制备TJ-1模拟月壤空心圆柱试样的新方法   总被引：1，自引：0，他引：1  

李立青  蒋明镜  苏佳兴  吴晓峰 《冰川冻土》2011,33(4):927-932

针对TJ-1模拟月壤颗粒级配跨度大、粒径〉2mm．的颗粒含量多,采用常规方法制备空心圆柱试样容易出现粗细颗粒分离、试样整体不均匀的特点,提出改良型制备方法．首先采用分层欠压法与冰冻法相结合制备出孔隙比e=1．0的实心圆柱试样,并对实心样的均匀性进行评价,得到分层制备相同孔隙比的TJ-1模拟月壤均匀试样时每层试样的高度;...  相似文献   

Noble Gas Diffusion Mechanism in Lunar Soil Simulant Grains:Results from ~4He~+ Implantation and Extraction Experiments     

付晓辉  邹永廖  郑永春  贺怀宇  欧阳自远 《中国地质大学学报(英文版)》2011,(5)

Experiments on ion implantation were performed in order to better characterize diffusion of noble gases in lunar soil.4He+ at 50 keV with 5×1016 ions/cm2 was implanted into lunar simulants and crystal ilmenite.Helium in the samples was released by stepwise heating experiments.Based on the data,we calculated the helium diffusion coefficient and activation energy.Lunar simulants display similar 4He release patterns in curve shape as lunar soil,but release temperatures are a little lower.This is probably a con...  相似文献   

Neogene basin development around Söke-Kuşadası (western Anatolia) and its bearing on tectonic development of the Aegean region     

Ömer Feyzi Gürer  Mustafa Bozcu  Kamil Yılmaz  Yücel Yımaz 《Geodinamica Acta》2013,26(1-3):57-69

The AMS study has been performed on various types of the basement – Variscan granitic and surrounding – Mesozoic sedimentary rocks in the Velká Fatra Mountains, Tatric Superunit of the Central Western Carpathians. The Velká Fatra Mts. provides good opportunity for AMS study because of composite S-type and I-type granite character of pluton and clear relations to Mesozoic sedimentary rocks in the cover and nappe positions. The granitic massif consists of the three types of weakly magnetic peraluminous granites (350 – 340 Ma in age), ranging from two-mica granites to biotite granodiorites in composition and carrying accessory monazite and ilmenite; whereby they resemble common S-type and/or Ilmenite Series granite. This pre-existing granitic body was intruded by relatively young (304 Ma old) metaluminous to subaluminous, strongly magnetic (due to magnetite) tonalitic intrusion of the I-type and/or Magnetite Series granite. In all S-types investigated as well as in the I-type tonalite body, the magnetic fabrics are not uniform, but slightly variable within a body and differing from body to body. The magnetic fabrics in all granitic rocks can be classified as mostly magmatic in origin, only subordinately affected by ductile deformation. The Alpine overprint of the magnetic fabric of the Variscan granite frequent in the central areas of the Central Western Carpathians was only weak in the Velká Fatra Mts. and the magnetic fabrics of these granites thus mostly comprise the original Variscan magmatic fabrics. On the other hand, in the marginal parts of the Velká Fatra Mts. the magnetic fabrics in granites are locally conformable to the deformational magnetic fabrics in surrounding sedimentary rocks (Mesozoic in age) thus indicating at least local effects of the Alpine deformation. The magnetic fabrics in Mesozoic sedimentary rocks covering the crystalline basement are partially (Cover Formation) to entirely (Nappe Units) deformational in origin.  相似文献   

Noise reduction methods in the analysis of near infrared lunar occultation light curves for high angular resolution measurements     

Tapas Baug  Thyagarajan Chandrasekhar 《天文和天体物理学研究(英文版)》2013,(11):1363-1380

A lunar occultation （LO） technique in the near-infrared （NIR） provides angular resolution down to milliarcseconds for an occulted source, even with ground- based 1 m class telescopes. LO observations are limited to brighter objects because they require a high signal-to-noise ratio （S/N ~40） for proper extraction of angular diameter values. Hence, methods to improve the S/N ratio by reducing noise using Fourier and wavelet transforms have been explored in this study. A sample of 54 NIR LO light curves observed with the IR camera at Mt Abu Observatory has been used. It is seen that both Fourier and wavelet methods have shown an improvement in S/N compared to the original data. However, the application of wavelet transforms causes a slight smoothing of the fringes and results in a higher value for angular diameter. Fourier transforms which reduce discrete noise frequencies do not distort the fringe. The Fourier transform method seems to be effective in improving the S/N, as well as improving the model fit, particularly in the fainter regime of our sample. These methods also provide a better model fit for brighter sources in some cases, though there may not be a significant imorovement in S/N.  相似文献   

伊舒地堑基底花岗岩的锆石U-Pb年代学及其构造意义   总被引：5，自引：0，他引：5  

许文良  裴福萍  高福红  杨德彬  卜永吉 《地球科学》2008,33(2):145-150

为了探讨伊舒地堑与松辽盆地基底的构造演化历史, 对位于伊舒地堑中的2个基底花岗岩进行了锆石LA-ICP-MS U-Pb定年研究, 并与松辽盆地基底花岗岩进行了对比.研究结果表明, 伊舒地堑基底花岗岩中的锆石呈自形或半自形, 并具有典型的岩浆生长环带, 个别发育有核边结构, 锆石的Th/U比值介于0.32 ~ 2.76, 暗示其岩浆成因.CH11井花岗岩中锆石18个测点206Pb/238U加权平均年龄为162±2 Ma, X13井花岗岩中锆石13个测点206Pb/238U加权平均年龄为159 ± 3 Ma, 其核部存在176 ±1 Ma的谐和年龄.上述结果表明, 伊舒地堑中基底花岗岩形成于中侏罗世晚期或晚侏罗世早期, 它们与松辽盆地基底中最晚期花岗岩的形成时间相同.这暗示伊舒地堑与松辽盆地自燕山期以来具有类似的基底演化历史. 176 ±1 Ma继承锆石的存在也证明了上述认识.   相似文献   

用于月面车辆力学试验的模拟月壤研究   总被引：9，自引：1，他引：8  

李建桥  邹猛  贾阳  陈斌  马文哲 《岩土力学》2008,29(6):1557-1561

研究月面环境下的车辆地面力学,对保证月球探测车辆的正常工作具有重要意义,而用于月面车辆力学试验的模拟月壤则影响其结果的准确度与可信度。用于月面车辆力学试验的模拟月壤,以月壤样本与JSC-1模拟月壤为参考标准,以吉林辉南县火山灰为主要原料、赤铁矿砂为辅料,通过调整试样的粒径分布与赤铁矿砂含量,使模拟月壤的比重、内摩擦角、凝聚力、承压特性、粒径分布、颗粒形态、矿物组成等参数接近JSC-1模拟月壤,并在月壤样本的参数变化范围之内,表明该模拟月壤可用于月面车辆力学试验研究。  相似文献   

陨石的矿物-岩石学特征及其分类   总被引：5，自引：3，他引：2       下载免费PDF全文

王道德  缪秉魁  林杨挺 《极地研究》2005,17(1):45-74

根据陨石的矿物岩石学特征、化学组成及结构可划分为球粒陨石及非球粒陨石质陨石两大类。球粒陨石进一步划分为碳质球粒陨石族(CI,CM,CO,CR,CB,CH,CV及CK球粒陨石)、普通球粒陨石族(H,L,LL球粒陨石)、顽辉石球粒陨石族(EH及EL球粒陨石)、R及K球粒陨石群,而非球粒陨石质陨石进一步划分为原始的无球粒陨石族(Acpulcoites,Lodranites,Wi nonaites,IAB硅酸盐包体及IIICD硅酸盐包体)和分异的陨石族。分异的陨石族包括:无球粒陨石(Angrites,Aubrites,Branchinites,橄辉无球粒陨石,HED灶神星陨石,SNCO火星陨石及月球陨石);石铁陨石(中铁陨石及橄榄陨铁);铁陨石(IAB,IC,IIAB,IIC,IID,IIE,IIIAB,IIICD,IIIE,II IF,IVA及IVB铁陨石化学群)。每一陨石族或陨石群,具有类似的成因或形成历史,并来自同一小行星体或行星体,藉此可建立不同陨石族或陨石群之间的成因联系,并可提供早期太阳星云的物理化学条件及其演化的信息。  相似文献   

硼同位素及其地质应用研究   总被引：25，自引：0，他引：25  

蒋少涌 《高校地质学报》2000,6(1):1-16

硼的两个稳定同位素（10B 和11B）相对质量差较大,因此,硼同位 素分馏较显著。由于分析测量技术方面的改进和创新, 硼同位素地球化学近年来有了长足 的发展。业已查明,自然界中δ11B值变化为 －37‰～+58‰。其中,较负的 δ11B值见于非海相蒸发硼酸盐矿物和某些电气石,而较正的δ11B值见 于某些盐湖卤水和蒸发海水。现代大洋水的δ11B值十分恒定 (+39,5‰)。原始 地幔的δ11B值估测为－10‰±2‰。陨石的δ11B值很不均一,变化 可达90‰。而月岩的δ11B值变化较小（－6‰～+4‰）。由于硼同位素存在大的 分馏和不同地质体中截然不同的δ11B值,硼同位素地质应用范围十分广泛。目 前,硼同位素在研究星云形成过程和宇宙事件,壳-幔演化和板块俯冲作用过程,判别沉积 环境,研究矿床成因,示踪古海洋和古气候条件,和判断环境污染源区等方面的研究中成效显著。  相似文献   

半地堑盆地演化机制的粘弹塑数值模拟   总被引：2，自引：1，他引：1  

汤良杰 《地学前缘》2000,7(4):441-448

利用新近完成的粘弹塑构造模拟软件包对盆地的动力学演化进行了一系列模拟。文中主要概述不同厚度的上地壳中由高角度平面正断层界定的半地堑盆地的演化模拟。模拟时上地壳被考虑成具有Byerlee型强度包络 ,并且位于无粘性基底之上 ,盆地中由密度比地壳密度小的沉积物充填。计算了以一定增量逐渐拉伸上地壳层时各个阶段的非静岩应力 (Nonlitho staticstress)、塑性破裂 (Plasticfailure)分布及挠曲剖面 (Flexureprofile)。塑性变形使得有效弹性厚度减小。到切穿破裂出现以前 ,断层断距一直增加 ,之后 ,断距基本停止增加。所以 ,地壳强度使沉降量和隆升量均有极限。上地壳层厚度和沉积物密度是控制盆地宽度和极限深度的两个重要因素 ,上地壳层厚度增加或者沉积物密度加大都使盆地宽度和深度增大。模拟结果可以解释一些大陆裂谷盆地的宽度和沉积深度。  相似文献   

Evolution of terrace risers along the upper Rhine graben inferred from morphologic dating methods: evidence of climatic and tectonic forcing   总被引：1，自引：0，他引：1  

B. Nivière  & Guy Marquis 《Geophysical Journal International》2000,141(3):577-594

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