宁芜盆地火山-次火山岩的锆石U-Pb年龄、Hf同位素组成及其地质意义

宁芜火山盆地是长江中下游重要的火山盆地之一,在盆地内自下而上依次发育龙王山组、大王山组、姑山组和娘娘山组火山岩和若干个同源次火山岩或小侵入岩体。本文对宁芜盆地火山-次火山岩进行了详细的锆石U-Pb年龄和Hf同位素地球化学研究。研究结果表明,大王山组粗安岩锆石U-Pb年龄为130.3±0.9Ma,姑山组两个粗安岩锆石U-Pb年龄分别为128.2±1.3Ma和128.5±1.8Ma,另外三个侵入岩年龄分别为127.1±1.2Ma、128.3±0.6Ma和128.2±1.0Ma,均为早白垩纪。综合前人成果,认为长江中下游地区火山盆地内火山活动的时限在135～124Ma之间,不存在侏罗纪岩浆活动。宁芜盆地火山岩和侵入岩的锆石176Hf/177Hf值在0.282502～0.282673范围内,εHf(t)变化为-6.9～-0.7,显示岩浆源自于岩石圈富集地幔部分熔融并在上升过程中受地壳物质的混染,为岩石圈伸展环境的产物。     

长江中下游成矿带溧水盆地(次)火山岩的年代学及其意义

溧水火山岩盆地是长江中下游地区众多中生代火山岩盆地之一,在盆地内自下而上发育有龙王山组、大王山组、姚家边组和甲山组粗面质火山岩和若干个同源的次火山侵入岩体。针对溧水盆地火山岩-次火山岩进行系统的锆石U-Pb年代学研究,结果显示,龙王山组玄武质粗面岩的锆石U-Pb年龄为135 Ma±1 Ma,大王山组粗安岩的锆石U-Pb年龄为131 Ma±1 Ma,姚家边组粗安岩的锆石U-Pb年龄为128 Ma±1 Ma,另外1个粗安斑岩体的年龄为131 Ma±1 Ma,它们均为早白垩纪岩浆活动的产物。上述年龄数据与长江中下游地区其他盆地火山岩的年龄基本一致,表明长江中下游地区中生代火山岩的喷发时代主要集中在135Ma~127Ma之间,均受制于中国东部岩石圈减薄的伸展构造背景。     

浙江丽水地区磨石山群火山岩时代归属

为查明浙江丽水地区中生代磨石山群火山岩的时代,在区域地质调查、火山机构划分的基础上,选择该群代表性火山岩进行锆石年龄测定。结果表明,大爽组底部流纹质晶屑熔结凝灰岩的SHRIMP锆石U-Pb年龄为154.9±5.5 Ma、LA-ICP-MS锆石U-Pb加权平均年龄为152.0±7.0 Ma,属晚侏罗世基默里奇阶;高坞组流纹质晶屑熔结凝灰岩SHRIMP锆石U-Pb年龄为131.6±2.7 Ma,两个火山机构的西山头组流纹质晶屑凝灰岩LAICP-MS锆石U-Pb加权平均年龄分别为128.6±1.7 Ma和139.5±2.5 Ma。认为浙南磨石山群火山岩时代:大爽组为晚侏罗世,高坞组、西山头组、茶湾组和九里坪组为早白垩世。     

江西德兴孔家—银山火山盆地的时代归属：锆石U-Pb年代学证据

江西银山铅锌多金属矿床是一个特大型火山-次火山热液矿床,容矿的孔家—银山火山盆地中火山-次火山岩通常被认为属于鹅湖岭组,但时代归属仍存在争议。本文对与银山火山岩伴生的英安斑岩进行了锆石LA-ICP-MS U-Pb年龄测定,获得了206Pb/238U年龄加权平均值为(181.3±2.1)Ma(MSWD=2.3,n=20),说明银山火山盆地形成于180 Ma左右,为早侏罗世的产物。对以往地质调查资料进行了分析,认为区域上鹅湖岭组为晚侏罗世有确切的地质证据,而早侏罗世孔家—银山火山盆地中火山-次火山岩不属于鹅湖岭组,该认识对研究区域地质演化及成矿规律有重要的意义。     

粤东桃子窝锡矿区火山-次火山岩和花岗岩锆石U-Pb年龄、Hf同位素特征及其意义

桃子窝锡矿位于莲花山断裂带西段,是典型的火山-次火山岩型锡矿。本文以桃子窝锡矿赋矿火山-次火山岩及花岗岩为研究对象,首次开展LA-ICP-MS锆石U-Pb定年和Hf同位素特征研究。获得两个次火山岩样品的锆石206Pb/238 U加权平均年龄为172.1±1.1 Ma和171.8±0.9 Ma,一个花岗岩样品的锆石206 Pb/238 U加权平均年龄为168.9±1.5 Ma,表明桃子窝锡矿火山-侵入岩为中侏罗世同一岩浆事件不同阶段的产物。锆石εHf(t)值大多数为负值,只有3个点的值大于0,变化于-13.96~9.53之间,平均值为-7.92。在εHf(t)-t图解上,εHf(t)值大多落在球粒陨石演化线之下,有3个点落在球粒陨石与亏损地幔演化线之间。二阶段模式年龄除3个点介于609.6~795.5 Ma外,其余点年龄为1 450.8~2 102.5 Ma,Hf同位素特征指示成岩物质主要来源于早中元古代古老地壳的部分熔融,还有新元古代新生地壳物质的加入。结合区内已有的研究成果,认为桃子窝锡矿及有关的火山-次火山岩与中生代太平洋板块向欧亚大陆俯冲有关。     

新疆东准噶尔石炭纪火山机构类型与时限

东准噶尔卡拉麦里大气田的主要储层是石炭纪火山岩,石炭纪古火山机构的样式与组合特征,与火山岩储层展布关系密切。野外调查表明,隐爆角砾岩是东准噶尔石炭纪古火山机构最常见的标志之一。东准噶尔石炭纪古火山机构类型主要有中心式、裂隙式和裂隙-中心式等样式。中心式火山机构以大石头层状火山、柯克巴斯套锥状火山最为典型;巴塔玛依内山附近沿断裂分布的带状火山岩具有裂隙式喷发的特征;东黑山火山具有火山口串珠状排列特征,是裂隙-中心式喷发的产物。大石头地区原缪林托凯陶山组火山岩的锆石SHRIMP U-Pb年龄为345.6±7.1 Ma,而已知巴塔玛依内山组火山岩年龄是350.0±6.3Ma,因此东准噶尔火山活动的主要时期是早石炭世。     

粤北河口岩体次英安斑岩锆石U-Pb年代学和Hf同位素特征及其地质意义

河口岩体位于贵东复式花岗岩体外围北东侧,也是粤北地区代表性火山岩-次火山岩,前人对其源区特征、成岩时代、构造背景研究程度相对较低。本文在野外地质调查基础上,选取次英安斑岩进行LA-ICP-MS锆石U-Pb年代学及Hf同位素组成特征研究。结果表明,次英安斑岩的锆石U-Pb年龄为428.6±2.2 Ma、429.6±2.4 Ma,属晚加里东期火山岩系,进一步证实粤北-赣南地区存在较大范围的加里东期火山岩-次火山岩。次英安斑岩的εHf(t)变化范围较小,呈明显负值,且集中在上下地壳的演化线之间,指示其形成于陆壳物质的部分熔融,并无明显地幔物质的加入。锆石Hf模式年龄(t DM 2)平均值分别为1756 Ma、1802 Ma,指示河口地区可能存在过早元古代的古老基底,次英安斑岩可能是早元古代的变质岩部分熔融的产物,形成于加厚地壳背景下的后碰撞拉张构造环境。     

大兴安岭北部上护林盆地恩和大岭火山机构特征与时代

大兴安岭北部上护林盆地恩和大岭火山机构主要由白音高老组酸性熔岩、火山碎屑岩、次火山岩及火山-沉积岩组成。实测剖面显示,该火山机构由侵出相、溢流相、爆发相、次火山岩相及火山沉积相构成,不同岩性、岩相围绕火山口大致呈对称分布,产状外倾,为中心式喷发的穹状火山。溢流相的流纹岩和次火山岩相的正长斑岩锆石U-Pb测年结果分别为(115.3±2.3)Ma和(114.3±1.6)Ma,表明恩和大岭火山机构形成于早白垩世晚期。该火山机构为一次简单的火山喷发旋回一个喷发期次,大致的火山活动过程可分为四个阶段,第一阶段为早期岩浆溢流阶段,形成溢流相流纹岩夹少量流纹质角砾凝灰岩;第二阶段为晚期火山爆发阶段,产生大量的爆发相火山碎屑岩;第三阶段为岩浆侵入阶段,分别形成侵出相松脂岩、次火山岩相正长斑岩等;第四阶段为火山活动的间歇阶段,形成火山沉积相火山-沉积岩。     

江西南部版石盆地火山岩SHRIMP锆石U-Pb年龄及其地质意义

应用SHRIMP锆石U-Pb定年方法,对江西南部三南-寻乌火山岩带版石盆地原鸡笼嶂组凝灰岩和原版石组流纹岩开展年代学研究.结果表明,凝灰岩SHRIMP锆石U-Pb年龄为(142.5±1.3)Ma,流纹岩SHRIMP锆石U-Pb年龄为(131.4±1.3)Ma.根据新的国际地层表,晚侏罗世与早白垩世的界线划在(145.5±4.0)Ma,版石盆地原鸡笼嶂组和原版石组均形成于早白垩世早期.版石盆地火山岩系属同一个火山旋回的产物,且岩石组合与江西北部峡江-广丰火山岩带武夷群一致,其中原鸡笼嶂组可归入鹅湖岭组,原版石组可归入石溪组.     

羌塘地块南部晚白垩世火山岩离子探针测年及其对红层时代的约束

羌塘地块南部广泛出露陆相红层,1:25万区域地质调查将大部分红层划归为中新统康托组,但缺乏可靠的年代学依据。野外观测发现火山岩与红层之间存在喷发不整合接触关系,室内从火山岩选出很多岩浆锆石;应用离子探针U-Pb同位素测年方法精确测定岩浆锆石年龄,能够为研究火山喷发期次和红层形成时代提供重要依据。对羌塘地块南部红层内部粗面安山岩夹层—比洛错火山岩和扎加藏布北侧红层上覆安山岩,挑选岩浆锆石进行高精度的离子探针U-Pb同位素测年,发现比洛错粗面安山岩锆石206Pb/238U同位素年龄为(83.3±1.3)Ma,扎加藏布北侧安山岩锆石206Pb/238U同位素年龄为(75.65±0.82)Ma。这些年龄良好地揭示了晚白垩世不同期次的火山喷发时代,同时为红层形成时代和红层盆地演化提供了重要的年代学约束。根据比洛错和扎加藏布北侧火山岩的锆石U-Pb同位素测年资料,将羌塘盆地南部红层时代归属上白垩统阿布山组,这对分析羌塘地块南部油气地质构造保存条件和构造地貌演化具有重要意义。     

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.     

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.     

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″.     

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。     

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。     

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.