静态测量方式的单颗粒锆石蒸发铅同位素定年方法     

王秀丽  李向辉王芳李秋立  陈福坤 《岩矿测试》2006,25(3):201-205

报道的单颗粒锆石蒸发定年方法是利用新型固体质谱计的多离子接收器配置实现的。改进的锆石蒸发^207Pb／^206Pb定年流程通过静态测量方式，在锆石蒸发过程中直接测定铅同位素比值，获得^207Pb／^206Pb年龄。应用该方法测定了元古代永宁组沉积岩的碎屑锆石，获得6颗锆石的^207Pb／^206Pb年龄值为1965—2590Ma。与传统的蒸发法流程相比，静态测量方法省时简捷，同时可以直观地观测到锆石内部的铅同位素组成变化。这些变化反映锆石结晶历史、后期事件叠加以及锆石成因等地质信息。  相似文献   

Magnetotail response during a strong substorm as observed by GEOTAIL in the distant tail     

A. Belehaki  R. W. McEntire  S. Kokubun  T. Yamamoto 《Annales Geophysicae》1998,16(5):528-541

Simultaneous energetic particle and magnetic field observations from the GEOTAIL spacecraft in the distant tail (X_GSM -150 Re) have been analysed to study the response of the Earths magnetotail during a strong substorm (AE 680 nT). At geosynchronous altitude, LANL spacecraft recorded three electron injections between 0030 UT and 0130 UT, which correspond to onsets observed on the ground at Kiruna Ground Observatory. The Earths magnetotail responded to this substorm with the ejection of five plasmoids, whose size decreases from one plasmoid to the next. Since the type of magnetic structure detected by a spacecraft residing the lobes, depends on the Z extent of the structure passing underneath the spacecraft, GEOTAIL is first engulfed by a plasmoid structure; six minutes later it detects a boundary layer plasmoid (BLP) and finally at the recovery phase of the substorm GEOTAIL observes three travelling compression regions (TCRs). The time-of-flight (TOF) speed of these magnetic structures was estimated to range between 510 km/s and 620 km/s. The length of these individual plasmoids was calculated to be between 28 Re and 56 Re. The principal axis analysis performed on the magnetic field during the TCR encountered, has confirmed that GEOTAIL observed a 2-D perturbation in the X-Z plane due to the passage of a plasmoid underneath. The first large plasmoid that engulfed GEOTAIL was much more complicated in nature probably due to the external, variable draped field lines associated with high beta plasma sheet and the PSBL flux tubes surrounding the plasmoid. From the analysis of the energetic particle angular distribution, evidence was found that ions were accelerated from the distant X-line at the onset of the burst associated with the first magnetic structure.  相似文献   

榆树林油田葡萄花油层砂体成因类型与分布特征          下载免费PDF全文

王俊玲  叶连俊 《地质科学》1997,32(4):515-520

在细分沉积微相的基础上,充分利用密井网开发井资料,通过精细地质解剖研究砂体几何形态及其内部结构,识别出榆树林油田葡萄花油层发育4种成因类型的砂体:水上分流河道砂体;水下分流河道砂体;河口坝砂体及席状砂砂体,并建立了不同成因砂体的垂向层序模式及砂体空间展布模式,为油田进一步开发提供了一定地质依据。  相似文献   

亚暴膨胀相近磁尾位形不稳定性模型Ⅱ.中磁尾等离子体流与近磁尾亚暴活动的关系   总被引：2，自引：0，他引：2       下载免费PDF全文

洪明华  濮祖荫 《地球物理学报》1997,40(2):154-163

在单流体MHD近似下，研究了有背景等离子体流存在时的近磁尾位形不稳定性．分析表明，等离子体地向流使两支漂移气球模DBM1和DBM2的不稳定增长更快．与卫星观测资料对比显示，诸多的观测观象与本模型的预言一致．这个结果对中磁尾磁场重联及高速等离子体流与亚暴膨胀相在近地触发之间的关系给出了新的解释．  相似文献   

控制网中观测元素作用的分析     

王建国 《武汉大学学报(信息科学版)》1987,(4)

本文阐述测量控制网中观测元素作用分析的理论,通过有关的四个数字指标对此进行了多个网例的定量分析,讨论了观测元素的作用与网形、与观测精度匹配等的关系。文中还给出了必要观测分量的几何意义。  相似文献   

A 2D MATHEMATICAL MODEL FOR THE BED DEFORMATION IN THE LOWER YELLOW RIVER   总被引：2，自引：0，他引：2  

Junqiang XIA  Guangqian WANG 《国际泥沙研究》2003,(2)

1 BANK EROSION IN THE LOWER YELLOW RIVER In alluvial rivers, riverbeds are always in a state of transition and development. Two kinds of deformations result for the fluvial process according to certain basic characteristics. One is longitudinal deformation that is characterized by the deformation of a riverbed in the direction of streamwise flow such as riverbed scour or deposition. The other is transverse or lateral deformation that is distinguished by the deformation of a riverb…  相似文献   

陆相断陷盆地的构造层序地层分析   总被引：10，自引：3，他引：7  

邓宏文  郭建宇  王瑞菊  谢小军 《地学前缘》2008,15(2):1-7

陆相盆地层序地层构型是构造运动、古气候、古湖平面变化与沉积物补给等动力学要素对沉积基准面控制的综合效应。其中,构造运动对盆地层序界面形成与层序内部充填起至关重要的作用。因此,陆相盆地层序地层研究须以构造层序地层为主线,即通过构造对层序形成与演化的控制分析解释层序地层构型,预测其内部充填特征。经研究,断陷盆地构造运动对层序地层的控制主要表现在:(1)断裂活动通过控制基底升降运动直接制约着盆地沉积物堆积的可容纳空间的变化及至层序地层构型;(2)构造转换带或调节带控制盆地主体物源补给方向和沉积体系分布;(3)断裂活动及其塑造的古地貌控制着沉积体系与砂体分布特征。  相似文献   

塔河油田奥陶系缝洞型碳酸盐岩储层预测研究   总被引：4，自引：1，他引：3  

温志新  王红漫  漆立新  于兴河 《地学前缘》2008,15(1):94-100

针对塔河油田奥陶系碳酸盐岩缝洞型储层的结构特点,以地质、钻井、测井及生产测试等资料分析为出发点,以各类储层地震响应为基础,分析了有利储层的地震属性特征、地震反射结构及波形相关特点,最终将有利储层综合划分为两类,并建立了各自的地震综合预测模式:Ⅰ类储层表现为串珠状、条带状振幅变化率异常和残丘高点+杂乱反射特征,相位角变化大于20°;Ⅱ类储层为弱或强振幅、高振幅变化率、弱相干、低速度和多种反射结构。提高了塔河油田及其周缘的钻井成功率。  相似文献   

长江河口河槽近期沉积特征及影响因子分析     

李一鸣  张国安  游博文  李占海 《地理学报》2019,74(1):178-190

随着流域和河口水利工程建设,长江河槽沉积环境发生了巨大改变,对河势演变和河槽冲淤均产生重要影响。依据长江河口河槽大面积表层沉积物采样和各河槽定点水文观测资料,分析各河槽沉积特征,探讨其影响因子及作用机制。结果表明:河槽沉积物类型以砂质粉砂和粉砂质砂分布最广,粒径分布纵向上呈自西向东减小、横向上自北向南减小趋势,河槽总体主槽粗、边滩细。涨落潮泥沙输运和沉降过程影响河槽纵向沉积分布特征,风浪作用强化了口门段河槽南北沉积环境的差异,北支、北港口门段河槽受到偏北方向风浪作用强烈,沉积物粗化明显。不同泥沙来源是造成河槽整体沉积环境差异的主导因素,南支、南港上段表现为流域来沙的沉积特征,北港、南槽、北槽则表现为流域与海域来沙的混合沉积特征,口外沉积物对口内河槽的影响主要是为口内河槽提供细颗粒物质来源。  相似文献   

Dynamics and local boundary properties of the dawn-side magnetopause under conditions observed by Equator-S     

M. W. Dunlop  A. Balogh  W. Baumjohann  G. Haerendel  K.-H. Fornacon  E. Georgescu  R. Nakamura  S. Kokubin 《Annales Geophysicae》1999,17(12):1535-1559

Magnetic field measurements, taken by the magnetometer experiment (MAM) on board the German Equator-S spacecraft, have been used to identify and categorise 131 crossings of the dawn-side magnetopause at low latitude, providing unusual, long duration coverage of the adjacent magnetospheric regions and near magnetosheath. The crossings occurred on 31 orbits, providing unbiased coverage over the full range of local magnetic shear from 06:00 to 10:40 LT. Apogee extent places the spacecraft in conditions associated with intermediate, rather than low, solar wind dynamic pressure, as it processes into the flank region. The apogee of the spacecraft remains close to the magnetopause for mean solar wind pressure. The occurrence of the magnetopause encounters are summarised and are found to compare well with predicted boundary location, where solar wind conditions are known. Most scale with solar wind pressure. Magnetopause shape is also documented and we find that the magnetopause orientation is consistently sunward of a model boundary and is not accounted for by IMF or local magnetic shear conditions. A number of well-established crossings, particularly those at high magnetic shear, or exhibiting unusually high-pressure states, were observed and have been analysed for their boundary characteristics and some details of their boundary and near magnetosheath properties are discussed. Of particular note are the occurrence of mirror-like signatures in the adjacent magnetosheath during a significant fraction of the encounters and a high number of multiple crossings over a long time period. The latter is facilitated by the spacecraft orbit which is designed to remain in the near magnetosheath for average solar wind pressure. For most encounters, a well-ordered, tangential (draped) magnetosheath field is observed and there is little evidence of large deviations in local boundary orientations. Two passes corresponding to close conjunctions of the Geotail spacecraft are analysed to confirm boundary orientation and motion. These further show evidence of an anti-sunward moving depression on the magnetopause (which is much smaller at Equator-S). The Tsyganenko model field is used routinely to assist in categorising the crossings and some comparison of models is carried out. We note that typically the T87 model fits the data better than the T89 model during conditions of low to intermediate K_p index near the magnetopause and also near the dawn-side tail current sheet in the dawnside region.  相似文献