柴达木北缘超高压变质带中的岛弧火山岩

青藏高原北部柴北缘发育一套与超高压变质带并行的早古生代岛弧火山岩带,岛弧火山岩以玄武岩类为主,包括一些中酸性岩类,岩石以普遍遭受绿片岩相蚀变为特征,区别于该地区普遍遭受角闪岩相区域变质的元古代的基性火山岩。该早古生代的岛孤火山岩显示三组地球化学特征:①VTG-Ⅰ,岛弧拉斑玄武岩(IAT);②VTG-Ⅱ,高Al次钙碱性-碱性过渡型玄武岩;③VTG-Ⅲ,较N-MORB更亏损的拉斑玄武岩(异常MORB)。研究认为前两组火山岩是成熟岛弧两个发育阶段的特征性产物:洋壳俯冲到陆壳的初用,由俯冲洋壳和地幔楔的部分熔融形成岛弧拉斑玄武岩(IAT),随着俯冲板块的速度加快和岛弧周围地壳的加厚,则形成钙碱性玄武岩(CA)、高Al玄武岩。第三组火山岩形成于弧间盆地,由亏损的地幔楔高度部分熔融形成比N-MORB亏损的的火山岩(异常MORB)。岛弧火山岩的锆石LA-ICP-MS法U-Pb年龄为514.2±8.5 Ma,说明柴北缘在早古生代发生过洋壳向陆壳的俯冲作用。鉴于该地区代表陆-陆俯冲作用的柴北缘超高压变质岩石也是形成于早古生代(494Ma),认为陆-陆俯冲作用发生在洋-陆俯冲作用之后,二者时间和空间相伴随。     

武夷地块中南平-宁化构造带南华纪弧火山岩属性及其对华夏板块多微地体拼合的启示

武夷地块中各地体的活动解析是认识华夏板块构造活动演化的窗口。南平-宁化构造带作为划分南武夷地体和北武夷地体的重要边界活动带,其构造属性对我们认识武夷地块中南、北武夷地体的构造演化具有重要意义。前人对南平-宁化构造带中变质火山岩类的研究和认识存在争议,限制了我们对南平-宁化构造带的构造属性的理解。因此,本文利用野外路线地质调查、年代学测定、同位素地球化学测试等手段,对该套变质火山岩做了重点研究,结合前人的研究成果,我们得到以下认识:南平-宁化构造带中的变质火山岩类主要形成于756～720 Ma,主要形成于活动大陆边缘或岛弧环境,表明南平-宁化构造带可能代表了南武夷地体和北武夷地体之间的一条南华纪的近东西向的岛弧火山活动带,结合带中构造变形反映的南北向对冲的汇聚极性,我们认为南武夷地体和北武夷地体之间在南华纪可能还存在洋-陆碰撞乃至陆-陆拼合过程,这也反映了多微地块、多期拼合过程可能更符合华夏板块大地构造演化的主旋律。     

火山活动与海侵影响下的典型湖相页岩有机质保存差异分析

黑色富有机质页岩是页岩油气生成和赋存的主要母体,是强还原环境水体的沉积产物,在其形成过程中,细菌硫酸盐还原作用(BSR)对水体环境影响明显,但BSR强度如何影响有机质的保存尚未得到关注。我国陆相湖盆富有机质泥页岩广泛发育,形成过程中常常伴随有火山活动或者海侵等事件,大量硫酸盐进入湖盆,改变水体的沉积环境,不同环境下BSR对黑色页岩有机质保存的影响明显不同。本次研究选取鄂尔多斯盆地延长组长7段页岩、松辽盆地青山口组和嫩江组页岩作为对象,同时与现代沉积物进行对比。研究表明,TOC与TS之间关系复杂,但细菌硫酸盐还原强度指数(SRI)与TOC呈现幂指数变化,且表现出两阶段变化的特征。当SRI大于1.375时,TOC整体偏低,指示了强硫酸盐还原作用消耗大量有机质;当SRI小于1.375时,TOC明显较高,指示了弱硫酸盐还原作用对有机质消耗相对较少,更有利于有机质保存。火山活动和海侵作用均向水体提供了大量硫酸盐,但对陆相湖盆页岩中有机质的保存影响不同。火山活动影响的长7段页岩SRI普遍小于1.375,BSR对有机质消耗相对弱,页岩TOC高。而受海侵影响的青山口组一段底部和嫩江组一段底部页岩SRI...     

IGNEOUS PETROLOGY

正20141376 Bian Xiongfei(Shenyang Institute of Geology and Mineral Resources,CGS,Shenyang 110034,China);Li Yongfei Zircon UPb Age,Geochemistry and Petrogenesis of the Jianshetun Volcanic Rocks in Eastern Inner Mongolia(Geology and Resources,ISSN1671-1947,CN21-1458/P,22(5),2013,p.360-366,6 illus.,2 tables,24 refs.)Key words:volcanic rocks,Inner Mongolia The LA-ICP-MS zircon U-Pb dating     

Mathematical identification of diffuse and localized instabilities in fluid‐saturated sands

The mathematical properties of diffuse and localized failure modes in fluid‐saturated sands are investigated. The granular medium is modeled as an elastoplastic solid, and a recently proposed set of scalar indices, here referred to as moduli of instability, is used to identify the onset of potential bifurcations of the incremental response. First, the analytical properties of these moduli are discussed, stressing their dependence on the kinematic constraints associated with the imposed deformation modes. Then, by using an elastoplastic model for sands, drained and undrained loading paths are simulated under axisymmetric, plane‐strain and simple shear conditions. For each deformation mode, the instability moduli are computed and monitored throughout the simulations, with the purpose of elucidating the consequences of changes in control conditions. In addition, it is illustrated that suitable linear transformations allow the same strategy to be used to perform drained or undrained shear band analyses and predict the interval of possible band inclinations. The final comparison against literature experiments on loose Hostun sand shows that the instability moduli are indicators of the loss of resistance against specific modes of deformation. As a result, they can be used to identify and explain a number of failure mechanisms that can be commonly observed in experiments. Copyright © 2013 John Wiley & Sons, Ltd.     

Silicates in evolved stars: the lrs-maser chronology revisited

Since the publication of our correlation (1990 Ap.J. 350, L45) suggesting a temporal relationship among: (a) shapes of 10 micron silicates seen in IRAS Low Resolution Spectra (LRS); (b) IRAS broad band colors; (c) light curve asymmetries, and (d) the types of masers associated with various Mira variable stars, the question has arisen whether the implied chronology refelcts the interval between thermal pulses, or the more lengthy ascent of the AGB. There is evidence in favor of the former interpretation. A strong implication of this idea is that variability among pre-silicate spectra should be significant. Several examples of this have been found in the extended LRS database, and are presented. Finally, plans are presented to continue monitoring of selected variables in the 10 micron region, to verify the variability suggested in the limited phase coverage provided in the LRS database. Monitoring will include use of our facilities at the Mt.Evans-Womble Observatory — highest in the world at 4313 meters altitude.     

The infrared colors of main sequence stars: how much circumstellar debris is normal?

We have been awarded NASA Key Project observing time on ISO, in order to establish the true frequency of far-infrared excesses in a volume-limited sample of main sequence and related stars, and address the relative success or failure of single stars in processes related to the forming of planetary systems. For a volume-limited subset of main sequence and related stars, PHT03 measurements at 3.6, 11.5, 20 and 60 micron will be obtained, using a 120 arsec aperture in all cases to eliminate possible companion confusion with differing apertures, to ascertain spectral energy distributions. For the M dwarfs, 100 micron observations will also be obtained. For some, brighter sources, more extensive wavelength coverage and improved spatial resolution will be attempted, using CAM and SWS. Spatially over-sampled PHOT observations will be made at 60 micron of the brightest and nearest Vega-like sources to measure the characteristic sizes of the emitting regions and obtain some information regarding their shapes and orientations. The goal is not a map, but scan profiles along 3 position angles which can be deconvolved to find the intrinsic size and shape of the half-maximum contour of the emitting region. Photometry of selected lines of sight through the zodiacal dust will also be carried out to look for outer solar system (Kuiper Belt) material. Observation at a range of wavelengths, ecliptic latitudes and at 2 epochs is designed to help untangle foreground Zodiacal from background Kuiper flux, not necessarily to look for individual macroscopic objects.     

千官岭金银矿区深部隐伏矿体的立体评价

本文在野外调查和前人资料的基础上，对新昌拨茅白垩纪火山盆地千官岭金银矿区深部隐伏矿体作了立体评价，指出了千官岭矿区具有2个成矿构造层；预测了深部隐伏矿体的可能位置；提出了在火山洼地中找矿，应注意在不同火山构造层中寻找不同类型矿床的观点，初步形成了陆缘火山盆地中金银矿床立体评价的基本思路。     

广西隆林县隆或金矿的地质特征和成因分析

隆林县隆或金矿属微粒型金矿，具有多层位、层状矿体为主、矿石和矿物成分简单、沉积结构构造特征，属典型层控矿床。矿床成因与生物礁的消失、滑塌事件、深水火山碎屑硅泥质上超盆地的叠覆、以及有机质的热解和分异有关。火山作用提供金的来源，火山～碎屑～浊积岩相为矿源层和含矿层，并受沉积盆地的关闭和开启影响，形成成岩矿床、成岩～后生或后生矿床     

生物传感器综述

本文介绍当前国际、国内生物传感器的发展及应用概况,并对生物传感器的市场前景和生物传感器技术的未来发展作了简单地论述。