived sediments and hydrous fluids. Our analysis provides a unified model for paired UHT and HP metamorphic orogens and presents a key to the associated thermal and fluid regimes.     

Post-Collisional Transition from Subduction- to Intraplate-type Magmatism in the Westernmost Mediterranean: Evidence for Continental-Edge Delamination of Subcontinental Lithosphere

Post-collisional magmatism in the southern Iberian and northwesternAfrican continental margins contains important clues for theunderstanding of a possible causal connection between movementsin the Earth's upper mantle, the uplift of continental lithosphereand the origin of circum-Mediterranean igneous activity. Systematicgeochemical and geochronological studies (major and trace element,Sr–Nd–Pb-isotope analysis and laser ⁴⁰Ar/³⁹Ar-agedating) on igneous rocks provide constraints for understandingthe post-collisional history of the southern Iberian and northwesternAfrican continental margins. Two groups of magmatic rocks canbe distinguished: (1) an Upper Miocene to Lower Pliocene (8·2–4·8Ma), Si–K-rich group including high-K (calc-alkaline)and shoshonitic series rocks; (2) an Upper Miocene to Pleistocene(6·3–0·65 Ma), Si-poor, Na-rich group includingbasanites and alkali basalts to hawaiites and tephrites. Maficsamples from the Si–K-rich group generally show geochemicalaffinities with volcanic rocks from active subduction zones(e.g. Izu–Bonin and Aeolian island arcs), whereas maficsamples from the Si-poor, Na-rich group are geochemically similarto lavas found in intraplate volcanic settings derived fromsub-lithospheric mantle sources (e.g. Canary Islands). The transitionfrom Si-rich (subduction-related) to Si-poor (intraplate-type)magmatism between 6·3 Ma (first alkali basalt) and 4·8Ma (latest shoshonite) can be observed both on a regional scaleand in individual volcanic systems. Si–K-rich and Si-poorigneous rocks from the continental margins of southern Iberiaand northwestern Africa are, respectively, proposed to havebeen derived from metasomatized subcontinental lithosphere andsub-lithospheric mantle that was contaminated with plume material.A three-dimensional geodynamic model for the westernmost Mediterraneanis presented in which subduction of oceanic lithosphere is inferredto have caused continental-edge delamination of subcontinentallithosphere associated with upwelling of plume-contaminatedsub-lithospheric mantle and lithospheric uplift. This processmay operate worldwide in areas where subduction-related andintraplate-type magmatism are spatially and temporally associated. KEY WORDS: post-collisional magmatism; Mediterranean-style back-arc basins; subduction; delamination; uplift of marine gateways     

A critical state model for sands dependent on stress and density

An elastoplastic model for sands is presented in this paper, which can describe stress–strain behaviour dependent on mean effective stress level and void ratio. The main features of the proposed model are: (a) a new state parameter, which is dependent on the initial void ratio and initial mean stress, is proposed and applied to the yield function in order to predict the plastic deformation for very loose sands; and (b) another new state parameter, which is used to determine the peak strength and describe the critical state behaviour of sands during shearing, is proposed in order to predict simply negative/positive dilatancy and the hardening/softening behaviour of medium or dense sands. In addition, the proposed model can also predict the stress–strain behaviour of sands under three-dimensional stress conditions by using a transformed stress tensor instead of ordinary stress tensor. Copyright © 2004 John Wiley & Sons, Ltd.     

西藏南部印度-亚洲碰撞带岩石圈:岩石学-地球化学约束

拟以岩石学和地球化学的研究为基础, 结合地球物理与构造地质学的研究成果, 从一个侧面探讨青藏高原岩石圈、特别是印度-亚洲主碰撞带岩石圈结构、组成及今后进一步的研究方向.印度-亚洲主碰撞带具有青藏高原最厚的地壳, 由初生地壳及再循环地壳两类不同性质的地壳构成; 青藏巨厚地壳是由于构造增厚及地幔物质注入(通过岩浆作用) 增厚两种机制形成的.碰撞以来藏南地壳加厚主要发生在约50~25Ma期间.青藏岩石圈地幔在地球化学和岩石学上是不均一的, 至少存在3种地球化学端元: (1) 新特提斯大洋岩石圈端元; (2) 印度陆下岩石圈端元; (3) 新特提斯闭合前青藏原有的岩石圈端元.在青藏高原还发现了一批壳幔深源岩石包体及高压-超高压矿物, 对于认识青藏深部有重要的意义.可以识别出青藏高原现今存在3种岩石圈结构类型: 第1种, 增厚的岩石圈(帕米尔型); 第2种, 减薄的岩石圈(冈底斯型); 第3种, 加厚-减薄-再加厚的岩石圈(羌塘型).这3类岩石圈是否在时间上具有先后顺序, 尚无明确的证据, 需要在今后加以注意.研究表明, 沿冈底斯带后碰撞钾质-超钾质火山活动, 可能与新特提斯洋俯冲板片在后碰撞阶段的断离及印度大陆岩石圈向青藏的持续俯冲作用有关, 但西段、中段与东段的动力学机制不相同.在青藏高原北部地区(羌塘、可可西里等地区), 后碰撞钾质-超钾质火山活动, 可能与波状外向扩展式的软流圈上隆引起的减压熔融有关.在高原北缘西昆仑、玉门等地区, 其形成机制可能为大规模走滑断层引起的减压熔融.青藏高原后碰撞火成活动具有明显而有规律的时空迁移.同碰撞的林子宗火山活动在65Ma左右始于冈底斯南部, 标志印度-亚洲大陆碰撞的开始.于45Ma左右火山活动向北迁移到羌塘-“三江”北段, 开始了后碰撞火山活动; 然后自内向外迁移, 即北向可可西里、南向冈底斯(在冈底斯内部又自西向东)、东向西秦岭迁移; 最后(6Ma以来), 再分别向高原的西北、东北、东南三隅迁移.结合已有地球物理资料, 一种可能的解释是它可能暗示由印度和亚洲大陆板块碰撞所诱发的深部物质(如中-下地壳、软流圈地幔物质) 流动.