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1.
矿集区找矿预测有着不同于典型矿床和区域性成矿预测的规律和特点,是在厘定区内主要类型矿床的成因类型基础上,以"三位一体"(即成矿地质作用与成矿地质体、成矿构造与成矿结构面、成矿作用特征标志)和成矿系统为主要内容开展工作。文章以辽宁青城子铅锌-金-银矿集区为例,系统总结了矿集区的矿床类型、岩浆-成矿系统、"三位一体"找矿预测要素等关键科学问题。青城子矿集区是中国重要的铅锌-金-银矿集区,由于多年的开采,青城子等矿山濒临危机,如何取得该地区找矿突破,是一个亟待解决的问题。对前人研究成果分析表明,该矿集区内铅锌矿床和金、银矿床的成因类型可能均属于岩浆热液型,而非元古代喷流沉积型,矿床的"层控"现象实为特定岩性界面控制的有利成矿结构面;成矿作用主要与印支期花岗斑岩有关,铅锌矿和金、银矿可能是同一岩浆系统演化的产物。在未来的找矿预测中,应重点开展以下5方面工作:(1)查明矿床的具体成矿地质体;(2)进一步提炼成矿期构造控矿规律和成矿结构面样式;(3)凝练有效的成矿作用特征标志,重点是与成矿有关的远程蚀变标志;(4)构建和完善矿集区中生代岩浆-成矿系统,并注意新矿种、新矿床类型的寻找;(5)探索研究矿集区的自然边界,扩大找矿范围和深度。  相似文献   

2.
漓渚铁多金属矿床处于钦杭构造带北东端北西侧,是一个典型的矽卡岩型Fe-Mo-Cu-Pb-Zn多金属矿床。在其形成的不同蚀变交代作用过程中,由于热流体的物理化学条件的改变,而形成一系列不同的蚀变矿物,这些蚀变矿物具有能反映其形成的地质环境的特征。其中能够直接指示矿体赋存位置的,对找矿预测具有特殊意义的标志为成矿作用特征标志,与成矿地质体、成矿构造与成矿结构面三者紧密联系,共同构成勘查区“三位一体”找矿预测地质模型的基本要素。本文根据漓渚铁矿床地质特征、地球化学特征和成矿作用过程的研究,对矿床成矿作用的成矿作用特征标志进行如下总结,以期对矿床进一步找矿勘查提供科学依据。  相似文献   

3.
MVT铅锌矿床和会泽型(HZT)铅锌矿床是全球最重要的铅锌矿床类型之一,其中大型矿床数量和铅锌金属储量均居于重要地位。基于勘查区找矿预测理论与方法,从“时间、空间、物质及其演化”四要素出发,厘定MVT铅锌矿床的成矿地质作用和成矿地质体,总结成矿结构面类型和矿化样式,概括成矿流体作用特征标志,并进一步揭示经典的MVT铅锌矿床“三位一体”的成矿规律:矿床产于前陆盆地地堑式构造带、不整合面上发育的溶塌角砾岩岩相组合、成矿正断层破碎带、区域性热卤水活动的“硅-钙面”成矿结构面中。在此基础上,综合构建经典的MVT铅锌矿床找矿预测地质模型:通过前陆盆地地堑式构造带研究确定勘查区找矿方向,通过成矿结构面研究判断矿体空间位置及其产状,硅-钙面等特征是判断矿床(体)存在的成矿流体作用标志。其勘查应用流程进一步概括为:看、查、识、厘、析、填、测、比、探、勘。该研究对同类矿床成矿规律研究和找矿预测评价具有启示意义。  相似文献   

4.
云南省保山市西邑铅锌矿床位于保山地块中北部,矿体主要赋存于下石炭统香山组构造破碎带中。应用"三位一体"勘查区找矿预测理论和方法,对保山西邑铅锌矿床开展了系统解剖,研究认为其成因类型为海底喷气沉积型(SEDEX型)+热液叠加改造型,成矿地质体为晚古生代(泥盆纪—早石炭世)保山盆地边缘的次级碎屑岩-碳酸盐岩沉积盆地,重磁推断矿区深部存在隐伏花岗岩体,对矿床形成产生了热液叠加改造;北东向或近南北向区域断层控制了沉积盆地的展布,其旁侧次级断层和断层破碎带为主要赋矿构造,矿体顶板主要为炭质泥岩、炭质板岩,含矿岩性为碳酸盐岩,显示硅钙面特征;成矿作用特征标志为矿化蚀变分带规律、北东(北西)侧伏规律;据此建立了地层+构造+硅钙面+蚀变分带组合"三位一体"找矿预测地质模型。利用该研究成果,在外围鲁图、广邑等地预测了有利成矿地段并提出勘查工作部署建议,其中鲁图和广邑预测区新发现了铅锌矿(化)体。  相似文献   

5.
沙坪沟整装勘查区位于安徽北淮阳成矿带内,是皖西地区最主要的钼铅锌多金属矿化集中区。研究区内已探明十余处铅锌矿,以小型矿为主,但缺乏较为系统的研究和总结。为了厘定区内铅锌矿与成矿地质体的关系以及成矿构造和成矿结构面的类型和属性,总结成矿作用特征标志,指导找矿预测,本文开展了区内典型矿床"三位一体"成矿特征的总结研究。研究结果揭示区内铅锌矿化类型分为角砾岩型、矽卡岩型、构造蚀变岩型和热液脉型4种,成矿地质体为燕山晚期中酸性岩浆岩,成矿构造为NE向和NW向断裂构造交会部位,成矿结构面主要为NE和NW断裂构造面、角砾岩筒、层间破碎带以及接触带等。在总结归纳铅锌矿成矿作用特征和找矿预测要素的基础上,建立起区内铅锌矿找矿预测地质模型,并对找矿潜力作出评价。  相似文献   

6.
通过贵州贞丰-普安金矿国家级整装勘查区的典型矿床研究,结合区域成矿地质背景,厘定了金矿成矿机制,构建了典型矿床成矿模式和区域成矿模式;通过成矿地质体、成矿构造与成矿结构面、成矿作用特征标志研究,构建了区域找矿预测地质模型和隐伏矿找矿的"五合一"技术应用示范体系;开展了找矿预测及靶区验证,新发现深埋800 1 000 m以下隐伏金矿体;整装勘查累计查明金资源量470 t,其中新增274 t,实现贵州金矿找矿历史性突破。  相似文献   

7.
周曙光 《安徽地质》2003,13(2):111-114
天马山硫金矿床位于铜官山矿田内,经铜陵有色(集团)公司的勘探和开发,对矿床的地质特征及成因有了新的认识。通过对矿床的成矿特征分析,认为矿体矿化类型有3种:层控夕卡岩型、夕卡岩型和热液型,它们是受统一成矿作用控制的产物。根据矿床中矿体的矿化类型不同以及不同矿化类型矿体的赋存空间位置不同等特征,提出了在天马山矿区及铜陵成矿区的地质找矿意义。  相似文献   

8.
安徽金寨汞洞冲铅锌矿是北淮阳地区重要的铅锌多金属矿床,文章分析研究了汞洞冲铅锌矿床区域地质背景、矿床地质特征,进一步结合前人所做的同位素地球化学、矿产勘查工作以及矿山开采实践等,讨论了铅锌矿床成因与区内构造-岩浆活动的联系,分析了其成矿地质体、成矿构造、成矿结构面以及成矿作用特征标志,建立了汞洞冲铅锌矿床"三位一体"成矿模型。成矿特征研究表明:区内铅锌矿床受构造-岩浆控制作用明显,燕山晚期的中酸性岩浆热液活动是其成矿来源,构造-岩浆带附近的断裂交汇部位是矿床形成的优越部位。此外,结合"三位一体"成矿理论分析,可以通过多种综合找矿手段在该区寻找深部隐伏铅锌矿体,从而扩大矿床规模。  相似文献   

9.
新平县好木冲铁矿矿体呈似层状、大型透镜状,赋存于中元古界昆阳群黑山头组与富良棚组在之间的断层破碎带中,含矿岩性为碳酸盐岩及火山碎屑岩。矿体受岩性、构造、岩浆岩三重因素控制,形成矿体+构造+岩体三位一体的格局,矿床的形成经历了沉积—变质—热液改造和表生富集等不同的成矿作用和成矿阶段,属沉积—改造型矿床。矿区找矿标志明显,成矿条件有利,找矿潜力较大。  相似文献   

10.
降低勘查风险、实现科学找矿一直是国内外矿产勘查界不断探索的前缘领域和研究热点,而勘查区找矿预测理论与方法是解决这一难题的有效途径。该方法将成矿作用内因(元素的地球化学特征)和外因(地质作用类型)相结合,构建以成矿地质体、成矿构造与成矿结构面和成矿作用特征标志为主要内容的找矿预测地质模型,通过大比例尺构造蚀变填图、物化探测量和专题研究等综合方法,预测推断矿体赋存位置,最后通过工程施工,发现并查明工业矿体(矿床)。依据勘查区找矿预测理论与方法,在四川拉拉铜矿、新疆玛尔坎苏锰矿带穆呼?玛尔坎土锰矿及内蒙古大兴安岭南段敖脑达坝地区锡多金属矿开展找矿预测,取得了较好效果。   相似文献   

11.
Tony Waltham 《Geology Today》2007,23(3):101-107
Switzerland's Lötschberg tunnels present a long story of both failure and success. Tunnelling that began 100 years ago ended in a massive disaster–which is a classic of engineering geology–but subsequent works were very much more successful.  相似文献   

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14.
This paper presents an elasto‐plastic model for non‐linear analyses of cement‐treated sand. Various laboratory tests were systematically carried out to investigate the pre‐peak and post‐peak behaviours of a cement‐treated sand. On the basis of these experimental results, the new model was built within the framework of a relatively simple elasto‐plastic theory. Two failure criteria are employed to express tensile and shear failure characteristics observed in the experimental results of the cement‐treated sand. The proposed model can describe strain‐hardening and strain‐softening responses under both failure modes. In the strain‐softening rules, the smeared crack concept is used, and a characteristic length is considered to avoid the issue of mesh‐size dependency. Since the failure criterion and strain‐hardening/softening rules are based on the experimental evidences, the model is relatively easy to understand and the parameters used in the model have clear physical meaning. The proposed model was applied to simulate the behaviour of cement‐treated sand in various laboratory tests, allowing for a reasonable comprehensive evaluation. It was demonstrated that the proposed model is suitable for describing both the tensile and shear failure behaviours of cement‐treated sand. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

15.
This paper reports a new 1° × 1° global thermal model for the continental lithosphere (TC1). Geotherms for continental terranes of different ages (> 3.6 Ga to present) constrained by reliable data on borehole heat flow measurements (Artemieva, I.M., Mooney, W.D. 2001. Thermal structure and evolution of Precambrian lithosphere: a global study. J. Geophys. Res 106, 16387–16414.), are statistically analyzed as a function of age and are used to estimate lithospheric temperatures in continental regions with no or low-quality heat flow data (ca. 60% of the continents). These data are supplemented by cratonic geotherms based on electromagnetic and xenolith data; the latter indicate the existence of Archean cratons with two characteristic thicknesses, ca. 200 and > 250 km. A map of tectono-thermal ages of lithospheric terranes complied for the continents on a 1° × 1° grid and combined with the statistical age relationship of continental geotherms (z = 0.04  t + 93.6, where z is lithospheric thermal thickness in km and t is age in Ma) formed the basis for a new global thermal model of the continental lithosphere (TC1). The TC1 model is presented by a set of maps, which show significant thermal heterogeneity within continental upper mantle, with the strongest lateral temperature variations (as large as 800 °C) in the shallow mantle. A map of the depth to a 550 °C isotherm (Curie isotherm for magnetite) in continental upper mantle is presented as a proxy to the thickness of the magnetic crust; the same map provides a rough estimate of elastic thickness of old (> 200 Ma) continental lithosphere, in which flexural rigidity is dominated by olivine rheology of the mantle.Statistical analysis of continental geotherms reveals that thick (> 250 km) lithosphere is restricted solely to young Archean terranes (3.0–2.6 Ga), while in old Archean cratons (3.6–3.0 Ga) lithospheric roots do not extend deeper than 200–220 km. It is proposed that the former were formed by tectonic stacking and underplating during paleocollision of continental nuclei; it is likely that such exceptionally thick lithospheric roots have a limited lateral extent and are restricted to paleoterrane boundaries. This conclusion is supported by an analysis of the growth rate of the lithosphere since the Archean, which does not reveal a peak in lithospheric volume at 2.7–2.6 Ga as expected from growth curves for juvenile crust.A pronounced peak in the rate of lithospheric growth (10–18 km3/year) at 2.1–1.7 Ga (as compared to 5–8 km3/year in the Archean) well correlates with a peak in the growth of juvenile crust and with a consequent global extraction of massif-type anorthosites. It is proposed that large-scale variations in lithospheric thickness at cratonic margins and at paleoterrane boundaries controlled anorogenic magmatism. In particular, mid-Proterozoic anorogenic magmatism at the cratonic margins was caused by edge-driven convection triggered by a fast growth of the lithospheric mantle at 2.1–1.7 Ga. Belts of anorogenic magmatism within cratonic interiors can be caused by a deflection of mantle heat by a locally thickened lithosphere at paleosutures and, thus, can be surface manifestations of exceptionally thick lithospheric roots. The present volume of continental lithosphere as estimated from the new global map of lithospheric thermal thickness is 27.8 (± 7.0) × 109 km3 (excluding submerged terranes with continental crust); preserved continental crust comprises ca. 7.7 × 109 km3. About 50% of the present continental lithosphere existed by 1.8 Ga.  相似文献   

16.
Assessing potential repositories for geologic sequestration of carbon dioxide using numerical models can be complicated, costly, and time-consuming, especially when faced with the challenge of selecting a repository from a multitude of potential repositories. This paper presents a set of simple analytical equations (model), based on the work of previous researchers, that could be used to evaluate the suitability of candidate repositories for subsurface sequestration of carbon dioxide. We considered the injection of carbon dioxide at a constant rate into a confined saline aquifer via a fully perforated vertical injection well. The validity of the analytical model was assessed via comparison with the TOUGH2 numerical model. The metrics used in comparing the two models include (1) spatial variations in formation pressure and (2) vertically integrated brine saturation profile. The analytical model and TOUGH2 show excellent agreement in their results when similar input conditions and assumptions are applied in both. The analytical model neglects capillary pressure and the pressure dependence of fluid properties. However, simulations in TOUGH2 indicate that little error is introduced by these simplifications. Sensitivity studies indicate that the agreement between the analytical model and TOUGH2 depends strongly on (1) the residual brine saturation, (2) the difference in density between carbon dioxide and resident brine (buoyancy), and (3) the relationship between relative permeability and brine saturation. The results achieved suggest that the analytical model is valid when the relationship between relative permeability and brine saturation is linear or quasi-linear and when the irreducible saturation of brine is zero or very small.  相似文献   

17.
A challenging computational problem arises when a discrete structure (e.g. foundation) interacts with an unbounded medium (e.g. deep soil deposit), particularly if general loading conditions and non‐linear material behaviour is assumed. In this paper, a novel method for dealing with such a problem is formulated by combining conventional three‐dimensional finite‐elements with the recently developed scaled boundary finite‐element method. The scaled boundary finite‐element method is a semi‐analytical technique based on finite‐elements that obtains a symmetric stiffness matrix with respect to degrees of freedom on a discretized boundary. The method is particularly well suited to modelling unbounded domains as analytical solutions are found in a radial co‐ordinate direction, but, unlike the boundary‐element method, no complex fundamental solution is required. A technique for coupling the stiffness matrix of bounded three‐dimensional finite‐element domain with the stiffness matrix of the unbounded scaled boundary finite‐element domain, which uses a Fourier series to model the variation of displacement in the circumferential direction of the cylindrical co‐ordinate system, is described. The accuracy and computational efficiency of the new formulation is demonstrated through the linear elastic analysis of rigid circular and square footings. Copyright © 2004 John Wiley & Sons, Ltd.  相似文献   

18.
Experimental observations clearly show that the relative humidity (hr) conditions influence significantly the creep behavior of cement‐based materials, indicating that the water present within these materials plays a crucial role. This work presents a creep model for hardened cement pastes (HCP), based on a multiscale homogenization approach. It takes into account both free and adsorbed water contained in the porosity and investigates their effects on the HCP macroscopic creep behavior. The calcium silicate hydrate phase is assumed to be linear viscoelastic, and the Mori–Tanaka scheme is applied in the Laplace–Carson space to the composite formed of porosity, calcium silicate hydrate, and the other main hydrated compounds (which behavior is linearly elastic) by making use of the correspondence principle. With this model, estimations of the evolution of the macroscopic creep behavior of HCP submitted to constant external loading are examined under different hr and compared with available experimental data. Finally, a method for implementing the model in a finite element code is proposed, and simulations of standard creep tests are performed to assess its validity. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

19.
In this paper we develop analytical solutions for scratch hardness–strength relations for cohesive‐frictional materials of the Mohr–Coulomb and Drucker–Prager type. Based on the lower bound yield design approach, closed‐form solutions are derived for frictionless scratch devices, and validated against computational upper bound and elastoplastic finite element solutions. The influence of friction at the blade–material interface is also investigated, for which a simple computational optimization is proposed. Illustrated for scratch tests on cement paste, we show that the proposed solutions provide a convenient way to determine estimates of cohesion and friction parameters from scratch data, and may serve as a benchmark to identify the relevance of strength models for scratch test analysis. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

20.
Paleothermometry is an essential tool for understanding past changes in climate. The ‘carbonate clumped isotope thermometer’ is a temperature proxy related to ordering of 13C and 18O in the carbonate lattice (based on measurements of 13C18O16O in CO2 produced by acid digestion of carbonate). This thermometer has been previously calibrated for inorganic calcite and aragonitic corals [Ghosh P., Adkins J., Affek H., Balta B., Guo W. F., Schauble E. A., Schrag D., and Eiler J. M. (2006) C-13-O-18 bonds in carbonate minerals: a new kind of paleothermometer. Geochim. Cosmochim. Acta70 (6), 1439-1456]. Here we determine the relationship between growth temperatures of aragonitic fish otoliths and abundances of 13C18O16O produced by acid digestion of those otoliths. Our calibration is based on analyses of otoliths from six species from four genera of modern fish sampled from a latitudinal transect of the Atlantic Ocean between 54° S and 65° N, plus one species from the tropical western Pacific. The temperatures at which fish otoliths precipitated were estimated by the mean temperature in the waters in which they lived, averaged over their estimated lifetimes. Estimated growth temperatures of our samples vary between 2 and 25 °C. Our results show that the abundance of 13C18O16O in CO2 produced by acid digestion of fish otolith aragonite is a function of growth temperature, following the relationship: , where Δ47 is the enrichment, in per mil, of 13C18O16O in CO2 relative to the amount expected for a stochastic (random) distribution of isotopes among all CO2 isotopologues, and T is the temperature in Kelvin. This relationship closely approaches that previously documented for inorganic calcite and aragonitic coral (Ghosh et al., 2006).  相似文献   

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