220kV盐津变电所填土边坡稳定性研究

针对该填土边坡,介绍了边坡的地质环境背景,描述了该边坡的变形特征,并从地形地貌、地层岩性、地质构造、水文地质条件等场地条件和人类活动等方面对边坡的变形机制进行了分析.结果表明:边坡变形模式是一种推移式蠕滑变形,场地平整填方加载是造成边坡变形的诱发因素,不良的地形地貌、地质结构和地下水条件是导致边坡蠕滑变形的内在因素.基于饱和三轴崮结不排水剪(CU)和排水剪(CD)试验、直剪与反复直剪试验以及岩块单轴抗压强度试验,通过反分析合理地确定了计算参数,通过有限差分软件FLAC3D如对填土边坡进行了变形破坏分析和加固后的稳定性评价.研究结果表明:天然状态下安全系数为1.10:填方堆载后其安全系数为1.03,坡体接近临界状态:抗滑加固后边坡的安全系数为1.27.因此,加固后边坡处于稳定状态.     

结构性吹填土剪切破坏的微结构效应

室内压缩试验、剪切试验和灵敏度试验分析表明吹填土的微观结构对其力学性质有很大的影响,是一种强结构性土。通过对剪切试验过程土样微观SEM照片进行微结构定量分析,探讨了孔隙和结构单元体微结构参数与轴向应变之间的关系。最后,对结构性吹填土剪切破坏的微结构效应进行了简要分析。结果表明,吹填土的剪切过程经历了孔隙气体压缩-水分运移、团粒散裂-颗粒滑移明显-结构破坏和新结构形成三个阶段。     

Resourcesat-1 mission planning,analysis and operations—Outline of key components

Resourcesat-1 is a global mission which provides continuity to the earth resources monitoring missions earlier launched by India. Resourcesat-1 is designed to have an improvement in the payload camera characteristics providing multi-spectral imaging capability in high resolution. This paper provides an overview of mission planning and analysis aiding spacecraft configuration, pre-launch simulations and operations, early-orbit operations and the on-orbit operational guidelines for Resourcesat-1. Mission planning involved integrating and inter-relating the efforts of space and ground systems in realizing the operational system which provides the continuity of satellite-based remote sensing data to the user community. Mission analysis related to contiguous imaging requirement of LISS-4 payload, resulted in a spacecraft yaw steering during imaging operations. Pre-launch simulation involved development of a software spacecraft simulator to be used as a tool for network tests, training of spacecraft operation personnel and validating the spacecraft health monitoring software. The required operations that were performed on the spacecraft to characterize and establish the on-orbit configuration for the normalization of daily operations are addressed in the sections relating to early orbit operations and on-orbit operational guidelines.     

Mechanical properties and time-dependent behaviour of sand-granulated rubber mixtures

The use of granulated recycled rubber as a lightweight material in civil engineering applications has been widely growing over the past 20 years. Processed waste tires mixed with soils have been introduced as lightweight fills for slopes, retaining walls, and embankments. It has also been considered as a damping material under foundations in seismic zones. Understanding the properties of sand-rubber mixtures is essential to evaluate its performance in geotechnical applications. Isotopically consolidated drained (CD) triaxial tests were conducted to investigate the effect of rubber size, content and saturation condition on the mechanical properties of sand-rubber mixtures. Moreover, the compressibility of the sand-rubber mixtures under sustained loading was investigated through one dimensional consolidation tests. The unit weight, shear strength and stiffness of sand-rubber mixtures decreased whereas deformability increased at increased rubber content. A non-linear stress-strain response was observed, that changed from brittle to ductile behaviour at increased rubber content. Sand-rubber mixtures, under one dimensional loading, exhibited significant settlement that increased as rubber content increased.     

The dynamical environment of Dawn at Vesta

Dawn is the first NASA mission to operate in the vicinity of the two most massive asteroids in the main belt, Ceres and Vesta. This double-rendezvous mission is enabled by the use of low-thrust solar electric propulsion. Dawn will arrive at Vesta in 2011 and will operate in its vicinity for approximately one year. Vesta's mass and non-spherical shape, coupled with its rotational period, presents very interesting challenges to a spacecraft that depends principally upon low-thrust propulsion for trajectory-changing maneuvers. The details of Vesta's high-order gravitational terms will not be determined until after Dawn's arrival at Vesta, but it is clear that their effect on Dawn operations creates the most complex operational environment for a NASA mission to date. Gravitational perturbations give rise to oscillations in Dawn's orbital radius, and it is found that trapping of the spacecraft is possible near the 1:1 resonance between Dawn's orbital period and Vesta's rotational period, located approximately between 520 and 580 km orbital radius. This resonant trapping can be escaped by thrusting at the appropriate orbital phase. Having passed through the 1:1 resonance, gravitational perturbations ultimately limit the minimum radius for low-altitude operations to about 400 km, in order to safely prevent surface impact. The lowest practical orbit is desirable in order to maximize signal-to-noise and spatial resolution of the Gamma-Ray and Neutron Detector and to provide the highest spatial resolution observations by Dawn's Framing Camera and Visible InfraRed mapping spectrometer. Dawn dynamical behavior is modeled in the context of a wide range of Vesta gravity models. Many of these models are distinguishable during Dawn's High Altitude Mapping Orbit and the remainder are resolved during Dawn's Low Altitude Mapping Orbit, providing insight into Vesta's interior structure. Ultimately, the dynamics of Dawn at Vesta identifies issues to be explored in the planning of future EP missions operating in close proximity to larger asteroids.     

Analysis of systematic error in “bead method” measurements of meteorite bulk volume and density

The Archimedean glass bead method for determining meteorite bulk density has become widely applied. We used well characterized, zero-porosity quartz and topaz samples to determine the systematic error in the glass bead method to support bulk density measurements of meteorites for our ongoing meteorite survey. Systematic error varies according to bead size, container size and settling method, but in all cases is less than 3%, and generally less than 2%. While measurements using larger containers (above 150 cm³) exhibit no discernible systematic error but much reduced precision, higher precision measurements with smaller containers do exhibit systematic error. For a 77 cm³ container using 40-80 μm diameter beads, the systematic error is effectively eliminated within measurement uncertainties when a “secured shake” settling method is employed in which the container is held securely to the shake platform during a 5 s period of vigorous shaking. For larger 700-800 μm diameter beads using the same method, bulk volumes are uniformly overestimated by 2%. Other settling methods exhibit sample-volume-dependent biases. For all methods, reliability of measurement is severely reduced for samples below ∼5 cm³ (10-15 g for typical meteorites), providing a lower-limit selection criterion for measurement of meteoritical samples.     

基于MapObjects和DLL的自定义地图面符号库的实现

地理信息软件远远不能满足我国的制图要求,在很多二次开发的地理信息系统中都需要使用地图符号库。因此详细地介绍基于VC和MapObjects组件来自定义地图面符号库,并将其编译成DLL。用户可以根据实际的需要来创建各种比例尺的地图面符号库,在实际工程中实现,同时对制作点线符号库也有很大的参考价值。     

现有业务系统建设GIS的模式分析与实践

随着信息化的发展,建设GIS的门槛已经逐步降低,GIS技术也越来越普及,如何在现有业务系统的基础上建设GIS已经成为普遍面临的一个问题。总结了3种建设模式,并对它们的主要区别和优缺点进行了比较分析,最后结合一个项目实践阐述了附加包装模式的具体实现过程。     

Influence of Water Pressure on the Stress State in Stopes with Cohesionless Backfill

The rapid increase of backfill use in underground mines requires a better understanding of the interaction between the fill material and the surrounding rock mass. This is a fairly complex issue as backfill materials are weak compared to the rock mass. This difference in the mechanical behavior induces a stress transfer along the contact area. Previous work conducted on backfilled trenches and mining stopes has shown that basic arching theory can be used to estimate earth pressures in narrow, vertical openings. In this regard, most existing solutions have been developed for dry backfills. However, in many cases, water is present in mine stopes, so its effect should be assessed. In this paper, the authors present a solution to evaluate the stress state in submerged or partially submerged backfilled stopes. The proposed analytical solution is validated against numerical modeling results.     

Late Mesozoic and Cenozoic rifting and its dynamic setting in Eastern China and adjacent areas

During the Late Mesozoic and Cenozoic, extension was widespread in Eastern China and adjacent areas. The first rifting stage spanned in the Late Jurassic–Early Cretaceous times and covered an area of more than 2 million km² of NE Asia from the Lake Baikal to the Sikhot-Alin in EW direction and from the Mongol–Okhotsk fold belt to North China in NS direction. This rifting was characterized by intracontinental rifts, volcanic eruptions and transform extension along large-scale strike–slip faults. Based on the magmatic activity, filling sequence of basins, tectonic framework and subsidence analysis of basins, the evolution of this area can be divided into three main developmental phases. The first phase, calc-alkaline volcanics erupted intensely along NNE-trending faults, forming Daxing'anling volcanic belt, NE China. The second phase, Basin and Range type fault basin system bearing coal and oil developed in NE Asia. During the third phase, which was marked by the change from synrifting to thermal subsidence, very thick postrift deposits developed in the Songliao basin (the largest oil basin in NE China).Following uplift and denudation, caused by compressional tectonism in the near end of Cretaceous, a Paleogene rifting stage produced widespread continental rift systems and continental margin basins in Eastern China. These rifted basins were usually filled with several kilometers of alluvial and lacustrine deposits and contain a large amount of fossil fuel resources. Integrated research in most of these rifting basins has shown that the basins are characterized by rapid subsidence, relative high paleo-geothermal history and thinned crust. It is now accepted that the formation of most of these basins was related to a lithospheric extensional regime or dextral transtensional regime. During Neogene time, early Tertiary basins in Eastern China entered a postrifting phase, forming regional downwarping. Basin fills formed in a thermal subsidence period onlapped the fault basin margins and were deposited in a broad downwarped lacustrine depression. At the same time, within plate rifting of the Lake Baikal and Shanxi graben climaxed and spreading of the Japan Sea and South China Sea occurred. Quaternary rifting was marked by basalt eruption and accelerated subsidence in the area of Tertiary rifting. The Okinawa Trough is an active rift involving back-arc extension.Continental rifting and marginal sea opening were clearly developed in various kind of tectonic settings. Three rifting styles, intracontinental rifting within fold belt, intracontinental rifting within craton and continental marginal rifting and spreading, are distinguished on the basis of nature of the basin basement, tectonic location of rifting and relations to large strike–slip faults.Changes of convergence rates of India–Eurasia and Pacific–Eurasia may have caused NW–SE-trending extensional stress field dominating the rifting. Asthenospheric upwelling may have well assisted the rifting process. In this paper, a combination model of interactions between plates and deep process of lithosphere has been proposed to explain the rifting process in East China and adjacent areas.The research on the Late Mesozoic and Cenozoic extensional tectonics of East China and adjacent areas is important because of its utility as an indicator of the dynamic setting and deformational mechanisms involved in stretching Lithosphere. The research also benefits the exploration and development of mineral and energy resources in this area.