Least Square Finite Element Method for Viscous Splitting of Unsteady Incompressible Navier–Stokes Equations

In order to solve unsteady incompressible Navier–Stokes(N–S) equations, a new stabilized finite element method,called the viscous-splitting least square FEM, is proposed. In the model, the N–S equations are split into diffusive and convective parts in each time step. The diffusive part is discretized by the backward difference method in time and discretized by the standard Galerkin method in space. The convective part is a first-order nonlinear equation.After the linearization of the nonlinear part by Newton's method, the convective part is also discretized by the backward difference method in time and discretized by least square scheme in space. C~0-type element can be used for interpolation of the velocity and pressure in the present model. Driven cavity flow and flow past a circular cylinder are conducted to validate the present model. Numerical results agree with previous numerical results, and the model has high accuracy and can be used to simulate problems with complex geometry.     

Binary Star Fractions from the LAMOST DR4

Stellar systems composed of single, double, triple or higher-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through comparing the radial velocity variations from multiepoch observations, we analyze the binary fraction of dwarf stars observed with LAMOST. Effects of different model assumptions, such as orbital period distributions on the estimate of binary fractions,are investigated. The results based on log-normal distribution of orbital periods reproduce the previous complete analyses better than the power-law distribution. We find that the binary fraction increases with Teff and decreases with [Fe/H]. We first investigate the relation between α-elements and binary fraction in such a large sample as provided by LAMOST. The old stars with high [α/Fe] dominate with a higher binary fraction than young stars with low [α/Fe]. At the same mass, earlier forming stars possess a higher binary fraction than newly forming ones, which may be related with evolution of the Galaxy.     

高密度聚乙烯/纳米辉钼矿复合材料性能研究

以径厚为30~45 nm的辉钼矿作为导电填料,采用熔融共混法制备高密度聚乙烯/纳米辉钼矿复合材料,应用高阻计ZC-36、SEM、XRD、TG等研究复合材料的电性能、晶体结构、界面微观形貌、热性能等。研究结果表明:当纳米辉钼矿含量为25%,复合材料的体积电阻率为5.1×109Ωcm,纳米辉钼矿高定向排列,呈链状集合体;复合材料tonset分解温度提高了35℃;辉钼矿的晶体结构发生变化,(002)晶面2θ右移了1.12°,面间距缩小0.257 nm。     

Facies character and geochemical signature in the late Quaternary meteoric diagenetic carbonate succession at the Xisha Islands,South China Sea

The late Quaternary shallow-water carbonates have been altered by a variety of diagenetic processes, and further influenced by high-amplitude global and regional sea level changes. This study utilizes a new borehole drilled on the Yongxing Island, Xisha Islands to investigate meteoric diagenetic alteration in the late Quaternary shallowwater carbonates. Petrographic, mineralogical, stable isotopic and elemental data provide new insights into the meteoric diagenetic processes of the reef limestone. The results show the variation in the distribution of aragonite,high-Mg calcite(HMC) and low-Mg calcite(LMC) divides the shallow-water carbonates in Core SSZK1 into three intervals, which are Unit I(31.20–55.92 m, LMC), Unit II(18.39–31.20 m, aragonite and LMC) and Unit III(upper 18.39 m of core, aragonite, LMC and HMC). Various degrees of meteoric diagenesis exist in the identified three units. The lowermost Unit I has suffered almost complete freshwater diagenesis, whereas the overlying Units II and III have undergone incompletely meteoric diagenesis. The amount of time that limestone has been in the freshwater diagenetic environment has the largest impact on the degree of meteoric diagenesis. Approximately four intact facies/water depth cycles are recognized. The cumulative depletion of elements such as strontium(Sr),sodium(Na) and sulphur(S) caused by duplicated meteoric diagenesis in the older reef sequences are distinguished from the younger reef sequences. This study provides a new record of meteoric diagenesis, which is well reflected by whole-rock mineralogy and geochemistry.     

土的本构理论和实验

引言爆炸波在土体中的传播规律可用连续介质力学的方法来求解.描述连续介质运动的方程可根据三个基本力学定律导出,即根据质量守恒定律、动量守恒定律和能量守恒定律导出.推导连续介质运动方程的方法有两种:其一是欧拉法,它能给出空间某一点在任意时刻的运动参数和状态参数;另一是拉格朗日法,它能给出每一个质点的运动参数和状态参数.在上述两种方法中,分别有和空间坐标或物质坐标相对应的应力应变量     

Theory of Elastoplastic Stress-Strain Model for Soil

This paper first introduces the currently adopted stress-strain symbols，some specific terms and their definitions，the commonly used stress-strain testing methods and the formulations for test results。Then，the incremental elastoplastic theories upen which mathematical models are finally given。     

华南金矿二元混合成矿模式

根据华南六个有代表性金矿的成矿时代、断裂构造、围岩、侵入岩、中基性岩墙、成矿类型、成矿阶段，矿石组成、成矿温度、包裹体成分以及稳定同位素等多方面研究，发现华南大部分金矿具有共同特征；主要成矿时代为燕山期，远落后于围岩时代；是沿地壳级大断裂形成的后生矿床，六个金矿的铅同位素组成可分出高值区（组）和低值区（组），表明成矿物质有深浅两个不同来源；不同金矿氢、氧同位素指示成矿热液水为深源岩浆水与古大气降水     

Gold concentration from well water by the hydroelectrical extraction method

An experimental survey of the gold concentrated from well water by a hydroelectrical extraction (HEE) method has been carried out in the famous Au metallogenic province in the eastern part of Shandong Province in northeastern China. This method is based on the existence of ionic Au in groundwater around ore bodies. Under the action of an external electric field, ionic Au migrates toward the cathode where the metal is absorbed by a special absorbent attached to the cathode. Promising areas for further exploration can be evaluated from the amount of Au in the absorbent.Distinct Au anomalies were discovered by the experimental survey. The results from the follow-up study of some of these anomalies have shown that most of them are related to the known placer Au deposits and to the primary Au occurrences. However, two new Au prospects and several new Au sources have been found which offer new targets for Au hunting in the area.The hydroelectrical extraction method is an effective technique of looking for Au in areas covered with transported overburden. Since the Au in well water can be concentrated on the cathode with the absorbent, the sensitivity requirement for Au analysis could be reduced. The method also provides a useful tool for the exploration of blind placer Au.     

新田宁远道县一带玄武质火山岩的地球化学研究

本文阐述了该区玄武质火山岩及其中包体的微量元素及同位素地球化学特征,并对玄武岩浆成因与演化进行了探讨。玄武岩与其中的包体具有不同的过渡金属元素分配型式。二辉橄榄岩包体具亏损地幔岩性质。玄武岩稀土元素的配分特点与世界上典型的大陆裂谷型玄武岩相似。锶、铅、氧同位素的初步研究结果对岩浆的幔源性质及所经受的同化混染作用提供了一些线索。     

四川的地热水资源

四川的地热水资源丰富，大多数热水出露于构造断裂带和洒谷地区，主要储集在三叠纪地层中的碳酸盐岩里。根据温（热）泉的分布状况、热水的类型和物理化学特征，对地热田进行了预测分区。