西南“三江”造山带大地构造相

西南“三江”造山带由多条缝合带及其间多个大小不等的中间陆块构成,其大地构造属性与划分方案历来受地学界关注与争论。本文以大地构造相理论为切入点,将西南“三江”造山带划分出11个一级及其若干二级大地构造相,包括俯冲、消减杂岩、仰冲等一级大地构造相以及与其相伴的后造山及走滑大地构造相。俯冲大地构造相类包括块体变质相、前陆褶冲相、前陆盆地相;消减杂岩大地构造相包括洋壳残片相、陆壳残片相、增生变质杂岩相、活化基底相、侵入岩相、上叠磨拉石相;仰冲板块大地构造相包括弧前盆地相、岛弧相、弧后及弧间盆地相。特提斯洋向北消减,使泛华夏大陆群各块体先拼接,其后弧后扩张、闭合、造山,从而形成了“三江”造山带“多缝合带”、“多陆体”特征。     

燕山板内造山带中生代构造演化特征

燕山地区自晚三叠世以来进入了板内造山带形成演化阶段，并具有分期演化的幕式特征。在时间演化序列上，可分出造山前期（T3）、造山主期（J1－J3）和造山后期（K1）等3个阶段。构造变形方面，燕山板内造山带的基本构造格局为一大型逆冲推覆系统组成的构造楔形体，呈前展式扩展，造成的地壳缩短量可达44.1%。动力变质作用以高压动力变质为特征，发育高压动力变质岩（榴辉岩和高压麻粒岩），形成于构造应力集中的逆掩断层上盘，由中－上地壳长英质岩石转变而成。岩浆岩属钙碱性岩石系列、中酸性岩石组合，其中岩石类型、稀土元素配分型式及所反映的构造运动强度均具有一定的特征。在造山带形成过程中伴生3期同造山磨拉石：杏石口期磨拉石（T3x)、后城期磨拉石（J3h)和青石砬期磨拉石（K1q)，它们反映了造山带的幕式演化特点和不同造山时期构造运动强度的不均一性。     

中央造山带东段岩石圈的构造格架

笔者讨论了大别—苏鲁超高压变质带地球物理调查剖面及相关地球物理成果。分析大别—苏鲁地体的深部地质构造与岩石圈主要特征,并与东秦岭地区前人的探测结果进行对比。结果认为,中央造山带东段的地壳构造反映了扬子克拉通向北的陆内深俯冲作用。陆壳俯冲的角度在20°～30°之间,由于角度较缓,中央造山带东段发育了开阔的后陆盆地,其下方基底构造仍保留有造山带板块会聚的特征。造山带核部上中地壳存在着规模很大的岩浆岩体的显示,与造山期后的地质作用有关。大别—苏鲁的早中生代超高压变质带在东秦岭可能仍埋藏在地壳深处,不会出露于地表。     

大巴山陆内造山带构造流体及其形成条件研究

构造脉体作为构造流体的宏观标志记录了与构造运动有关的流体来源、形成环境条件和动力学等信息。大巴山构造带是一个典型的陆内造山带,发育了代表构造前、同构造期和构造后3期构造流体的方解石脉(V1、V2和V3)。本文在对构造后伸展背景下形成的方解石脉(V3)野外产状、几何特征和围岩力学性质统计分析基础上,通过其形成古应力场恢复和同位素地球化学分析,研究V3脉体形成环境条件及其流体来源。结果表明,V3脉体走向以NE SW向为主,脉体倾角较陡,大多近于直立,其形成的主应力轴σ1,σ2和σ3方位分别为67°∠76°、200°∠13°和293°∠10°,形成时的应力场为NW SE向拉张。V3脉体形成时流体压力pf<σ2<σ1,流体超压Δsi在92～167 MPa,形成最大深度为1.8～7.2 km。δ13C δ18O反映V3方解石脉形成与围岩碳酸盐岩脱CO2作用有关,V3方解石脉流体包裹体水的δD δ18O同位素分析表明其为盆地内部变质建造水向浅部迁移并有浅部表生水的参与。结合大巴山前陆构造广泛存在的异常高压流体,认为大巴山前陆在晚白垩世-古近纪时期处于伸展构造背景下,原来封存在深部的异常高压流体超压Δsi突破围岩形成裂缝,并上升到浅部与表生流体混合沉淀形成了V3脉体。     

Tectonic burial and exhumation in a foreland fold and thrust belt: the Monte Alpi case history (Southern Apennines,Italy)

The Monte Alpi area of the Southern Apennines represents the only sector of the thrust belt where the reservoir rocks (i.e. Apulian Platform carbonates) for major hydrocarbon accumulations in southern Italy are interpreted to crop out. Tectonic evolution and exhumation of this area were analysed by integrating stratigraphic and structural data with different organic and inorganic parameters which record the burial and thermal evolution of the sediments (vitrinite reflectance, fluid inclusions, and I/S mixed layers in clayey sediments). Our analyses suggest that the presently exposed Monte Alpi structure suffered a loading of ca. 4000 m, owing to the emplacement of allochthonous units in Early Pliocene times. Available geological data indicate that erosion of the tectonic load occurred since the Late Pliocene, when the area first emerged. This implies an average exhumation rate in excess of 1 mm/year. A model can be constructed which matches the maturity indices and also takes into account intermediate stages of the evolution, resulting from combined structural and fluid inclusion data. By this model, a first stage of exhumation would have taken place at an average rate of about 0.36 mm/year. This was controlled by uplift and erosion associated with both: (i) thrusting at depth within the Apulian carbonates (Late Pliocene), and (ii) strike-slip faulting (Early Pleistocene). A second exhumation stage would have occurred in the last 700 ky at a much faster rate (ca. 4 mm/year) as a result of extensional tectonics.     

Tectonic implications from Re-Os dating of Mesozoic molybdenum deposits in the East Qinling-Dabie orogenic belt

The East Qinling-Dabie molybdenum belt is part of a larger East-West trending metallogenic belt in eastern China. Most of the molybdenum deposits occur as porphyry or porphyry-skarn type, but there are also some vein type deposits. Following systematic Re-Os dating of molybdenite from 13 deposits and comparisons with two previously dated deposits, we have recognized that the molybdenum mineralization in the East Qinling-Dabie belt was developed during hydrothermal activity linked to magmatism and the emplacement of granitoid stocks. Three pulses of granitoid magmatism and Mo mineralization are recognized corresponding to significant tectonic events in the East Qinling-Dabie belt. Vein type deposits dated at 233-221 Ma were formed in detachment fractures, indicating localized extension within the collisional setting of the North China and Yangtze Cratons. I-type and transitional I- and S-type granites and related mineralization dated at 148-138 Ma may have formed part of a continental magmatic arc, with widespread magmatism and back-arc extension caused by subduction of the Izanagi or Paleopacific plate beneath the Eurasian continent in a WNW-ESE direction in the Late Jurassic-Early Cretaceous. Both S-type and transitional S- and I-type granite-associated porphyry molybdenum deposits dated at 131-112 Ma are part of an extensive mineralization event throughout East China that can be ascribed to regional large-scale lithospheric thinning, delamination and thermal erosion.     

论东天山觉罗塔格造山带的大地构造属性

觉罗塔格造山带位于吐哈盆地和中天山地块之间，长期以来，关于该造山带的大地构造属性争论较多，有晚古生代岛弧带、弧后盆地、裂陷槽、古生代陆缘增生带、石炭纪火山岩型被动陆缘等不同认识。基于晚古生代早期觉罗塔格地区处于板内拉张的动力学背景，而非挤压碰撞环境，结合对带内早石炭世雅满苏组火山—沉积建造较为系统的岩石学、岩石化学及岩石地球化学研究，认为觉罗塔格造山带应为一拉张型构造—岩浆岩带。     

阿尔泰造山带南缘基性杂岩的形成背景及其动力学含义

新疆北部阿尔泰造山带南缘出露-套基性杂岩,它们呈透镜状存在于晚古生代片麻状花岗岩中。阿拉尕克基性杂岩的~40Ar/39~Ar坪年龄为262．7±1．1Ma。基性杂岩的地球化学分析结果显示阿勒泰阿拉尕克、塔尔浪乡样品的轻、重稀土元素基本上没有发生分异,富蕴县乌恰沟基性岩的轻、重稀土元素发生了中一弱的分异；在微量元素特征方面,富集Th、Rb。通过地球化学图件判别,认为该基性杂岩形成于海山的构造环境。结合前人获得的花岗岩锆石SHRIMP的年代集中在400～410Ma左右,而花岗岩~40Ar/39~Ar坪年龄为240Ma左右,作者认为基性杂岩的~40Ar/39Ar坪年龄代表了晚二叠世时期的一次构造事件的年龄,基性杂岩寄生于花岗岩中是通过构造混杂作用实现的。在此基础上,提出了形成过程的两个阶段,即：晚古生代早期的俯冲阶段,为花岗岩与含海山玄武岩的增生楔形成阶段,晚二叠世的强烈碰撞阶段,导致花岗岩和增生楔物质的变形和构造混杂。     

天山-兴蒙造山带主要钼矿床Re-Os定年和地质意义

天山-兴蒙钼矿带是中亚成矿域的重要组成部分,该成矿带主要呈近东西向分布;本文通过对天山-兴蒙钼矿带4个典型矿床Re-Os同位素精确定年,结合前人区域动力学背景的研究,揭示天山-兴蒙造山带钼矿床的成矿作用主要与岩浆侵入形成的花岗岩热液作用有关,并识别出兴蒙造山带3期岩浆活动、钼成矿作用和构造热事件;Re-Os定年结果揭示出晚古生代铜-钼矿床与俯冲-增生作用有关,三叠纪钼的成矿形成于西伯利亚板块与塔里木-华北克拉通碰撞背景下,而侏罗纪-早白垩世的钼成矿作用与古太平洋板块西向俯冲作用有关。     

Uplift and cooling magnetisation record in the Bamble and Telemark terranes,Sveconorwegian orogenic belt,SE Norway,and the Grenville-Sveconorwegian loop

The ~ 1100 Ma Sveconorwegian orogenic belt comprises allochthonous terranes juxtaposed by major fault zones and emplaced against, and onto, the south-western margin of the Fennoscandian Shield. To resolve the magnetic signature acquired during post-orogenic uplift and cooling and evaluate wider correlations with the contemporaneous Grenville belt of North America, this study reports a regional palaeomagnetic study on a range of rock types from sectors of the medium-high metamorphic grade Bamble terrane (48 sites and 390 cores) and the adjoining medium-low grade Telemark terrane (33 and 240 cores) juxtaposed by an orogen-parallel (Porsgrunn- Kristiansand) fault zone with major vertical displacement. Magnetite and ilmeno-hematites are magnetic carriers with the latter more significant in the higher metamorphic grades. Magnetic intensities are stronger in the higher-grade terrane presumably due to the growth of metamorphic ferromagnets, but are an order lower than values predicted for the lower continental crust and indicate that an additional mechanism is responsible for high magnetisations in deep crust. Anisotropy of magnetic susceptibility (AMS) largely reflects the NE–SW tectonic grain of the last stage of Sveconorwegian ductile deformation. The magnetisation record is filtered by excluding magnetisations possibly acquired during regional Mesozoic dyke emplacement, development of the Permo-Carboniferous Oslo Rift and Late Proterozoic magmatism. The remaining record is a dual polarity signature summarised by mean poles at 31.9°N, 50.9°E, (N = 191 components) in the Bamble terrane and at 34.2°N, 58.9°E (N = 151 components) in the Telemark terrane. However these means are non-Fisherian and embrace arcuate distributions of magnetic components acquired during protracted exhumation cooling of the orogen with the best-defined parts comprising clockwise trajectories correlating with each another but indicating that cooling in Telemark was more protracted; in each case directions of more shallow NW-direction tend to be derived from lower unblocking temperature components. The geochronological evidence indicates that regional temperatures had fallen to permit acquisition of magnetisation by ~ 950–900 Ma and the two swathes define the younger limb of a clockwise (Grenville-Sveconorwegian) APW loop embracing the approximate interval 940–850 Ma; the outward path of this loop (~ 1020–940 Ma) is probably at present recorded only in dyke swarms from the Finnish sector of the shield. Correlation of APW between Laurentia and Fennoscandia confirms that the two shields broke apart shortly after culmination of the Sveconorwegian orogeny when Fennoscandia rotated rapidly clockwise into a secondary configuration adjacent to the eastern margin of Laurentia; the Grenville and Sveconorwegian orogenic frontal zones formed in alignment were reoriented at a high angle to one another in a coupling that appears to have persisted during most of the remainder of Neoproterozoic times.     

秦岭—大别造山带(湖北段)重力场特征与造山带构造

利用区域重力资料,通过位场分离、转换技术,揭示了造山带深部构造特征。正的线状重磁异常带及各阶小波细节,清晰地反映了桐柏—大别及东秦岭造山带南缘缝合带的位置,特别是重力异常小波四阶逼近,深部构造特征更加醒目。在鄂西北地区岩石圈所呈现出的"立交桥式"双层结构中,自由空间、均衡重力、剩余重力异常及小波各阶细节明显地反映出相对浅部的造山带近东西向延伸的构造特征;各阶逼近结果则反映了相对深部的地壳-岩石圈地幔南北向伸展的构造特征。应用地球物理资料来研究地球岩石圈结构、构造,除深层地震外,区域重力也是最有效方法手段之一。特别是近年来二维小波变换技术日趋成熟,为应用区域重力资料解决诸如造山带深部构造等疑难问题提供了新的手段和工作思路。     

陆—陆碰撞造山带中压型变质作用的pT轨迹——以南秦岭佛坪地区为例

依据石榴石的环带特征反演了南秦岭造山带中压型变质作用的pT轨迹，表明石榴石的环带记录了峰期变质前的温压条件递增过程，其最高温度与最大压力一致，这一过程可能与地壳的持续加厚过程相对应。峰期变质以后即出现有构造作用参与的快速抬升过程，pT轨迹表现为ITD型。这一研究可以加深入们的对造山带发生中压型变质作用过程的理解。     

北秦岭造山带中的拆沉作用

秦岭造山是一个非常有特色的碰撞造山带,来自地球物理、地球化学以及地质学的证据说明秦岭造山带中发生过拆沉作用,笔者主要讨论了北秦岭造山发生拆沉作用地地球物理、地球化学以及地质学证据,重点运用北秦岭地壳的地球化学特征进行对经,并用拆沉作用解释商丹地区的一些特殊地质现象。     

秦岭岩群中两类斜长角闪岩的性质和时代及其地质意义

在北秦岭造山带核部秦岭岩群内发育两类不同产状的斜长角闪岩.一类与秦岭岩群中的大理岩紧密共生,呈规模较大的似层状或较小块体产于大理岩内,另一类则呈密集岩墙群型式侵入于秦岭岩群南段二云母石英片岩中.不同的产出状态表明两类斜长角闪岩的成因和时代存在显著差异,也具有不同的地质构造意义.地球化学上,两类不同产状的斜长角闪岩的原岩皆为玄武岩质的.侵入秦岭岩群二云母石英片岩中的斜长角闪岩墙群形成于板内拉张环境,SHRIMP锆石U-Pb测年揭示该类斜长角闪岩形成于晚奥陶世(449±11Ma),Sr-Nd同位素特征显示其岩浆源区为亏损地幔源区,40Ar/39Ar热年代学研究显示该类斜长角闪岩的角闪岩相变质作用发生于石炭纪末期(301.3±6.4Ma).地球化学和Sr-Nd同位素特征显示与秦岭岩群大理岩共生的似层状或块状斜长角闪岩的形成环境与侵入云母石英片岩中的斜长角闪岩墙群的存在显著差异,其形成于洋岛(OIB)或海山环境.40Ar/39Ar热年代学研究显示该类斜长角闪岩于晚二叠世(258.1±5.7Ma)发生了角闪岩相变质作用.不同性质、形成和变质时代、相似的变质作用等特点表明,秦岭岩群中的两类角闪岩分属不同性质的构造块体,秦岭岩群高级变地质地体可能是一个构造拼合地体.斜长角闪岩岩墙为晚奥陶世(449±11Ma)侵入秦岭岩群云英片岩中的基性岩墙群,是北秦岭晚加里东期后造山期热收缩而致的地壳伸展或岩圈拆离减薄的产物.与秦岭岩群大理岩共生的斜长角闪岩则可能是洋隆体的基性喷出岩+碳酸盐岩帽组合,是中二叠世(312～260Ma)期间构造移置而来的外来块体.     

Intracontinental tectonic melange in Southern Apennines

On the axial zone of the Southern Apennines the major tectonic boundary between the inner platform (Western platform unit) and the pelagic (Lagonegro units) domains is represented by a thick level of highly deformed rock‐assemblage. Structural analysis reveals that this tectonic unit represents an intracontinental melange complex characterized by a block‐in‐matrix fabric that contains blocks from both hangingwall platform and footwall basin units. This unit comprises different sets of structures that, caused by shearing processes, developed at depths ranging from about 8–9 km to the surface. These tectonites represent the product of a crustal shear zone developed at the major boundary between platform‐basin domains of Adria during the thick‐skinned tectonic processes controlling the Southern Apennines mountain building.     

Influence of syn-sedimentary faults on orogenic structures in a collisional belt: Insights from the inner zone of the Northern Apennines (Italy)

This paper discusses the possible influence of syn-sedimentary structures on the development of orogenic structures during positive tectonic inversion in the inner Northern Apennines (Italy). Examples from key areas located in southern Tuscany provided original cartographic, structural and kinematics data for Late Oligocene-Early Miocene thrusts, organized in duplex systems, verging in the opposite direction of the foreland propagation (back-thrusts), which affected the Late Triassic-Oligocene sedimentary succession of the Tuscan Domain, previously affected by pre-orogenic structures. These latter consist of mesoscopic-to cartographic-scale Jurassic syn-sedimentary normal faults and extensional structures, which gave rise to effective stratigraphic lateral variation and mechanical heterogeneities. Structural analysis of both syn-sedimentary faults and back-thrusts were therefore compared in order to discuss the possible role of the pre-existing anisotropies in influencing the evolution of the back-thrusts. As a result, it can be reasonably proposed that back-thrusts trajectories and stacking pattern were controlled by relevant syn-sedimentary normal faults; these latter were reactivated, in some cases, if properly oriented. Such an issue adds new inputs for discussing the potential role of structural inheritance during tectonic inversions, and helps to better understand the processes suitable for the development of back-thrusts in the inner zones of orogenic belts, as it is the case of the inner Northern Apennines.     

The geology of part of the Southern foreland of the Damara orogenic belt in South West Africa and Botswana

A characteristic feature of the Damara geosyncline in northern South West Africa is the gradual transgression from the relatively undeformed sediments of the miogeosynclinal facies to the metamorphosed eugeosynclinical facies. A crude mirror-image of the arc separating the two facies is present along the southern foreland of the Damara geosyncline and conforms quite clearly with the northern limit of the Kalahari craton. However, owing to the presence of major thrust-faulting which eliminates the transition-beds between the two facies a direct correlation is not possible. The pre-Damara rocks on the southern side of the Damara geosyncline have been divided into the Marienhof Formation and the Dordabis Group in central South West Africa, and the Kgwebe Group in Botswana. These rocks form the base on which the strata constituting the Damara geosyncline have been deposited, and have been subjected to metamorphism both before and during the Damara orogenesis. The term Southern Marginal Facies is proposed for the unmetamorphosed strata deposited unconformably on the pre-Damara rocks along the southern flanks of the Damara geosyncline. These unmetamorphosed strata are composed of the Klein Aub, Witvlei, Ghanzi and Tsumis Formations which are regarded as the equivalent of the Nosib Group. They are unconformably overlain by the Nama Group which is considered to be, at least in part, the equivalent of the Hakos and Khomas Formations. Copper mineralization associated with calcareous shale, limestone and argillite occurs within the Klein Aub, Witvlei and Lower Ghanzi Formations. The mineralized strata closely resemble that of the Zambian Copper-belt with which they may well be correlated.     

喜马拉雅造山带东构造结拉布拉多期和格林威尔期造山作用的记录

位于喜马拉雅东构造结西北部的南迦巴瓦复合体,是构造应力最强、隆升和剥蚀最快、新生代变质和深熔作用最强的地区。为厘定该地区早期的变质岩浆作用,本文对南迦巴瓦复合体北部的花岗片麻岩和混合岩进行了岩石学和年代学研究。花岗片麻岩原岩为富钾的偏铝质花岗岩,具有岩浆弧花岗岩的成分特征。花岗片麻岩中的锆石具有岩浆锆石的环带结构,记录了487.9±1.6Ma的一期构造岩浆事件;混合岩的锆石具有明显的核-边结构,核部和边部的不协和线交点年龄分别为1559±13Ma、1154±12Ma。对比印度大陆东部的西隆高原、东高止造山带,发现三者都经历了拉布拉多期、格林威尔期以及泛非期的造山作用。因此,我们认为喜马拉雅东构造结与这两个地区密切相关,可能是他们向北的延伸,这三者可能组成统一的印度大陆东部造山带,一起经历了哥伦比亚超大陆、Rodinia和冈瓦纳超大陆的聚合与裂解过程。     

喜马拉雅造山带变泥质岩系及其地球化学特征

高喜马拉雅结晶岩系和北喜马拉雅穹隆都发育高角闪岩相-麻粒岩相变泥质岩,岩石组合以富铝质片麻岩类为主,伴生钾质花岗片麻岩、大理岩及基性麻粒岩等.元素地球化学特征表明,其原岩主要为较富铝的长石质砂岩和石英岩质砂岩及少量粘土岩,形成于大陆边缘浅海相沉积环境.这些变泥质岩具有相似的微量元素和稀土元素地球化学特征,表现为大离子亲石元素相对高场强元素较富集,轻稀土较重稀土富集,稀土总量较高,具有较显著的Eu负异常.在变质矿物组合、元素地球化学特征及锆石组成等特征上,它们与青藏高原北缘的康西瓦和阿尔金孔兹岩系相似,可能是来源于冈瓦纳大陆边缘的同一套岩石.