A Preliminary Study on Fluid Inclusions and Mineralization of Xitieshan Sedimentary-Exhalative (SEDEX) Lead-Zinc Deposit     

WANG Lijuan  ZHU Xinyou  WANG Jingbin  DENG Jiniu  WANG Yuwang  ZHU Heping 《《地质学报》英文版》2008,82(4):838-844

The Xitieshan lead-zinc deposit is located at the northern margin of the Qaidam Basin, Qinghai Province, China, and had developed a complete marine sedimentary-exhalative system. Our preliminary study of ore-forming fluids shows that fluid inclusions in quartz from altered stockwork rocks that represent the pipe facies have a wide range of temperature and salinity. The intense fluid activities are characteristics of the pipe facies of the exhalative system. Fluid inclusions in carbonates near the unstratified ore bodies hosted in the thick-bedded marble which represents vent-proximal facies are large in size and have moderate to high temperatures. They represent unerupted sub-seafloor fluid activity. Fluids in altered stockwork rocks and carbonates have similar H2O-NaCl-CO2 system, both belonging to the sedimentary-exhalative system. The fluids migrate from the pipe facies to the unstratified ore bodies. Boiling of the fluids causes the separation of CO2 vapor and liquid H2O. When the fluids migrate into the unconsolidated thick-bedded marble, the escape of CO2, decreasing temperature and pressure as well as some involvement of seawater into the fluids result in the unmixing of fluids with high and low salinity and deposition of ore-forming materials. The two unmixed fluids were trapped in unconsolidated carbonates and the ore-forming materials were deposited in the unconsolidated carbonates to form the sedimentary-exhalative type unstratified ore bodies. The ore-forming temperature of unstratified ore bodies is up to high temperature indicating that there is a huge ore-forming potential in its deep.  相似文献   

ASTER多光谱波段与SPOT全色波段融合方法研究     

喻怀义  朱谷昌  杨自安  石菲菲  王如涛 《矿产与地质》2008,22(1):69-73

遥感图像融合可以发挥多源遥感数据的优势。但由于不同传感器的遥感数据有着不同的特征,不同数据所采用的融合方法也应不同。文章探讨了ASTER多光谱波段与SPOT全色波段数据融合的方法,通过对PCA融合、IHS融合和基于小波的IHS融合方法的对比研究,得出基于小波的IHS融合法在提高空间分辨率的同时较好地保持了地物的多光谱信息。  相似文献   

成像光谱矿物填图精度兼与矿物丰度关系初探     

唐攀科  郑跃鹏  李永丽 《矿产与地质》2008,22(4):364-369

成像光谱遥感技术在岩石矿物识别和矿物填图方面发挥着越来越大作用,而成像光谱矿物填图的精度问题一直是研究的焦点。文章利用高光谱数据HyMap对新疆东天山地区的矿物填图结果,通过引入矿物填绘分布强度的概念,探索性的分析了成像光谱矿物填图与填绘矿物丰度的关系。  相似文献   

Erratum to: Late Cenozoic Volcanism at the Northeastern Flank of the South Khangai Volcanic Region (Central Mongolia): Geochronology and Formation Conditions     

V. V. Yarmolyuk  E. A. Kudryashova  A. M. Kozlovsky  V. A. Lebedev  V. M. Savatenkov 《Doklady Earth Sciences》2008,419(2):531

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快速城镇化进程中珠江三角洲高铵地下水赋存环境及驱动因素          下载免费PDF全文

吕晓立  刘景涛  韩占涛  朱亮  杨明楠  李海军 《中国地质》2021,48(6):1770-1780

地下水中高浓度的铵态氮对生活饮用水安全及生态环境存在潜在威胁。相比较硝态氮，高浓度的铵态氮不仅有各种人为来源，天然沉积环境更是造成高铵地下水的主要成因。本文以城镇化快速发展的珠江三角洲为研究区，运用数理统计、主成分分析等方法深入探讨了研究区高铵地下水的赋存环境特征及驱动因素。结果表明，研究区地下水中NH₄⁺质量浓度介于未检出~180 mg/L。研究区1539组地下水样品中，NH₄⁺质量浓度大于10 mg/L的高铵地下水69组，其中含NH₄⁺质量浓度大于30 mg/L的高铵"肥水"23组。对比2005-2008年历史水化学数据，2009-2018年新增建设用地孔隙含水层高铵地下水样品比例增加25%。高铵地下水呈斑块状分布于三角洲平原区第四系底部低洼的基底、洼地等退积层序发育的淤泥质含水层中。淤泥层等富含有机质和总有机碳的沉积层是珠江三角洲地区的"生铵层"，有机氮的矿化是三角洲平原区城市化孔隙含水层中高铵地下水的主要驱动力。城镇化扩张引起生活污水及富铵工业废水的泄漏入渗是城乡结合部高铵地下水铵氮的重要来源。三角洲平原区中性至弱碱性富含有机质的还原环境是高铵地下水的主要成因。风化溶滤、阳离子交换吸附、海陆交互作用是珠江三角洲高铵地下水质演变的主要水文地球化学过程。  相似文献   

甘肃代家庄铅锌矿的地质特征与找矿意义   总被引：4，自引：1，他引：4  

祝新友  汪东波  卫冶国  邱小平  王瑞廷 《地球学报》2006,27(6):595-602

位于甘肃宕昌县的代家庄矿床曾被认为是西成矿田铅锌找矿的重大进展,矿床产于秦岭西成盆地西北端泥盆系浅海相的富含生物化石的细碎屑岩—灰岩中。矿体不规则受NW向断裂的控制,呈角砾状分布于下部碎屑岩与上部厚层灰岩界面附近灰岩一侧。矿石的矿物共生组合为闪锌矿 方铅矿 少量黄铁矿 少量白铁矿 方解石,不含石英。硫化物发育大量的胶状、球粒状、草霉状微晶结构,部分显现出微生物化石结构特点。对代家庄与西成主要类型铅锌矿床地质地球化学特征的对比发现,二者在容矿围岩沉积环境、矿石形态、结构构造以及同位素地球化学等多方面存在明显的差异,代家庄矿床成因属于碳酸盐岩容矿的低温热液矿床,不同于西成矿田的主要SEDEX类型。主要控矿因素为灰岩—碎屑界面附近、NW向断裂等。  相似文献   

Late Neoproterozoic,Ordovician and Carboniferous events recorded in monazites from southern-central Madagascar     

《Precambrian Research》2006,144(3-4):278-296

The evolution of the basement of southern Madagascar north and south of the Ranotsara shear zone was investigated using (U + Th)/Pb electron probe monazite age dating in combination with petrographic constraints. Several monazite grains show a stepwise progression of younger ages towards the rim indicating partial and complete resetting during tectonic, metamorphic and/or fluid events. The oldest ages, ranging from 630–2400 Ma, occur relatively rare in relic cores. A first, clear age-population is dated at 550–560 Ma. Most ages fall in two populations at 420–460 and 490–500 Ma, which in some samples overlap in error. We interprete these ages as dating low-pressure and high-temperature metamorphism. We have also clear evidence for Carboniferous (300–310 Ma) monazite overgrowth rims, which can not directly be related to macroscopic structures or metamorphic parageneses. In combination with literature data, we propose that the observed monazite age populations are related to Gondwana amalgamation and subsequent rifting events during the break up of Gondwana. Our study confirms that only the electron or ion microprobe yields sufficient spatial resolution to date individual shells of multiple zoned monazites in the polymetamorphic basement of Madagascar.  相似文献   

Tin mineralization in the Dajing tin–polymetallic deposit, Inner Mongolia, China     

Y.W. Wang  J.B. Wang  L.J. Wang  Y.Z. Chen 《Journal of Asian Earth Sciences》2006,28(4-6):320-331

Dajing is a large-scale tin–polymetallic deposit that hosts the largest tin mine in North China. It is a hydrothermal vein-type deposit containing Sn, Cu, Pb, Zn, Ag, and minor components Co and In. The deposit consists of more than 690 veins hosted within Upper Permian sedimentary rocks.Three mineralization stages and six ore types are recognized with cassiterite constituting the dominant tin mineral. The SnO₂ content of cassiterite increases in the sequence of mineralization stages shear-deformation→cassiterite–quartz→cassiterite–sulfide (or chalcopyrite–pyrite) stage, while the content of FeO, TiO₂, Nb₂O₅, Ta₂O₅, and In₂O₅ tends to decrease with increases in NiO and Ga₂O₅. It is considered that the negative correlation between SnO₂ and FeO, Nb₂O₅, Ta₂O₅, and In₂O₅ results from elemental substitutions. The early stage cassiterite is much richer in Ta and the later stage cassiterite is much poorer in Ti and Fe than is usual in hydrothermal vein type tin deposits. This is interpreted to indicate that the component of early stage cassiterite reflects a granitic magma source while the composition of later stage cassiterite has a more obvious strata source. The compositional variation of cassiterite corresponds to decreasing crystallization temperatures within each stage and between sequential stages with time. The characteristics of REE in cassiterite from two stages are in accord with that of subvolcanic rocks and the Linxi formation. It suggests that tin transported during the cassiterite–quartz stage may have originated from subvolcanic dikes (e.g., dacite porphyry), while in the cassiterite–sulfide stage, tin may have been derived from wallrock (e.g. siltstone) of the Upper Permian-age Linxi Formation.  相似文献   

农牧交错带典型区农业与牧业用地互动关系研究   总被引：13，自引：0，他引：13  

高清竹  何立环  江源  王家骥 《地球科学进展》2002,17(2):209-214

利用1989年和2000年的两期Landsat-TM数据和相关的统计资料以及气候数据，应用转移距阵和多元回归分析等研究方法，对地处典型农牧交错带地区的兴和县土地利用变化进行研究，结果表明：农田和草地是研究区域中最主要的土地利用类型，Landsat-TM卫星影像数据和统计数据比较一致地反映农田和草地面积的变化；农田和草地的相互转换率在各种用地相互转化中非常剧烈；农业与牧业用地的互动特征具有明显的区域差异；农业和牧业用地的互动特点是自然因素和社会经济因素同时影响的结果。  相似文献   

Chemical composition of stars in the galactic halo     

S. V. Ermakov  V. G. Klochkova  V. E. Panchuk  G. Zhao 《Astronomy Reports》2002,46(11):874-886

The chemical compositions of the atmospheres of six metal-poor stars are analyzed. Spectra with signal-to-noise ratios of no less than 100 and a resolution of R≈17 000 were obtained using the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. The abundances of Li, O, α-process elements (Mg, Si, Ca, Ti), Na, K, Sc, iron-peak elements (Cr, Mn, Fe, Ni, Cu, Zn), and s-process elements (Y, Ba) are derived. The star G251-54 ([Fe/H]=?1.55, T _eff=5541 K, logg=3.58) is deficient in some elements compared to both stars with similar metallicities and the Sun. The atmosphere of G251-54 has the following elemental abundances relative to iron: [O/Fe]=+0.47, [α/Fe]≈?0.3, [Na/Fe]=?0.60, [Sc/Fe]=?0.57, [Cr, Ni, Fe]≈0, [Zn/Fe]=+0.16, [Cu/Fe]=?0.66, [Y/Fe]=?0.70, and [Ba/Fe]=?1.35. The remaining five stars have metallicities in the range ?1.6<[Fe/H]相似文献