雅鲁藏布江缝合带西段仲巴地区俯冲—增生过程

雅鲁藏布江缝合带是新特提斯洋俯冲消亡的残余,记录了新特提斯洋打开—闭合的全过程。本文以雅鲁藏布江缝合带西段仲巴地区南侧的纳久混杂岩为研究对象,进行了详细的放射虫年代学,砂岩碎屑锆石U-Pb同位素年代学以及碎屑组分统计研究。我们的数据表明,纳久混杂岩中硅质岩含有大量保存较好的放射虫化石,包含Pseudodictyomitra carpatica带典型分子,根据放射虫时代组合确定其时代为早Barremian阶;混杂岩中砂岩岩块主要为岩屑砂岩,不同样品碎屑锆石得出的最大沉积年龄介于95～73 Ma之间。碎屑锆石U-Pb年龄源区分析表明,碎屑物质来自北侧的冈底斯岩浆弧和拉萨地体。纳久混杂岩南侧的砂岩沉积时代为早白垩世,碎屑锆石U-Pb年龄源区表明具有典型的特提斯喜马拉雅特征。我们的数据表明,纳久混杂岩基质时代为早白垩世,砂岩岩块时代为晚白垩世,与北侧的早白垩世蛇绿岩共同组成了白垩纪的增生楔,随着印度与欧亚大陆的碰撞仰冲到特提斯喜马拉雅之上。     

西藏南部绒布地区晚白垩世宗卓组沉积相与沉积环境演化

宗卓组地层作为中生代海相沉积的重要组成部分,记载了西藏南部地区白垩纪古海洋、古气候等重要地质历史信息。通过对砂岩进行镜下观察、物源分析、粒度分析等方面的研究,本文对绒布地区宗卓组的沉积相类型和沉积环境演化有了新的认识。粒度分析指示沉积时期水体搬运动力较弱、存在浊流沉积;宗卓组内3种不同类型的砂岩镜下特征、地球化学特征和锆石U- Pb年龄,指示3类砂岩的物源不同。本文在宗卓组共识别出陆棚相、大陆斜坡相和深海盆地3类沉积相,并对其进行了更为详细的划分。晚白垩世新特提斯洋壳向北俯冲,俯冲结束后印度—亚洲大陆发生初始碰撞。结合研究区构造背景分析,本文推测这是导致研究区沉积环境由半深海环境变为深海环境的原因。对研究区宗卓组地层和砂岩来源进行分析后得出：在洋壳俯冲阶段,宗卓组为被动大陆边缘沉积;在之后印度—亚洲陆陆碰撞的初始碰撞阶段,特提斯喜马拉雅被动陆缘已不复存在,并完全过渡为前陆盆地。     

藏南江孜县白沙地区宗卓混杂岩：岩石组成与物源区分析

藏南宗卓混杂岩是印度-欧亚大陆早期碰撞过程的重要地质记录.本文对江孜县白沙地区宗卓混杂岩进行了详细的野外和室内岩石学研究.该混杂岩由岩块和“基质”组成,岩块岩石类型有砂岩、硅质岩、玄武岩、砾岩等,“基质”以未变质的黑色页岩、泥岩为主.砂岩碎屑统计显示,其碎屑成分为火山岩屑和沉积岩屑,与日喀则弧前盆地类似.砂岩碎屑锫石年...     

藏南仲巴地区早白垩世日朗组物源分析及其构造意义

藏南仲巴地区早白垩世日朗组出露于特提斯喜马拉雅北亚带,整体为黄绿色火山岩屑砂岩,局部层位可见页岩与泥岩,分析为一套深海海底扇沉积组合。本文仔细分析了日朗组砂岩岩石学特征及鲍马序列和槽模沉积构造等沉积学特征,结果表明:日朗组砂岩成分成熟度和结构成熟度均不高,具有近源物源的特点;槽模构造古水流数据统计表明古流向由南向北,指示物质组分来源于南侧特提斯喜马拉雅和/或印度克拉通。砂岩碎屑组分统计结果表明日朗组的物源区构造背景属于克拉通内部及石英再旋回区。碎屑锆石U-Pb年龄频谱图对比进一步表明其物源区为印度稳定大陆边缘,外加一套早白垩世火山碎屑物质的输入。仲巴地区日朗组物源特征反映了印度大陆北缘早白垩世由深部断裂引起的一次强烈的火山事件,可能与印度大陆从澳大利亚-南极大陆裂解有关。     

西藏札达地区上白垩统-下始新统达机翁组:对冈底斯弧前盆地演化的制约

冈底斯弧前区域地层沉积记录,对新特提斯洋消亡和印度-亚洲碰撞过程的研究具有十分重要的意义。位于西藏南部札达地区的达机翁组,北邻冈底斯岩浆弧,南靠雅鲁藏布江缝合带。岩石组成主要包括砾岩、岩屑砂岩、泥页岩和灰岩等。沉积环境分析认为达机翁组形成于扇三角洲相环境。火山灰锆石U-Pb定年、碎屑锆石最年轻年龄以及底栖有孔虫化石组合共同约束达机翁组的形成时代为晚白垩世-始新世早期(即ca.73～49Ma)。物源区分析结果表明达机翁组物源类似于区域上分布的日喀则弧前盆地沉积,直接以北侧冈底斯岩浆弧为主要物质源区。通过与区域弧前沉积对比,为冈底斯弧前盆地海相地层时代提供制约,结果显示新特提斯洋在亚洲大陆南缘的弧前海退存在东西方向上的穿时性,即海水自东向西逐渐退出,并最终在～49Ma退出冈底斯-拉达克弧前区域。     

藏南古近纪甲查拉组物源分析及其对印度-欧亚大陆碰撞启动时间的约束

位于特提斯喜马拉雅北亚带的江孜地区古近纪甲查拉组角度不整合于晚白垩世宗卓组之上,系该地区最高(时代最晚)海相地层。运用岩石学和地球化学方法对其进行分析研究结果表明该组物源区主要为近源再旋回造山带,岩屑的母岩类型主要是岩浆弧成因的中性、中酸性安山质火山岩。新生代以前,特提斯喜马拉雅属于印度板块的被动大陆边缘,从特提斯喜马拉雅南亚带向北亚带显示了一种从浅水陆棚到深水盆地的变化,在侏罗-白垩纪时其陆源碎屑物主要是成熟度极高的石英砂岩,所以甲查拉组的碎屑物质只能来源于当时的冈底斯弧地区,所获有限的古水流证据也指示了这一点。从欧亚大陆侵蚀下来的碎屑物质被带到原印度大陆地区沉积,暗示该区的特提斯洋壳已经完全消失,印度与欧亚大陆在特提斯喜马拉雅中、东部产生了初始的陆-陆碰撞,其碰撞的启动时间为甲查拉组开始沉积的65 M a±。     

西藏林周盆地中侏罗统却桑温泉组碎屑锆石U-Pb年代学及地质意义

林周盆地位于冈底斯板块中部，对其进行盆地分析将为理解冈底斯板块构造演化过程提供重要的沉积学证据。本文以林周盆地中侏罗统却桑温泉组为研究对象，开展岩石学和碎屑锆石U-Pb年代学研究，结果显示却桑温泉组岩屑石英砂岩最年轻碎屑锆石年龄为169 Ma，存在620～540 Ma,1 220～1 055 Ma等年龄峰值，其中最年轻碎屑锆石年龄是对特提斯洋壳俯冲引发的岩浆事件的响应。碎屑锆石区域对比研究表明却桑温泉组物源主要来自冈底斯中部唐加-松多造山带，为特提斯洋向北俯冲、向南增生过程的沉积记录。     

藏南柳区砾岩的沉积环境及物源分析:对雅鲁藏布缝合带古近纪隆升的约束

沿雅鲁藏布江缝合带分布的柳区砾岩是喜马拉雅造山作用过程中重要的沉积记录。然而,目前对该套地层的构造属性仍存在不同的认识,因为尚未发现来自冈底斯中酸性的火山岩砾石,部分学者认为其是在印度和洋内岛弧碰撞形成的。本次工作对柳区出露的柳区砾岩进行了详细的剖面实测、沉积学观察和物源区分析。地层由厚层的砾级到巨砾级的砾岩以及相对较薄层的砂岩和泥岩组成,砾石包括硅质岩、基性-超基性岩、石英砂岩、岩屑砂岩以及板岩和千枚岩。砾岩分选差,磨圆差,颗粒支撑和基质支撑均发育,根据岩相组合判断其形成于冲积扇和辫状河环境。较大的砾径以及极低的结构成熟度表示为近源堆积,暗示雅鲁藏布江蛇绿岩带为该套砾岩的重要源区,而特提斯喜马拉雅带为板岩和片岩的主要源区。岩屑砂岩的碎屑颗粒统计结果显示岩屑的含量为82%~85%,其中沉积岩屑为主(82%~95%),石英颗粒以单晶石英为主。碎屑锆石U-Pb年龄有453~579Ma和737~889Ma二个主要的范围,而缺少200~400Ma的锆石年龄。上述观测都说明日喀则弧前盆地、雅鲁藏布蛇绿岩带和特提斯喜马拉雅为柳区砾岩的重要物源区。由于柳区砾岩内部含有日喀则弧前盆地提供的物源,所以柳区砾岩是印度-欧亚板块碰撞之后沉积的。而柳区砾岩内各成分的变化反应源区对物源贡献的变化,同时记录了造山带隆升的历史,具体表现为印度-欧亚板块碰撞后,首先雅鲁藏布江蛇绿岩带和日喀则弧前盆地相对较快隆升,并遭受剥蚀,为柳区砾岩的沉积提供初始的物源,随着印度板块的俯冲,特提斯喜马拉雅带开始隆升,成为了柳区砾岩的物源,主要提供板岩和千枚岩。进一步的俯冲使得蛇绿岩带大幅度隆升而阻碍了日喀则弧前盆地和冈底斯继续提供物源,使得柳区砾岩上段石英砂岩中缺少火山岩石英和再旋回的石英颗粒。     

古新世特提斯喜马拉雅南亚带石英砂岩成因及其构造意义:以藏南岗巴地区古新统基堵拉组为例

特提斯喜马拉雅南亚带作为印度被动大陆北缘的主要构造单元,相较于其他类似构造单元发育着多套特殊的石英砂岩,意味着被动大陆边缘物源区陆源碎屑供应能力的多次变化,而引起印度被动大陆北缘石英砂岩沉积的构造背景和构造意义尚不明确。以特提斯喜马拉雅南亚带的岗巴地区古新统基堵拉组石英砂岩为例,通过砂岩碎屑成分分析、古流向恢复、重矿物分析和碎屑锆石年代学方法,对基堵拉组石英砂岩的沉积学及物源区特征,以及蕴含的成因和构造意义进行探讨。从沉积相分析结果来看,在早古新世岗巴地区所属的板块为印度被动大陆边缘,处于新特提斯洋的海岸线附近,以滨岸相为主,显示了一种浅海陆棚到陆相的变化。从砂岩岩相学的结果分析,基堵拉组的陆源碎屑物主要是成熟度极高的石英砂岩,同时古水流近NNE方向。从碎屑锆石年代学数据分析结果可知,基堵拉组的碎屑锆石年龄特征与早白垩世德干高原地区相吻合。故认为基堵拉组石英砂岩的形成是由于印度北缘的陆源碎屑供应量突然增多与被动大陆边缘物源区构造抬升导致,而引起被动大陆边缘物源区构造抬升的原因主要与德干大火成岩省形成相关。最终认为石英砂岩的发育成因与印度大陆北缘德干大火成岩省形成时构造隆升所导致的稳定克拉通再活化有关。     

西藏冈底斯带中部南木林地区林子宗群火山岩锆石U-Pb年龄和地球化学特征

林子宗群火山岩广泛分布在冈底斯带上,其岩石学特征及所代表的区域不整合事件被认为与特提斯洋俯冲消减到印度-亚洲大陆碰撞转变有关。对冈底斯带南木林地区的林子宗群火山岩进行了LA-ICP-MS锆石U-Pb测年及地球化学研究,获得林子宗群火山岩帕那组LA-ICP-MS锆石U-Pb年龄为46.08±0.47Ma、49.00±1.30Ma,对比冈底斯带其他地区已发表的年龄数据,认为印度-亚洲大陆碰撞(在西藏南部)的时间,东部可能依次早于中部和西部。地球化学特征表明,冈底斯带南木林地区林子宗群火山岩具有碰撞后地壳加厚背景下产生的弧火山岩特征,应为新特提斯洋俯冲消减到印度-亚洲大陆碰撞构造背景下形成的。     

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.