论中国陆相侏罗系——白垩系界线   总被引：2，自引：2，他引：2  

季强柳永清  姬书安陈文吕君昌  尤海鲁袁崇喜 《地质通报》2006,25(3):336-339

介绍了中国学者近几年在陆相侏罗系-白垩系界线研究领域的最新成果,讨论了陆相侏罗系-白垩系界线研究的原则和方法,指出了目前工作中存在的问题,初步认为在建立中国陆相中生界区域年代系统时要特别注意系、统的界线必须与国际接轨,时间上应与国际系、统界线相一致.如果国际地质科学联合会和国际地层委员会最终采用135Ma作为国际侏罗系-白垩系界线的年龄值,那么冀北-辽西地区陆相侏罗系-白垩系界线推测应在张家口组底部,与区域不整合面相一致,表明热河生物群的时代肯定为早白垩世.如果国际侏罗系-白垩系界线的年龄值将来确定为145Ma,那么冀北-辽西地区陆相侏罗系-白垩系界线推测位于土城子组的上部,意味着冀北地区缺失凡兰吟阶的地层,辽西地区可能缺失凡兰吟阶和欧特里沃阶的地层.  相似文献   

Detection of iodine monoxide radicals in the marine boundary layer using laser induced fluorescence spectroscopy     

Lisa K. Whalley  Kate L. Furneaux  Tom Gravestock  Helen M. Atkinson  Catherine S. E. Bale  Trevor Ingham  William J. Bloss  Dwayne E. Heard 《Journal of Atmospheric Chemistry》2007,58(1):19-39

A Laser Induced Fluorescence (LIF) instrument has been developed to detect iodine monoxide (IO) radicals in the atmosphere. An all solid-state Nd:YAG pumped Ti:Sapphire laser operating at approximately 445 nm was used to excite the (2,0) band of the IO A²Π_3/2 ← X²Π_3/2 electronic transition, with off-resonance fluorescence in the (2,5) band detected at 521 nm. The sensitivity of the instrument was determined by calibration. IO (between 10 and 150 pptV) was generated following the 184.9 nm photolysis of N₂O/CF₃I/N₂ mixtures with O₃ actinometry used to determine the photolysis flux. The detection limit was determined to be 0.3 pptV for a 300 s integration period, with an uncertainty of 23% (1σ). The instrument was deployed in August/September 2006 during the RHaMBLe (Reactive Halogens in the Marine Boundary Layer) campaign in Roscoff, France. Located on a small jetty, a few metres from the water’s edge at high tide, the instrument measured significant levels of IO on 11 days, with a maximum of 27.6 ± 3.2 pptV observed on one day (averaged over 10 s) representing the highest IO mixing ratio recorded in the marine boundary layer to date. IO displayed a clear diurnal profile with a maximum at low tide during the daytime. These results represent the first point measurements of IO in the atmosphere by LIF.  相似文献   

活动构造研究中相关速率的原地宇宙成因核素年代学约束     

张会平  张培震  郑文俊  郑德文  陈正位 《地震地质》2007,29(2):418-430

活动构造研究中获得的相关速率是解释活动构造运动方式和幅度的重要基础,同时也能够提供检验和建立有关运动学和动力学模型的必要参数。原地宇宙成因核素年代学是近几十年来随着加速质谱的出现而逐渐发展并不断广泛应用于地学,特别是地表过程以及活动构造研究中来的。由于仪器测试费用高以及处理流程比较复杂,国内早期相关研究没有得以广泛开展,然而目前正呈现逐渐升温的趋势。在样品采集以及精细野外地质调查测量的基础上,活动构造研究中的活动断裂运动速率,活动构造区的河流水系侵蚀下切速率以及古地震事件,活动火山喷发事件等均可以通过原地宇宙成因核素年代学定量约束。文中在概述原地宇宙成因核素年代学基本原理的基础上,总结了国内外有关该年代学在活动构造研究应用中的最新成果和资料,重点介绍了基于原地宇宙成因核素年代学方法获取和解释活动构造研究中相关速率的成果  相似文献   

白云鄂博碳酸岩脉的显微共聚焦激光拉曼光谱分析     

秦朝建  裘愉卓  周国富  王中刚  张台荣  肖国望 《矿物学报》2007,27(3):400-405

白云鄂博矿区发育的脉状稀土碳酸岩，由于其结晶迅速，矿物颗粒细微，其中的微小矿物的鉴定一直是一个难题。应用显微共聚焦激光拉曼光谱仪则能较好地解决这一问题。研究表明，白云鄂博地区存在富稀土白云质岩浆碳酸岩脉，早期阶段形成碱性长石和铁白云石，无稀土矿化；铁白云石常常出溶铁质而自身则形成方解石。霓石和方解石形成略晚，常常与氟碳铈矿等稀土矿物共生，出现强烈的稀土矿化；而无解理的方解石则形成于更晚的岩浆期后热液阶段，发育大量的流体包裹体，并出现强烈的铌、稀土矿化。铌铁矿分布在氟碳铈矿中和赤铁矿边缘，为热液交代作用的产物。早期结晶的矿物如碱性长石、铁白云石稀土矿化弱，岩浆晚期分异出大量的流体相，稀土元素和Sr等进入岩浆热液中，并在热液结晶矿物中富集，甚至在非平衡结晶的石英中产生强烈的稀土矿化。结合岩相学显微观察，显微拉曼探针很好的揭示了这一地质过程。同时为白云鄂博矿床铌、稀土矿化的热液交代成因提供了依据。  相似文献   

Ilmenite composition in the Tellnes Fe–Ti deposit,SW Norway: fractional crystallization,postcumulus evolution and ilmenite–zircon relation     

Bernard Charlier  Øyvind Skår  Are Korneliussen  Jean-Clair Duchesne  Jacqueline Vander Auwera 《Contributions to Mineralogy and Petrology》2007,154(2):119-134

Major and trace element XRF and in situ LA-ICP-MS analyses of ilmenite in the Tellnes ilmenite deposit, Rogaland Anorthosite Province, SW Norway, constrains a two stage fractional crystallization model of a ferrodioritic Fe-Ti-P rich melt. Stage 1 is characterized by ilmenite-plagioclase cumulates, partly stored in the lower part of the ore body (Lower Central Zone, LCZ), and stage 2 by ilmenite-plagioclase-orthopyroxene-olivine cumulates (Upper Central Zone, UCZ). The concentration of V and Cr in ilmenite, corrected for the trapped liquid effect, (1) defines the cotectic proportion of ilmenite to be 17.5 wt% during stage 1, and (2) implies an increase of D _V^Ilm during stage 2, most likely related to a shift in fO₂. The proportion of 17.5 wt% is lower than the modal proportion of ilmenite (ca. 50 wt%) in the ore body, implying accumulation of ilmenite and flotation of plagioclase. The fraction of residual liquid left after crystallization of Tellnes cumulates is estimated at 0.6 and the flotation of plagioclase at 26 wt% of the initial melt mass. The increasing content of intercumulus magnetite with stratigraphic height, from 0 to ca. 3 wt%, results from differentiation of the trapped liquid towards magnetite saturation. The MgO content of ilmenite (1.4–4.4 wt%) is much lower than the expected cumulus composition. It shows extensive postcumulus re-equilibration with trapped liquid and ferromagnesian silicates, correlated with distance to the host anorthosite. The Zr content of ilmenite, provided by in situ analyses, is low (<114 ppm) and uncorrelated with stratigraphy or Cr content. The data demonstrate that zircon coronas observed around ilmenite formed by subsolidus exsolution of ZrO₂ from ilmenite. The U-Pb zircon age of 920 ± 3 Ma probably records this exsolution process. Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorized users.  相似文献   

GRACE和SLR观测的地球动力学扁率最大熵谱及小波相关分析          下载免费PDF全文

张子占  陆洋  许厚泽 《地球物理学报》2007,50(5):1383-1389

卫星重力测量技术的实现为测定地球动力学扁率提供了新的方式和途径，GRACE卫星是目前最新的重力测量卫星，据其恢复的低阶重力场较以往精度得到大大提高，然而其观测地球动力学扁率（二阶项）却与卫星激光测距（SLR）结果相差较大.本文采用最大熵谱和小波分析方法对GRACE和SLR观测的地球动力学扁率时间序列信号进行定量比较分析，结果表明：GRACE观测的地球动力学扁率年际周期变化振幅仅为SLR观测结果的25%，并且目前GRACE观测的地球动力学扁率数据中含有系统输入信息和相位差，但前者较后者包含有较强的短周期（2～6月）信息.造成这种差异的主要原因可能来自于GRACE与SLR全球观测数据时空分布不同.  相似文献   

Laser Scanning的基本原理及其应用前景     

WANG Ren    XU Qing 《测绘学院学报》2007,(Z1)

首先介绍了激光测距仪的发展历程,针对应用领域的不同,分别对3维激光成像仪和机载/星载激光测高仪的测量原理进行了阐述,并分别介绍了两种激光测距仪的工作流程以及数据处理流程,最后对两种激光测距仪的应用范围进行了阐述,并把两种激光测距技术和普通摄影测量进行了比较,指出了激光测距技术相对于普通摄影测量的优点,即高精度性、穿透性、实时性。  相似文献   

Determination of the distribution of size of irregularly shaped particles from laser diffractometer measurements     

Claudio L. Schneider  Reiner Neumann  Alan S. Souza 《International Journal of Mineral Processing》2007

The formal stereological transformation equation for particle sieve size distribution from measurements in lower dimensional spaces is applied to laser diffractometer measurements. The transformation function for iron ore particles is measured experimentally, and modeled. The solution is tested against the measured transformation function data as well as synthetic composite distributions of the original sample. The natural size distribution of a sample taken from a grinding circuit stream was measured by a combination of standard sieving and cyclosizer, and the result is compared to the transformed size distribution calculated from laser diffractometer measurements. The stereological transformation technique performed well in all cases.  相似文献   

CLSM技术应用于化石硅藻微构造的尝试研究     

王金星  李家英 《地球学报》2007,28(1):79-85

首次采用激光扫描共聚焦显微系统(Confocal Laser Scanaing Microsystem)的新方法对西藏化石硅藻进行了微构造的尝试研究,通过对标本不同层面的系列扫描和三维重组立体图像的观察,揭示了采自西藏阿里地区和山南地区湖相沉积剖面的化石硅藻的微构造及形态特征,发现了某些对硅藻分类、示相特征的新标识,并在CLSM技术的应用方面获得了新的认识.  相似文献   

Laser microprobe for the study of noble gases and nitrogen in single grains: A case study of individual chondrules from the Dhajala meteorite   总被引：1，自引：0，他引：1  

R. R. Mahajan  S. V. S. Murty 《Journal of Earth System Science》2003,112(1):113-127

A laser microprobe capable of analysing nitrogen and noble gases in individual grains with masses less than a milligram is described. It can be used in both continuous wave (CW) mode, useful for stepwise heating of an individual grain, as well as in pulsed mode, useful for ablating material from a small selected area of a sample, for gas extraction. We could achieve low blanks (in ccSTP units) for 4He(4.8 x 10{-12}),²²Ne(1.0 x 10{-12}),³⁶Ar(1.0 x10 ^-13),⁸⁴Kr(2.9 x 10{-14}),¹³² Xe(2.6 x 10{-14}), and N (87 pg), using this system. Preliminary data for individual chondrules from the Dhajala meteorite show that noble gases and nitrogen from grains as small as 170 microgram can be analysed using the present laser microprobe setup. The amount of trapped neon in Dhajala chondrules is very small, and nitrogen in the chondrules is isotopically heavier as compared to the bulk meteorite.  相似文献