围岩蚀变对内生金属矿床勘查的意义

围岩蚀变对于研究热液矿床元素富集规律、指导找矿都具有极其重要的意义。文章从围岩蚀变是矿质沉淀的重要机制、围岩蚀变是重要的找矿标志、围岩蚀变在地球物理、地球化学找矿信息提取中的响应等方面阐述围岩蚀变对成矿与找矿的贡献。     

南美典型铁矿床遥感找矿模型研究

针对南美地区两种典型铁矿—苏比利尔湖型和阿尔果玛型铁矿,基于ETM+遥感数据,采用光谱角方法提取研究区的羟基、铁染蚀变信息;通过影像增强,波段合成等预处理结合人工解译,进行赋矿地层和控矿构造信息提取。总结分析示矿信息规律和特征,建立遥感找矿模型,圈定2处遥感找矿靶区,缩小了野外地质调查范围。     

基于铜陵矿集区遥感影像的地质解译及成矿远景区圈定研究

本文对铜陵矿集区的landsat 7 ETM+遥感影像进行综合分析,获取影像波谱特性,运用波段比值和主成分分析的方法提取铁染和羟基蚀变信息,利用彩色密度分割得到蚀变异常图像,清晰显示铜陵矿集区的成矿有利区域。并对遥感解译结果和铜陵地区地质构造与现有矿点对比,验证提取结果。圈定的11个成矿有利区域中:3个A类区蚀变信息明显,具备有利成矿条件,成矿潜力巨大;4个B类区蚀变信息中等,具备有利成矿条件,具有一定成矿潜力;4个C类区蚀变信息离散,成矿条件不明显,具有成矿可能,但是潜力不大。     

Selection of Less Biased Threshold Angles for SAM Classification Using the Real Value–Area Fractal Technique

The accuracy of classification of the Spectral Angle Mapping (SAM) is warranted by choosing the appropriate threshold angles, which are normally defined by the user. Trial‐and‐error and statistical methods are commonly applied to determine threshold angles. In this paper, we discuss a real value–area (RV–A) technique based on the established concentration–area (C–A) fractal model to determine less biased threshold angles for SAM classification of multispectral images. Short wave infrared (SWIR) bands of the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) images were used over and around the Sar Cheshmeh porphyry Cu deposit and Seridune porphyry Cu prospect. Reference spectra from the known hydrothermal alteration zones in each study area were chosen for producing respective rule images. Segmentation of each rule image resulted in a RV–A curve. Hydrothermal alteration mapping based on threshold values of each RV–A curve showed that the first break in each curve is practical for selection of optimum threshold angles. The hydrothermal alteration maps of the study areas were evaluated by field and laboratory studies including X–ray diffraction analysis, spectral analysis, and thin section study of rock samples. The accuracy of the SAM classification was evaluated by using an error matrix. Overall accuracies of 80.62% and 75.45% were acquired in the Sar Cheshmeh and Seridune areas, respectively. We also used different threshold angles obtained by some statistical techniques to evaluate the efficiency of the proposed RV–A technique. Threshold angles provided by statistical techniques could not enhance the hydrothermal alteration zones around the known deposits, as good as threshold angles obtained by the RV–A technique. Since no arbitrary parameter is defined by the user in the application of the RV‐A technique, its application prevents introduction of human bias to the selection of optimum threshold angle for SAM classification.     

云南会泽HZT 型铅锌矿床蚀变白云岩特征及岩石-地球化学找矿标志

蚀变白云岩是会泽超大型铅锌矿床的赋矿围岩。通过矿区调研和近矿围岩典型剖面精细测量,矿区蚀变中-粗晶白云岩从颜色上可分为4种类型:肉红中粗晶白云岩、米黄色针孔状粗晶白云岩、灰白孔洞状粗晶白云岩、纯白色粗晶白云岩;前三者与矿体产出关系密切,从远矿到近矿依次为:肉红中粗晶白云岩→米黄色针孔状粗晶白云岩→灰白孔洞状粗晶白云岩→铅锌矿石;总结了3个带主要矿物组合、组构特征,认为3个带在白云石重结晶程度、显微构造、黄铁矿、晶洞充填物及裂隙等具明显差异,据此可作为辨识赋矿白云岩的重要标志。同时,对比了摆佐组白云岩(矿化粗晶白云岩、粗晶白云岩、白云石化灰岩)主量元素变化特征,分析了近矿蚀变白云岩主量元素及其比值与矿体距离的相关性,以及CaO与其他主量元素相关性,确定了热液蚀变参数有SiO2、MgO/CaO、K2O/CaO、Al2O3/TFe等,为找矿预测提供理论依据。     

遥感信息与化探在湘南地区找矿预测中的应用

湘南地区是我国重要的有色金属成矿带之一,在该区针对ETM图像采用主成份分析、掩膜等遥感图像处理方法进行遥感蚀变信息提取,并针对该区的水系沉积物,采用迭代法确定地球化学背景值与异常下限,利用MapGIS、Section及DGSS软件提取化探异常信息,研究了该区的地质成矿背景。结合以上两种方法,圈定找矿靶区,为地质勘察工作明确了找矿的方向。     

马超营断裂带地质及地球化学特征

根据对马超营断裂带系统进行的地质—地球化学剖面研究，探讨了该带断裂构造活动及其元素地球化学迁移富集规律与构造地球化学分异之间的关系；分析了蚀变、矿化与成矿的关系，认为早期面型蚀变伴有成矿元素的活化和迁移，但无矿化富集，后期带状蚀变伴有金的富集成矿且以硅化、绢云母化为主要标志。从而，为马超营断裂带这一重要的以金为主成矿带的进一步工作、研究，提供了地球化学方面的依据。     

卢氏西虎岭黄铁矿床围岩蚀变特征及其找矿意义

文章通过对西虎岭黄铁矿床围岩蚀变的研究认为，围岩蚀变大致可分为６种基本蚀变类型，５个蚀变阶段，３个蚀变带。各蚀变带以矿体为中心对称分布，各带之间呈渐变过渡关系。同时认为矿床成因类型属中低温热液充填型，并指出围岩蚀变的找矿意义。     

Trace element and Nd isotope analyses of apatite in granitoids and metamorphosed granitoids from the eastern Central Asian Orogenic Belt: Implications for petrogenesis and post-magmatic alteration

We present in situ trace element and Nd isotopic data of apatites from metamorphosed and metasomatized (i.e., altered) and unaltered granitoids in the Songnen and Jiamusi massifs in the eastern Central Asian Orogenic Belt, with the aim of fingerprinting granitoid petrogenesis, including both the magmatic and post-magmatic evolution processes. Apatites from altered granitoids (AG) and unaltered granitoids (UG) are characterized by distinct textures and geochemical compositions. Apatites from AG have irregular rim overgrowths and complex internal textures, along with low contents of rare earth elements (REEs), suggesting the re-precipitation of apatite during epidote crystallization and/or leaching of REEs from apatite by metasomatic fluids. ε_Nd(t) values of the these apatites are decoupled from zircon ε_Hf(t) values for most samples, which can be attributed to the higher mobility of Nd as compared to Sm in certain fluids. Apatites from UG are of igneous origin based on their homogeneous or concentric zoned textures and coupled Nd-Hf isotopic compositions. Trace element variations in igneous apatite are controlled primarily by the geochemical composition of the parental melt, fractional crystallization of other REE-bearing minerals, and changes in partition coefficients. Sr contents and Eu/Eu* values of apatites from UG correlate with whole-rock Sr and SiO₂ contents, highlighting the effects of plagioclase fractionation during magma evolution. Apatites from UG can be subdivided into four groups based on REE contents. Group 1 apatites have REE patterns similar to the host granitoids, but are slightly enriched in middle REEs, reflecting the influence of the parental melt composition and REE partitioning. Group 2 apatites exhibit strong light REE depletions, whereas Group 3 apatites are depleted in middle and heavy REEs, indicative of the crystallization of epidote-group minerals and hornblende before and/or during apatite crystallization, respectively. Group 4 apatites are depleted in heavy REEs, but enriched in Sr, which are features of adakites. Some unusual geochemical features of the apatites, including the REE patterns, Sr contents, Eu anomalies, and Nd isotopic compositions, indicate that inherited apatites are likely to retain the geochemical features of their parental magmas, and thus provide a record of small-scale crustal assimilation during magma evolution that is not evident from the whole-rock geochemistry.     

基于高光谱数据的甘肃花西山金矿蚀变特征分析与找矿预测应用

利用地物光谱仪识别具有光谱诊断性吸收特征的蚀变矿物,并分析其空间分布及组合特征,是后续利用航空、航天高光谱遥感开展找矿预测的重要理论依据。本文以位于甘肃柳园地区花牛山矿集区的花西山金矿床为例,首先利用FieldSpecPro FR便携式光谱仪对采集样品进行光谱测量,通过The Spectral Geologist 8软件对获得的光谱数据进行分析解译,揭示了与矿化关系密切的地表蚀变矿物为绢云母（白云母和多硅白云母）+黄钾铁矾+赤铁矿+针铁矿,外围蚀变矿物主要为绢云母（钠云母）+绿帘石+绿泥石+蒙脱石+水铝石。基于这一认识,对矿区及周边开展CASI/SASI航空高光谱遥感蚀变矿物信息提取,综合地表及航空高光谱解译信息,建立了花西山式金矿床的高光谱遥感找矿预测模型,并基于该找矿预测模型在外围圈定了预测区1处,经野外查证,预测区内发现有明显金异常。研究结果表明,在分析和总结调查区成矿地质背景和蚀变特征的基础上,结合高光谱遥感信息可快速地、更有针对性地发现成矿有利区段,为矿产勘查部署提供重要参考资料。