广西昭平县湾岛金矿地质特征及找矿方向

广西昭平湾岛金矿受断裂破碎带和花岗斑岩接触带的控制,主要围岩蚀变为硅化和绢云母化,矿化类型分为石英脉型和硅化蚀变岩型.金矿床属中低温热液构造蚀变岩型金矿.     

新疆尼勒克县哈勒尕提铜铁矿地质特征及找矿前景

文章介绍了新疆尼勒克县哈勒尕提铜铁矿成矿地质背景和矿区地质特征、矿体特征、矿物成分、微量元素分布特征等,指出该矿具备大型矿床的成矿条件,有较大的找矿前景.     

肃南县羊露河上游似鞍山式铁矿地质特征及找矿方向

羊露河上游铁矿位于北祁连西段加里东褶皱带西段.铁矿体赋存于下元古界长城系上岩组含铁角闪片岩中,含矿层位严格受地层层位控制,矿石构造具有同生沉积特征,并显示了热液富集作用特点,具"似鞍山式"铁矿成因特征,矿石品位较高,盲矿体存在的可能性较大,因此具有重要的找矿意义.     

会泽铅锌矿床中自然锑的发现及伴生元素的分布特征

文章对会泽铅锌矿床的主要矿体进行了系统观察、采样，对其矿石进行了岩矿鉴定、化学分析(包括部分单矿物)和电子探针分析，并对其成矿作用做了探讨。首次在矿石中发现了自然锑，初步查明整个矿床中Ag，Cd，Ge，Cu，Sb等伴生元素的平均含量(wB／10^-6)分别为121．77、660．99、62．10、203．78和169．87，认为它们是晚成矿阶段形成的。     

阿尔金北缘大平沟金矿床成因

大平沟金矿是阿尔金北缘地区近年来新发现的一个中型金矿床。它受韧性剪切带构造的控制,矿化类型为蚀变糜棱岩型夹少量钾长石石英脉型。文章通过地质地球化学的研究,探讨了该矿床的成因。稀土元素、硫同位素、铅同位素和锶同位素地球化学特征反映成矿物质主要来源于变质岩;流体包裹体和氢氧同位素反映成矿流体主要来源于变质水,有少量重熔岩浆水和大气降水的混入,成矿温度198～2 90℃,成矿流体密度0 .791～0 .971g/cm3 ;盐度w(NaCleq) =2 .0 3%～5 .5 % ,成矿压力(42 0～72 0 )×10 5Pa ,成矿深度为1.6 1～2 .6 8km。石英流体包裹体Rb_Sr等时线年龄表明成矿时代为加里东期。大平沟金矿床属于中温动力变质热液成因矿床。     

新疆哈密维权银(铜)矿床地质特征和成矿时代

维权银(铜)矿床是2000年发现的一个独立中型银矿。经过野外及室内研究,发现矿床产于塔里木板块北缘活动带觉罗塔格晚古生代岛弧带的南侧,赋矿地层为中石炭统土古土布拉克组浅海相中酸性、基性火山岩、碎屑岩和碳酸盐岩,受区域早期热蚀变作用而发生不含矿的角岩化;受晚期岩体侵入活动作用形成Ag、Cu等矽卡岩矿化;容矿岩石为钙铁榴石矽卡岩,是一个远离侵入体的以银为主的多金属矽卡岩型矿床。采集维权银(铜)矿东南部花岗岩进行单颗粒锆石的SHRIMPU_Pb年龄测定,结果为(297±3)Ma,是矿床成矿年龄的上限。     

个旧锡矿大马芦层间氧化矿床地质特征及找矿方向研究

个旧锡矿层间氧化矿床品位高、工业利用价值大，加强这类矿床地质特征的研究，对于矿山深部及外围的锡矿找矿具有重要的指导意义。通过对个旧锡矿层间氧化矿床产出的地质特征、控矿因素的分析与研究，探讨了其矿床成因，并总结出：“背-突式”、“向-断-凹式”、“断-互式”及“断裂式”四种成，矿模式。按这些模式的找矿实践表明，找矿效果极佳。     

黔西北猫猫厂-榨子厂铅锌矿区地质特征及找矿方向

猫猫厂铅锌矿系黔西北铅锌银矿集区主要矿床之一，产于NW向与NE向构造交切复合部位，赋矿地层主要为石炭系白云岩、白云质灰岩。通过对矿床地质特征的总结及与邻区典型矿床类比分析，认为深部找矿潜力大，应加大找矿力度。     

Efficiency of heavy liquid separation to concentrate magnetic particles

Low-temperature rock magnetic measurements have distinct diagnostic value. However, in most bulk marine sediments the concentration of ferrimagnetic and antiferromagnetic minerals is extremely low, so even sensitive instrumentation often responds to the paramagnetic contribution of the silicate matrix in the residual field of the magnetometer. Analysis of magnetic extracts is usually performed to solve the problems raised by low magnetic concentrations. Additionally magnetic extracts can be used for several other analyses, for example electron microscopy or X-ray diffraction. The magnetic extraction technique is generally sufficient for sediments dominated by magnetite. In this study however, we show that high-coercivity components are rather underrepresented in magnetic extracts of sediments with a more complex magnetic mineralogy. We test heavy liquid separation, using hydrophilic sodium polytungstenate solution Na₆[H₂W₁₂O₄₀], to demonstrate the efficiencies of both concentration techniques. Low-temperature cycling of zero-field-cooled, field-cooled and saturation isothermal remanent magnetization acquired at room temperature was performed on dry bulk sediments, magnetic extracts, and heavy liquid separates of clay-rich pelagic sediments originating from the Equatorial Atlantic. The results of the thermomagnetic measurements clarify that magnetic extraction favours components with high spontaneous magnetization, such as magnetite and titanomagnetite. The heavy liquid separation is unbiased with respect to high- and low-coercive minerals, thus it represents the entire magnetic assemblage.     

Improved magnetic anomalies of the Antarctic lithosphere from satellite and near-surface data

The Antarctic magnetic anomaly map compiled marine and airborne surveys collected south of 60°S through 1999 and used Magsat data to help fill in the regional gaps between the surveys. Ørsted and CHAMP satellite magnetic observations with greatly improved measurement accuracies and temporal and spatial coverage of the Antarctic, have now supplanted the Magsat data. We combined the new satellite observations with the near-surface survey data for an improved magnetic anomaly map of the Antarctic lithosphere. Specifically, we separated the crustal from the core and external field components in the satellite data using crustal thickness variations estimated from the terrain and the satellite-derived free-air gravity observations. Regional gaps in the near-surface surveys were then filled with predictions from crustal magnetization models that jointly satisfied the near-surface and satellite crustal anomalies. Comparisons in some of the regional gaps that also considered newly acquired aeromagnetic data demonstrated the enhanced anomaly estimation capabilities of the predictions over those from conventional minimum curvature and spherical harmonic geomagnetic field models. We also noted that the growing number of regional and world magnetic survey compilations involve coverage gaps where these procedures can contribute effective near-surface crustal anomaly estimates.