滇西区域构造应力场分析

云南地处印度板块、欧亚板块—中国大陆碰撞带东缘,地壳运动剧烈,主要受到印度板块NE向挤压与川滇菱形块体SSE滑移的联合作用.在构造上,云南地区可以划分为滇缅泰板块、印支板块、扬子板块、华南板块等4个一级构造单元和腾冲块体、保山块体、兰坪—思茅弧后盆地、盐源—丽江陆缘坳陷、滇中坳陷、康滇古隆起、滇东坳褶等7个二级构造单元...     

吉林延边小西南岔铜(金)矿床早白垩世中—酸性岩浆岩年代学、地球化学及其成因探讨

小西南岔铜(金)矿床位于吉林省延边地区东部,通过对小西南岔铜(金)矿床早白垩世中—酸性岩浆岩进行野外地质、岩相学、年代学和地球化学等方面的研究,进一步探讨延边乃至东北地区中生代大地构造演化。年代学研究结果表明：其同位素年龄分别为(101.69±0.61) Ma(石英闪长岩)、(101.14±0.58) Ma(英云闪长岩)、(100.82±0.62) Ma(花岗闪长岩)和(100.20±1.10) Ma(闪长玢岩),岩浆作用发生在早白垩世末期(102～100 Ma),是同一构造演化过程的产物。岩石地球化学研究表明,闪长玢岩具有典型埃达克质岩石的地球化学特征,其w(SiO₂)=61.419%～62.153%,w(Al₂O₃)=16.872%～17.329%,w(MgO)=2.339%～2.643%,w(Na₂O)=5.749%～6.623%,w(K₂O)=1.483%～1.786%,w(Sr)=(691～888)×10^-6,w(Yb)=(0.71～0.83)×...     

自动气象站采集器数据质量控制程序的改进设计

讨论自动气象站采集器的数据质量控制问题,以气温、风向、风速和降水量等4个代表性气象要素为例,提出自动气象站采集器数据质量控制程序的改进方案.在遵循向下兼容性、低运算量等要求下,改进设计在现有自动气象站采集器软件整体框架内进行.     

塔城盆地地下水氟分布特征及富集机理

塔城盆地位于新疆维吾尔自治区西北部,干旱少雨,蒸发强烈.但相对于新疆其他盆地,塔城盆地地下水水质相对较好,溶解性总固体和F-含量相对较低.为解译这种差异及盆地内高氟地下水的成因,本文在对盆地地下水样品水化学组分系统分析的基础上,结合多种水文地质调查数据,利用数理统计、离子比及主成分分析等手段,研究高氟水的成因及其分布规...     

一种利用机载激光点云的河流横纵断面自动提取方法

传统的河流断面测量方法具有周期长、成本高、外业多等不足,为此提出一种基于机载激光点云的河流横纵断面自动提取方法.首先,使用渐进三角网滤波器从机载点云中分离出地面点,用以构建三角网模型,并将其转化成数字高程模型数据.接着,利用洼地填充、流向分析、流量分析、河流栅格提取、矢量化等水文分析模块,从数字高程模型数据中自动提取出...     

The electromagnetic and gravitational-wave radiations of X-ray transient CDF-S XT2

Binary neutron star(NS)mergers may result in remnants of supra-massive or even stable NS,which have been supported indirectly by observed X-ray plateau of some gamma-ray burst(GRB)afterglows.Recently,Xue et al.(2019)discovered an X-ray transient CDF-S XT2 that is powered by a magnetar from merger of double NS via X-ray plateau and following stepper phase.However,the decay slope after the plateau emission is slightly larger than the theoretical value of spin-down in electromagnetic(EM)dominated by losing its rotation energy.In this paper,we assume that the feature of X-ray emission is caused by a supra-massive magnetar central engine for surviving thousands of seconds to collapse into a black hole.Within this scenario,we present the comparisons of the X-ray plateau luminosity,break time,and the parameters of magnetar between CDF-S XT2 and other short GRBs with internal plateau samples.By adopting the collapse time to constrain the equation of state(EOS),we find that three EOSs(GM1,DD2,and DDME2)are consistent with the observational data.On the other hand,if the most released rotation energy of magnetar is dominated by GW radiation,we also constrain the upper limit of ellipticity of NS for given EOS,and its range is[0.32-1.3]×10^-3.Its GW signal cannot be detected by Advanced LIGO or even for more sensitive Einstein Telescope in the future.     

Simulating the effect of hydrate dissociation on wellhead stability during oil and gas development in deepwater

It is well known that methane hydrate has been identified as an alternative resource due to its massive reserves and clean property. However, hydrate dissociation during oil and gas development (OGD) process in deep water can affect the stability of subsea equipment and formation. Currently, there is a serious lack of studies over quantitative assessment on the effects of hydrate dissociation on wellhead stability. In order to solve this problem, ABAQUS finite element software was used to develop a model and to evaluate the behavior of wellhead caused by hydrate dissociation. The factors that affect the wellhead stability include dissociation range, depth of hydrate formation and mechanical properties of dissociated hydrate region. Based on these, series of simulations were carried out to determine the wellhead displacement. The results revealed that, continuous dissociation of hydrate in homogeneous and isotropic formations can causes the non-linear increment in vertical displacement of wellhead. The displacement of wellhead showed good agreement with the settlement of overlying formations under the same conditions. In addition, the shallower and thicker hydrate formation can aggravate the influence of hydrate dissociation on the wellhead stability. Further, it was observed that with the declining elastic modulus and Poisson’s ratio, the wellhead displacement increases. Hence, these findings not only confirm the effect of hydrate dissociation on the wellhead stability, but also lend support to the actions, such as cooling the drilling fluid, which can reduce the hydrate dissociation range and further make deepwater operations safer and more efficient.     

基于灰色关联分析与RBF神经网络的水面蒸发量预测

利用灰色关联度法分析了影响水面蒸发量的主要气象因素,并通过RBF神经网络建立了水面蒸发量的经验预测模型.计算结果表明,所建立的模型简单易行,精度较高,可以应用于生产实践中.     

云南白登浅海相磷块岩与青龙哨陆相磷块岩的对比研究

白登磷矿是我国重要的浅海相磷块岩矿床,而青龙哨磷矿是我国重要的陆相磷块岩矿床.两地磷矿品位高,储量大,是滇池地区正在开采的2个重要磷矿基地.野外工作研究发现,青龙哨角砾状磷块岩顶板的磷锶铝石矿层和高岭土黏土岩二者呈超覆式不整合接触.深入研究发现其具有陆相磷块岩的许多特征,而没有浅海相磷块岩的原生沉积构造特征.同时,白登磷矿见上下2层工业矿体,而青龙哨磷矿仅见1层工业矿体.对此二矿床特点进行了对比分析.     

Post-Newtonian effect on the variation of time of periastron passage of binary stars in three gravitational theories

The equation for the variation of the time of a periastron passage of binary stars has been solved by using the perturbation approach. The post-Newtonian effect on the variation of the time of a periastron passage has been examined within three gravitational theories. The results clearly show that the periastron passage of a binary star occurs earlier (advances) at each revolution. This effect has been calculated and discussed for ten binary stars.