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1.
河南萑香洼金矿原生晕地球化学特征和深部找矿预测 总被引：3，自引：1，他引：3
河南熊耳山地区是豫西重要的金矿化集中区,萑香洼金矿是该成矿带近几年新发现的金矿床.通过运用地球化学成矿指数、聚类分析和因子分析的理论与方法,解析了萑香洼金矿的地球化学场,得出如下主要研究成果:①金矿床F985矿脉呈现以Au、Ag为主,伴有Pb、Zn、Cu、Bi、As、Sb等多元素的综合原生晕;②厘定金矿床的地球化学原生晕的轴向分带、横向分带和纵向分带;③原生晕轴向分带序列:头晕元素组合为As、Sb、Ba,主成矿晕元素组合为Au、Ag、Pb、Zn、Cu、Mo,尾晕元素组合为Co、Ni、Bi;④依据综合原生晕异常套合的特征,优选了4个找矿靶区,对深部隐伏矿体进行定位预测. 相似文献
2.
通过与国内外及哈图齐Ⅰ热液型金矿的对比,筛选出齐Ⅲ成矿成晕指示元素Hg、Au、Ni、Pb、As、Sb、Cu、W、Zn、Ag、Mo、Bi等。利用格氏分带指数法和相关性聚类分析,获得齐Ⅲ金矿矿体原生晕轴向分带序列为:(Sb)-(Ni-Cu-Zn-Ag-Pb-Bi)-(Mo-As)-(Au-Hg-W),相关性聚类为:Pb-Bi,W-Au-Sb-As,Cu-Zn-Ni和Hg-Ag。结合前人研究成果和剔除叠加结构的影响,获得该矿前缘晕指示元素组合是Hg-As-Sb,近矿元素组合Pb-Ag-Cu-Zn-Bi,尾晕组合W-Ni-Mo。根据原生晕分布特征及前沿晕与尾晕元素累加比的变化趋势,推测深部可能存在隐伏矿体。 相似文献
3.
甘肃文县阳山金矿是产于勉略缝合带内的超大型卡林-类卡林型金矿床。为探讨矿区深部找矿潜力和成矿远景评价,文章对葛条湾-安坝矿段30号勘探线剖面的成矿及伴生元素原生晕地球化学特征进行研究,结果表明:该矿段原生晕的轴(垂)向分带序列自上而下为:Pb—Co—Cu—Zn—Mn—Bi—Mo—Sb—Au—As—Ag。矿体中部原生晕具有反向分带特征,原生晕出现前缘晕、尾晕叠加,显示具有多阶段热液叠加成矿作用的特征。在深部1400 m标高,前缘晕并未消失,并向深部强度增大,尾晕仅为弱异常。同时,原生晕地球化学参数(As×Sb)/(Mo×Bi)、(As+Sb)/(Mo+Bi)比值发生转折并升高,前缘晕因子得分在深部有很强的高值异常,进一步证实深部具有盲矿体存在的可能性。综上表明,阳山金矿矿区深部找矿前景较好。 相似文献
4.
陕西省铧厂沟金矿主要赋存于海底基性火山喷流细碧岩中.在野外地质工作的基础上,进行了数学地质分析和原生晕分带序列计算.结果表明,Sb、Hg、As、Cu为前缘晕元素组合,Au、Ag、Bi、Pb、Zn为近矿晕元素组合,Co、Ni、W、Mo、Mn、Cd为尾晕元素组合;北矿带原生晕轴向分带序列从上至下为:Hg-Bi-Mo-Au-Ag-As-Cu-Pb-Co-W-Mn-Sb-Ni-Zn-Cd.结合微量元素衬值空间变化规律,建立了北矿带的原生晕叠加理想模型:在950m中段到830 m中段之间自上而下发育A、B、C 三个小矿体;A矿体尾部和B矿体头部叠加在一起,而B、C两个矿体间隔的距离较大;830m中段已经到达矿体尾部,矿体向深部延伸较小. 相似文献
5.
《物探与化探》2015,(5)
对龙门店银矿K4矿体Au、Ag、Cu、Pb、Zn、W、Mo、Hg、As、Sb、Bi等11种微量元素的原生晕特征进行研究,为矿体深部成矿预测提供理论依据。微量元素统计学分析表明,Pb、Zn可作为矿体主要的近矿指示元素,矿体的成矿过程具有多期次叠加的特点;分析K4矿体原生晕地球化学参数垂向变化规律,发现矿体前缘和中部分别表现出明显的尾晕指示元素强异常和前缘晕指示元素强异常;计算得到矿体自上而下的轴向分带序列为W—Mo—Au—Hg—Cu—As—Bi—Zn—Ag—Sb—Pb,出现了明显的"前尾晕共存"和"反向分带"现象。依据上述K4矿体原生晕特征,建立了矿体原生叠加晕模型,并预测矿体深部存在规模较大的盲矿体,909 m标高以下有较大的找矿潜力。 相似文献
6.
小西南岔金铜矿床为浅成金铜共生大型矿床,受岩体-地层-构造联合控制,以叠加富集为主.矿区分为南山和北山两个矿段.矿化主要发育在闪长岩和斜长花岗岩中的北北西向断裂带及岩体接触带中,矿化以含金铜石英硫化物脉型及密集细脉为主.矿区水系沉积物异常元素为Au、Cu、Ag、Bi、Zn、Mo（W、Sb、As）;土壤异常元素为Cu、Mo、Au、Ag、Bi;岩石地球化学异常为Au、Cu、Ag、Bi、Ta、Ba、Sr（As、Sb、Zn、Co、Ni、W、Mo）.原生晕中轴向分带序列为（Bs、Sr）-As-Ag-Pb-Sn-W-Au-Bi-Cu-Sb-CoTe-Ni-Zn-Mo.南山矿段水平分带序列为Au-Cu-Bi-Te-Ag-Pb-Zn-As-Co-Ni-W-Sb-Mo-Sn;北山矿段为Au-Cu-Bi-Te-AgAs-Sb-Mo-Pb-Zn-Co-W-Ni-Sn.矿床地球化学异常特征及其分带性显示北山矿段矿体剥蚀程度大于南山矿段,矿区北西部矿体剥蚀强度大于南东部,表明向矿区南部仍有较大找矿远景. 相似文献
7.
为预测和评价那仁陶勒盖金矿的成矿潜力,运用多元统计方法,结合地球化学各参数信息,对那仁陶勒盖金矿原生晕进行系统研究.结果显示:那仁陶勒盖金矿赋矿花岗闪长岩中Au、Ag、Bi等元素浓集克拉克值明显偏高,与那仁陶勒盖金成矿作用关系密切;矿石中Au与Sb、Cu、Pb、Ag、Hg、Zn、As、Bi等关系最为密切;矿体原生晕轴向分带序列出现尾晕元素W、Sn等与前缘晕元素As叠加的现象,同时(As+Sb)/(Bi+Mo)、100Sb/(Bi·Mo)等分带性指数出现转折,指示深部存在盲矿体.依据上述矿体原生晕特征,建立矿体叠加晕预测模型,预测盲矿体赋存位置在海拔710m以下的岩体与地层接触带附近. 相似文献
8.
《四川地质学报》2019,(Z1):160-161
四川子杠坪铅锌矿床位于松潘～甘孜地槽褶皱系的东南缘,处于滴痴山背斜的西翼。矿区发现了一条铅锌矿体,赋存于二叠系下统甲黄沟群片岩地层的层间断裂带中,呈似层状产出,具显著的层控特征,成因类型为沉积变质叠加热液改造型。对I号矿体6个中段的56件矿样的副样分析,通过数理统计分析、分带序列研究、建立矿体深部预测模型等方法,系统研究了矿体原生晕地球化学特征。研究表明成矿主要指示元素为Pb、Zn、Cu、Co、Ag、Sb、Hg,次要指示元素为Au、As、Mo、Ni、Bi、W、Sn。原生晕分布特征显示了单一期次成矿作用前缘晕指示元素为As、Sb、Hg,近矿晕指示元素为Pb、Zn、Ag、Bi、Co,矿体下部及尾晕元素为Au、W、Mo、Cu。矿体原生晕综合轴向分带序列为:As―Sb―Ni―Bi―Ag―Ba―Zn―Sr―Mo―Au―W―Co―Pb―Sn―Cu―Hg,出现反分带现象。地球化学参数评价指标变化趋势为由大到小再变大,叠加作用明显,前缘晕元素Ag、Sb、Hg的含量在最下部中段有增大趋势,推测矿体向下延伸很可能再次富集膨大,膨大部位较远。建立了矿体深部预测模型,结合成矿指示元素浓度分布情况,预测了矿体在深部呈囊状展布,在P08-P16勘查线向下可能再次膨大,往东西两端则有逐渐尖灭趋势。 相似文献
9.
《四川地质学报》2022,(Z1):160-170
四川子杠坪铅锌矿床位于松潘～甘孜地槽褶皱系的东南缘,处于滴痴山背斜的西翼。矿区发现了一条铅锌矿体,赋存于二叠系下统甲黄沟群片岩地层的层间断裂带中,呈似层状产出,具显著的层控特征,成因类型为沉积变质叠加热液改造型。对I号矿体6个中段的56件矿样的副样分析,通过数理统计分析、分带序列研究、建立矿体深部预测模型等方法,系统研究了矿体原生晕地球化学特征。研究表明成矿主要指示元素为Pb、Zn、Cu、Co、Ag、Sb、Hg,次要指示元素为Au、As、Mo、Ni、Bi、W、Sn。原生晕分布特征显示了单一期次成矿作用前缘晕指示元素为As、Sb、Hg,近矿晕指示元素为Pb、Zn、Ag、Bi、Co,矿体下部及尾晕元素为Au、W、Mo、Cu。矿体原生晕综合轴向分带序列为:As―Sb―Ni―Bi―Ag―Ba―Zn―Sr―Mo―Au―W―Co―Pb―Sn―Cu―Hg,出现反分带现象。地球化学参数评价指标变化趋势为由大到小再变大,叠加作用明显,前缘晕元素Ag、Sb、Hg的含量在最下部中段有增大趋势,推测矿体向下延伸很可能再次富集膨大,膨大部位较远。建立了矿体深部预测模型,结合成矿指示元素浓度分布情况,预测了矿体在深部呈囊状展布,在P08-P16勘查线向下可能再次膨大,往东西两端则有逐渐尖灭趋势。 相似文献
10.
《矿产与地质》2017,(2)
针对矿区地表及井下四个中段共采集地层和构造蚀变岩样品194件,分析Ti、V、Cr、Mn、Co、Ni、Au、Ag、Cu、Pb、Zn、W、Sn、Mo、Bi、As、Sb、Hg等18种微量元素含量,编制各元素地球化学0号勘探线横剖面图,综合利用地球化学图件分析法与格里戈良分带指数法,确定元素的轴向分带序列。通过地质地球化学资料可知,石英闪长岩、构造蚀变岩中Cu、Ag、As、Au、Mo、Sn元素含量高,变异系数大,表明这些元素参与成矿蚀变作用。矿区原生晕轴向分带序列为:(Zn、Cr1、Hg1、Ni、As)→(Pb、V、Mn、W、Cr_2、Ti)→(Hg_2、Sb、Co、Bi、Sn、Ag、Au、Mo、Cu),根据元素地球化学横剖面图中主成矿元素异常高值带向下延伸未封闭、矿体向下未尖灭、特征前缘晕元素Hg、成矿晕元素Cu出现矿尾晕等特征,说明矿体向下仍有一定的延伸,预示着深部具有一定的找矿潜力。 相似文献
11.
奥地利安东帕有限公司 《岩矿测试》2009,28(3):306-306
最新的流行病学研究表明,空气中较高浓度的悬浮细颗粒可能对人类的健康有不利的影响。根据该项研究显示,由于心脏病、慢性呼吸问题和肺功能指标恶化而导致死亡率的升高与细尘粒子有关。这些研究结果已经促使欧盟于1999年4月出台了限制空气中二氧化硫、二氧化氮、氧化氮、铅和颗粒物含量的法案(1999/30/EC),对各项指标包括对可吸入PM10颗粒的浓度提出了新的限制性指标。PM10颗粒是指可以通过预分级器分离采集的气体动力学直径小于10μm的细颗粒。目前研究的兴趣重点逐步偏向PM2.5这些更细微颗粒物,PM2.5这种颗粒物对健康有明显的不利影响。在欧盟指令2008/50/EC中,对PM10和PM2.5都提 相似文献
12.
Joseph Clancy White 《Contributions to Mineralogy and Petrology》1993,113(4):524-532
The textural relationships and structural states of optically isotropic labradorite from the Manicouagan, Quebec, impact structure have been examined by light (optical) and transmission electron (TEM) microscopy. Two distinct diaplectic glasses have been recognized based on their contrasting morphology, timing and the inferred modes of formation. The earliest isotropic bands and grain-scale isotropism (maskelynite) optically exhibit a gradational,in situ transformation from crystalline plagioclase with preservation of relict textures (twins, grain boundaries). The same transformation from crystalline to amorphous structure is observed in TEM to occur heterogeneously at scales on the order of the unit cell. The progressive transformation of optical properties reflects an increase in the volume fraction and eventual coalescence of these amorphous units. This maskelynite-type diaplectic glass is interpreted to form in the solid-state directly from crystalline material during the compressional phase of the shock wave. The other isotropic material occurs in spatially discrete tensiongashes and planar deformation features (PDFs) that overprint the maskelynite-type glass. This second type of diaplectic glass (PDF-type) is developed homogeneously within a given glass band and exhibits sharp crystal-glass boundaries, in contrast to the gradational boundaries of the maskelynite-type glass. PDF-type glass is interpreted to form by melting in tensional release zones during passage of the rarefaction wave. These observations emphasize the ability of naturally shocked rocks to preserve subtle evidence of variations in the shock process from highly transient events. 相似文献
13.
A catastrophic rockslide-debris flow in Wulong, Chongqing, China in 2009: background, characterization, and causes 总被引：7，自引：3，他引：4
Qiang Xu Xuanmei Fan Runqiu Huang Yueping Yin Shengshan Hou Xiujun Dong Minggao Tang 《Landslides》2010,7(1):75-87
On June 5, 2009, a catastrophic rockslide-debris flow occurred at the crest of the Jiweishan Mountain in Wulong, Chongqing,
China. Approximately five million cubic meters of limestone blocks slid along a weak interlayer of bituminous and carbonaceous
shale. The source mass descended from the upper part of the slope rapidly, crossing a 200-m wide and 50-m deep creek in front
of it. Blocked by the opposite steep creek wall, the sliding mass changed its direction and traveled a further 2.2 km along
the creek in debris-flow mode, finally forming a large accumulation zone with an average depth of 30 m. This is one of the
most catastrophic rockslide events in recent years in China. It buried 12 houses and the entrance of an iron mining tunnel
where some 27 miners were working inside. Ten people died, 64 missing, and eight wounded. Immediately after this disaster
happened, the government organized an expert team to assist the rescue work. As one of the geological experts, the author
did a lot of field investigations and collected first-hand information. Multi-methods including the remote sensing, 3D laser
scanning, geophysical exploration, and numerical modeling were used for analyzing the characteristics and the triggering mechanism
of the Wulong rockslide. The preliminary investigation results reveal that this rockslide with poor geological conditions
was mainly induced by the gravitation and the karst effect and also affected by the previous mining activities. The research
in this paper is meaningful and useful for further research on such kind of rockslides that are geologically similar to the
Wulong rockslide. 相似文献
14.
S. Viswanathan K. Surya Prakash Rao B. Mahabaleswar 《Journal of the Geological Society of India》2013,82(6):621-627
Komatiites are mantle-derived ultramafic volcanic rocks. Komatiites have been discovered in several States of India, notably in Karnataka. Studies on the distribution of trace-elements in the komatiites of India are very few. This paper proposes a simple, accurate, precise, rapid, and non-destructive wavelength-dispersive x-ray fluorescence (WDXRF) spectrometric technique for determining Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Y, Zr, Nb, Ba, Pb, and Th in komatiites, and discusses the accuracy, precision, limits of detection, x-ray spectral-line interferences, inter-element effects, speed, advantages, and limitations of the technique. The accuracy of the technique is excellent (within 3%) for Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Zr, Nb, Ba, Pb, and Th and very good (within 4%) for Y. The precision is also excellent (within 3%) for Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Y, Zr, Nb, Ba, Pb, and Th. The limits of detection are: 1 ppm for Sc and V; 2 ppm for Cr, Co, and Ni; 3 ppm for Cu, Zn, Rb, and Sr; 4 ppm for Y and Zr; 6 ppm for Nb; 10 ppm for Ba; 13 ppm for Pb; and 14 ppm for Th. The time taken for determining Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Y, Zr, Nb, Ba, Pb, and Th in a batch of 24 samples of komatiites, for a replication of four analyses per sample, by one operator, using a manual WDXRF spectrometer, is only 60 hours. 相似文献
15.
Xiaoyu ZHAO Wuyi WANG Hairong LI Fujian FENG Lizhen WANG 《中国地球化学学报》2006,25(B08):80-81
Brick-tea-type fluorosis is a peculiar endemic disease in China, which had been discovered in minority areas of western China since 1980, and distributed mainly in Tibet, Inner Mongolia, Gansu, Xinjiang, Qinghai and parts of Sichuan Province. The prevalence rate of fluorosis in Tibetan and Mongolian nationality people was higher. Epidemiological investigation showed that fluorosis morbidity and degrees were different in different brick-tea drinking areas, and it was probably caused by drinking various kinds of brick tea from different regions. Therefore, we collected 33 samples of brick tea from six provinces where minority nationalities were accustomed to drinking a large quantity of brick tea. F concentrations were determined by the combustion hydrolysis-ion selective electrode method. The results showed that among the brick teas, the F concentrations ranged from the minimum 74.1 mg/kg in Yunnan Province to the maximum 991.2 mg/kg in Sichuan Province. Besides, there was a great difference among the various kinds of brick tea, and F concentrations decreased in the order of Kang brick tea, Green brick tea, Black brick tea, Mi brick tea, Fu brick tea, Chitsu ping tea, Puerh tea, and Tuo tea. The average F concentration in brick teas was 431.92 mg/kg. 相似文献
16.
Natural Hazards - Despite the application of various methods to calculate uncertainty in flood vulnerability assessments, the challenge of uncertainty remains. The main purpose of this study was to... 相似文献
17.
L. I. Mashonkina A. B. Vinogradova D. A. Ptitsyn V. S. Khokhlova T. A. Chernetsova 《Astronomy Reports》2007,51(11):903-919
We derived Sr, Y, Zr, and Ce abundances for a sample of 74 cool dwarfs and subgiants with iron abundances, [Fe/H], between 0.25 and ?2.43. These estimates were obtained using synthetic spectra, assuming local thermodynamic equilibrium (LTE) for Y, Zr, and Ce, allowing for non-LTE conditions for Sr. We used high-resolution (λ/Δλ?40 000 and 60 000) spectra with signal-to-noise ratios between 50 and 200. We find that the Zr/Y, Sr/Y, and Sr/Zr ratios for the halo stars are the same in a wide metallicity range (?2.43 ≤ [Fe/H] ≤ ?0.90), within the errors, indicating a common origin for these elements at the epoch of halo formation. The Zr/Y ratios for thick-disk stars quickly decrease with increasing Ba abundance, indicating a lower rate of production of Zr compared to Y during active thick-disk formation. The thick-disk and halo stars display an increase in the [Zr/Ba] ratio with decreasing Ba abundance and a correlation of the Zr and Eu overabundances relative to Ba. The evolutionary behavior of the abundance ratios found for the thick-disk and halo stars does not agree with current models for the Galaxy’s chemical evolution. The abundance ratios of Y and Zr to Fe and Ba for thin-disk stars, as well as the abundance ratios within each group, are, on average, solar, though we note a slight decrease of Zr/Ba and Zr/Y with increasing Ba abundance. These results provide evidence for a dominance of asymptotic-giant-branch stars in the enrichment of the interstellar medium in heavy elements during the thin-disk epoch, in agreement with the predictions of the nucleosynthesis theory for the main s-process component. 相似文献
18.
Arsenic concentrations of less than 5 ppb to as large as 1,260 ppb in stream waters and from 5 ppm to 4,000 ppm in stream
sediments were found in the Pedro Dome-Cleary Summit area, Alaska. Waters from three of 20 wells sampled had arsenic concentrations
exceeding the U.S. Public Health Service recommended limit of 50 ppb. The high arsenic levels are a consequence of arsenic
enrichment in the rocks of the area. Placer and lode-gold mining may increase the arsenic content of the waters by exposing
arsenic-containing rocks to surface waters and by increasing the load of arsenic-rich sediments in the streams. Finding these
disturbingly large concentrations of arsenic in the waters of the Fairbanks area was the major result of this work, inasmuch
as a subsequent study (to be published) revealed arsenic concentrations as large as 10 ppm in domestic wells and prompted
an extensive study by Federal and State agencies of the health hazard posed by these arsenic-rich waters. 相似文献
19.