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Abstract. Scanning electron microscopy-cathodoluminescence (SEM-CL) imaging of vein quartz in the Cu-mineralised, Shuteen Complex (South Gobi, Mongolia) has revealed a complex history of crystal growth, dissolution and microfracture healing, associated with several hydrothermal events that could not be detected using other observational techniques (e.g. transmitted/reflected light microscopy, back-scattered electron imaging, or secondary electron imaging).
The quartz initially grew as CL-bright/grey crystals in a 345±30C liquid reservoir, as inferred by the analysis of primary liquid fluid inclusions (average Th of 343C; 6.6∼7.7 wt% NaCleq ). Quartz precipitation occurred at the edge of the crystals as reservoir fluids cooled to 260±25C, as indicated by micron-scale CL-dark/CL-bright quartz growth bands containing abundant fluid inclusions (with an average Th values of 261C). Pressure fluctuations were the likely cause of dissolution, as SEM-CL imaging reveals the quartz have corroded or rounded crystal edges, and precipitation of later quartz into open space. SEM-CL imaging shows the quartz contains healed microfractures that trapped low salinity fluids (3.9 wt% NaC1eq ) with Th values of 173±15C.
SEM-CL imaging provides a means of deciphering the thermal and chemical evolution of the fossil Shuteen hydrothermal system, and the nature of hydrothermal quartz vein-forming processes, by facilitating the correlation of distinct fluid inclusion populations and their relative chronology, with specific hydrothermal events. 相似文献
The quartz initially grew as CL-bright/grey crystals in a 345±30C liquid reservoir, as inferred by the analysis of primary liquid fluid inclusions (average Th of 343C; 6.6∼7.7 wt% NaCl
SEM-CL imaging provides a means of deciphering the thermal and chemical evolution of the fossil Shuteen hydrothermal system, and the nature of hydrothermal quartz vein-forming processes, by facilitating the correlation of distinct fluid inclusion populations and their relative chronology, with specific hydrothermal events. 相似文献
105.
The Clementine spacecraft orbited the Moon and acquired science data for 10 weeks in the Spring of 1994. During this time
it collected global 11-band multispectral images and near global altimetry. Select areas of the Moon were imaged at 25 m/pixel
in visible light and 60 m/pixel in thermal wavelengths. From these datasets a new paradigm for the evolution of the lunar
crust emerged. The Moon is no longer viewed as a two-terrane planet, the Apollo samples were found not to represent the lunar
crust as a whole, and the complexity of lunar crustal stratigraphy was further revealed. More than ten years later the Clementine
datasets continue to significantly advance lunar science and will continue to do so as new measurements are returned from
planned missions such as Chandrayaan, SELENE, and Lunar Reconnaissance Orbiter. This paper highlights the scientific research
conducted over the last decade using Clementine data and summarizes the influence of Clementine on our understanding of the
Moon. 相似文献
106.
S. C. Tarantino M. Zema F. Maglia M. C. Domeneghetti M. A. Carpenter 《Physics and Chemistry of Minerals》2005,32(8-9):568-577
A suite of (Mn1-x
Fe
x
)Nb2O6 (x=0, 0.05, 0.25, 0.50, 0.75, 1) columbite samples has been prepared by solid-state reaction from oxides. X-ray diffraction
and spectroscopic investigations have been carried out in order to gain different perspectives on how the solid solution adapts
at different length scales to cation mixing. X-ray powder diffraction and powder absorption IR spectroscopy data are presented.
The powder diffraction data show that there is no significant excess volume of mixing on the Fe–Mn columbite join. All the
unit-cell parameters decrease linearly as a function of increasing Fe content. Substitution of Fe2+ for the larger Mn2+ cation causes a decrease in the volume of the A polyhedron, which also becomes more regular with respect to both bond-length
and edge-length distortion parameters. No significant variation of the B site has been observed. Wavenumber shifts of the
IR peaks nearly all vary linearly with composition, consistent with linear variations of the lattice parameters. Line broadening
has been quantified by autocorrelation analysis of the IR spectra. This is interpreted as suggesting that there is some element
of local strain or positional disorder at the length scale of second or third nearest neighbours around sites occupied by
Fe. 相似文献
107.
X射线荧光光谱法分析不同类型岩石中10种主量元素的测试能力验证 总被引:4,自引:3,他引:1
以28个不同类型岩石标样作外标,用玻璃熔片法制样,采用经验系数法进行基体校正,建立了X射线荧光光谱法(XRF)测定不同类型岩石中硅铝钙镁等10种主量元素的分析方法。该方法被用于参与GeoPT分析测试能力验证,15年来分析了23个不同类型的岩石验证样品。经验证该方法对SiO_2、Al_2O_3、K_2O和CaO具有非常好的分析效果(所有测定结果的|Z|2);对于MgO、MnO、TiO_2和Na_2O四个元素,尽管各有一个样品的分析结果的|Z|2,这主要是样品与标样的基体差异较大造成了低含量样品测定结果超差,但依然可获得好的分析效果;当TFe_2O_31.0%,P_2O_5含量在0.08%~0.80%区间时,分析结果的|Z|2,满足分析期望。总体上所建立的XRF分析方法稳定,可满足应用地球化学实验室测试不同类型岩石中10种主量元素的分析期望。 相似文献
108.
X射线荧光光谱-电子探针在中酸性火山岩鉴定中的应用 总被引:2,自引:1,他引:1
中酸性火山岩多具斑状结构,基质可见微晶状结构、隐晶状结构、玻璃质结构等,由于基质矿物颗粒多细小,常用的偏光显微镜受放大倍数的限制,很难准确鉴定矿物种属及含量,这类岩石仅依靠偏光显微镜分类命名会存在误差。本文采用X射线荧光光谱(XRF)、电子探针(EMPA)和偏光显微镜下观察相结合的方法,对中酸性火山岩进行鉴定。结果表明:对于基质呈隐晶质、显微晶质的中酸性火山岩,基质特征相似,偏光显微镜下无法确定长石、石英的含量,因此无法对岩石准确命名;再通过XRF进行主量元素分析,并对分析结果进行标准矿物QAPF双三角图解分类、TAS图解分类及李氏火山岩定量分类,对比结果显示三种分类命名方法存在差异;通过电子探针对矿物进行校验显示,QAPF及李氏火山岩定量分类图解与显微镜下鉴定相符,TAS图解与其他分析结果存在一定偏差。因此,对于中酸性火山岩准确命名,应采用多种分析方法相结合的方式,避免测试单一引起的误差。 相似文献
109.
该文回顾了环境气象卫星可见光红外光学成像遥感仪器50多年的发展历程,从不同时期在轨运行的近百台 (套) 仪器中选择了12种作为代表,结合仪器功能性能技术指标和应用需求梳理分析了其历史发展脉络和主流业务发展趋势,并初步探讨了创新发展方向。50多年的发展可以分为3个阶段:早期探索20年, 美国第1代探索性仪器,开创了气象卫星对地观测的先河;初步应用20年, 基本形成初步应用格局,欧洲、中国等开始发展自己的环境气象卫星光学成像遥感仪器;稳定应用和进步发展10多年。新一代极轨卫星可见光红外光学成像遥感仪器,其典型特征是光谱波段20个以上,谱段带宽窄,光谱范围全面覆盖0.4~15 μm,辐射测量精度高,空间分辨率为200~1000 m,其改进型仪器代表了未来极轨气象卫星主流业务发展趋势。静止气象卫星可见光红外光学成像遥感仪器未来主流业务发展方向的典型特点是光谱波段15个以上,谱段带宽较窄,光谱范围全面覆盖0.4 ~15 μm,辐射测量精度高,空间分辨率为500~2000 m,圆盘图成像速度可达到分钟级,区域扫描速度更快。 相似文献
110.