西藏拉萨地块过铝质花岗岩中继承锆石的物源区示踪及其古地理意义

富含继承锆石的过铝质花岗岩一般来源于富铝质岩石(如变泥质岩)的部分熔融,因而分析这些继承锆石的U-Pb年龄可以像分析沉积岩碎屑锆石的U-Pb年龄一样,提供过铝质花岗岩源区物质中碎屑沉积物物源区的丰富信息。本文报道了中部拉萨地块早侏罗世过铝质花岗岩的全岩地球化学和锆石U-Pb年代学数据,结合拉萨地块已有二叠纪和晚三叠世过铝质花岗岩的继承锆石年代学数据,总结了目前已有的拉萨地块过铝质花岗岩的继承锆石U-Pb年龄特征(共199个谐和测点)。这些过铝质花岗岩属强过铝质S型花岗岩,其中的继承锆石定义了1250~1100Ma(峰值1181±14Ma)和550~450Ma(峰值494±7Ma)2个最突出的年龄群,分别可比于拉萨地块古生代沉积岩的碎屑锆石年龄峰值(约1170Ma)和寒武纪火山岩的侵位时代,明显不同于西羌塘、安多和特提斯喜马拉雅新元古代-古生代沉积岩中的碎屑锆石年龄频谱。拉萨地块过铝质花岗岩中约1181Ma的继承锆石,可能与拉萨地块古生代沉积岩中的同期碎屑锆石一样,都来自澳大利亚南西部Albany-Fraser造山带和东南极Wilkes等地,而约494的继承锆石,既可能来自澳大利亚西部,也可能来自拉萨地块本地。本文提供了拉萨地块与澳大利亚大陆北缘具有古地理联系的过铝质花岗岩继承锆石U-Pb年龄证据。拉萨地块的研究实践表明,采用过铝质花岗岩继承锆石和古生代沉积岩碎屑锆石相结合的锆石U-Pb年代学方法,可为重建冈瓦纳大陆北缘其它微陆块的古地理和构造岩浆演化提供重要约束。     

滇西保山地块早古生代碎屑锆石U-Pb-Hf同位素研究及其对冈瓦纳大陆重建的制约

滇西地区出露的古生界公养河群和孟定街群分别位于保山地块的西部和东部,其沉积时代、构造归属、碎屑物质来源及在早古生代冈瓦纳大陆重建中的古地理位置具有重要研究意义。本文对公养河群2个砂岩样品和孟定街群的4个变质砂岩样品的碎屑锆石进行U-Pb定年和Lu-Hf同位素分析。其中,公养河群的碎屑锆石年龄谱范围是3862～533Ma,ε_(Hf)(t)值的范围是-37. 8～+11. 0,最小年龄峰期为549～533Ma,表明该群的最大沉积年龄为早寒武世早期,该群可能为寒武系地层。孟定街群的碎屑锆石年龄谱范围是3097～542Ma,ε_(Hf)(t)值的范围是-39. 5～+10. 5,其最小年龄峰期(576～458Ma)将该群的沉积下限时代限制在晚奥陶世。结合保山地块的其他古生代地层的碎屑锆石研究,我们认为保山地块在早古生代位于冈瓦纳大陆北缘,物源主要来自印度大陆,但～1. 17Ga年龄峰的出现说明其东部可能接受了一定比例来自西澳大利亚的沉积物质。这一结果表明保山地块在冈瓦纳大陆北缘重建中的位置应该靠近印度大陆,而其东缘接近澳大利亚大陆。     

临沧地体亲缘性及南段组物源——来自泥盆纪—石炭纪南段组碎屑锆石U-Pb年龄的证据

对临沧地体泥盆纪—石炭纪南段组的沉积岩开展碎屑锆石LA-ICP-MS U-Pb定年研究结果表明,所有样品的U-Pb年龄谱存在3个主要峰值:泛非期(530~680Ma)、晚格林威尔期(900~980Ma)和早格林威尔期(1100~1300Ma)。次要峰值年龄为1550~1730Ma和2350~2630Ma,反映了物源区构造-岩浆事件的复杂性。南段组碎屑岩锆石年龄图谱明显区别于思茅地块泥盆纪—石炭纪碎屑锆石年龄图谱,临沧地块南段组碎屑锆石的年龄表明其物源来自东冈瓦纳超大陆,临沧地体应该是来自东冈瓦纳北缘的微地块,这也与其生物特征相吻合。     

滇西腾冲地块高黎贡群变质沉积岩时代与原特提斯洋俯冲/增生：来自碎屑锆石U- Pb定年和岩石地球化学证据

滇西腾冲地块高黎贡群变质沉积岩时代和构造背景的厘定对正确认识原特提斯构造域演化过程及腾冲地块与冈瓦纳大陆之间的关系十分关键。岩石学、岩石地球化学结果表明,高黎贡群变质岩由变质沉积岩和变质岩浆岩组成,前者以片岩和副片麻岩为主,夹少量大理岩和石英岩,其原岩由一套杂砂岩、泥岩夹少量灰岩、硅质岩岩石组合,为深海-半深海相沉积物,形成于活动大陆边缘环境。碎屑锆石LA-ICP-MS U-Pb定年结果表明高黎贡群变质沉积岩中的锆石主要来源于与罗迪尼亚、冈瓦纳超大陆拼合及原特提斯洋俯冲有关的岩浆岩(900~1000Ma和500~600Ma),少量来源于中元古代地层(1500~1600Ma和2300~2400Ma)。4件样品中最年轻碎屑锆石群的加权平均年龄(507~510Ma)及没有出现有意义的小于470Ma碎屑锆石,表明高黎贡群变质沉积岩原岩形成于510~470Ma,是晚寒武世-早奥陶世早期原特提斯洋壳向冈瓦纳大陆下俯冲过程中,在俯冲带上盘沉积的含有大量该期火成岩碎屑的斜坡相沉积物。     

云开地块东缘寒武系-泥盆系不整合界面上下的碎屑锆石U-Pb年代学记录及对物源转换的响应

云开地块东缘粤西圭岗镇附近寒武系之上不整合覆盖一套灰白色石英砾岩-含砾砂岩,由于缺乏化石和年龄依据,这套岩石的时代长期存有争议.利用LA-ICP-MS U-Pb测年手段,对该套含砾碎屑沉积岩及其上下层位进行了U-Pb测年,4件样品共获得300组有效数据,年龄变化于2 900~400 Ma,不整合面之下样品主要集中于1 100~700 Ma,不整合面之上最年轻碎屑锆石年龄集中于450~400 Ma.新的测年数据结合前人研究成果表明,云开地块东缘不整合面下伏及上覆地层的时代分别为寒武纪和泥盆纪.研究区寒武纪时期物源特征与印度、东南极洲和澳大利亚西部相似,指示该时期研究区同冈瓦纳东北缘相连,物源来自东冈瓦纳北缘南极洲、印度地块和澳大利亚之间的造山带,而泥盆纪物源主要来自邻近的云开地块.寒武系和泥盆系之间的不整合面是早古生代郁南运动与广西运动叠加的产物.      

东特提斯喜马拉雅下白垩统碎屑锆石U-Pb年代学及其古地理

东特提斯喜马拉雅在中生代位于东冈瓦纳大陆的结合部位,其古地理对于了解东冈瓦纳大陆裂解至关重要.对东特提斯喜马拉雅塔嘎地区沉积地层进行了详细的碎屑锆石U-Pb年代学研究.结果表明,东特提斯喜马拉雅塔嘎地区采样剖面沉积下限为126.6±2.7 Ma.碎屑锆石年龄谱显示东特提斯喜马拉雅塔嘎地区采样地层主要包含~520 Ma、~890 Ma和~1 200 Ma的特征峰值年龄,对比结果表明东特提斯喜马拉雅塔嘎地区沉积地层碎屑锆石年龄谱与印度东部和澳大利亚西南部地层碎屑锆石年龄谱具有一定的相似性.结合东冈瓦纳岩浆活动记录以及该剖面下部玄武岩年龄,东特提斯喜马拉雅塔嘎地区地层沉积于东特提斯喜马拉雅从东冈瓦纳大陆分离时期,其物质来源可能为印度东部、澳大利亚西南部以及南极大陆.      

福建上杭盆地发现3.4Ga碎屑锆石

碎屑锆石已经成为研究区域地质演化的一种重要手段。本文对华夏地块东部上杭盆地底部产出的含砾石英砂岩中的碎屑锆石开展了LA-MC-ICP-MS U-Pb测年和Hf同位素测量。结果表明,这些碎屑锆石主要是岩浆锆石,锆石年龄变化于328~3 403 Ma,至少记录了10期的岩浆活动事件,表明该地区曾经历了长期复杂的地质演化历史。与华夏地块其他地区的碎屑锆石或捕获锆石一样,上杭盆地这些碎屑锆石年龄数据记录下了诸如晚太古代—早元古代地壳生长事件、哥伦比亚超大陆和Rodinia超大陆的汇聚与裂解、冈瓦纳大陆的聚合等全球主要地质事件,以及具有华夏地块特征的早古生代强烈的板内造山运动(武夷—云开运动)。最高峰值年龄出现在450 Ma,表明研究区附近最为强烈的事件是加里东运动(当地称作武夷—云开运动,或者广西运动)。Hf同位素数据表明,?Hf(t)=-27.2~19.8,绝大多数εHf(t)值小于0,两阶段亏损地幔Hf模式年龄(tDM2)介于1 124~3 979 Ma,峰值1 800~1 900 Ma,表明其早期岩浆活动主要与大规模的新生地壳有关,而晚期主要表现为对早期形成地壳的大规模改造,古老物质的再循环,很少有新生地壳增生。     

保山地体新元古代——早古生代沉积岩碎屑锆石年代学及其构造意义

滇西潞西地区位于青藏高原东南缘,大地构造位置上属于保山地体。由于新生代强烈的陆内变形作用,保山地体与青藏高原腹地体的对应关系难以确定。野外观察及LA-ICP-MS锆石U-Pb测年结果表明,潞西新元古代—早古生代地层(震旦系—寒武系蒲满哨群及下奥陶统大矿山组)大部分碎屑锆石Th/U0.1,说明其大多为岩浆成因。U-Pb年龄跨度较大,太古宙—早古生代都有分布,且具有明显的562Ma、892Ma及2265Ma年龄峰,以及较弱的1680Ma和2550Ma年龄峰。保山地体潞西地区沉积岩碎屑锆石年龄分布特征与特提斯喜马拉雅、南羌塘沉积地层碎屑锆石年龄分布特征相似,说明其具有相同的物源——冈瓦纳大陆北部的印度大陆。在新元古代晚期—早古生代,保山地体位于印度大陆北缘,与南羌塘、喜马拉雅地体相邻。伴随着俯冲相关的增生造山过程,保山地体形成相应的新元古代末期—早古生代沉积地层。     

昌宁-孟连结合带弄巴地区泥盆系、石炭系的时代及沉积环境:放射虫、碎屑锆石U-Pb年龄和Hf同位素约束

造山带中远洋深水沉积物是恢复古大洋的重要依据之一,昌宁-孟连古特提斯结合带存在大量海相沉积物,但是否存在大洋盆地相的远洋沉积还不清楚.对弄巴地区被认为最可能是洋盆相沉积的石炭系岩片和海相泥盆系岩片进行了岩石学、放射虫时代、碎屑锆石U-Pb年龄和Hf同位素研究.石炭系岩片放射虫硅质岩中鉴定出放射虫6属8种,时代为早石炭世早-中期.LA-ICP-MS锆石U-Pb定年结果显示,泥盆系岩片岩屑石英杂砂岩碎屑锆石年龄范围为387~3 266 Ma,最年轻一组年龄为387~413 Ma;石炭系岩片中与放射虫硅质岩共生的基性凝灰岩碎屑锆石年龄为341~3 403 Ma,最年轻一组年龄为341~354 Ma.综合锆石年龄和化石资料,限定泥盆系岩片原始沉积时代为早-中泥盆世,石炭系岩片时代为早石炭世早-中期.碎屑锆石U-Pb年龄谱特征和Hf同位素组成指示泥盆系岩片和石炭系岩片具有相似的物质源区,主要来源于亲冈瓦纳的陆壳,少量来自于古生代特提斯域新生岛弧.早-中泥盆世地层岩片原始沉积于亲冈瓦纳的大陆斜坡环境;早石炭世地层岩片原始沉积于亲冈瓦纳的大陆斜坡至古特提斯洋盆边缘环境,不是远洋深水的大洋盆地环境.寻找以远洋深水沉积物为代表的大洋盆地相沉积并开展研究是当前昌宁-孟连古特提斯研究的重要方向之一.      

Lower Paleozoic detrital zircon U-Pb geochronological characteristics of the Baoshan Block in western Yunnan and its constraints on the Proto-Tethys tectonic evolutionSCIEI北大核心CSCD

滇西保山地块是东特提斯构造域的主要微陆块之一,但对其物源和古地理位置仍存在较大争议。本文通过对保山地块西缘早古生代地层进行碎屑锆石U-Pb定年来约束其物源及古地理位置,并进一步探讨原特提斯洋早古生代构造演化模式。保山地块西缘早古生代地层具有相似的年龄分布模式,主年龄峰期为-0.95Ga、次级年龄峰期为-1.2Ga和-2.5Ga。寒武系公养河群最小锆石年龄为526Ma,结合其上部年龄为499.2Ma的火山岩夹层,约束其沉积时代为早寒武世早期。对比保山地块不同区域早古生代地层的碎屑锆石年龄数据,它们都具有相似的锆石年龄分布模式和年龄峰值。-0.95Ga主年龄峰期和-2.5Ga的次级年龄峰期指示保山地块早古生代的沉积物主要来自于印度大陆,而-1.2Ga的次级年龄峰期表明有部分沉积物来自于西澳大利亚,其早古生代古地理位置位于印度和西澳大利亚之间。结合沉积学证据及滇西地区广泛发育的早古生代岩浆作用,本文认为早古生代冈瓦纳大陆北缘为活动大陆边缘。     

Unity of the national and the international in the socio-cultural development of the peoples of the USSR

International unity is becoming ever stronger in this country owing to an increasing similarity in the development of the cultural environment. This comprises the provision of all the country's republics with a sufficient number of schools, theatres, and other institutions and cultural information media in accordance with the needs of the population. An important part is played by the rise in ‘the general educational level, as well as the level of professional qualifications and skills. Among all the Soviet nations and nationalities, this rise being more rapid among formerly backward peoples. Prominent among the factors of internationalization is the progressive development of the nationalities’ cultural resources, while professional culture is being increasingly brought within the reach of the masses.The implementation of the nationalities policy promotes the all-round development of all Soviet nations and nationalities, their drawing together, the upsurge of the individual capabilities of every Soviet citizen.     

Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth

It is known from observations that the center of mass of the Moon does not coincide with the geometric center of its figure, and the line connecting these two centers is not aligned with the direction toward the center of the Earth, instead deviating toward the Southeast. This stationary deviation of the axis of the inertia ellipsoid of the Moon to the South of the direction toward the Earth is analyzed. A system of five linear differential equations describing the physical libration of the Moon in latitude is considered, and these equations are derived using a new vector method taking into account perturbations from the Earth and partly from the Sun. The characteristic equation of this system is obtained, and all five oscillation frequencies are found. Special attention is paid to the fifth (zero) frequency, for which the solution of the latitude libration equations are stationary and represents a previously unknown additional motion of the rotational axis of theMoon in a cone with a small opening angle. In contrast to the astronomical precession of the Earth, the rotation of the angular-velocity vector is in the positive direction (counter-clockwise), with the period T ₃ = 27.32 days. On this basis, this phenomenon has been named “quasi-precession.” This quasi-precession leads to a stationary inclination of the major axis of the inertia ellipsoid of theMoon to the South (for an observer on Earth), making it possible to explain one component of the observed deviation of the center of mass of the Moon from the direction toward the Earth. The opening angle of the quasiprecession cone is approximately 0.834″.     

Global repeating events in the history of the Earth and the motion of the Sun in the Galaxy

Chronological analyses of correlations between certain global repeating events (mass extinctions of marine organisms, meteorite impacts, and flashes in the frequency of geomagnetic reversals) during the Phanerozoic Eon and the motion of the solar system in the Galaxy are presented for five rotationally symmetrical models for the regular Galactic gravitational field. Thirteen of sixteen mass-extinction events can be described by a repetition interval of 183±3 million years. This is in agreement with the anomalistic period (interval between two subsequent passages of the Sun through the apocenter of its Galactic orbit) in the model of Allen and Martos. The positions of the minima and maxima in Gaussian functions approximating the frequency distribution for geomagnetic reversals also agree with the times of passage of the Sun through the apocenter and pericenter, respectively, of its Galactic orbit in this model. The maximum in the distribution of the deviations of the dates of mass extinctions from the nearest dates of impacts of large, crater-forming bodies is close to zero, providing evidence that many such events are correlated. As a rule, extinctions follow impact events. The impacts of large bodies have occurred most often when the solar system passes through the Galactic plane, while mass extinctions occur more often at some distance from the Galactic plane (about 40 pc). As a rule, intervals of increases in the frequency of geomagnetic reversals coincide with dates of impacts of large bodies. At the same time, these intervals do not show a clear correlation with the dates of mass extinctions. The intensity of mass extinctions, like the energy released by impacts, is consistently higher in periods when the Sun is moving from the apocenter toward the pericenter of its orbit, than when it is moving from the pericenter toward the apocenter. Thus, there is evidence for a variety of relationships between repeating global events in the Phanerozoic and the motion of the Sun in the Galaxy. Long-period variations in the frequency of geomagnetic reversals are correlated with the orbital motion of the Sun, and increases in the frequency of geomagnetic reversals are correlated with impacts. Mass extinctions are correlated with the impacts of large bodies, whose motions may have been perturbed by clouds of interstellar material concentrated toward the Galactic plane and by the shock front associated with the Perseus spiral arm, through which the solar system passes. The velocity of the Sun relative to the spiral pattern is estimated.     

摩擦桩基桩土间极限摩阻力取值问题探讨

通过对广珠东线高速公路横沥大桥的试桩及土体的工程地质条件分析,总结出影响摩擦桩基桩土间极限摩阻力取值的一般问题以及解决问题的方法和措施。     

从榴辉岩与围岩的关系论苏鲁榴辉岩的形成与折返

位于华北和扬子两板块碰撞带中的苏鲁榴辉岩形成的温压条件不但是超高压，而且是高温。榴辉岩的PTt轨迹表明其为陆-陆磁撞俯冲带的产物。榴辉岩的区域性围岩花岗质片麻岩为新元古代同碰撞期花岗岩，榴辉岩及其他直接围岩皆呈包体存在于其中，并见新元古代花岗岩呈脉状侵入榴辉岩包体中。区域性围岩新元古代花岗岩的锆石中发现有柯石英、绿辉石等包裹体，表明新元古代花岗岩的组成物质也经受过超高压变质作用，且榴辉岩与围岩新元古代花岗岩的锆石U-Pb体系同位素年龄基本相同。但新元古代花岗岩所记录的变质作用和变形作用期次（或阶段）却少于榴辉岩。椐上述可得如下推断：超高压榴辉岩与新元古代花岗岩岩浆是同时在碰撞带底部（俯冲板块前部）形成的；榴辉岩的第一折返阶段是由新元古代花岗岩岩浆携带上升的，其第二折返阶段是和新元古代花岗岩一起由逆冲及区域性隆起而上升，遭受剥蚀。     

某高速公路下伏煤矿采空区稳定性分析

在论述某高速公路下伏砦脖煤矿采空区地质、采矿和工程地质特征的基础上, 进行了稳定性数值模拟分析, 定性与定量地分析与评价了该煤矿采空区的地表变形特征及稳定性。研究结果表明: 该煤矿采空区的变形尚未完成, 对拟建的高速公路将产生很大的危害, 必须采取相应的工程治理措施。      

The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads

In order to characterise the influence of the heavyrains on the observed landslides during the 1996–1997hydrological cycle, rainfall records for the last 100years are analysed from 104 stations in easternAndalusia. Regarding the amounts of rain recordedbetween October 1996 and March 1997 in the 104stations studied, 31 presented new all-time records;15 presented values that were 80–100% of thepre-1995 record; 49 stations, 80–50%; and 9stations, < 50%. A map has been devised of thesusceptibility of the materials through which thesouth-eastern Andalusian road network crosses,together with an inventory of the damage caused byinstability phenomena on banks and cuttings of theroad network during the winter of 1996–1997. Therelationships between the rainfall during the studyperiod, the damage caused to the road network and thesusceptibility of the materials affected are analysed.The results indicate that there is a clearcorrespondence between the rainfall recorded and thesusceptibility of the materials with the inventorieddamage. It is concluded that the widespread seriousdamage caused in early 1997 to the roads andsurrounding areas in the Alpujarra region and thecoast of the Province of Granada was mainly caused bythe extraordinarily heavy rains. However, considerablyless damage was observed where the susceptibility ofthe terrain is low, thus highlighting the extremeusefulness of terrain-susceptibility maps for riskprevention and territorial planning.     

On the consistency of proposed models for the Pyrenees with the structure of the eastern parts of the belt

The structure of the eastern Pyrenees consists mainly of south-directed thrusts involving basement and cover rocks. An antiformal stack developed by the piling up of basement thrust sheets which outcrop in the Axial zone. These structures account for a thin-skinned thrust model rather than a vertical fault model in which the Axial zone would be essentially autochthonous, and the North-Pyrenean fault the axial plane of a fan thrust system. New data from the Eastern Pyrenees and the thin-skinned model suggest that(1) the structure east of the Pedraforca nappe is similar to that of the Central Pyrenees; (2) the cover rocks of the South-Pyrenean units and of the Axial zone-after restoration—built up a northwards-thickening prism consistent with the existence of a unique Pyrenean sedimentary basin during Mesozoic time; (3) the Axial zone is only a complex antiformal stack developed as a part of South-Pyrenean system related to the Paleogene thrusting-tectonics. The Axial zone palaeogeographic area had no special meaning during Mesozoic time.