共查询到18条相似文献，搜索用时 125 毫秒
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针对找矿指标的有效性和找矿模型的普适性问题,研究引入热磁技术,以乌努格吐山铜矿和丰山洞铜矿为例,对比分析了土壤热磁组分与岩石、岩石热磁组分与黄铁矿的元素组合。试验表明,在确定成矿指示元素组合方面,土壤热磁组分是一种可行的介质,相比岩石具有更高的元素含量,可以挖掘出更多的异常信息;而岩石热磁组分与黄铁矿则具有一致的元素组合,比较而言,岩石热磁组分具有更宽的适用范围(如风化岩石)。作为一种人工方法分离组分,热磁组分弥补了岩石或黄铁矿等自然介质本身所固有的一些不足,为成矿指示元素的选择提供了一个新的研究平台;对于确定同一类型矿床有效指示元素组合,解决找矿模型的普适性问题,开拓了一种新思路。 相似文献
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利用光学显微镜和带能谱的扫描电子显微镜（SEM）等方法研究了土壤热磁组分的形貌特征、结构、表面性质及矿物组成,并与化学分析相结合,探讨了土壤热磁组分对矿化指示元素的富集作用和机理。研究结果表明,土壤热磁组分以铁锰氧化物为主,是由土壤中非晶质铁锰氧化物转化而来的。通过对土壤、土壤热磁组分、土壤非磁性组分中铁锰氧化物与成矿及其伴生元素的相关关系分析,证实了土壤热磁组分对矿化指示元素的富集作用,为深化土壤热磁组分测量方法的基础理论提供了依据。对比试验结果表明,土壤热磁组分测量较常规土壤测量具有更强的发现由深部矿体引起的微弱矿化信息的能力。 相似文献
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雄安新区地热资源潜力大,碳酸盐岩是雄安新区深部地热资源的有利储层,综合地球物理勘查方法是查明深部构造与碳酸盐岩热储特征地层结构的有效途径。本文针对深部碳酸盐岩热储勘查目标,提出了“面—线—点”分层次渐进式地球物理探测模式,先利用高精度重力和航磁资料研究碳酸盐岩分布范围及地层厚度、深大断裂分布、基岩起伏等信息,然后利用大地电磁开展热储地层低阻异常特征分析,再利用二维地震剖面精细刻画热储地层,分析地热田异常区速度结构和区域构造特征。根据重力、航磁、大地电磁、地震等地球物理方法在地热资源勘查的不同阶段勘探的精度及可靠性,以及施工成本、施工效率等因素,开展了地球物理方法探测深部岩溶热储经济适用性分析,并建议在碳酸盐岩地热勘探采用“重力+磁法+大地电磁”的地球物理勘探技术组合方式。 相似文献
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针对运积物覆盖区找矿面临的技术难题,引入土壤热磁组分测量方法,以冀北蔡家营热液型铅锌银矿、东天山沙泉子岩浆型铜镍硫化物矿以及野马泉地区矽卡岩型铁铜多金属矿为例,选择运积物覆盖地段开展剖面及面积性方法试验研究。蔡家营与沙泉子研究区实验结果表明,与常规土壤测量方法获得的弱小异常相比,热磁组分测量地表异常显著,能够很好地反映出深部矿体空间位置及展布形态,具有强化弱异常、发现新异常的优势;野马泉地区试验结果表明,在运积物覆盖达百米以上的已知矿区或勘查区,热磁组分测量均有异常显示,异常元素空间套合较好,并为已知区外围覆盖区找矿勘查提供了新的找矿靶区。经实验证实,土壤热磁组分测量技术为解决运积物覆盖区找矿难题提供了一种行之有效的方法。 相似文献
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本文旨在研究探讨无论借助传统方法，还是借助新的热磁法对包气带土壤和土石受到石油产品地下晶体污染地段制图的可能性。指出热磁方法的显著优点，即热磁法的高速度、大范围采用的可能性、经济实用。 相似文献
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安徽铜陵冬瓜山矿床中磁黄铁矿矿石结构特征及其成因意义 总被引：9，自引：3，他引：6
安徽铜陵冬瓜山矿床是长江中下游地区具有代表性的大型层状硫化物矿床,磁黄铁矿为矿床中的主要硫化物矿物.该矿床主要由层状硫化物矿体组成,伴有矽卡岩型和斑岩型矿体.在层状矿体上部,磁黄铁矿主要为块状构造,而层状矿体下部,磁黄铁矿多为层纹状、条带状构造,具有显著的沉积结构构造特征.野外地质观察及室内矿相学研究表明,层状矿体中磁黄铁矿矿石遭受了强烈的变质作用及热液交代作用.进变质过程中形成的结构主要为胶黄铁矿转变为黄铁矿以及进一步变质转变为磁黄铁矿、磁铁矿时形成的交代残留结构.退变质过程则以磁黄铁矿的退火、黄铁矿变斑晶的生长和单纯六方磁黄铁矿的形成为特征.岩浆热液对单纯六方磁黄铁矿的交代作用形成了单斜和六方磁黄铁矿的交生结构.这些结构特征表明层状矿体中的磁黄铁矿并不是岩浆热液成因,而主要为石炭纪同生沉积胶黄铁矿、黄铁矿在燕山期岩浆侵入所引起的热变质作用下脱硫所形成,并在热变质作用之后又受到岩浆热液的叠加交代.磁黄铁矿的结构特征显示冬瓜山矿床的形成经历了同生沉积、热变质、热液交代等多个阶段,支持其为同生沉积-叠加改造型矿床. 相似文献
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准苏吉花斑岩型铜钼矿床是内蒙古中北部新近发现的铜钼多金属矿床之一。这里对矿区地表土壤热磁组分中元素含量及异常特征进行了研究,结果表明元素异常在平面上出现明显的分带性,以地表矿化露头为中心向外依次为Mo-Cu-W-Te带、Ag-Bi-In-Zn-Cd带及As-Pb-Mn-Sb带,所有元素异常均包含在Fe2O3异常之内。通过土壤热磁组分地球化学测量,共圈出七个多元素组合异常,经野外异常查证,认为土壤热磁组分地球化学异常为有效的地质异常。因此,在风成沙覆盖区应用土壤热磁组分地球化学测量方法,配合多重分形(含量-求和法)和地质累积指数(Igeo)等统计方法,可最大限度消除风成沙干扰,快速、有效地确定异常下限,圈定多元素组合异常,提供有利找矿靶区。 相似文献
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Picroilmenite samples from five kimberlite pipes of the Yakutian kimberlite province have been studied. Point microprobe analyses of two mutually perpendicular profiles of each sample were carried out to study the compositional inhomogeneity of picroilmenite. Thermomagnetic curves were also recorded for each sample. A model for the processing of thermomagnetic curves is proposed on the basis of the relationship between the Curie point of picroilmenite and the content of the hematite end-member. The compositions determined by the thermomagnetic curves and microprobe analysis are rather similar. The conclusion has been drawn that thermomagnetic analysis can be used for the rapid determination of the picroilmenite composition. The possibilities and restrictions of this method are shown. 相似文献
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《Russian Geology and Geophysics》2014,55(3):397-404
A thermomagnetic analysis has been performed for 737 picroilmenite samples from the cores of eight boreholes in the N-S-striking drilling profile of the Zarnitsa kimberlite pipe in the Daldyn kimberlite field, Yakutia. Based on the shapes of thermomagnetic curves and the Curie points, 29 samples were chosen for detailed microprobe studies of chemical composition and elucidation of the dependence of their thermomagnetic parameters on the content of the hematite end-member in the picroilmenites. The thermomagnetic curves of most of the studied picroilmenite samples are approximated by a two-component model for the hematite end-member distribution: the main and supplementary distribution. The average hematite end-member content in the main distribution coincides with the probe microanalysis data and is always lower than the average content in the supplementary distribution. The relative hematite end-member contents in the main and supplementary distributions within the picroilmenite grains are indicators of the dynamics of mineral formation in different parts of the Zarnitsa pipe. The data obtained testify to the multistage formation of the pipe under unstable thermodynamic conditions, which explains the intricate distribution pattern of picroilmenite. 相似文献
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T. A. Sherendo V. Ya. Mitrofanov P. S. Martyshko V. A. Vazhenin L. A. Pamyatnykh A. V. Alekseev 《Doklady Earth Sciences》2014,456(1):563-566
The ore and accessory chrome-spinels from metamorphosed dunites of the Cr-bearing Klyuchevskoi alpine-type ultramafic massif are studied. As a result of use of thermomagnetic analysis in the range of 4–900 K, magnetic resonance spectroscopy, and magnetic-force microscopy, secondary magnetic Fe3+-enriched microphases chaotically distributed in the primary nonmagnetic mineral were revealed for the first time in accessory chrome-spinels. It was established that the metamorphosed accessory chrome-spinels produce the magnetic properties of the host rocks and the primary nonmagnetic chrome-spinels forming ore bodies remains almost unaltered. This originates the contrast of magnetic properties between the ore body and host rocks and provides the geomagnetic anomaly in the ore-hosting zone. 相似文献
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N. S. Bezaeva D. D. Badyukov M. A. Nazarov P. Rochette J. Feinberg 《Geochemistry International》2013,51(7):568-574
This paper presents the distribution of magnetic susceptibility, χ0, in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtained by standard magnetic techniques for the meteorite material, including thermomagnetic analysis, measurements of natural remanent magnetization (NRM) and saturation isothermal remanent magnetization (SIRM), as well as the spectra of their alternating field demagnetization at amplitudes up to 170 mT, measurements of hysteresis loops and back-field remanence demagnetization curves at temperatures from 10 K to 700°C etc. The mean logχ0 values for the light-colored (main) lithology of the meteorite material and impact-melt breccia from our collection are 4.54 ± 0.10 (n = 66) and 4.65 ± 0.09 (n = 38) (×10?9 m3/kg), respectively. According to international magnetic classification of meteorites, Chelyabinsk falls within the range of LL5 chondrites. The mean metal content was estimated from the saturation magnetization, M s, of the light- and dark-colored lithologies as 3.7 and 4.1 wt %, respectively. Hence, the dark lithology is richer in metal. The metal grains are multidomain at room temperature and show low coercive force, B c (<2 mT) and remanent coercive force, B cr (15–23 mT). The thermomagnetic analyses of the samples showed that the magnetic properties of the Chelyabinsk meteorite are controlled mainly by taenite and kamacite at temperatures >75 K. In the temperature range below 75 K, magnetic properties are controlled by chromite; the magnetic hardness of the samples is maximal at 10 K and equals to 606 and 157 mT for the light- and dark-colored lithologies, respectively. 相似文献
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《International Geology Review》2012,54(10):1475-1481
Titanium magnetite and ilmenite begin to crystallize first, but most of these minerals come down concurrently with ferrohedenbergite, after phenocrysts of olivine have already appeared. Crystallization of the ferromagnetic minerals ceases upon solidification of the glass. Evolution and order of crystallization of the magmatic melt itself are indicated by different states of oxidation and decay of the ferromagnetic minerals captured by phenocrysts of olivine, ferrohedenbergite, and sanidine. A primary magnetic origin of independent grains of ilmenite is suggested by their abundance and shape, but thermomagnetic evidence indicates that some of them are products of degradation-oxidation of titanium magnetite. 相似文献
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A. A. Plyashkevich P. S. Minyuk T. V. Subbotnikova A. V. Alshevsky 《Doklady Earth Sciences》2016,467(2):380-383
Newly obtained data from microscopic, geochemical, and thermomagnetic studies of the large Kolyma fulgurite are presented here: the fulgurite was formed in the Holocene as a result of lightning affected black shale alluvium. The composition is very close to that of glass formed from a melt. The glass has elevated concentrations of Y, Zr, Nb, and REEs. The newly formed mineral phases have been identified: those are Al–Si glass, α-cristobalite, moissanite, native iron with a phosphorus admixture, nickel-less shreibersite (?), troilite, and possibly cohenite. The formation of these minerals is related to the melt fractionation and the effects of element concentration and segregation of ore components under conditions of the rock melting caused by the effect of high-energy plasma (lightning strike). 相似文献