玉石沟铬铁矿床的成因

玉石沟铬铁矿床产于北祁连蛇绿岩型超镁铁岩中，可分为产于堆积超镁铁岩中的堆积铬铁矿床和产于地幔橄榄岩中的豆荚状铬铁矿床两种类型。堆积铬铁矿床由玄武岩浆分离结晶作用形成，位于辉长岩下约２０ｍ处的纯橄岩或辉石岩中；豆荚状铬铁矿床由地幔岩部分熔融作用形成，产于地幔橄榄岩上部或顶部基性程度最高的纯橄岩或纯橄岩－斜辉辉橄岩杂岩带，位于堆积杂岩下约２００～１７００ｍ范围内。     

西藏罗布莎蛇绿岩中不同产出的纯橄岩及成因探讨

罗布莎蛇绿岩中的纯橄岩有三种产出情况,除了与豆荚状铬铁矿伴生的薄壳状纯橄岩外,还有产在方辉橄榄岩底部被认为是堆晶岩的厚层状纯橄岩和方辉橄榄岩中的透镜状纯橄岩。厚层状纯橄岩约700～1000m厚,以橄榄石富镁(Fo93～95),单斜辉石低铝富镁(Al2O30.47%～0.85%,Mg#95～97),铬尖晶石高铬低镁(Cr#值平均77,Mg#平均51)为特征。该纯橄岩中的浸染状铬铁矿也是高铬低镁型,但Mg#值(平均59)高于厚层状纯橄岩的副矿物铬尖晶石。薄壳状纯橄岩与厚层状纯橄岩成分相近,其橄榄石Fo92～94,单斜辉石Al2O3<1%和Mg#95～97;铬尖晶石的Cr#值平均71,Mg#值平均52。与薄壳状纯橄岩伴生的块状铬铁矿为高镁高铬型,但Mg#值(平均68)相对更高些,Cr#值平均79。透镜状纯橄岩的特征是橄榄石Fo(91～92)和铬尖晶石Cr#(60左右)均低于前两类纯橄岩,但单斜辉石的Al2O3(1.41%～1.71%)则高于前两者。透镜状纯橄岩的矿物成分与方辉橄榄岩重叠,两者为渐变过渡关系。研究对比表明,罗布莎厚层状纯橄岩不同于经典的蛇绿岩的超镁铁质堆晶岩,认为将其成因解释为拉斑玄武质熔体与地幔橄榄岩的反应较为合理。透镜状纯橄岩与方辉橄榄岩存在成生联系,可能是地幔橄榄岩高度部分熔融的产物,或熔体和方辉橄榄岩在原位发生反应的产物;薄壳状纯橄岩成因与厚层状纯橄岩相同,但与其相伴的块状铬铁矿是否由拉斑玄武质熔体与方辉橄榄岩反应形成,值得商榷。     

南祁连大道尔吉早古生代弧后盆地型蛇绿岩的年代学、地球化学特征及意义

大道尔吉蛇绿岩是中祁连地块和南祁连褶皱带之间蛇绿混杂岩带的重要组成部分。出露的岩石单元包括地幔橄榄岩、镁铁–超镁铁质堆晶杂岩和玄武安山岩。其中镁铁–超镁铁质堆晶杂岩包括三个堆晶旋回,单个堆晶旋回底部为含铬尖晶石纯橄岩,向上逐渐变为透辉石岩(辉石橄榄岩)→辉长岩等。堆晶杂岩中辉石橄榄岩Sm-Nd同位素等时线年龄为441±58 Ma,为加里东中期岩浆活动的产物。地球化学特征显示:地幔橄榄岩MgO(40.41%~40.96%)、Cr(3590×10~(–6)~7340×10~(–6))、Ni(1480×10~(–6)~1710×10~(–6))含量高,而Al_2O_3(0.35%~0.59%)、TiO_2(0.03%~0.04%)和∑REE(0.81×10~(–6)~1.84×10~(–6))含量低,具亏损地幔岩的特征;镁铁–超镁铁质堆晶杂岩的主量元素变化大,重稀土元素富集,正Eu异常(δEu=1.22~2.15);玄武安山岩SiO_2为54.90%~57.76%,MgO为3.50%~5.45%,TiO_2为0.72%~1.12%,Na_2O/K_2O1,∑REE为24.9×10~(–6)~53.4×10~(–6),LaN/YbN=1.0~1.7,具平坦稀土配分模式,与E-MORB相似,同时富集Ba、Rb、Th等大离子亲石元素,亏损Nb、Ta、Zr、Ti等高场强元素,具弧后盆地火山岩地球化学特征。综合区域地质、岩石组合和地球化学特征,认为大道尔吉蛇绿岩属构造肢解的蛇绿岩残片,具有俯冲带(SSZ)型蛇绿岩的特征,形成于弧后盆地环境,为奥陶纪柴北缘洋向中祁连地块俯冲,引起弧后扩张形成。     

西藏日喀则蛇绿岩大竹曲豆荚状铬铁矿形成机制

为了研究蛇绿岩型豆荚状铬铁矿床的成因和构造环境,对西藏雅鲁藏布构造带中段的日喀则蛇绿岩大竹曲岩体中的铬铁矿化进行了研究。通过岩相学和地球化学研究,发现大竹曲地幔橄榄岩中铬尖晶石为不规则它形,且全岩的CaO和Al_2O_3含量与铬尖晶石Cr~#分别呈正相关和负相关关系,这表明地幔橄榄岩中铬尖晶石为地幔部分熔融的残余。然而,纯橄岩和矿石中铬尖晶石显示自形-半自形,并可见橄榄石包裹自形铬尖晶石,且纯橄岩与矿石的CaO和Al_2O_3和Cr~#均无相关性,均说明纯橄岩和铬铁矿石形成于岩石-熔体反应。高Cr~#矿石和纯橄岩的母岩浆性质接近于玻镁安山质熔体,而低Cr~#纯橄岩的母岩浆则类似于MORB,表明大竹曲铬铁矿可能形成于弧后扩张中心。     

藏南罗布莎铬铁矿床铬尖晶石矿物学与矿床成因研究

西藏罗布莎铬铁矿床是我国目前研究程度最高、规模最大、地幔橄榄岩相对新鲜的豆荚状铬铁矿床,主要工业矿体产于蛇绿岩壳-幔边界(即岩石莫霍面)以下方辉橄榄岩相带一定层位中,主要有块状、浸染状和豆状等矿石类型。罗布莎铬尖晶石成分变化范围大,依据铬尖晶石的化学成分与矿物学研究至少可识别出3个期次铬尖晶石:(1)成矿前期铬尖晶石,主要以熔蚀残斑晶、出溶晶及少量自形晶形式产于方辉橄榄岩中,以富Al₂O₃为特征,Cr^#值变化范围大(17.19~66.30),且大部分小于60,并与Mg^#值呈负相关关系,由出溶晶,残斑晶到自形晶铬尖晶石,总体表现向富Cr、Fe的方向演变;(2)成矿主期铬尖晶石,可分为早、晚2个阶段。早阶段铬尖晶石主要以它形晶产于不同类型铬铁矿石中,部分呈自形-半自形晶产于铬铁矿体的纯橄岩外壳中,主要以富铬为特征,矿石中Cr^#值变化范围小(70.08~87.03),均大于60,其中块状铬铁矿具有最高的Cr^#和Mg^#,由纯橄岩外壳中副矿物铬尖晶石向豆状、浸染状矿石以及块状矿石演变过程中,铬尖晶石化学成分总体向更富Cr、富Mg方向演变;晚阶段铬尖晶石:主要以自形-半自形晶产于具堆晶结构的纯橄岩相带中,成份上以更加富而贫Al₂O₃,且具有最低Mg^#(18.79~44.77)值为特征;(3)成矿晚期铬尖晶石,主要以网状集合体产于豆状-网脉状(眼眉状)矿石中,以更贫Al、富Fe为特征,具有最高的Cr^#值和低的Mg^#值。综合研究表明,罗布莎铬铁矿中的铬主要来自原始地幔岩本身,且主要来自于地幔橄榄岩中2种辉石的不一致熔融和对副矿物铬尖晶石的改造,原始富铬矿物可能来自地幔深部的八面体硅酸盐矿物。罗布莎豆荚状铬铁矿的成矿作用具有多期次、多成因、多种构造背景下成矿特征,成矿作用过程经历了由大洋中脊(MOR)扩张环境向岛弧体系俯冲环境的转变过程,洋内俯冲带之上(SSZ)的弧间盆地环境是形成冶金级豆荚状铬铁矿的最为有利构造环境。研究提出了罗布莎铬铁矿的"三阶段"成矿模式,即,经历了大洋中脊预富集阶段,俯冲带之上主成矿阶段及之后的构造抬升改造阶段。纯橄岩与方辉橄榄岩接触带之下的方辉橄榄岩相带是寻找较大规模铬铁矿床的有利地带。     

豆荚状铬铁矿床的研究现状及进展

豆荚状铬铁矿床是工业上冶金级铬铁矿石的最主要来源,对于其成因研究依然是各国地质学家最为关注的热点之一。文章着重概述了近年来国内外地质学者对豆荚状铬铁矿床成因研究的现状和最新进展。最新研究表明,显生宙以来的豆荚状铬铁矿床具有一定的成矿专属性,主要赋存于蛇绿岩套底部(壳-幔边界,即岩石莫霍面)地幔橄榄岩中的一定层位中。世界上含矿的地幔橄榄岩普遍具有垂直熔融分带特征,即上部偏基性,下部偏酸性。豆荚状铬铁矿床与纯橄岩-方辉橄榄岩相密接相关,却很少见有豆荚状铬铁矿床产于二辉橄榄岩中。豆荚状铬铁矿的成矿作用经历了由洋中脊(MOR)扩张环境向岛弧体系俯冲环境的转变过程,而岛弧环境(岛弧、弧后盆地、弧前盆地等)是形成冶金级豆荚状铬铁矿的最为有利的构造环境。富铬铬铁矿与纯橄岩、玻安岩(Boninite)均为亏损地幔橄榄岩再次高度熔融的最终产物,而玻安岩普遍产于岛弧环境。虽然玻安岩不是铬的有效载体,但玻安岩的熔离促使铬铁矿达到进一步的富集。铬铁矿中的铬来自原始地幔,主要来自于地幔橄榄岩中两种辉石的不一致熔融及其对副矿物铬尖晶石的改造。随着部分熔融程度的增高,地幔橄榄岩逐渐向富镁方向演变,而对应的造矿铬尖晶石也逐渐向富镁、富铬方向演变。     

大道尔吉式铬铁矿

正成矿区带:中祁连成矿带(Ⅲ-22)。建造构造:奥陶纪形成的野人沟、大道尔吉和小道尔吉3个超基性岩体群呈透镜状挤入蓟县系大理岩之断裂带中。大道尔吉岩体分为:变质地幔橄榄岩带,由纯橄岩和方辉橄榄岩(m/f为10.16～11.14)组成;堆晶杂岩带由纯橄岩-含辉纯橄岩(m/f为7.34～9.11)、透辉岩-易剥橄榄岩-辉长岩组成(m/f为3.16～     

对豆荚状铬铁矿床成因及评价准则的新认识

产于蛇绿岩套地幔橄榄岩中的豆荚状铬铁矿床，有高铬及高铝两种类型；前者属于ＰＰＧ蛇绿岩系列，后者属于ＰＴＧ蛇绿岩系列。作者的最新研究成果表明，高铬型铬铁矿是原始地幔岩高度熔融再造的产物。高熔系指随熔融程度的增高，原始地幔岩中的单斜辉石斜方辉石，借助于不一致熔融转变为橄榄石和铬尖晶石，导致了纯橄的形成。     

对富铝型豆荚状铬铁矿矿床成因的新认识一一以新疆萨尔托海铬铁矿矿床为例

萨尔托海铬铁矿矿床产于萨尔托海蛇绿岩块的地幔橄榄岩中,属于富铝型豆荚状铬铁矿床。该矿床与一套橄长岩和辉长岩类岩石紧密伴生,矿体周围常被一薄的绿泥石壳所包裹。本区铬铁矿的形成包括两个阶段:第一阶段是原始地幔岩经高度熔融形成富铬铬铁矿;第二阶段形成富铝铬铁矿。交代作用伴随着新生单斜辉石和斜长石的形成。原始地幔岩的高度熔融以及基性熔体在地幔橄榄岩中的形成和存在是萨尔托海铬铁矿形成的先决条件。     

北秦岭松树沟橄榄岩与铬铁矿矿床的成因关系

松树沟橄榄岩体是秦岭造山带中规模最大的赋存铬铁矿床的超基性岩体。松树沟橄榄岩主要由细粒橄榄岩质糜棱岩和中粗粒橄榄岩组成。本文通过对松树沟橄榄岩的岩相学、主微量、稀土元素地球化学的系统研究,认为松树沟细粒方辉橄榄岩为洋脊扩张过程中地幔岩减压-近分离熔融产生的残留体,细粒纯橄岩主要由地幔橄榄岩熔融残留橄榄石、消耗辉石的减压熔融反应:aCpx+bOpx+cSpl=dOl+1Melt生成的橄榄石和少量的地幔方辉橄榄岩残留体组成,但均受到了后期渗滤熔体的再富集作用;中粗粒纯橄岩和方辉橄榄岩主要为上述反应产生的渗滤熔体被圈闭在迁移通道或减压扩容带内在热边界层(TBL)通过反应:MeltA=Ol+MeltB冷凝结晶而成,属堆晶橄榄岩。Pb-Sr-Nd同位素地球化学的证据显示,松树沟橄榄岩与基性岩具有共同的地幔源区,二者同为松树沟蛇绿岩的重要组成部分。通过矿床地质特征及铬铁矿电子探针测试研究,认为松树沟铬铁矿床是产于中粗粒堆晶纯橄岩中的层状铬铁矿床,形成于格林威尔期松树沟洋盆的扩张过程中,是中粗粒纯橄岩在热边界层(TBL)的冷凝结晶过程中岩浆分异作用的产物。     

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.     

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。      

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。     

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.