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71.
西藏驱龙斑岩铜钼矿地球化学异常特征 总被引:6,自引:0,他引:6
驱龙铜矿发育多元素的岩石地球化学异常.成矿元素Cu、Mo、(Ag)异常强、规模大,异常与矿化区一致;伴生元素Au、Bi、Pb、As、Sb、Hg异常在Cu、Mo异常边部并套合产出的B Co、Ni Mn Zn的异常主要分布铜钼矿化带外侧.Na2O在矿化区显示负异常,K2O为正异常.从异常元素组合、水平分带性和贫Na2O、富K2O的成矿环境表明,矿床属典型的斑岩型铜矿地球化学特征,并受到了强烈的剥蚀. 相似文献
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区域土壤环境地球化学研究——异常成因判别·环境质量·污染程度评价的思路与方法 总被引:8,自引:2,他引:8
从概念内涵和应用目标出发,认为土壤环境地球化学质量评价应该分为质量现状和污染程度两个方面.在此基础上探讨了区域地球化学资料在土壤环境现状质量评价、异常成因识别、污染元素累积速率和土壤污染程度评价研究的基本思路和方法. 相似文献
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化探异常中选优评价成为目前地质勘查中的关键技术难题之一,以东疆觉罗塔格成矿带库姆塔格—沙泉子测区岩屑地球化学综合异常优选排队为例,讨论了化探异常优选排队新方法。在区域成矿地质背景和地球化学背景研究的基础上,采用地质地球化学预测系统新技术思路和方法,对本区130个化探异常进行了优选排队,筛选出36个有望异常和7个成矿远景区。对优选出的有望异常进行检查评价和工程验证均发现地表含金铜蚀变矿(化)体,说明所提出的化探异常优选排队新方法是有效可行的。 相似文献
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Merapi Volcano (Central Java, Indonesia) has been frequently active during Middle to Late Holocene time producing basalts and basaltic andesites of medium-K composition in earlier stages of activity and high-K magmas from 1900 14C yr BP to the present. Radiocarbon dating of pyroclastic deposits indicates an almost continuous activity with periods of high eruption rates alternating with shorter time spans of distinctly reduced eruptive frequency since the first appearance of high-K volcanic rocks. Geochemical data of 28 well-dated, prehistoric pyroclastic flows of the Merapi high-K series indicate systematic cyclic variations. These medium-term compositional variations result from a complex interplay of several magmatic processes, which ultimately control the periodicity and frequency of eruptions at Merapi. Low eruption rates and the absence of new influxes of primitive magma from depth allow the generation of basaltic andesite magma (56–57 wt% SiO2) in a small-volume magma reservoir through fractional crystallisation from parental mafic magma (52–53 wt% SiO2) in periods of low eruptive frequency. Magmas of intermediate composition erupted during these stages provide evidence for periodic withdrawal of magma from a steadily fractionating magma chamber. Subsequent periods are characterised by high eruption rates that coincide with shifts of whole-rock compositions from basaltic andesite to basalt. This compositional variation is interpreted to originate from influxes of primitive magma into a continuously active magma chamber, triggering the eruption of evolved magma after periods of low eruptive frequency. Batches of primitive magma eventually mix with residual magma in the magmatic reservoir to decrease whole-rock SiO2 contents. Supply of primitive magma at Merapi appears to be sufficiently frequent that andesites or more differentiated rock types were not generated during the past 2000 years of activity. Cyclic variations also occurred during the recent eruptive period since AD 1883. The most recent eruptive episode of Merapi is characterised by essentially uniform magma compositions that may imply the existence of a continuously active magma reservoir, maintained in a quasi-steady state by magma recharge. The whole-rock compositions at the upper limit of the total SiO2 range of the Merapi suite could also indicate the beginning of another period of high eruption rates and shifts towards more mafic compositions. 相似文献
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William J. Chazey III Clive R. Neal Jinesh C. Jain William S. Kinman 《Geostandards and Geoanalytical Research》2003,27(2):181-192
The geochemical reference material BHVO-1 was analysed by a variety of techniques over a six year period. These techniques included inductively coupled plasma-mass spectrometry and atomic emission spectroscopy (ICP-MS and ICP-AES, respectively), laser ablation ICP-MS and spark source mass spectroscopy. Inconsistencies between the published consensus values reported by Gladney and Roelandts (1988, Geostandards Newsletter) and the results of our study are noted for Rb, Y, Zr, Pb and Th. The values reported here for Rb, Y, Zr and Pb are generally lower, while Th is higher than the consensus value. This is not an analytical artefact unique to the University of Notre Dame ICP-MS facility, as most of the BHVO-1 analyses reported over the last ten to twenty years are in agreement with our results. We propose new consensus values for each of these elements as follows: Rb = 9.3 ± 0.2 μg g-1 (compared to 11 ± 2 μg g-1), Y = 24.4 ± 1.3 μg g-1 (compared to 27.6 ± 1.7 μg g-1), Zr = 172 ± 10 μg g-1 (compared to 179 ± 21 μg g-1), Pb = 2.2 ± 0.2 μg g-1 (compared to 2.6 ± 0.9 μg g-1) and Th = 1.22 ± 0.02 μg g-1 (compared to 1.08 ± 0.15 μg g-1). 相似文献
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