宾川小龙潭斑岩铜矿找矿方向思考     

张金学  王文超  雷阳艾  梅朴莲 《云南地质》2009,28(4):409-414

小龙潭近东西向核桃箐断层对岩体的控制起主导作用。核桃箐沟以北的斑岩露头总体为“模式”的外带。结合核桃箐沟断层的性质及其对地貌的影响,提出进一步找矿重点应转移至核桃箐沟南侧探寻斑岩体核部,打破在F2以北找矿的瓶颈,有望取得找中大型斑岩铜矿的突破。  相似文献   

Sound velocity of Fe3C at high pressure and high temperature determined by inelastic X-ray scattering     

《Comptes Rendus Geoscience》2019,351(2-3):190-196

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Classification of lacustrine sediments based on sedimentary components   总被引：2，自引：12，他引：2  

Douglas Schnurrenberger  James Russell  Kerry Kelts 《Journal of Paleolimnology》2003,29(2):141-154

This paper introduces a flexible sediment classification scheme for modern and ancient lake sediments employed at the Limnological Research Center, University of Minnesota. Our classification scheme emphasizes the macroscopic structure and microscopic components of the sedimentary matrix (clastic, chemical and biological) and can be applied to a wide range of lacustrine settings. Such a classification scheme is necessary to i) facilitate communication and collaboration between the highly interdisciplinary community of scientists that study lacustrine archives, ii) create a structure for comparative lacustrine sedimentological studies, and iii) take greater advantage of the great potential information recorded by changing depositional environments. Such a development is needed in light of current and planned Global Lake Drilling efforts and to expedite the creation of on-line, searchable databases of global lacustrine archives. A more comprehensive treatment of the topics discussed in this paper is available at: http://lrc.geo.umn.edu/services/handbook/sedclass.html.  相似文献   

Evidence and cause of climate cycles in polar motion     

H. Jochmann  E. Felsmann 《Journal of Geodesy》2001,74(10):711-719

 The long-term variation of polar motion contains a number of periods similar to climate cycles. Two possible causes for these long-term variations are mass redistributions produced by variations of atmospheric and oceanic circulation, and mass exchanges between the cryosphere and hydrosphere. Inner-core wobble, which can be inferred from the observed motion of the geomagnetic pole, is another phenomenon with periods similar to climate cycles. Only observations relating to mass redistributions caused by atmosphere dynamics and inner-core wobble are available for sufficiently long periods of time to investigate their influence on climate cycles in polar motion. Both processes contribute to climate cycles in polar motion, but they cannot completely explain these cycles. Possible sources of climate cycles are discussed. Received: 20 December 1999 / Accepted: 28 August 2000  相似文献   

Closure of the Fe-S-Si liquid miscibility gap at high pressure     

C. Sanloup 《Physics of the Earth and Planetary Interiors》2004,147(1):57-65

A high pressure investigation of melting relationships in the Fe-S-Si system has been conducted in a multi-anvil apparatus from 10 to 27 GPa and up to 2343 K. At 1 atm, the Fe-S-Si ternary system exhibits a vast miscibility gap [Raghavan, V., 1988. Phase diagrams of ternary iron alloys. Part 2: Ternary systems containing iron and sulphur. Indian Institute of Metals, Calcutta]. Quenched samples from experiments conducted at 10 and 12 GPa show an emulsion of immiscible liquids (an Fe-S melt and an Fe-Si melt). The liquid miscibility gap persists to at least 2343 K at 10 GPa. At 15 GPa, only one liquid is quenched, with a fine homogeneous dendritic texture. The results provide a mechanism to incorporate both S and Si as the light elements into the Earth’s core during a moderately high-pressure differentiation, consistent with geochemical models predicting up to 15 wt.% of light elements in the Earth’s core with 2-5 wt.% S and 7-10 wt.% Si. In contrast, for small planets such as Mars and Ganymede, differentiation took place within the pressure range of the miscibility gap. The composition of these cores is likely to be S-rich but Si-poor.  相似文献   

中国沉积学的今后发展:若干思考与建议   总被引：4，自引：0，他引：4  

颜丹平  周美夫  宋鸿林  刘敦一  王彦斌  汪昌亮  董铁柱 《地学前缘》2005,12(2):0-0

出露于北京西山房山岩体南北两侧的官地杂岩,主要由正片麻岩、斜长角闪岩组成,局部具混合岩化特征。对官地杂岩的形成时代及出露原因一直存在很大的争议。一种观点认为官地杂岩形成时代为太古宙,出露于中生代早期的区域伸展体制下,另一种观点则认为官地杂岩是中新元古界或古生界泥质变质岩,在房山岩体侵位过程中发生接触变质作用的产物。研究表明,官地杂岩是一套正片麻岩,其中的锆石核部为岩浆成因,而外部普遍发育较窄的浅色边。SHRIMP II锆石铀铅年龄测定获得锆石的一致曲线与不一致曲线上交点年龄值为(2 521 ±20) Ma,代表了新太古代的岩浆结晶年龄,从而证明官地杂岩原岩形成于新太古代。构造分析表明,官地杂岩与上覆中元古代蓟县系至早古生代地层间为剥离断层接触关系,并为房山岩体侵位和改造,证明是一个形成于房山岩体侵位前的变质核杂岩构造。但房山岩体的侵位并未对锆石的岩浆年龄和变质年龄产生明显影响。  相似文献   

Orientation,composition, and entrapment conditions of fluid inclusions in the footwall of the northern Snake Range detachment,Nevada     

《Journal of Structural Geology》2015

Footwall rocks of the northern Snake Range detachment fault (Hampton and Hendry's Creeks) offer exposures of quartzite mylonites (sub-horizontal foliation) that were permeated by surface fluids. An S–C–C′ mylonitic fabric is defined by dynamically recrystallized quartz and mica. Electron backscatter diffraction analyses indicate a strong preferred orientation of quartz that is overprinted by two sets of sub-vertical, ESE and NNE striking fractures. Analyses of sets of three perpendicular thin sections indicate that fluid inclusions (FIs) are arranged according to macroscopic fracture patterns. FIs associated with NNE and ESE-striking fractures coevally trapped unmixed CO₂ and H₂O-rich fluids at conditions near the critical CO₂–H₂O solvus, giving minimum trapping conditions of T = 175–200 °C and ∼100 MPa H₂O-rich FIs trapped along ESE-trending microcracks in single crystals of quartz may have been trapped at conditions as low as 150 °C and 50 MPa indicating the latest microfracturing and annealing of quartz in an overall extensional system. Results suggest that the upper crust was thin (4–8 km) during FI trapping and had an elevated geotherm (>50 °C/km). Footwall rocks that have been exhumed through the brittle-ductile transition in such extensional systems experience both brittle and crystal-plastic deformation that may allow for circulation of meteoric fluids and grain-scale fluid–rock interactions.  相似文献   

The wetting ability of Si-bearing liquid Fe-alloys in a solid silicate matrix—percolation during core formation under reducing conditions?     

Ute Mann  Daniel J. Frost  David C. Rubie 《Physics of the Earth and Planetary Interiors》2008,167(1-2):1-7

The wetting characteristics of liquid Fe–Si alloys in a matrix of the respective predominating stable silicate mantle mineral (forsterite or silicate perovskite) at pressures of 2–5 and 25 GPa and temperatures of 1600–2000 °C were studied by determining the liquid metal–solid silicate contact angles. The median angle values from texturally equilibrated samples were found to be independent of pressure, temperature, silicate mineralogy and the Si content in the metal fraction and range between 130° and 140° which is far above the critical wetting boundary of 60°. This shows that within the studied range of conditions dissolved Si does not lower the surface energies between Fe-rich liquids and silicate mantle grains. As a consequence, under reducing conditions the presence of Si in the metal phase of planetary bodies would not have enhanced percolative flow as an effective metal–silicate separation process.  相似文献   

Effects of an outer thin stably stratified layer on planetary dynamos     

Sabine Stanley  Aylia Mohammadi 《Physics of the Earth and Planetary Interiors》2008,168(3-4):179-190

The presence of outer stably stratified layers in planetary cores has been suggested for Earth, Saturn and Mercury. In this study, we use a 3-D numerical dynamo model to investigate the effects of a thin stable layer surrounding a convecting interior on the produced magnetic field. We find that a stable layer can destabilize the field morphology through a thermal wind that produces unfavorable zonal flows throughout the core. The direction of these zonal flows is prograde in equatorial regions, unlike a model with no stable layer that has retrograde equatorial flows. Our models therefore suggest that the Earth does not have a stable layer since we observe a westward drift as opposed to an eastward drift. For Saturn, we find that due to coupling of the flows in the stable and unstable layers, the layer does not act to shear out the non-axisymmetry in the observed magnetic field, and therefore cannot explain Saturn’s axisymmetric magnetic field. For Mercury, we find that if the stable layer is thin, it can actively produce strong or weak surface fields and not necessarily attenuate smaller scale features through the skin effect.  相似文献   

东南印度洋中脊(108°—134°E区域)断层构造与岩浆活动关系     

刘守金  林间  罗怡鸣 《热带海洋学报》2019,38(4):70-80

东南印度洋脊(Southeast Indian Ridge, 简称SEIR)是中速扩张洋中脊, 在其中的108°—134°E区域的全扩张速率为72~76 mm·a ^-1。但在接近澳大利亚-南极洲不整合带(Australian-Antarctic Discordance, 简称AAD)区内, 海底地貌沿洋中脊的变化强烈, 其变化范围涵盖了从慢速到快速扩张洋中脊上常见的例子, 且出现了明显的地球物理与地球化学异常, 说明洋中脊在AAD区附近的岩浆供应量极不均匀。文章定量分析了高精度多波束测深数据, 计算了洋中脊不同段的地形坡度、断层比例以及平面与剖面的岩浆参数M值, 结合研究区内剩余地幔布格重力异常以及洋中脊轴部地球化学指标Na_8.0、Fe_8.0等资料, 分析与讨论了研究区的断层构造与岩浆活动特征的关系。研究发现, 东南印度洋脊108°—134°E区域的B区(在AAD区内)及C5段(在AAD区外西侧)发育有大量的海洋核杂岩, 而且B区的海洋核杂岩单体规模更大, 其中最大的位于B3区, 沿洋中脊扩张方向延伸约50km。研究结果首次系统性地显示, 相比东南印度洋的其他区域, B和C5异常区具有偏低的平面与剖面M值、偏高的断层比例、偏正的地幔布格重力异常以及偏高的Na_8.0值与偏低的Fe_8.0值, 这些异常特征可能反映了B区和C5段的岩浆初始熔融深度较浅以及岩浆熔融程度较低, 因此导致其岩浆供应量异常少, 形成较薄的地壳。研究结果同时表明, 在岩浆供应量极少的洋中脊, 构造伸展作用有利于海洋核杂岩的发育, 导致地壳进一步减薄。  相似文献