路堤侧向变形性状及预测模型研究

结合大量实测资料和已有的研究成果,分析了路堤荷载作用下水平向应变随深度的变化规律,得出了侧向变形沿深度呈“弓”型分布的变化规律;提出了符合该变化规律的预测模型及参数求解方法,模型中a、b和c等3个待定参数能简单地求出。工程实践表明,该预测模型不仅反映了侧向变形随深度的变化规律,且有一定的精度,能反映出最大侧向变形发生的位置,应用效果良好。     

DX14井区火山岩气藏水平井适应性分析

KL气田DX14井区为一火山岩气藏,现有4口水平井。通过对该区火山岩气藏水平井地质条件适应性和设计适应性进行分析,结合已投产2口水平井的生产情况,预测即将投产2口水平井生产效果。提出了该区水平井适应性的评价指标：1、应从气藏类型、气藏深度、气层有效厚度、气层各向异性指数等8个方面,来分析气藏水平井开发的地质适应性;2、认为该区水平井段应沿气层上部部署,水平段长度应根据火山岩体范围控制在600--800m左右,效果较好。     

水平井开采煤层气藏生产动态计算新数学模型

基于朗格缪尔模型、菲克第二扩散定律和达西定律,综合考虑重力和气体压缩效应的影响,推导出描述煤层气和水渗流规律的基本偏微分方程组(并给出定解条件),且利用有限差分法对该数学模型进行了数值求解。计算结果表明,该模型能够有效模拟煤层气水平井的生产动态。通过对比是否考虑非稳态扩散和气体压缩效应时不同裂隙渗透率下的产气动态可知,忽略非稳态扩散和压缩效应,将人为缩短达到气体峰值产量的时间,增大产气峰值;将降低气体膨胀能,低估气井后期产能。煤岩裂隙渗透率越高,气井产能受渗透率回归效应影响越大,峰值产量的持续时间越短且产量下降速度快。因此在煤层气藏开采过程中,应根据气井的产气动态调整井底流压,建立合理的储层压力系统,以降低渗透率回归效应带来的不利影响。     

A new algorithm for distance cartogram construction

A distance cartogram is a diagram that visualizes the proximity indices between points in a network, such as time–distances between cities. The Euclidean distances between the points on the distance cartogram represent the given proximity indices. This is a useful visualization tool for the level of service of transport, e.g. difference in the level of service between regions or points in a network and its improvement in the course of time. The two previously proposed methods—multidimensional scaling (MDS) and network time–space mapping—have certain advantages and disadvantages. However, we observe that these methods are essentially the same, and the merits of both these methods can be combined to formulate a generalized solution. In this study, we first formulate the time–space mapping problem, which includes the key features of both of the above stated methods, and propose a generalized solution. We then apply this solution to the time–distances of Japan's railway networks to confirm its applicability.     

Internet teaching foundation for the Remote Sensing Core Curriculum program

The Remote Sensing Core Curriculum (RSCC) was initiated in 1993 to meet the demands for a college-level set of resources to enhance the quality of education across national and international campuses. The American Society of Photogrammetry and Remote Sensing adopted the RSCC in 1996 to sustain support of this educational initiative for its membership and collegiate community. A series of volumes, containing lectures, exercises, and data, is being created by expert contributors to address the different technical fields of remote sensing. The RSCC program is designed to operate on the Internet taking full advantage of the World Wide Web (WWW) technology for distance learning. The issues of curriculum development related to the educational setting, with demands on faculty, students, and facilities, is considered to understand the new paradigms for WW-influenced computer-aided learning. The WWW is shown to be especially appropriate for facilitating remote sensing education with requirements for addressing image data sets and multimedia learning tools. The RSCC is located at http://www.umbc.edu/rscc     

水平面代替水准面对两井贯通的影响

理论结合实际,用详实的数据说明了在两井贯通时,把水准面当作水平面处理的界限,避免了盲目应用而产生严重后果.     

Globular clusters and the Mira period–luminosity relation

A globular cluster distance scale based on Hipparcos parallaxes of subdwarfs has been used to derive estimates of M _K for cluster Miras, including one in the Small Magellanic Cloud (SMC) globular cluster NGC 121. These lead to a zero-point of the Mira infrared period–luminosity (PL) relation, PL( K ), in good agreement with that derived from Hipparcos parallaxes of nearby field Miras. The mean of these two estimates together with data on LMC Miras yields a Large Magellanic Cloud (LMC) distance modulus of     in evident agreement with a metallicity-corrected Cepheid modulus     .
The use of luminous asymptotic giant branch (AGB) stars as extragalactic population indicators is also discussed.     

低渗透储层水平井—直井联合布井极限注采井距研究

低渗透储层水平井—直井联合布井技术具有广泛的应用前景,其布井方式至关重要。首先利用劈分流场的方法直观地给出常规储层水平井—直井联合布井的产能评价方法;然后针对低渗透储层的渗流特点,在考虑启动压力梯度条件下建立新的井网渗流物理模型并求解得到产能评价公式;最后经分析计算给出启动压力梯度影响的面积井网极限注采井距关系曲线。研究结果为低渗透储层部署水平井—直井联合井网提供理论依据。     

Distant field blue horizontal branch stars – III. Identification of a probable outer halo stream at Galactocentric distance r= 70 kpc

We present FOcal Reducer/low dispersion Spectrograph-1 spectra (from the European Southern Observatory's Very Large Telescope) of a sample of 34 faint  20.0 < g * < 21.1  A-type stars selected from the Sloan Digital Sky Survey Early Data Release, with the goal of measuring the velocity dispersion of blue horizontal branch (BHB) stars in the remote Galactic halo,   R ∼ 80 kpc  . We show that colour selection with  1.08 < u *− g * < 1.40  and  −0.2 < g *− r * < −0.04  minimizes contamination of the sample by less luminous blue stragglers. In classifying the stars we confine our attention to the 20 stars with spectra of signal-to-noise ratio >15 Å⁻¹. Classification produces a sample of eight BHB stars at distances  65–102 kpc  from the Sun (mean 80 kpc), which represents the most distant sample of Galactic stars with measured radial velocities. The dispersion of the measured radial component of the velocity with respect to the centre of the Galaxy is  58 ± 15 km s⁻¹  . This value is anomalously low in comparison with measured values for stars at smaller distances, as well as for satellites at similar distances. Seeking an explanation for the low measured velocity dispersion, further analysis reveals that six of the eight remote BHB stars are plausibly associated with a single orbit. Three previously known outer halo carbon stars also appear to belong to this stream. The velocity dispersion of all nine stars relative to the orbit is only  15 ± 4 km s⁻¹  . Further observations along the orbit are required to trace the full extent of this structure on the sky.     

新疆比勒提地区断裂构造磁异常信息提取及解释

比勒提地区位于新疆西南天山,以该区1：50000高精度磁测数据为基础,采用解析延拓、方向导数等技术手段提取与断裂构造有关的磁异常信息,对区域内构造进行识别,结合标本物性参数统计,对引起磁异常的原因进行分析。对区域磁异常向上延拓及求一阶导数后进行对比,圈定4个特征异常带A1-A4,结合地质资料,识别出4条断裂构造FW1-FW4,FW1和FW2对应喀拉铁克断裂及其次级断裂,FW3为构造动力作用产生的强片理化带,FW4为隐伏断裂,表明高精度磁法测量在本区能有效识别断裂并反映其分布。