地面人影作业决策指挥系统建设的技术问题探讨   总被引：1，自引：0，他引：1  

王以琳  张新华  贾斌  王化玲  于金源 《气象科技》2011,39(4):502-506

为做好地面人工影响天气决策指挥系统的研究和开发,提出各级人影办的职责和作业流程。在市级人影办指挥地面作业的体制内,省级人影办主要做好潜势预报和作业预警等项工作;市级人影办建立以GIS、雷达图像、作业点位置叠加为基础,作业指标为核心,高炮、火箭射程计算作业参数为关键,利用GPRS通信完成指挥中心到作业点的指令下达任务;县级人影办主要负责作业监测、部分作业点的指挥、作业和灾情信息上报,作业点管理等项工作。该方案可以提高形成作业指令的科学性和指令下达速度,使其进入业务应用。  相似文献   

内蒙古乌斯尼黑蛇绿混杂岩带形成时代的地质新证据   总被引：3，自引：0，他引：3  

鲍庆中  张长捷  吴之理 《地质与资源》2011,20(1):16-20

贺根山-乌斯尼黑蛇绿混杂岩带的属性和形成时代存在明显的认识上的分歧.早期认为是二叠纪侵入的超镁铁质岩体.该超镁铁质岩体侵入了下二叠统格根敖包组,并被哲斯组地层不整合覆盖,形成时代为二叠纪.20世纪80年代以来,通过中国北方板块构造研究,在硅质岩中采集到的一系列化石资料表明,贺根山地区蛇绿混杂岩的形成时代应为中-晚泥盆世...  相似文献   

东昆仑南缘布青山构造混杂岩带哥日卓托闪长岩体年代学、地球化学特征及其地质意义   总被引：5，自引：0，他引：5  

李佐臣  裴先治  刘战庆  李瑞保  裴磊  陈国超  刘成军  陈有炘  高景民 《地质学报》2013,87(8)

对东昆仑南缘布青山构造混杂岩带哥日卓托闪长岩体进行了锆石U-Pb年代学和岩石地球化学研究,以便对其形成时代和岩石成因进行约束.结果表明,哥日卓托闪长岩锆石Th/U比值(0.63～1.28)较高,阴极发光图像显示锆石内部发育振荡环带,具岩浆成因特点;LA-ICP-MS锆石U-Pb年龄为225.8±1.5Ma(MSWD=0.53),表明其形成时代为晚三叠世早期.岩体的SiO2含量在53.07％～58.74％之间,Al2O3(14.66％～16.17％)含量相对较高,全碱含量较低(4.76％～6.04％),高钾(1.60％～2.90％),里特曼指数σ在1.69～2.66之间,属高钾钙碱性系列.稀土元素总量(∑REE)为158.36×10-6～211.50×10-6,δEu为0.85～0.97,稀土元素配分曲线呈右倾型,具有弱的负铕异常.高场强元素(Nb、Ta、P等)和大离子亲石元素(Ba、Sr、Ti等)具有明显的负异常,而Rb、U、La、Hf、Nd等元素具有明显的正异常.哥日卓托闪长岩形成于高温环境(800℃±),具有后碰撞岩浆活动的特征,是东昆仑地块与巴颜喀拉地块碰撞后地壳部分熔融的产物.  相似文献   

新疆西准噶尔萨尔托海蛇绿混杂岩形成时代及构造环境分析          下载免费PDF全文

何世平  时超  王超  于浦生  辜平阳  查显锋 《地质科学》2013,48(4):1033-1049

萨尔托海蛇绿混杂岩是西准噶尔地区达拉布特蛇绿混杂岩带的重要组成部分,其形成时代和构造环境颇具争议。通过LA-ICP-MS锆石微区原位U-Pb同位素测年,获得其中辉长辉绿岩的 ²⁰⁶Pb/²³⁸U 加权平均年龄为388.8±1.1 Ma,确定该蛇绿混杂岩形成于中泥盆世。岩石地球化学分析表明,纯橄岩(蛇纹岩)属于低Si、低碱、高Mg的变质橄榄岩,REE呈∑REE 偏低的平坦型分布模式,Cr、Ni和Co含量较高,变玄武岩属于高Ti、富Mg、富Fe、偏碱的拉斑系列,REE分布模式呈现 ∑REE 偏低、Eu异常不明显的平坦型曲线,微量元素分布模式为K、Cs、Th、Nb和P相对亏损的平坦型曲线,Zr/Nb比值低,总体表现出与E-MORB相似的特征。综合判断认为,萨尔托海蛇绿混杂岩形成于大陆裂谷向洋盆转化的构造环境,类似于"红海式"洋盆,为进一步深入认识新疆地区众多蛇绿混杂岩的形成构造环境提供了新思路。  相似文献   

设定地震及其烈度影响判别   总被引：1，自引：0，他引：1  

聂树明  周克森 《华南地震》2008,28(2):47-52

设定地震常用于震害预测、地震小区划和重大工程选址,烈度衰减模型反映了地震引起的地面震动及其影响的强弱程度分布。设定地震包括确定性和非确定性设定两种方法,确定性方法基于构造或历史地震,非确定性方法是基于概率危险性方法,用于估计区域或城市未来可能遭遇的地震危险。缺失等震线或震害记载不详的历史地震和概率设定地震都不能确切地反映地震破坏影响,借助于烈度衰减关系模型和GIS,可直观地判别其影响分布情况,便于设定地震的取舍。  相似文献   

某水电站坝基G23挤压蚀变破碎带成因及工程性质分析   总被引：4，自引：0，他引：4  

孟国涛  徐卫亚  杨圣奇  刘金堂  晏新春 《岩土力学》2008,29(6):1691-1696

G23挤压蚀变破碎带是某水电站坝基的主要工程地质问题。通过对该水电站枢纽区新构造运动及构造体系特征的综合分析,探讨了G23挤压蚀变破碎带的成因机制。基于典型岩样的物相及微形貌试验成果,分析了G23带构造岩的岩性特征,明确了G23带岩体的物理性质及其转变特征,预测了该挤压蚀变破碎带在工程作用下的变化趋势。结合蚀变岩样三轴压缩试验的变形破坏规律,阐述了G23带对工程作用的响应及其对工程的影响。  相似文献   

Stability of dense hydrous magnesium silicate phases in the systems Mg2SiO4-H2O and MgSiO3-H2O at pressures up to 27 GPa     

E. Ohtani  H. Mizobata  H. Yurimoto 《Physics and Chemistry of Minerals》2000,27(8):533-544

We conducted high-pressure phase equilibrium experiments in the systems MgSiO₃ with 15 wt% H₂O and Mg₂SiO₄ with 5 wt% and 11 wt% H₂O at 20 ∼ 27 GPa. Based on the phase relations in these systems, together with the previous works on the related systems, we have clarified the stability relations of dense hydrous magnesium silicates in the system MgO-SiO₂-H₂O in the pressure range from 10 to 27 GPa. The results show that the stability field of phase G, which is identical to phase D and phase F, expands with increasing water contents. Water stored in serpentine in the descending cold slabs is transported into depths greater than 200 km, where serpentine decomposes to a mixture of phase A, enstatite, and fluid. Reaction sequences of the hydrous phases which appear at higher pressures vary with water content. In the slabs with a water content less than about 2 wt%, phase A carries water to a depth of 450 km. Hydrous wadsleyite, hydrous ringwoodite, and ilmenite are the main water reservoirs in the transition zone from 450 to 660 km. Superhydrous phase B is the water reservoir in the uppermost part of the lower mantle from 670 to 800 km, whereas phase G appears in the lower mantle only at depths greater than 800 km. In cold slabs with local water enrichment greater than 2 wt%, the following hydrous phases appear with increasing depths; phase A to 450 km, phase A and phase G from 450 km to 550 km, brucite, superhydrous phase B, and phase G from 550 km to 800 km, and phase G at depths greater than 800 km. Received: 4 August 1999 / Accepted: 1 March 2000  相似文献   

广西加里东运动构造古地理问题   总被引：24，自引：3，他引：21       下载免费PDF全文

吴浩若 《古地理学报》2000,2(1):70-76

广西历来被认为是我国加里东运动的典型地区,志留纪末的造山运动使早泥盆世莲花山组砾岩不整合于下伏地层之上。但是,实际上莲花山组只分布于广西中部的大明山－大瑶山地区和东北部扬子地块边缘,并且,它不具备同造山期磨拉石沉积特征,而是古陆剥蚀面上新海侵序列底部的滨海相沉积。广西西部的晚古生代台地相区,泥盆系底部为泥岩或粉砂岩,超覆于寒武系台地相沉积层之上。滇东南和越南北部邻区情况类似。推测在早古生代时它们属于一个地块,可称为“桂滇－北越地块”。早奥陶世云开地块和桂滇－北越地块、扬子地块的会聚和挤压,形成了大明山－大瑶山地体寒武系东西向的线形褶皱带。这是广西加里东运动的主幕。晚奥陶世-早志留世华夏地块和扬子地块的碰撞带在广西仅限于它的东北部,表现为震旦系-下志留统近南北向的线形褶皱带。志留纪末并无造山运动的证据。早泥盆世开始,可能由于地幔柱活动而使桂滇－北越地块裂解,形成北越地块、靖西台地和其他更小的块体。  相似文献   

Surface motion in the pulsating DA white dwarf G29‐38     

M. H. van Kerkwijk  J. C. Clemens  Y. Wu 《Monthly notices of the Royal Astronomical Society》2000,314(2):209-219

We present time-resolved spectrophotometry of the pulsating DA white dwarf G29-38. As in previous broad-band photometry, the light curve shows the presence of a large number of periodicities. Many of these are combination frequencies, i.e. periodicities occurring at frequencies that are sums or differences of frequencies of stronger, real modes. We identify at least six real modes, and at least five combination frequencies. We measure line-of-sight velocities for our spectra and detect periodic variations at the frequencies of five of the six real modes, with amplitudes of up to 5 km s⁻¹. We argue that these variations reflect the horizontal surface motion associated with the g-mode pulsations. No velocity signals are detected at any of the combination frequencies, confirming that the flux variations at these frequencies do not reflect physical pulsation, but rather reflect mixing of frequencies owing to a non-linear transformation in the outer layers of the star. We discuss the amplitude ratios and phase differences found for the velocity and light variations, as well as those found for the real modes and their combination frequencies, both in a model-independent way and in the context of models based on the convective-driving mechanism. In a companion paper, we use the wavelength dependence of the amplitudes of the modes to infer their spherical degree.  相似文献   

Compton-thick X-ray absorption in the Seyfert galaxies Tololo 0109383 and ESO 138G1     

M. J. Collinge  W. N. Brandt 《Monthly notices of the Royal Astronomical Society》2000,317(2):L35-L39

We present analyses of the ASCA X-ray spectra of two Seyfert galaxies, Tololo 0109383 and ESO 138G1. In both cases, spectral fitting reveals two statistically acceptable continuum models: Compton reflection and partial covering. Both spectra have strong iron K lines, with equivalent widths greater than 1.5 keV. These large equivalent widths are suggestive of heavier obscuration than that directly indicated by the partial-covering models (  210²³ cm^-2),  with the actual column densities being 'Compton-thick' (i.e.   N _H1.510²⁴ cm^-2).  We use the hard X-ray/[O  iii ] flux correlation for Seyferts and data from the literature to provide additional support for this hypothesis. Since Tololo 0109383 is known to have optical type 1 characteristics such as broad Balmer line components and Fe  ii emission, this result marks it as a notable object.  相似文献