基于曲线拟合的线要素综合数据整体处理方法

讨论了线要素综合后数据的整体处理与按弧段分区平差两种解算方案，详细推导了按弧段分区平差解算的各种条件方程。通过算例验证，本方法是合理的、实用的。     

黄河上游某电站上新统石膏夹层对坝基岩体稳定性影响评价

拟建的黄河上游某水电站在勘查过程中发现在河床以下存在一层厚约2m的石膏层。石膏岩遇水易溶解,工程地质性质较差,力学强度较低,是水电建设中的不良岩体。本文对石膏岩的物理力学性质和化学成分做了仔细分析,分析了石膏溶蚀后对坝基稳定性的影响,找出防止石膏溶蚀的判断标准,最后得出防治措施。     

监测数据远程传送的方法——全站仪数据远程监测系统简介

随着上海市政建设的发展,自动化监测在工程施工变形中越来越重要。“全站仪数据远程监测系统”能够利用现有互联网络,在远端通过联网计算机实时查看现场的工程数据和相关图表,掌握现场的变形数据变化情况,提高监测工作的效率,满足业主的要求。     

线路坐标计算的通用模型

介绍了一种适合电算的线路坐标计算通用模型。首先,引入了曲线元的概念,使线路的平面线形三要素(直线、圆曲线、缓和曲线)得到了统一。然后,以曲线元作为组成线路的最小单元,推导了线路坐标计算的通用数学模型。该模型形式简单,易于编程实现。不但能解算S型、卵型、复合型、C型等复杂组合线形的任意指定点的坐标,而且能将线路中桩、边桩以及与线路非正交交叉的特殊点位(如桥墩、电线杆等)的坐标解算统一了起来。     

Kinematic parameters of young subsystems and the galactic rotation curve

We analyze the space velocities of blue supergiants, long-period Cepheids, and young open star clusters (OSCs), as well as the H I and H II radial-velocity fields by the maximum-likelihood method. The distance scales of the objects are matched both by comparing the first derivatives of the angular velocity Ω′ determined separately from radial velocities and proper motions and by the statistical-parallax method. The former method yields a short distance scale (for R₀=7.5 kpc, the assumed distances should be increased by 4%), whereas the latter method yields a long distance scale (for R₀=8.5 kpc, the assumed distances should be increased by 16%). We cannot choose between these two methods. Similarly, the distance scale of blue supergiants should be shortened by 9% and lengthened by 3%, respectively. The H II distance scale is matched with the distance scale of Cepheids and OSCs by comparing the derivatives Ω′ determined for H II from radial velocities and for Cepheids and OSCs from space velocities. As a result, the distances to H II regions should be increased by 5% in the short distance scale. We constructed the Galactic rotation curve in the Galactocentric distance range 2–14 kpc from the radial velocities of all objects with allowance for the difference between the residual-velocity distributions. The axial ratio of the Cepheid+OSC velocity ellipsoid is well described by the Lindblad relation, while σ_u≈σ_v for gas. The following rotation-curve parameters were obtained: Ω₀=(27.5±1.4) km s^?1 kpc^?1 and A=(17.1±0.5) km s^?1 kpc^?1 for the short distance scale (R₀=7.5 kpc); and Ω₀=(26.6±1.4) km s^?1 kpc^?1 and A=(15.4±0.5) km s^?1 kpc^?1 for the long distance scale (R₀=8.5 kpc). We propose a new method for determining the angular velocity Ω₀ from stellar radial velocities alone by using the Lindblad relation. Good agreement between the inferred Ω₀ and our calculations based on space velocities suggests that the Lindblad relation holds throughout the entire sample volume. Our analysis of the heliocentric velocities for samples of young objects reveals noticeable streaming motions (with a velocity lag of ～7 km s^?1 relative to the LSR), whereas a direct computation of the perturbation amplitudes in terms of the linear density-wave theory yields a small amplitude for the tangential perturbations.     

基于双差观测序列曲线拟合实现GPS静态定位基线实时解算

对于ＧＰＳ静态差分定位的实时算法而言,能否实时地解决观测数据的存储、卫星失锁、载波相位周跳、多径效应以及计算速度等问题是保证基线的实时解算和定位成功率的重要因素。本文利用载波相位双差观测时间序列可用直线或高次曲线进行很好拟合的特性,设计了一种静态定位的实时算法,能解决上述实时定位中的特殊问题。     

利用GIS实现区化扫面采样点地质代码自动识别

本文主要介绍利用ＧＩＳ对地质图进行数字化采集和编辑,填写每个区的地质属性信息,将区化扫面中涉及的采样点与区进行拓扑分析,从而完成采样点地质代码的自动填写。并介绍了处理过程中的技术难点,为今后化探扫面中地质代码的填写提供了新的方法。     

东营通61断块沙河街组二段储层物性参数展布特征研究

本文在沉积相研究基础上对通６１断块内下第三系沙河街组二段地层的孔隙度、渗透率值做平面展布,统计主要沉积微相的储层物性参数分布规律,分析各沉积微相的储层特征,揭示了沉积微相对储层物性参数展布的控制作用,并指出研究区内的有利砂岩储集层。     

大地电磁标定曲线的畸变及校正

以野外实际工作为例,对大地电磁测深系统中磁探头的响应函数进行分析,总结了转角频率的偏高或偏低与视电阻率和相位曲线畸变之间的关系,提出了合理的校正方案。