玉龙铜矿带马拉松多斑岩体岩石学及成岩成矿系统年代学分析   总被引：9，自引：4，他引：5  

梁华英  莫济海  孙卫东  张玉泉  曾提  胡光黔  Charllote ALLEN 《岩石学报》2009,25(2):385-392

马拉松多斑岩铜钼矿床是玉龙斑岩铜矿带中第二大的大型斑岩铜钼矿床,本文分析了岩体化学组成及用锆石LA-ICP-MS U-Pb法以及黑云母K-Ar法测定了成岩成矿体系同位素年代。赋矿岩体可分为早晚两期, 早期岩体主要由石英二长斑岩及碱长花岗斑岩组成,晚期岩体主要由碱长花岗斑岩组成。早期岩体和晚期岩体在化学组成上有一定的差异,早期岩体富Al₂O₃、MgO、CaO、Na₂O、Fe ₂O₃、TiO₂,晚期岩体则相对富SiO₂及K₂O;马拉松多早期岩体锆石LA-ICP-MS U-Pb年龄(36.9±0.4Ma, MSWD=1.52)与晚期岩体锆石LA-ICP-MS U-Pb年龄（36.9±0.3Ma, MSWD=1.38）相同,也和黑云母K-Ar年龄（36.9±0.6Ma）及前人的辉钼矿Re-Os年龄一致。早期和晚期岩体是在现有同位素体系难以区别的相同的时间间隔内脉动侵入形成的,马拉松多成岩成矿系统在很短时期内从高温（800℃,锆石U-Pb封闭温度）冷却至中低温（300℃黑云母Ar同位素体系的封闭温度）,成岩成矿时间跨度小于1Ma。玉龙矿带主要赋矿岩体锆石年龄表明,玉龙斑岩铜矿带岩浆活动时间跨度4.3Ma内,约发生过四次成岩成矿事件。  相似文献   

西藏冈底斯南部陆陆碰撞早期成矿作用分析   总被引：4，自引：0，他引：4  

黄文婷  梁华英  伍静  王春龙  邹银桥  王秀璋  许继峰  Charllote M ALLEN 《岩石学报》2013,29(4):1439-1449

冈底斯带南部发育有大量的斑岩铜钼矿床和矽卡岩型铜铅锌多金属矿床,形成了斑岩铜矿带和多金属矿带.前人的研究表明,成矿带内的矿床形成年代大都小于30Ma,处于碰撞后期伸展构造环境.本文对冈底斯带中南部的甲龙矽卡岩型铁矿、撒当金银矿床(点)和多底沟矽卡岩型钼矿床(点)开展了年代学研究,结果显示:甲龙铁矿黑云母二长花岗斑岩的锆石LA-ICP-MS U-Pb年龄为61.1 ±0.4Ma,MSWD=0.94;撒当赋矿安山岩锆石LA-ICP-MS U-Pb年龄为62.6±0.5Ma,MSWD=1.51;多底沟钼矿床(点)3件辉钼矿Re-Os模式年龄为64.3±0.8Ma ～ 69.2±3.3Ma,加权平均模式年龄为66.7±6.4Ma(MSWD=8.1).三个矿床(点)的同位素年龄表明成岩成矿事件和印度-欧亚板块陆陆碰撞早期构造岩浆事件有关.结合前人工作,我们提出冈底斯中南部发生了大规模与陆陆碰撞早期岩浆事件有关的成矿作用,形成了大面积分布的矿床,具有良好的找矿前景,应引起更多关注.  相似文献   

INTENSITY OF DEPOSITION FROM AVALANCHES AND THE LOOSE PACKING OF AVALANCHE DEPOSITS     

J. R. L. ALLEN 《Sedimentology》1972,18(1-2):105-111

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A strong regional temperature signal in low‐elevation Huon pine     

K. J. ALLEN  D. M. DREW  G. M. DOWNES  R. EVANS  E. R. COOK  M. BATTAGLIA  P. J. BAKER 《第四纪科学杂志》2013,28(5):433-438

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Modelling of cyclic tidal rhythmites (Carboniferous of Indiana and Kansas, Precambrian of Utah, USA) as a basis for reconstruction of intertidal positioning and palaeotidal regimes   总被引：4，自引：0，他引：4  

ALLEN W. ARCHER  TROY W. JOHNSON 《Sedimentology》1997,44(6):991-1010

Analyses are presented for a variety of ancient cyclic tidal rhythmites, which exhibit well developed neap-spring tidal periods. Many such rhythmites were formed within the upper intertidal zone and exhibit truncated cycles that contain relatively few discrete lamina per neap-spring cycle. In such cases it can be difficult to determine if the originated palaeotidal system was diurnal or semidiurnal. Based on sedimentological controls observed in modern analogues, the development of cyclic tidal rhythmites can be modelled by use of predicted tidal-height information. The modelling used a 19-year-long series of tidal heights, which were subsequently used to approximate tidal velocities and rhythmite sedimentation. Modelling was based on a range of diurnal to semidiurnal regimes and comparisons were performed at a number of levels within the intertidal zone. This modelling produced a long series of simulated laminae-thickness series which could be cross-correlated with ancient laminae-thickness series measured directly from ancient rhythmites. This approach involved 1.6 × 10⁶ comparisons of each ancient rhythmite series to the series simulated from the predictive tidal-height information. The high correlations derived for such comparisons indicate that reasonable approximations to the palaeotidal systems can be made. In some cases, it is possible to determine the diurnal or semidiurnal nature of the originating palaeotidal system.  相似文献   

Two-stage corona growth during Precambrian granulite facies metamorphism of Smitbson Bjerge, north-west Greenland     

ADAM A. GARDE  WILLIAM E. GLASSLEY  ALLEN P. NUTMAN 《Journal of Metamorphic Geology》1984,2(3):237-247

Abstract Late Archaean orthogneisses and aluminous and iron-rich metasedimentary rocks intruded by anorthosite and a ferrodiorite-granite suite were completely recrystallized during Proterozoic granulite facies metamorphism. Geobarometry and geothermometry indicate P-T conditions of around 7.5kbar. 700°C, with a CO₂-rich fluid phase and logfO₂ at or below -16. A two-stage high-grade history of near isochemical corona growth is preserved in metasediments with the reaction cycle opx + plag + H₂O → hbl+gar+SiO₂→ opx+plag+H₂O. End product compositions resemble those of the initial phases, and the only mobile components were SiO₂ and/or H₂O. The coronas reflect shortlived fluctuations in chemical activity at essentially constant P and T, contrary to simple progressive change in equilibrium parameters recorded by most corona-bearing textures.  相似文献   

A Study on Retrieving Atmospheric Profiles from EOS/AIRS Observations   总被引：5，自引：0，他引：5  

GUAN Li  ALLEN Huang  LI Jun 《Acta Meteorologica Sinica》2005,19(1):112-119

1. IntroductionThe development of global climate and weathermodels requires accurate monitoring of atmospherictemperature and moisture profiles, as well as the con-tents of trace gases and aerosols. It is quite difficultto monitor continuously these parameters on a globalscale.Until recently. AIRS (Atmospheric InfraredSounder) offers a new opportunity to improve globalmonitoring of temperature, moisture, and ozone distri-butions and changes therein. The high spectral resolu-tion (v/Δv ? 12…  相似文献   

青藏高原东缘中新生代龙门山前陆盆地动力学及其与大陆碰撞作用的耦合关系   总被引：15，自引：1，他引：15  

李勇  P.A.ALLEN  周荣军  A.L.DENSMORE  M.A.ELLIS 《地质学报》2006,80(8):1101-1109

位于青藏高原东缘的龙门山前陆盆地是中国典型的前陆盆地之一。自晚三叠世以来,该盆地充填了厚度大于1万余米的海相至陆相沉积物,以不整合面为界可将其划分为6个构造层序,根据几何形态将构造层序区分为两种类型,即楔状构造层序和板状构造层序,其中晚三叠世、晚侏罗世、晚白垩世—古近纪构造层序为楔状构造层序,其余为板状构造层序。研究结果表明楔状构造层序为逆冲构造负载的产物,板状构造层序为走滑剥蚀卸载的产物。本次以晚三叠世前陆盆地为典型的楔状前陆盆地开展了逆冲构造负载系统的弹性挠曲动力学模拟,以晚新生代龙门山前陆盆地为典型的板状前陆盆地开展了与走滑剥蚀卸载系统的弹性挠曲动力学模拟,并计算了龙门山构造负载系统向扬子克拉通的推进速率,结果表明龙门山造山楔的推进速率在早期较快(如晚三叠世最大推进速率达15mm/a),晚期较慢(如晚侏罗世、晚白垩世—古近纪最大推进速率仅为6.7mm/a)。进而推测龙门山幕式逆冲作用的构造驱动力来自于青藏高原中生代以来的基麦里大陆加积碰撞和印度与亚洲板块碰撞作用,其中晚三叠世楔状构造层序是羌塘板块与亚洲大陆碰撞的产物,晚侏罗世楔状构造层序是拉萨板块与亚洲大陆碰撞的产物,晚白垩世—古近纪楔状构造层序是科希斯坦板块、印度板块与亚洲大陆碰撞的产物。  相似文献   

Resedimentation of cold pumiceous ignimbrite into water: facies transformations simulated in flume experiments     

S. R. ALLEN  A. FREUNDT† 《Sedimentology》2006,53(4):717-734

Deposits and transport processes resulting from the resedimentation of cold, unconsolidated ignimbrite into water were simulated by flume experiments. The ignimbrite sample used was poorly sorted (σ = 2·4–3), fine ash‐rich (< 63 μm, 17–30 wt%) and included both dense lithic clasts (> 2000 kg m^?3) and pumice (500 to ca 1300 kg m^?3). As a result of the binding forces of the ash matrix, the experiments involved resedimentation from a steep front onto the floor (with or without an initial ramp) of the water‐filled tank under both still and wave‐generated conditions. Larger discrete collapse events were induced by oversteepening the sample front and by undercutting from wave action. The mass of the collapse and proportion of pore–space water strongly influenced the style of resedimentation and the deposits. Initial collapse events were from the top of the steep front and fell onto the floor. The largest, densest clasts were deposited as a lithic lag in a proximal sediment wedge or rolled down to a break‐in‐slope. Fine ash was transported in dilute turbidity currents, and coarse unsaturated pumice clasts floated off. Moderate collapse events generated high‐density turbidity currents, trapping pumice in the flow, causing them to saturate. These low‐density pumice clasts were easily remobilized by wave activity and passing currents and accumulated on the gentle slope at the bottom of the resedimented deposit. Large collapse events slumped, producing poorly sorted mounds similar in texture to the original starting material. As the matrix of the ignimbrite sample became saturated with water, moderate and large collapse events generated debrisflows and slurries that deposited massive, poorly sorted deposits. Furthermore, once more gentle slopes were established between the sample and deposit, small cascading grainflows deposited lithic clasts on the upper slopes and levees of pumice at the terminus of low‐relief, ash channels. The experiments show that, excluding large collapse events and debrisflows, resedimenting ignimbrite in water is effective at segregating low‐density pumice clasts from dense lithic clasts and fine ash. Experiments using fine‐ash poor ignimbrite and well‐sorted quartz sand for comparison formed an inherently unstable initial steep front that immediately collapsed by continuous grain avalanches. The grainflow deposits had textures similar to the fines‐poor starting material.  相似文献   

Wave-generated structures in the Devonian lacustrine sediments of south-east Shetland and ancient wave conditions     

PHILIP A. ALLEN 《Sedimentology》1981,28(3):369-379

The most common wave-generated structures in the nearshore lacustrine sediments of the south-east Shetland basin are cosets of undulatory and unidirectional ripple cross-lamination. The undulatory lamination was produced at relatively high oscillatory flow strengths by accretion of rolling grain (post-vortex) ripples, and the unidirectional cross-sets were formed by the migration of vortex (orbital) ripples at lower strengths. Unidirectional solitary lenses were generated under moderate but discontinuous wave activity on a partly sand-starved substrate. Some lenses were reworked during periods of more prolonged wave activity. The Inman-Komar plot of near-bottom orbital diameter versus ripple spacing (λ= 0.80d₀ for small d₀, or λ= 0.65d₀ as modified by Miller & Komar) may only be used in estimating ancient wave conditions for vortex ripples with low Vertical Form Indices and small wavelengths. This laboratory based relationship (minimum d₀ conditions) is utilized in this study since wave periods in lakes are small. The estimation of ancient wave conditions suggests that the ripples were produced in water depths of up to 10 m and in most cases less than 5 m. The formative waves possessed periods of up to 3.4 sec and suggest that the lake was relatively small, perhaps of the order of 20 km wide.  相似文献