元岭金矿蚀变破碎带特征及其找矿意义     

刘红樱  周顺之  胡受奚  王群昌 《河南国土资源》1996,(2)

根据对元岭金矿三条蚀变破碎带一般地质特征、微量元素特征的对比研究，并借鉴邻近矿区蚀变破碎带的矿化特征，本文阐明了元岭蚀变破碎带矿化的有利构造部位，总结了蚀变破碎带特征与矿化强度之间的关系，指出蚀变破碎带的矿化蚀变元素为中低温组合，矿化蚀变愈强则参与元素的种类愈多、数量愈大。围岩性质对矿化蚀变有一定影响，围岩中的易迁移亲铜元素和亲硫铁族无素对矿化有利。据此，为进一步成矿预测、评价蚀变破碎带的含矿性提供依据。  相似文献   

云南省红土型金矿床找矿前景     

吕伯西 《四川地质科技情报》1997,(1):27-29

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地壳不同时代构造单元黑色页岩层含金性的比较分析     

龙长林  余新 《国外铀金地质》1996,13(1):33-42

碳质陆源火山岩层中常产有大型金矿床，目前对研究黑色页岩层的含金性给予很大的注意。本文研究了西伯利亚地台元古代盆地中金矿田碳质陆源岩石内金的分布和含铜的碳质陆源建造内岩石的金分布，还收集了地球上其他地区有关碳质生成物的本底含金性。在此基础上，发现具有不同矿化黑色页岩建造的地球化学差异，以及地壳不同构造单元内同类型碳质岩石中金含量的时代变异性。  相似文献   

冲积扇形砂金矿床     

檀国平 《国外铀金地质》1992,(2):25-26

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内蒙额仁陶勒盖银矿床含银性的红外光谱评价     

张培萍  朱钟秀 《长春地质学院学报》1993,23(3):319-322

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东坪金矿黄铁矿晶体形态填图与评价预测          下载免费PDF全文

张齐道 《地质与勘探》1993,29(7):40-41

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发展超硬材料产业是地勘延伸业走向市场的有利趋向          下载免费PDF全文

舒全安 《地质与勘探》1993,29(7):54-55,34

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谈地勘经济改革与发展的现状和走势          下载免费PDF全文

张自俊  许智迅 《地质与勘探》1993,29(5):1-5

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金矿床的热液流体特征研究     

王建国  孙丽娜  赵玉山  侯根群  赵纯福 《国土资源》1993,(4)

通过对中国东部金成矿区域地质特征的分析,根据氢氧同位素及流体包裹体数据特征,表明中国东部金矿床成矿流体主要来自大气降水,其次为变质作用过程释放的水和岩浆分异水;成矿金属组分主要来自太古宙变质岩系。  相似文献   

Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions     

Chang－XiZhang  G.B.Gelfreikh 《中国天文和天体物理学报》2002,2(3):266-276

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.  相似文献