共查询到20条相似文献，搜索用时 328 毫秒
1.
河南省新县姚冲钼矿床流体包裹体研究 总被引：1，自引：1，他引：0
河南省新县姚冲钼矿床产于大别造山带,属于陆-陆碰撞体制的斑岩型矿床,其流体成矿过程可以分为早、中、晚三个阶段,分别以石英+钾长石±黄铁矿±磁铁矿、石英±钾长石+辉钼矿±其他硫化物和石英±碳酸盐±萤石组合为标志.热液石英和萤石中发育纯CO2包裹体(PC型)、CO2-H2O型包裹体(C型)、水溶液包裹体(W型)和含子晶多相包裹体(S型).早阶段石英中发育纯CO2包裹体、CO2-H2O型包裹体和含子晶多相包裹体,中阶段的石英则发育CO2-H2O型包裹体、水溶液包裹体和含子晶多相包裹体,在晚阶段的无矿石英脉中发育水溶液包裹体和少量的CO2-H2O型包裹体,石英-碳酸盐-(萤石)脉石英与萤石中只发育水溶液包裹体.早阶段流体包裹体的均一温度为277～ 380℃,集中于300～ 360℃,盐度变化于3.0％～10.3％ NaCleqv之间.中阶段包裹体均一温度介于185 ～ 351℃之间,集中在260～ 320℃,盐度介于2.4％ ～9.3％NaCleqv;晚阶段包裹体均一温度为139 ～245℃,盐度介于0.7％ ～6.3％ NaCleqv之间.中阶段多相包裹体中常见黄铜矿和其他透明子矿物,表明流体具有还原性、过饱和的特征,是矿石矿物沉淀的主要阶段.估算早、中阶段流体捕获压力分别集中于47 ～ 131MPa和26 ～118MPa,所对应的成矿深度分别约为4.7km和2.6～4.2km.上述流体包裹体的研究表明姚冲钼矿床的初始成矿流体具有高温、高盐度、富CO2的特征,同时预测了深部找矿潜能. 相似文献
2.
新疆东天山白山钼矿床流体包裹体研究 总被引：5，自引：3，他引：2
白山钼矿位于东天山觉罗塔格成矿带东段,是新疆极具代表性的大型-超大型斑岩钼矿.根据矿物共生组合和脉体穿插关系,脉体发育顺序依次为:早期石英-钾长石脉、石英-钾长石-辉钼矿脉、石英-辉钼矿脉、石英-多金属硫化物脉和晚期石英-碳酸盐-萤石脉.早期石英-钾长石脉中主要发育纯CH4包裹体(PC型)、CH4-H2O型包裹体(C1型)和水溶液包裹体(W型),均一温度集中在320 ～420℃,盐度为1.98％ ～ 8.79％ NaCleqv;石英-钾长石-辉钼矿脉中发育含子晶包裹体(S型)和W型包裹体,均一温度集中在260～ 400℃,盐度为1.49％～8.65％ NaCleqv;石英-辉钼矿脉和石英-多金属硫化物脉发育W型、S型和CO2-H2O型包裹体(C2型),均一温度分别为200～ 240℃和140 ～ 240℃,盐度分别为2.14％ ～8.10％ NaCleqv和0.33％～ 10.22％ NaCleqv,不包括不熔子矿物的贡献;晚期石英-碳酸盐-萤石脉只发育W型包裹体,均一温度和盐度明显下降,分别为100～ 160℃和0.17％～4.86％ NaCleqv.估算的石英-钾长石脉体和石英-多金属硫化物脉形成压力分别为105 ～ 221 MPa和15 ～ 285MPa.成矿流体由高温、富碳质、还原的岩浆流体向低温、低盐度、贫碳质的大气降水热液演化.成矿阶段温度下降,早期流体中的CH4还原HMoO4-的高价钼,从而形成辉钼矿,可能是导致成矿物质沉淀的重要因素. 相似文献
3.
岔路口超大型斑岩钼矿床位于大兴安岭北部,是目前中国东北地区最大的钼矿床,矿体赋存于中酸性杂岩体及侏罗系火山-沉积岩内,其中花岗斑岩、石英斑岩、细粒花岗岩与钼矿化关系密切.流体包裹体研究表明,岔路口矿床主要发育富液两相包裹体、富气两相包裹体和含子矿物多相包裹体.花岗斑岩石英斑晶中流体包裹体的形成温度集中在230 ～ 440℃和470～510℃两个温度区间,盐度分别介于0.7％ ～ 53.7％ NaCl eqv和6.2％～61.3％ NaCl eqv两个区间;成矿早阶段钾长石-石英-磁铁矿脉中流体包裹体的形成温度集中在320～440℃、盐度介于4.2％ ～ 52.3％NaCl eqv;成矿中阶段石英-辉钼矿脉和角砾岩中流体包裹体的形成温度集中在260～410℃、盐度介于0.4％～52.3％ NaCleqv;成矿晚阶段石英-萤石-方铅矿-闪锌矿脉中流体包裹体的形成温度集中在170～320℃、盐度介于0.5％ ～ 11.1％ NaCleqv.成矿流体具高温、高盐度及高氧逸度的特征,总体上属于富F的H2O-NaCl±CO2体系.成矿流体的δ 18Ow值为-4.5‰～3.2‰,δDw值为-138‰～-122‰,表明成矿流体为岩浆水与雨水的混合流体.金属硫化物的δ34S值介于-1.9‰～+3.6‰,均值为+1.6‰,表明成矿物质主要来自深源岩浆.多期次的流体沸腾作用是该矿床的主要成矿机制. 相似文献
4.
比利亚谷矿床是内蒙古额尔古纳成矿带内新发现的一个铅锌（银）矿床,具有大型矿床的成矿潜力。主矿体呈脉状产于上侏罗统塔木兰沟组和满克头鄂博组火山岩地层中,受NW,NWW向张性断裂构造控制;主要金属矿物有方铅矿、闪锌矿、黄铁矿、黄铜矿、辉银矿等。为确定该矿床的成矿流体特征及成因类型,对矿石中的石英、重晶石和闪锌矿开展了流体包裹体的岩相学观察、显微测温和激光拉曼光谱分析。结果表明,上述矿物中主要发育富液相、CO2三相和少量含子矿物三相包裹体;富液相包裹体的均一温度与盐度分别为102℃～378℃和0．2％～10．5％NaCleqv,CO2三相包裹体的均一温度和盐度分别为124℃～256℃和1．8～11．2％NaCleqv,舍子矿物三相包裹体的均一温度与盐度分别为220℃和42．4％NaCleqv。单个流体包裹体气相成分的激光拉曼光谱分析显示,除石英中的部分富液相包裹体的气体成分含CO2外,不同矿物中的富液相包裹体的气体成分均为H2O。此外,该矿床成矿流体的盐度范围波动较大,重晶石中包裹体的均一温度分布范围较广,因此成矿流体属不均匀流体,流体混合作用是该矿床的重要成矿机制。综合认为,比利亚谷铅锌（银）矿床应属赋存于中生代火山岩中的与浅成一超浅成岩浆作用有关的中低温热液脉型矿床。 相似文献
5.
浙江八面山萤石矿床流体包裹体地球化学研究 总被引：2，自引：1，他引：1
八面山萤石矿床流体包裹体可分为三大类型:Ⅰ气液包裹体,Ⅱ气体包裹体,Ⅲ含子矿物的多相包裹体;矿床成矿温度变化不大,主要集中在120～240°C之间。细粒条带状萤石矿石包裹体温度变化在115～250℃之间;巨晶块状萤石矿石和石英脉型萤石矿石包裹体温度集中在135～170℃之间。萤石矿床流体包裹体以低盐度成矿流体为主。成矿过程中起作用的成矿流体为KCl-H2O体系和CO2-CaF2-H2O体系,成矿溶液的离子类型属K+-Ca2+-HCO--F-型,KCl-H2O体系反映岩浆期后热液作用的结果,而CO2-CaF2-H2O体系可能反映了寒武纪矿源层成矿体系。通过包裹体研究,认为八面山萤石矿床是受地层-岩体-层间断裂共同控制"三位一体"的热液成因矿床。 相似文献
6.
安徽庐枞盆地泥河铁矿床成矿流体特征及其对矿床成因的指示 总被引：13，自引：10，他引：3
庐枞盆地位于长江中下游断陷带内,地处扬子板块北缘,是长江中下游成矿带中重要的铁铜多金属成矿区.庐枞盆地西北部勘探新发现的大型泥河铁硫硬石膏矿床,矿床中硬石膏在不同蚀变-矿化阶段均广泛发育,具有鲜明的成矿特色,是玢岩型铁矿床成矿流体研究的理想对象.本次工作在详细野外地质和室内研究基础上,对矿床不同成矿阶段硬石膏等脉石矿物中流体包裹体开展较系统的包裹体岩相学、显微测温学和拉曼光谱学研究.鉴定出矿床中的包裹体类型有Ⅰa型原生包裹体(L+G),Ⅰb型次生包裹体(L+G)和Ⅱ型包裹体(L),均属盐水体系.拉曼探针分析结果显示包裹体的主要成分为盐水溶液,气相成分含有微量的CO2、N2和CH4.各成矿阶段矿物中包裹体测温工作表明,硬石膏-辉石-磁铁矿阶段、硬石膏-黄铁矿-磁铁矿阶段、高岭石-硬石膏-石英-黄铁矿阶段和重晶石-方解石-硬石膏阶段成矿流体温度的峰值分别为460.0～ 380.0℃、350.0～ 270.0℃、250.0～190.0℃和190.0～150.0℃,成矿流体盐度的平均值分别为14.11％ NaCleqv,10.73％NaCleqv,4.03％ NaCleqv和3.26％ NaCleqv,成矿流体经历了从中高温中等盐度流体向中低温低盐度流体的演化过程.在此基础上初步分析了矿床成矿流体系统的演化过程和成矿机理,建立了泥河矿床的成矿模式. 相似文献
7.
小秦岭文峪金矿床流体包裹体研究及矿床成因 总被引：5，自引：2，他引：3
文峪金矿位于小秦岭矿田南部,其产出受脆-韧性剪切带控制,赋矿围岩为太华群变质杂岩.根据脉体穿切关系和矿物交代关系,可以将文峪金矿流体成矿过程分为早、中、晚三个阶段,其热液石英中发育CO2-H2O型、纯CO2型和H2O溶液型三种类型流体包裹体.平阶段石英中原生包裹体主要是CO2-H2O型和纯CO2型,其成分为CO2+H2O±N2±CH4,均一温度集中在290～330℃,盐度为1.02％～9.59％ NaCleqv;中阶段为主成矿阶段,该阶段石英中包含了所有3种类型的包裹体,其中以CO2-H2O型包裹体为主,获得CO2-H2O和水溶液包裹体均一温度集中在250～290℃,盐度为0.02％～12.81％NaCleqv;晚阶段石英仅发育水溶液型包裹体,具有较低的均一温度(114～239℃)和盐度(4.18％～8.95％ NaCleqv).根据CO2-H2O型包裹体计算早、中阶段压力分别为130 ～ 178MPa和85 ～ 150MPa,对应的成矿深度分别为4.7～6.5km和3.1～5.5km.总体而言,文峪金矿的初始流体具有中高温、富CO2、低盐度的变质流体特征,晚成矿阶段流体演化为低温、低盐度水溶液流体,流体的不混溶导致了主成矿期矿质的大量沉淀,文峪金矿为中浅成的造山型矿床. 相似文献
8.
河南王坪西沟铅锌矿床流体包裹体特征和矿床成因类型 总被引：9，自引：6，他引：3
王坪西沟铅锌矿床隶属于东秦岭外方山钼铅锌多金属成矿区,位于车村-鲁山断裂北侧。矿床赋存于中元古代熊耳群鸡蛋坪组火山岩系中,受断裂控制,呈脉状产出;矿石主要由金属硫化物,少量石英和碳酸盐组成;成矿过程分为早、中、晚三个阶段,分别以石英-黄铁矿组合、金属硫化物和碳酸盐为标志。流体包裹体研究表明,成矿流体为CO2-H2O-NaCl±CaCl,体系,石英或闪锌矿中可见CO2-H2O型、含子晶型和水溶液型三类包裹体,CO2-H2O型包裹体集中在早阶段产出。早、中、晚阶段流体包裹体均一温度分别为280～386℃、180～350℃和120-230℃,从早到晚逐渐降低;盐度分别集中在3％～7％NaCl eqv．、3．55％～17．43％NaCl eqv．和3．06％-13．51％NaCleqv．。含子晶型流体包裹体主要出现在中阶段,子晶为方解石,该阶段为成矿主要阶段,可见CO2-H2O型包裹体与富液相水溶液包裹体共存,均一温度相近,指示流体沸腾,发生CO2的逃逸,成矿物质快速沉淀。总之,王坪西沟铅锌矿床地质特征与造山型矿床一致,成矿机理可由碰撞成岩成矿与流体作用（CMF）模式所解释。 相似文献
9.
内蒙古林西县水头大型萤石矿床位于索伦-林西缝合带北侧,产于二叠系火山沉积岩中,矿体主要受NNE向断裂破碎带控制。文中从流体包裹体和H O S同位素研究出发,讨论了该矿床成矿流体的特征、演化与成矿过程。萤石中主要发育液相H2O包裹体,包裹体均一温度集中在140~220 ℃,盐度变化于0.4%~2.8% NaCleqv,密度平均为0.87 g/cm3。包裹体成分以H2O为主,其次为CO2、H2,含有CH4、C2H6和C3H6等有机组分。成矿流体属中低温、低盐度、中低密度的NaCl H2O体系。成矿流体的δDH2O SMOW值为-140.1‰~-120.5‰,δ18OH2O SMOW值为-6.7‰~2.3‰,主体属大气降水热液;矿石中黄铁矿的δ34S值为1.2‰~3‰,指示硫的来源可能与岩浆活动有间接联系。综上推断,成矿热液主要来源于被加热的大气降水和地下水,水岩反应很可能是萤石沉淀的主要机制,矿床属断裂控矿、中低温热液裂隙充填型萤石矿床。 相似文献
10.
河南省栾川南泥湖斑岩型钼钨矿床流体包裹体研究 总被引：20，自引：11，他引：9
河南省栾川县南泥湖超大型钼钨矿床形成于秦岭造山带的燕山期大陆碰撞体制,流体成矿过程包括早、中、晚3个阶段,分别以石英+钾长石±辉钼矿±黄铁矿、石英+多金属硫化物±碳酸盐和石英+碳酸盐+萤石组合为标志,矿石矿物主要沉淀于中阶段.早、中阶段石英中可见纯CO_2包裹体、CO_2-H_2O型包裹体、水溶液包裹体和含子晶多相包裹体,但晚阶段萤石中只发育水溶液包裹体.早阶段流体包裹体均一温度集中于350～460℃,盐度为5.68 wt%～17.87 wt% NaCl.eqv.中阶段包裹体均一温度集中在250～380℃,盐度为3.00 wt%～38.16 wt% NaCl.eqv;中阶段多相包裹体中常见石盐、黄铜矿和未知种类的子矿物,指示流体具有沸腾所致的还原性、过饱和特征;盐度相差悬殊的含子晶多相包裹体、富气相水溶液包裹体和富液相水溶液包裹体共存,在相近温度下异相均一,表明流体沸腾的存在.晚阶段流体包裹体均一温度集中在115～265℃,盐度介于0.53 wt%～1.23 wt%NaCl.eqv之间.估算早、中阶段流体捕获压力分别为70～300MPa和30～150MPa,推测成矿深度约为3km.总之,成矿流体具高温、高盐度、高氧逸度、富CO_2的特征;流体沸腾导致CO_2逃逸,氧化性降低,成矿物质沉淀. 相似文献
11.
Guboglo M. N. 《GeoJournal》1980,4(1):53-58
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. 相似文献
12.
13.
Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth
B. P. Kondratyev 《Astronomy Reports》2017,61(8):709-714
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″. 相似文献
14.
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. 相似文献
15.
16.
摩擦桩基桩土间极限摩阻力取值问题探讨 总被引：1，自引：0，他引：1
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。 相似文献
17.
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。 相似文献
18.
某高速公路下伏煤矿采空区稳定性分析 总被引：10，自引：0，他引：10
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。 相似文献
19.
The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads 总被引：3，自引：1，他引：2
Clemente Irigaray Francisco Lamas Rachid El Hamdouni Tomás Fernández José Chacón 《Natural Hazards》2000,21(1):65-81
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. 相似文献
20.
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. 相似文献