共查询到20条相似文献，搜索用时 78 毫秒
1.
南秦岭旬阳盆地下古生界铅锌成矿作用 总被引：1，自引：0，他引：1
近年来,南秦岭旬阳盆地志留系铅锌矿集区铅锌矿床勘查取得重大突破,备受关注.旬阳盆地下古生界中的铅锌矿床主要赋存于志留系梅子垭组和双河镇组,受地层控制明显,矿体形态简单,主要为层状和似层状,矿石结构简单,矿物成分单一,围岩蚀变弱且不对称;闪锌矿δ34S组成平均为6.83‰,方铅矿δ34S组成平均为5.95‰,黄铁矿矿石δ34S为1.1‰,志留系泥质岩石中黄铁矿的δ34S平均为15.64‰,硫主要来源于海水硫酸盐;208Pb/204Pb为37.93%～38.95%,207Pb/204Pb为15.55%～15.69%,反映铅的来源为上地壳.成矿温度为135～297 o C,属于中低温,成矿流体成分主要以K+、Na+、Ca2+、Mg2+、F-、Cl-、SO2-4为主,Na+/ K+值小于1,F-/ Cl-值很小,主要来自于海水.因此,热水沉积成矿作用是旬阳盆地下古生界铅锌矿床形成的主要原因. 相似文献
2.
青海虎头崖铅锌矿床是祁漫塔格成矿带矽卡岩型多金属矿的典型代表之一,该矿区岩浆活动强烈,具有Fe、Cu、Mo、Pb、Zn等多金属成矿元素组合。本文通过电子探针对该矿床中闪锌矿化学成分标型特征进行了详细研究,探讨其中Fe、Cd等元素的分布状态和富集规律。研究表明,矿床中闪锌矿可分为3个世代,从早到晚闪锌矿颜色由黑色逐渐变为浅黄色,矿物组合由闪锌矿-(方铅矿-黄铜矿)-黄铁矿-磁黄铁矿→闪锌矿-方铅矿-黄铜矿-黄铁矿-(磁黄铁矿) →闪锌矿-方铅矿-方解石或石英。早阶段形成的闪锌矿以富Fe贫Zn和Cd为特征,而晚阶段形成的闪锌矿相对贫Fe,富Zn和Cd。通过闪锌矿中的FeS含量估算获得成矿温度范围为148～262℃。随着成矿阶段的演化,3个世代闪锌矿中FeS含量逐渐降低,表明对应成矿温度的不断降低,分别为262～258、260～200、248～148℃。结合Zn/Cd含量比值变化范围,认为虎头崖铅锌矿床应属于中温热液矿床。在空间分布上,沿着热液流动方向,闪锌矿中Zn含量逐渐增加,Fe含量逐渐减少,Zn/Cd变化范围增大,指示矿床中热液流动方向为由北西西到南东东,由深部到浅部,与矿体走向一致。通过与国内其他不同类型铅锌矿床的对比,发现虎头崖铅锌矿床闪锌矿中Zn、Fe、Mn、Cd等化学成分具有典型中温矽卡岩型矿床中闪锌矿化学成分的特征,明显不同于层控型矿床、喷流沉积型矿床等其他类型矿床闪锌矿。结合该矿床地质特征和成矿作用过程,我们认为虎头崖铅锌矿床为矽卡岩型矿床。 相似文献
3.
昊星铅锌矿床位于黔西北威宁县境内的云炉河坝地区,毗邻川滇黔接壤铅锌矿集区内第二大的毛坪铅锌矿床。该矿床赋存于泥盆系碳酸盐岩中,矿体呈似层状、透镜状及脉状产出,与赋矿地层产状基本一致,受NE向构造控矿明显。硫化物矿石的Pb品位为1. 5%42. 80%,平均2. 89%,Zn品位为1. 5%35. 92%,平均9. 86%。可见,昊星铅锌矿床的成矿特征与会泽、毛坪和天桥等川滇黔铅锌矿集区内的其他典型矿床较相似。昊星铅锌矿床硫化物(黄铁矿、闪锌矿和方铅矿)的δ34SCDT值介于-57. 21‰+3. 93‰,则明显不同于会泽、毛坪和天桥等矿床(5‰%25‰),暗示昊星铅锌矿床的还原硫可能具有不同的来源或形成机制。通过分析认为,该矿床的硫很可能是海相硫酸盐生物还原过程(BSR)的产物,而黄铁矿异常低的δ34S可能是非封闭体系BSR批式分离的结果,即BSR过程形成的还原硫分批随着流体迁移至异地参与成矿。方铅矿的Pb同位素组成显示,昊星铅锌矿床的成矿金属主要由基底岩石提供。因此,本文认为昊星铅锌矿床是流体混合的产物,起源或流经基底岩石的成矿流体与BSR过程形成的还原性流体在异地发生混合,伴生部分TSR和水/岩相互作用过程,赋矿沉积岩中的蒸发岩和金属元素参与到了成矿之中,最终形成昊星铅锌矿床。 相似文献
4.
茂租铅锌矿床主要发育3个矿体(群),主矿体呈层状、似层状。闪锌矿、方铅矿和黄铁矿δ34S值介于+8.84‰～19.86‰,富集重硫,表明硫主要来源于海相硫酸盐热化学还原;Pb同位素组成较均一,投点主要落入基底Pb同位素组成范围内,暗示其来源单一或混合均匀,成矿主要来源于昆阳群和会理群基底岩石。结合区域铅锌矿床地质地球化学特征,川滇黔地区铅锌矿床赋存在不同时代地层中,成矿流体性质颇为相似,推测该区铅锌矿床形成于同一时期,成矿与均一化流体的贯入有关。 相似文献
5.
在详细的野外调研及岩相学研究基础上,通过电子探针分析(EMPA)和电感耦合等离子体质谱分析(ICPMS),系统研究云南会泽铅锌矿不同成矿阶段闪锌矿化学成分特征,探讨Zn、Fe、Cd、Ge、In、Ag的富集规律及其指示意义。研究表明,该矿床的热液成矿作用可划分为4个阶段,依次为细粒黄铁矿阶段、多金属硫化物阶段、黄铁矿-方铅矿阶段和碳酸盐阶段,其中闪锌矿的形成可划分为两个阶段,从早到晚颜色由黑色变为红色。早阶段闪锌矿富Fe,贫Ge、In、Ag、Zn和Cd;晚阶段闪锌矿富Ge、In、Ag、Zn和Cd,相对贫Fe。闪锌矿中Cd、Ge等有用组分均已达到工业综合利用要求,主要替代Fe进入闪锌矿晶格。闪锌矿中Fe S含量从早到晚呈降低趋势,估算早期成矿温度为170~262℃,晚期成矿温度低于203℃,结合Zn/Cd含量比值变化范围,认为该矿床属于中温热液矿床,其成矿温度由早至晚逐渐降低。空间上,Zn、Fe含量及Zn/Cd值均指示矿床形成时热液由深部向浅部流动。将该矿床闪锌矿中In、Cd、Ga、Ge、Zn/Cd、Ga/In、Ge/In等特征元素及其比值与典型铅锌矿进行对比,显示会泽铅锌矿与MVT型铅锌矿床类似。 相似文献
6.
闽中梅仙丁家山铅锌矿床硫化物微量元素地球化学特征及其成矿意义 总被引：1，自引：1，他引：0
梅仙丁家山铅锌矿床是闽中新元古代马面山群中多个大中型铅锌多金属矿床的典型代表.本文以丁家山铅锌矿床两类矿石(含磁黄铁矿矿石和含磁铁矿矿石)内的闪锌矿和黄铁矿为研究对象,通过电子探针及LA-ICP-MS微量元素分析技术,揭示二者的微量元素组成和赋存状态,探讨成矿温度及矿床成因方面的重要信息.分析结果显示:闪锌矿内Fe、Mn、Cd、Cu、In、Pb、Bi元素较为富集,两类矿石内的闪锌矿除Fe元素含量相差较大以外(平均值分别为9.3％和1.7％),其他元素含量并无明显差异;电子探针面扫描和LA-ICP-MS剥蚀图像显示元素Mn、Cd、In以类质同象形式存在,而Fe、Cu、Pb、Bi则有类质同象和显微包体2种存在形式.黄铁矿微量元素含量整体较低,元素Co、Ni、Pb、Bi相对富集,Ni、Mn主要以类质同象形式存在,Cu、Co有类质同象替换和显微包体2种形式,Pb、Bi主要以方铅矿包体形式存在.两类矿石中的闪锌矿Zn/Cd比值分别在120～150之间和93～210之间,均指示中温成矿条件.两类闪锌矿内Fe、Cd、Mn元素含量特征与典型矽卡岩型矿床内的闪锌矿相吻合;矿床内硫化物硫同位素组成揭示成矿物质来自于岩浆岩.上述证据共同支持梅仙丁家山铅锌矿矿床属矽卡岩型矿床. 相似文献
7.
贵州普定纳雍枝铅锌矿矿床成因:S和原位Pb同位素证据 总被引：12，自引：5，他引：7
通过近五年(2011~2015)勘查实现找矿重大突破的贵州普定纳雍枝铅锌矿床,位于扬子陆块西南缘,五指山背斜南东翼北中部,是黔西北铅锌成矿区的重要组成部分。矿区内已发现20余个铅锌矿体,探获铅锌金属资源储量超135万吨,是川滇黔接壤铅锌矿集区贵州境内目前已发现和探明规模最大的铅锌矿床。主矿体多呈层状、似层状、透镜状和陡倾斜脉状产出,除了陡倾斜脉状矿体产于F7断层破碎带,其余(似)层状矿体均产于下寒武统清虚洞组和上震旦统灯影组白云岩中,与围岩产状一致,层控特征明显。其矿石类型主要有块状、角砾状、细脉状和浸染状等,矿石矿物以闪锌矿为主,其次为方铅矿和黄铁矿,脉石矿物以方解石、白云石为主,含少量石英,偶见重晶石。本次研究表明,该矿床硫化物δ~(34)S_(CDT)值介于15.94‰~25.49‰之间,均值为22.41‰(n=21),其中黄铁矿δ~(34)S_(CDT)值为22.06‰,闪锌矿δ~(34)S_(CDT)值为19.37‰~25.49‰,均值为23.17‰(n=17),方铅矿δ~(34)S_(CDT)值为15.94‰~19.70‰(n=3),均值为18.23‰。各类硫化物δ~(34)S值部分重叠,总体上不具有δ~(34)S黄铁矿δ~(34)S闪锌矿δ~(34)S方铅矿的特征,暗示硫同位素在硫化物矿物间的分馏未达到平衡。此外,矿石存有少量硫酸盐矿物(重晶石),暗示成矿流体的δ~(34)S3∑S值应高于硫化物的平均δ4S值(22.41‰),接近赋矿地层中海相硫酸盐岩的δ~(34)S值(22‰~28‰)。因此,成矿流体中的还原硫最可能为海相硫酸盐岩热化学还原的产物,来源于赋矿地层中的蒸发岩。应用飞秒激光剥蚀多接收器等离子体质谱法首次获得了纳雍枝铅锌矿中方铅矿原位Pb同位素数据,结果显示Pb同位素组成非常集中(~(206)Pb/204Pb=17.828~17.860,均值17.841,~(207)Pb/204Pb=15.648~15.666,均值15.659,~(208)Pb/204Pb=37.922~37.979,均值37.960,n=32),位于上地壳平均Pb演化曲线上,表明其成矿物质具壳源特征,可能来源于基底岩石。综合矿床地质、矿物学、S和原位Pb同位素数据,本文认为纳雍枝铅锌矿床S主要来源于其赋矿地层,Pb等金属元素主要来源于基底岩石,这两组流体的混合是导致其金属硫化物沉淀成矿的重要机制,成矿流体具后生、低温热液等特征,属于密西西比河谷型(MVT)矿床,很可能形成于燕山期,与右江盆地演化有关。 相似文献
8.
对新疆霍什布拉克铅锌矿床硫化物硫、铅同位素测定,获得成矿早期黄铁矿的δ34S值为-12.1‰～-8.5‰,闪锌矿的δ34S值为-17.6‰,方铅矿的δ34S值为-18.8‰;晚期黄铁矿的δ34S值为+12.8‰～+22.2‰,闪锌矿的δ34S值为+20.0‰～+24.2‰,方铅矿的δ34S值为+14.4‰+22.2‰.成矿从早到晚,硫同位素由大的负值变化到大的正值,方铅矿的206 Pb/204 Pb比值为17.900-18.086,207Pb/204Pb比值为15.586-15.732,208Pb/204Pb比值为37.997-38.381;黄铁矿的206Pb/204Pb比值为17.950,207 pb/204Pb比值为15.633,208 pb/204 Pb比值为38.144.灰岩的206pb/204 Pb比值为18.156-18.875,207Pb/204Pb比值为15.396-15.855,208Pb/204Pb比值为37.631-38.967.硫同位素指示硫来源于海水硫酸盐还原硫.铅同位素指示至少有两上以上来源. 相似文献
9.
10.
《矿产与地质》2017,(2)
马元铅锌矿床位于扬子板块北缘碑坝穹窿构造的南缘,是区域上重要的碳酸岩型铅锌矿,矿体赋存于震旦系灯影组白云岩中。通过对马元铅锌矿床中矿石矿物闪锌矿、方铅矿和黄铁矿的硫、铅同位素系统研究,探讨其成矿物质来源。研究表明:马元铅锌矿床中矿石矿物的δ~(34)S值为15.4‰~19.6‰,平均为17.67‰,重晶石的δ~(34)S值为33.2%~33.5%,平均为33.3%,显示S主要形成于海相硫酸盐的热化学还原作用;矿石矿物的~(206)Pb/~(204)Pb值、~(207)Pb/~(204)Pb值和~(208)Pb/~(204)Pb值分别为17.62%~18.02%、15.49%~15.65%和37.57%~38.35%,组成较为均一,Pb主要来自于壳幔混合的造山带,基底岩系可能是马元铅锌矿床成矿物质的重要来源。 相似文献
11.
东濮凹陷北部沙三中亚段广泛发育盐岩和烃源岩,这两个看似不能共存的物质却在这里互层共生。该时期研究区沉积特征为多盐韵律与多层烃源岩互层共生、连续沉积,单个盐韵律厚度从几米到十几米,烃源岩有机质丰度高、类型好。平面上,两者在湖盆沉积沉降中心共生;垂向上,高有机质丰度、好干酪根类型与高盐度地层具有较好的对应关系。因而成为恢复古气候和古环境的重要研究对象。通过岩石学、古生物学以及Sr/Ba、B/Ga、(V+Ni+Mn)、Fe/Mn、Sr/Cu、Mg/Ca、V/(V+Ni)、稀土元素含量和氯同位素等方法对凹陷北部沙三中亚段的沉积环境进行研究。结果表明,凹陷北部沙三中亚段为深水沉积的还原环境,古盐度较高,达到半咸水-咸水沉积;微量元素和孢粉化石特征表明研究区沙三中亚段为温暖潮湿的环境。 相似文献
12.
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
13.
郯庐断裂南段研究进展与断裂性质讨论 总被引：13，自引：3，他引：13
据1：5万区域地质调查和专题研究资料，就郯庐断裂带是否南延与消失的原因，其与大别—苏鲁造山带交截形成的假位错效应，以及与中新生代沉积盆地形成演化的关系等作了新的阐述。在此基础上，讨论了郯庐断裂带是否为巨大的左行平移断层或转换断层。认为郯庐断裂带可能是在“古郯庐带”的基础上于早侏罗世重新活动、白垩纪强烈活动的地堑型枢纽断裂带。 相似文献
14.
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
15.
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
16.
17.
Jiayu Rong Michael Melchin S. Henry Williams Tatyana N. Koren Jacques Verniers 《《幕》》2008,31(3):315-318
The Global Stratotype Section and Point （GSSP） for the base of the Silurian System was defined in 1985. Since that time, a number of researchers have suggested that this section has serious deficiencies for use as a GSSP. As a result, in 2000, the Subcommission on Silurian Stratigraphy （SSS） proposed undertaking a formal restu@ of this GSSP, which was subsequently approved by the International Commission of Stratigraphy （ICS）. The result of this restudy was the formal proposal that the current GSSP, at 1.6 m above the base of the Birkhill Shale, at Dob＇s Linn, Scotland, should be maintained as the same locality and stratigraphic level, but the bios- tratigraphical definition of the boundary should be revised. The previously defined, basal Silurian grapto- lite zone, the Parakidograptus acuminatus Zone, should be subdivided into a lower Akidograptus ascensus Zone and a higher E acuminatus Zone. The base of the A. ascensus Zone, marked by the first appearance of A. ascensus, should be regarded as the biostratigraphic mark for the base of the Silurian. This proposal has now been formally approved by the SSS and ICS, and ratified by International Union of Geological Sciences. This is the first GSSP to undergo formal restudy and redefini- tion, and the proposal also included a recommended procedure for restudy of GSSPs. 相似文献
18.
Dean S. Oliver 《Mathematical Geology》1998,30(7):911-933
In reservoir characterization, the covariance is often used to describe the spatial correlation and variation in rock properties or the uncertainty in rock properties. The inverse of the covariance, on the other hand, is seldom discussed in geostatistics. In this paper, I show that the inverse is required for simulation and estimation of Gaussian random fields, and that it can be identified with the differential operator in regularized inverse theory. Unfortunately, because the covariance matrix for parameters in reservoir models can be extremely large, calculation of the inverse can be a problem. In this paper, I discuss four methods of calculating the inverse of the covariance, two of which are analytical, and two of which are purely numerical. By taking advantage of the assumed stationarity of the covariance, none of the methods require inversion of the full covariance matrix. 相似文献
19.
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
20.
正Artemia cysts are an extremely important component of aquaculture diets.It is well established that the cultivation of fish and shellfish derive substantial health and growth advantages when Artemia are included in the diets of the 相似文献