根据GPS和InSAR数据反演2001年昆仑山口西地震同震破裂分布

利用干涉合成孔径雷达（interferometric synthetic aperture radar, InSAR）技术可以获取空间连续的地表形变监测结果,但仅能得到真实三维形变在雷达视线方向上的一维投影,降低了地表形变解译的可靠性。全球导航卫星系统（global navigation satellite system, GNSS）可提供高精度的三维形变结果,但其空间分辨率较低。因此可通过融合InSAR和GNSS来实现高精度高空间分辨率的三维地表形变监测。提出利用方差分量估计(variance component estimation, VCE)方法对经典的联合大地和卫星同步形变测量值的应变张量估计(simultaneous and integrated strain tensor estimation from geodetic and satellite deformation measurements, SISTEM)方法进行改进,发挥SISTEM方法可以考虑相邻点地表形变的空间相关性的优势,优化了函数模型中InSAR和GNSS观测的构成比例,引入VCE方法精确估计了各类观测值的后验方差,进而实现了高精度的三维地表形变测量。首先通过设计模拟实验对所提方法进行了验证,然后将该方法应用于2007年夏威夷基拉韦厄火山喷发案例中。相较于SISTEM方法,该方法在东西、南北、垂直向解算的形变精度均有大幅提升。     

准饱和多孔介质中圈闭气体对渗透系数的影响

含圈闭气体的地下水流称为准饱和流,准饱和流中的圈闭气体对含水层渗透系数有重大影响。通过柱试验开展了粉砂、细砂、中砂和粗砂4种介质圈闭气体饱和度与准饱和渗透系数关系的研究。结果表明:圈闭气体饱和度明显受介质的粒径影响,在细粒介质中圈闭气体饱和度明显较大;4种介质圈闭气体饱和度在0~15%范围内,准饱和渗透系数与完全饱和相比减少了32.82%~56.38%,且准饱和渗透系数与圈闭气体饱和度之间可表达为一个负线性相关的经验公式;该公式与Faybishenko公式等效,但形式简单,参数较少,使用方便;准饱和渗透系数的变化规律可概化为圈闭气体占据了原有的有效孔隙,造成原有效孔隙度减少,从而使渗透系数减小。利用该理论,Kozeny-Carman方程能较准确地描述准饱和渗透系数的变化规律,而基于哈根-泊肃叶方程的渗透系数公式则存在较大误差,不适用于描述准饱和渗透系数;试验结果证明了室内测定饱和渗透系数时排除圈闭气体的必要性。     

Design of environmental decision support system and its application to water quality management

1 IntroductionEnvironmental decision support systems could be divided into two categories by their organizational form and system functions. One is regional environmental analytical system based on commercial GIS and assisted by environmental models, such as BASINS developed by the American NEPA using ARC/VIEW as its user platform and including QUAL2E and NPSM as its prediction tools. The other is environmental information and prediction system based on mathematical models, such as…     

Long-term changes in water quality and phytoplankton characteristics in port shelter, Hong Kong, from 1988-1998.

This study analysed monthly physico-chemical and phytoplankton data collected from 10 marine monitoring stations in Port Shelter Hong Kong, from 1988 to 1998. Cluster analysis based on all water quality parameters measured shows that the 10 monitoring stations can be grouped into three clusters: Cluster I consists of stations located in Outer Port Shelter; Cluster II consists of stations located in Inner Port Shelter and Cluster III consists of a single station in Hebe Heaven, a well-sheltered Bay in Inner Port Shelter. Factor analysis shows high positive loadings for nutrients and nutrient ratios in the first two factors of the three clusters, which indicates that the stations of the three clusters were primarily grouped according to their respective nutrient conditions. In Inner Port Shelter, and particularly Station PM5 in the sheltered Hebe Haven, the influence of surface runoff and pollution loading from the surrounding catchment area was apparent. Five stations located along a transect from Inner to Outer Port Shelter were selected for trend analysis. An increasing trend for temperature and a decreasing trend for pH are observed in all Stations except PM10 which is at the mouth of Port Shelter. The results of canonical analysis revealed that temperature and pH could also play an important role in determining the density and biovolume of the minor algal groups in Port Shelter.     

AV Hydrae: A Near-Contact Semi-Detached Binary with Possible Massand Angular Momentum Loss

The photoelectric observations of the neglected binary AV Hya published by Srivastava and Kandpal (1980) have been re-analyzed using Wilson-Devinney's synthetic light-curve program. The binary turns out to be a near-contact semi-detached system. The primary, more massive, more luminous and greater component, eclipsed at primary minimum, is detached from its Roche lobe (85%). The secondary fills its Roche lobe and has a temperature difference of T=,-3414 K. As with other semi-detached binaries, the secondary is more evolved than that of the primary. Thetimes of light minima of the eclipsing have been analyzed,showing that the orbital period of AV Hya undergoes acontinuous decrease with a rate of dP/dE=-8.26×10^-8 day/year. The mass transfer between the twocomponents can not explain the present orbital period variationsince the secondary component is filling the Roche lobe. Theorbital period change demonstrates that the system may undergoa secular mass and angular momentum loss and the system mayevolve from the present short-period near-contact system intoan A-type contact binary.     

基于栅格数字高程模型自动提取黄土地貌沟沿线技术研究

从数字高程模型中提取具有精确定位特征的连续的沟沿线是构建黄土沟壑丘陵地区土壤侵蚀,泥沙搬运和径流过程的空间分布式机理－过程模型的关键技术。本文提出了基于地貌形态学特征的地貌提取技术,在提取具有代表性的黄土丘陵沟壑区山西离石王家沟流域汇流网络的基础上,自动提取了该流域完整的沟沿线,得到了满意的结果。     

基于集体记忆的红色旅游地地方性建构

红色历史的集体记忆嵌入动态的地方建构和空间生产过程,成为地方性重构的有力素材。文章以云南省宾川县新庄红军村为例,通过参与式观察和访谈文本分析等质性方法,从地方性景观与话语的再建构,以及地方性情境创设的空间实践,探讨新庄村的地方性建构机制。研究发现：具体的地方要素在地方-记忆的互动关系中起中介承启作用。地方要素既促进红色旅游情境下记忆的唤起、存储与再创造,又对集体记忆重新建构的地方特质、意义与场所精神进行地方性元素表达。旅游情境创设与地方性展演使集体记忆不断得到投影、表达与重构,推动差异化的地方叙述与体验。     

More than two hundred and fifty thousand spectroscopic binary or variable star candidates discovered by LAMOST

About 786.4 thousand stars were observed by LAMOST twice or more during the first stage of its spectroscopic survey. The radial velocity differences for about 256 thousand targets are larger than10 km s^-1 and they are possible spectroscopic binary or variable candidates(SBVCs). It is shown that most SBVCs are slightly metal poorer than the Sun. There are two peaks in the temperature distribution of SBVCs around 5760 K and 4870 K, while there are three peaks in the distribution of the gravitational acceleration at 2.461, 4.171 and 4.621 cm s^-2. The locations of SBVCs on the [Fe/H]-T, [Fe/H]-log g, log g-T and H-R diagrams are investigated. It is found that the detected SBVCs could be classified into four groups. The first group has higher log g～4.621 and lower T ～ 4870 K which are mainly cool red dwarf binaries. The second group of SBVCs has logg around 4.171 cm s^-2 that includes binaries and pulsating stars such as δSet and γ Dor variables. The gravitational accelerations of the third group of SBVCs are higher and some of them are below the zero-age main sequence. They may be contact binaries in which the primary components are losing energy to the secondaries in the common envelopes and are at a special stellar evolutionary stage.The last group is composed of giants or supergiants with log g around 2.461 cm s^-2 that may be evolved pulsating stars. One target(C134624.29+333921.2) is confirmed as an eclipsing binary with a period of 0.65 days. A preliminary analysis suggests that it is a detached binary with a mass ratio of 0.46. The primary fills its critical Roche lobe by about 89%, indicating that mass transfer will occur between the two components.     

天文用电荷耦合器件的实验室检测

介绍云南天文台ＣＣＤ检测实验室检测天文用ＣＣＤ系统的方法,检测参数主要包括：线性、噪声、增益、量子效率以及转移效率等．     

康滇地轴中南段铀成矿条件及远景分析

本文对康滇地轴中南段铀矿化划分出３种类型（砂岩型、钠交代岩型和元古代浅变质岩型），并阐明其主要特征。提出了元古代地壳演化曾经历了原始古陆形成阶段、沉降活动阶段和基底再团结阶段，认为中元古界昆阳群是有别于典型的含铀碳硅泥岩沉积建造。通过对该区部分岩石原始铀含量进行研究，提出了有关岩石可作为该区铀源岩的新认识；划分出碱性和酸性两大类型的热液蚀变，指出本区以发育碱性蚀变地段的成矿前景较好。指出该区铀成矿前景：（１）该区不具备形成澳加式元古代不整合面型铀矿床的地质条件；（２）非澳加式元古代不整合面型的铀成矿前景较差；（３）本区碱（钠）交代岩型铀矿化具有一定的找矿前景。