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1.
陕西沉积型磷矿主要分布在华北陆块西南缘、秦祁昆造山系南缘及华南陆块北缘,赋矿地层主要为震旦系、寒武系。通过总结省内景福山式、胡家沟式、天台山式等5个类型磷矿成矿时代、含磷岩系地层、岩石组合、矿石类型的成矿地质特征,划分了沉积型磷矿成矿远景区,分析了找矿潜力,对寻找新的磷矿产地应具有一定的指导意义。  相似文献   

2.
中南地区锡、锰、铅锌、金、稀土等资源找矿潜力大,成矿条件有利,中国地质调查局组织实施了扬子陆块及周缘地质矿产调查工程和七个二级项目,全力支撑找矿突破战略行动锰、锡等重点矿种勘查目标的实现。扬子工程近两年来新发现大量矿化点,圈定了一批找矿靶区,总结了区域成矿规律,在扬子古陆核及其东南缘、北缘、华夏陆块群等构造演化等成矿地质背景研究取得较多进展,一批地质调查项目圈定的有利找矿靶区转入矿产勘查。依据国土资源部及地质调查局的工作部署,本文提出下一阶段工作的初步规划,继续在成矿区带开展1∶5万地质矿产调查和科技创新工作,聚焦华南陆块聚散过程中的资源效应和资源潜力评价,助力华南大宗矿种与战略性新兴矿种资源新格局和重要矿产资源基地建设。  相似文献   

3.
大巴山地区水系沉积物地球化学特征及找矿方向   总被引:2,自引:1,他引:1       下载免费PDF全文
大巴山地区跨秦岭、扬子两个一级构造单元,基于1:5万水系沉积物测量成果,统计计算了成矿元素地球化学参数,分析研究了元素分布特征、元素相关性及异常元素组合特征,认为研究区Pb、Zn、Ba、Cu、Mn找矿潜力较大,推断研究区所在的秦岭构造单元成矿类型主要为与震旦系—下寒武统黑色岩系有关的低温热液锌铜矿和沉积型钡矿;研究区所在的扬子构造单元成矿类型主要为与寒武系碳酸盐地层有关的低温热液铅锌矿和与震旦系碳酸盐岩有关的沉积型锰矿;在此基础上,划分出杨家坪—葛洞钡锌成矿远景区、镇坪钡锌成矿远景区、黄安坝—迷魂阵锌铜成矿远景区、百羊坪铅锌成矿远景区和修齐镇—石坊乡锰成矿远景区。  相似文献   

4.
吴波 《地质与勘探》2013,49(2):250-256
利用2009年贵州省矿产资源利用现状调查磷矿成果数据库,以核查块段为基础,通过块段品位和块段资源储量数据对全省磷矿核查矿区平均品位统计,掌握了全省核查矿区高中低品位磷矿石的分布,并对块段品位数据区间分段统计吨位频率,建立了寒武系磷矿层和震旦系磷矿层品位-吨位模型。统计结果表明,寒武系磷矿层的矿区平均品位总体较低,震旦系磷矿层矿区平均品位总体较高,全省磷矿吨位频率服从正态分布,寒武系磷矿层吨位峰值区间较窄,震旦系磷矿层吨位峰值区间较宽。综合研究表明,开阳-息烽片区和瓮安-福泉片区震旦系磷矿层高品位矿石资源储量多,矿石质量好,可作为全省磷矿资源开发利用布局的重点地区,铜仁-松桃片区和清镇-织金片区寒武系磷矿层品位低、贫矿石资源储量多,矿石质量差,应加强低品位矿石和贫矿石的选矿技术研究。  相似文献   

5.
安徽省东至地区金矿类型及找矿方向   总被引:4,自引:0,他引:4  
安徽省东至地区位于扬子陆块北缘,跨下扬子前陆带和江南隆起带两个次级构造单元,独特的大地构造环境造就了本区有利的金矿成矿地质条件,形成多种类型的金矿床,其成因类型主要包括岩浆热液型和风化壳型,工业类型主要有破碎带蚀变岩型、含金石英脉型、微细粒浸染型及红土型。各类型金矿分类聚集,形成两个主要的金矿成矿带。沿赵家岭断层带以破碎带蚀变岩型为主,伴有含金石英脉型,中畈—戴家一带,赵家岭—杨家山一带均具较大找矿潜力,是本区金矿勘查重点地区,九华庄等地也具一定的找矿潜力;沿高坦断裂以微细粒浸染型为主,伴有破碎带蚀变岩型及红土型,查册桥地区是其重点勘查区,铜锣尖、小河等地找矿潜力也较大。  相似文献   

6.
四川汉源地区磷矿成矿类型均属浅海相沉积型,烂泥三湾磷矿位于大洪山短轴向斜西翼,严格受寒武系下统梅树村组地层控制,通过对汉源地区磷矿矿床成因分析,总结了成矿规律和找矿标志,初步划分了找矿远景区和找矿靶区,对该区磷矿资源勘查具有重要的指导意义。  相似文献   

7.
通过本次对雷波县莫红磷矿区以往地质资料的收集、整理分析研究,初步掌握了其形成机理及磷质富集成矿规律。我国磷矿主要集中于中一上扬子陆块湖北、云南、贵州、四川和湖南5省,震旦纪一寒武纪是海相沉积磷块岩矿床的主要成矿时期。四川马边一雷波地区的磷矿床赋存于寒武系下统麦地坪组,早寒武世梅树村期是其重要成磷期。查明其成磷期,含磷层位,可为进一步开展磷资源的普查找矿起到积极推动作用。  相似文献   

8.
四川省昆阳式磷矿位于上扬子台拗峨眉山断拱和凉山陷褶束,属川滇早寒武世成磷带北段,磷矿赋存于下寒武统麦地坪组(€1 m)的中下部,层状延伸,其产状与含磷层一致,层位稳定,分布广,资源储量规模大,具有巨大的找矿潜力.在收集、整理前人研究资料和勘查项目成果的基础上,通过总结矿床地质特征及其矿床分布规律,分析成矿古构造、古地理...  相似文献   

9.
在中朝准地台、塔里木准地台边缘深断裂附近和台中隆起带以及天山-兴安、祁连-秦岭、额尔古纳几个地槽褶皱区的中间地带,不同程度地具备中国北方三种主要类型磷矿的成矿条件。研究分析认为中国北方的内生磷矿具有良好的找矿前景,绿岩带型磷矿和古元古代沉积变质磷矿显示一定的找矿潜力,沉积型磷矿一般品位低、规模小。通过归纳,在中国北方划分出磷矿的二级城矿区4个、三级成矿带15个、四级成矿亚带19个。圈定成矿预测区A级2个,B级C级各23个。确定了21处可开展进一步工作的地区。  相似文献   

10.
张英利  贾晓彤 《地质学报》2024,98(2):363-380
扬子陆块西缘寒武系主要为一套碎屑岩- 碳酸盐岩的岩石组合,前人研究多认为形成于相对稳定的克拉通盆地。但同时期出现的大陆岩浆作用显然与前期认定的克拉通盆地性质不符,需要借助扬子西缘的物质来源探讨构造背景。基于野外露头等资料,本文通过对扬子陆块西缘会泽和会东附近寒武系3件砂岩样品进行重矿物分析、电气石电子探针和碎屑锆石U- Pb测年分析,确定扬子西缘寒武纪沉积物的源区;并结合沉积序列等综合探讨扬子陆块西缘寒武纪的构造背景。沉积序列表明,扬子西缘寒武系沧浪铺组、西王庙组和二道水组主要由砂岩和白云岩等组成,沉积环境为滨岸—潮坪。细—粗砂岩碎屑颗粒为次棱角状—次圆状,分选较差;碎屑组分主要为石英,岩屑几乎全部为燧石,长石含量较少。测试分析结果表明:重矿物分析指示扬子西缘寒武系砂岩重矿物主要由锆石、赤—褐铁矿、电气石、钛铁矿、金红石、磷灰石等组成,重矿物组合指示岩浆岩为其主要母岩;电气石电子探针分析结果表明,物源主要来自于贫锂花岗岩和变砂岩、变泥岩;碎屑锆石测年分析表明物源区母岩主要为983~540 Ma岩浆岩。碎屑锆石年龄对比等综合分析表明,寒武系沉积物部分源自康滇古陆983~708 Ma的岩浆岩和变沉积岩,部分源自冈瓦纳大陆东非造山带663~540 Ma的岩石,物源区岩石经历再旋回产物作用。扬子西缘寒武系的沉积序列、碎屑锆石年龄谱图和碎屑组成等特征综合分析表明,扬子陆块西缘寒武系形成于前陆盆地。  相似文献   

11.
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.
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   

14.
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   

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  
陈银生 《世界地质》1999,18(1):54-59
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.
从榴辉岩与围岩的关系论苏鲁榴辉岩的形成与折返   总被引:4,自引:1,他引:4       下载免费PDF全文
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.
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   

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