天文经纬度和天文方位角测定的基本原理

大地天文测量无论在基础科学,还是在国民经济和国防建设中都具有重要的意义。随着空间大地测量技术(VLB、ILLR、SLR和GPS等)的发展,虽然天文测量在应用上有所减少,但在大地测量的绝对定位和中远程武器的发射等领域中仍然是不可替代的技术。本文详细地介绍了天文经纬度和天文方位角测量的基本原理和方法,综述了天文测量目前的发展状况和存在的问题。本文的工作可为天文大地测量的研究提供一定的参考和依据。     

基于大视场光学测量设备的多星观测和解算天文经纬度研究

本文提出了一种新的基于大视场光学测量设备和GPS测量点位天文坐标的方法,即测量多个星体方位角相对于主光轴方位角的增量,然后通过非线性最小二乘法解算出点位的天文坐标。采用该方法不仅可以避免讨论大气蒙气差的修正问题,而且能够满足高精度天文坐标的测量要求。     

Deflection of the vertical and refraction in three-dimensional adjustment of terrestrial networks

Summary In this paper statistical tests are exploited in order to verify the hypotheses about the refraction and the deflection of the vertical pertaining to a geometrical model for the three-dimensional adjustment of terrestrial networks. The deflections of the vertical and the refraction coefficients can be assumed either as unknowns or fixed input data, at some or all the points of the network. The geometrical model, reported in the appendix for convenience, assumes as observables the slant distances, zenith and horizontal angles, without any reduction neither to the marks on the ground nor to the surface of reference. Further, the observation equations are derived and linearized in terms of Cartesian coordinates in Geocentric or Topocentric system; direction cosines of the vertical and of the ellipsoidal normal are adopted as the relevant direction parameters. Finally, an application to a network from Hradilek (1984), performed under different assumptions about the unknowns and the corrections of the angular observations due to the deflections of the vertical, shows the effectiveness of the proposed approach.     

Simple and highly accurate formulas for the computation of Transverse Mercator coordinates from longitude and isometric latitude

A conformal approximation to the Transverse Mercator (TM) map projection, global in longitude λ and isometric latitude q, is constructed. New formulas for the point scale factor and grid convergence are also shown. Assuming that the true values of the TM coordinates are given by conveniently truncated Gauss–Krüger series expansions, we use the maximum norm of the absolute error to measure globally the accuracy of the approximation. For a Universal Transverse Mercator (UTM) zone the accuracy equals 0.21  mm, whereas for the region of the ellipsoid bounded by the meridians  ±20° the accuracy is equal to 0.3  mm. Our approach is based on a four-term perturbation series approximation to the radius r(q) of the parallel q, with a maximum absolute deviation of 0.43  mm. The small parameter of the power series expansion is the square of the eccentricity of the ellipsoid. This closed approximation to r(q) is obtained by solving a regularly perturbed Cauchy problem with the Poincaré method of the small parameter. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.     

天文经纬度归心实用算式推证

文中分析天文经纬度归心公式中各变量的特点,推导基于2000国家大地坐标系统简单实用的归心计算公式,进一步给出由已确定变量推求归心元素测量精度的数学关系式。验证实用公式计算的归心改正数满足专用工程天文经纬度的计算精度需求。     

基于LightGBM的全球海洋次表层温盐遥感预测

随着卫星遥感技术的发展,越来越多的卫星观测数据被应用于预测海洋内部温盐结构信息,而如何有效提高海洋内部温盐信息的预测精度仍是一个挑战。本文应用LightGBM算法结合随机森林算法构建全球海洋次表层（0—1000 m）温度异常（STA）与盐度异常（SSA）的预测模型,模型使用海表卫星观测数据（海表高度异常（SSHA）、海表温度异常（SSTA）、海表盐度异常（SSSA）和海表风场异常水平和垂直分量（USSWA、VSSWA）,结合经纬度信息（LON、LAT）作为预测变量,使用Argo次表层温盐数据作为模型训练与测试标记。本文使用五参数模型（SSTA、SSHA、SSSA、USSWA、VSSWA）、带纬度六参数模型（LAT、SSTA、SSHA、SSSA、USSWA、VSSWA）、带经度六参数模型（LON、SSTA、SSHA、SSSA、USSWA、VSSWA）与带经纬度七参数模型（LON、LAT、SSTA、SSHA、SSSA、USSWA、VSSWA）来着重分析LON与LAT在STA、SSA遥感预测中发挥的作用。结果表明LON与LAT在STA、SSA各自预测中发挥不同的作用。在单时相和时序预测STA中LON与LAT对模型的贡献随着深度的增加逐渐增大,而在单时相和时序预测SSA中LON与LAT对不同深度预测模型始终保持较大的贡献。在单时相预测STA与SSA中LON较LAT对模型贡献更大,而在时序预测STA与SSA中LAT较LON对模型贡献更大。经纬度信息是全球海洋次表层温盐机器学习预测的重要参数,可以提高模型的预测精度。同时,LightGBM较随机森林在预测海洋次表层温盐异常时精度更高鲁棒性更强。     

Method of simultaneous determination of astronomic latitude,azimuth and longitude by observing only time and horizontal angles between a pair of stars near elongation and a south star near meridian

Summary This paper endeavours to evolve a method of simultaneous determination of astronomic latitude, azimuth and longitude from observations of a star-pair near their times of east and west elongations and a south star near its time of meridian transit. The star-pair of observation being within a short distance of elongation, either east or west, their motion in azimuth then is extremely slow and the small error in time has therefore insignificant effect on their azimuth, and in addition, the south star with its azimuth known from observations of the previous star-pair, being very fast-moving, the method is especially suitable for determining the astronomic latitude, azimuth and longitude by observing only the time and horizontal angees between them, and also a reference mark for ensuring the orientation of the horizontal circle side by side.     

地图中国界线与经纬线关系表示方法探究

国界线是地图中的重要内容。经纬线不仅用于确定位置和方向,也用于国家之间划分国界线。地图上绘制国界线不仅要遵循相关法规、条约及标准,还应当正确处理好国界线与经纬线的关系。本文通过介绍地图中绘制国界线的依据,重点梳理国界线与经纬线关系容易出错的几个重点区域,对相关地图编制和地图审查部门起到一定的借鉴作用。     

World geodetic datum WD 1 and WD 2 from satellite and terrestrial observations

By minimizing the global distance between the (quasi-) geoid and an ellipsoid of revolution, the best parameters of an ellipsoid and its location parameters are estimated. Input data are the absolute value of the geopotential at (quasi-) geoid level, a set of harmonic coefficients from satellite, terrestrial or combined observations, the mean rotational speed of the earth, and approximate values of the seminajor axis and the eccentricity of the ellipsoid. The output ranges from 6378137,63 m and 6378141,62 m for the best semimajor axis and from 298.259758 and 298.259651 for the reciprocal value of the best ellipsoidal flattening within WD 1 and WD 2. The best translational parameters are 6.4 cm (Greenwich-direction), 0.8 cm (orthogonal to Greenwich-direction), and 1.9 cm (parallel to rotational axis of the earth); the best rotational parameters are −0.2” (around Greenwich-direction) and 1.1” (around orthogonal to Greenwich-direction). The dependence of the datum of the (quasi-) geoid geopotential is studied in detail.     

利用天测与测地VLBI观测建立天球与地球参考架

本文讨论了利用天测与测地 VLBI观测建立天球与地球参考架过程中所面临的问题及解决的技术途径 ,涉及天球参考架与地球参考架原点与定向的确定、地球参考架时间演变的确定等。并通过实测数据分析与结果比对证明解决途径的有效性。     

Problems of accuracies in combined terrestrial and statellite control networks

Summary The combination of terrestrial and satellite aided network observations requires hybrid models of two kinds: a hybrid functional model and a stochastic model being able to process the heterogeneous observations approapriately. An appropriate combination of stochastic information means to adjoin proper weights to the various types of observations on one hand and on the other hand to separate the relelevant internal accuracy from that accuracy which is affected by a number of network external influences. The first task can be overcome by the technique of estimating variance components of the individual observation groups, the second one can be handled by applying S-transformations to covariance matrices. The paper deals with problems of the hybrid stochastic model. Examples are given.     

地面LiDAR技术与移动最小二乘法在三维建模中的应用

地面LiDAR不仅能够快速获得建筑物表面精确三维坐标点云信息,并且利用自身所携带的相机同时采集建筑物的影像信息,这使得地面LiDAR在城市三维建模与古建筑精细模型制作中得到广泛应用。然而地面Li-DAR采集的点云数据巨大,离散点之间没有关系,这给建模带来了困难。本文通过将地面LiDAR数据进行预处理得到建筑物点云数据,再通过移动最小二乘法来拟合建筑面构建建筑物模型,实验证明移动最小二乘法拟合得到的建筑物模型光滑准确,能够将建筑物的细节信息表达出来。     

Determination of GPS orbits using double difference carrier phase observations from regional networks

Summary Carrier phase measurements are potentially the most precise observations available from theGPS satellite system, the formal precision being of the order of one centimeter per observation. If the so called double differences are used as the basic observable, the analysis is relatively simple, since satellite- and receiver-clocks may be represented by basic models. We investigate the feasibility of double difference phase observations for orbit determination using the material of the 1985 High Precision Baseline Test, where the coordinates of the so called fiducial points (Haystack, Ft. Davis Richmond and Mojave) are held fixed.TI-4100 andAFGL-receiver observations were used in the same orbit determination process. Although no surface weather data had been available to us, the orbit quality seems to be of the order of0.1 ppm. When we use these orbits to estimate the coordinates of the five “non-fiducial points” Owens Valley, Hat Creek Mammoth Lake, Austin and Dahlgren we get a repeatability of the order of5 cm for latitude and longitude and10 cm for height, if the observations of the first four days of the campaign are compared to those of the second four days. If we use our orbits estimated withTI andAFGL observations to process the Mojave—Owens Valley baseline (length245 km) measured by the twoSERIES-X receivers, we obtain day to day repeatabilities of1.6 cm (0.06 ppm) in length,2 cm (0.08 ppm) in latitude,4 cm (0.16 ppm) in longitude and7 cm (0.29 ppm) in height. Since there are indications that regional networks will be realized in the near future, the results presented here should encourage the realization of regional high precision orbit determination services.     

地面LiDAR数据模拟及单木LAI反演

地面激光雷达Li DAR可以快速获取高精度、高密度的点云数据,在植被结构参数获取方面的应用越来越广泛。为了定量分析地面激光雷达点云数据获取单木结构参数的能力和精度,本文提出利用光线跟踪结合植被真实结构模拟地面3维激光扫描仪的单木点云数据(以RIEGL VZ-1000为例),并结合间隙率模型反演单木叶面积指数LAI。在点云模拟过程中,充分考虑了脉冲特性,包括光斑大小、波束发射角以及回波探测强度。重点分析了光斑大小和最小探测强度对LAI反演的影响,并采用根河实测单木数据进行了验证。结果表明,光斑大小和最小探测强度的设定对于LAI反演结果存在很大影响,该结论对于提高地面激光雷达点云数据反演植被结构参数精度具有重要意义。     

Estimating regional deformation from a combination of space and terrestrial geodetic data

We discuss an approach for efficiently combining different types of geodetic data to estimate time-dependent motions of stations in a region of active deformation. The primary observations are analyzed separately to produce loosely constrained estimates of station positions and coordinate system parameters which are then combined with appropriate constraints to estimate velocities and coseismic displacements. We define noninteger degrees of freedom to handle the case of finite constraints and stochastic perturbation of parameters and develop statistical tests for determining compatibility between different data sets. With these developments, we show an example of combining space and terrestrial geodetic data to obtain the deformation field in southern California. Received: 23 January 1997 / Accepted: 30 September 1997     

Aboveground total and green biomass of dryland shrub derived from terrestrial laser scanning

Sagebrush (Artemisia tridentata), a dominant shrub species in the sagebrush-steppe ecosystem of the western US, is declining from its historical distribution due to feedbacks between climate and land use change, fire, and invasive species. Quantifying aboveground biomass of sagebrush is important for assessing carbon storage and monitoring the presence and distribution of this rapidly changing dryland ecosystem. Models of shrub canopy volume, derived from terrestrial laser scanning (TLS) point clouds, were used to accurately estimate aboveground sagebrush biomass. Ninety-one sagebrush plants were scanned and sampled across three study sites in the Great Basin, USA. Half of the plants were scanned and destructively sampled in the spring (n = 46), while the other half were scanned again in the fall before destructive sampling (n = 45). The latter set of sagebrush plants was scanned during both spring and fall to further test the ability of the TLS to quantify seasonal changes in green biomass. Sagebrush biomass was estimated using both a voxel and a 3-D convex hull approach applied to TLS point cloud data. The 3-D convex hull model estimated total and green biomass more accurately (R² = 0.92 and R² = 0.83, respectively) than the voxel-based method (R² = 0.86 and R² = 0.73, respectively). Seasonal differences in TLS-predicted green biomass were detected at two of the sites (p < 0.001 and p = 0.029), elucidating the amount of ephemeral leaf loss in the face of summer drought. The methods presented herein are directly transferable to other dryland shrubs, and implementation of the convex hull model with similar sagebrush species is straightforward.     

基于TLS技术的典型建筑物震害信息三维建模分析——以彭州市白鹿中学为例

传统光学及雷达遥感技术在地震灾害损失评估中无法获取建筑物立面破坏信息,对结构已遭破坏,但顶面基本完好的建筑物识别能力较差。三维激光扫描技术(terrestrial laser scanning,TLS)可以获取建筑物结构破坏状况的高精度三维信息。利用2013年10月23日RIEGL VZ-1000三维激光扫描仪采集到的汶川地震震后彭州市白鹿中学的精细点云数据,通过不规则三角网建模和纹理贴图等处理进行三维建模分析,在此基础上对建筑物的典型破坏特征及地表破裂情况进行了详细建模研究,真实再现了白鹿中学破坏场景,实现了震害信息的永久保存。研究结果表明:位于断层上盘的勤学楼整体无明显破损;位于下盘的求知楼损毁相对严重,普遍出现"X"形的共轭剪切裂缝、构造柱断裂及露筋等现象;地震陡坎沉降量不大,高程剖面显示现今该陡坎最低高度为205 cm,最高为231 cm,与GPS测量结果大致吻合。