国际南极大地参考框架的构建与进展   总被引：10，自引：2，他引：8  

鄂栋臣  张胜凯 《大地测量与地球动力学》2006,26(2):104-108

回顾了南极大地参考框架发展的历史,总结了由国际南极研究科学委员会(SCAR)组织的历次南极地区大地测量观测活动的成果,并结合2007~2008第四次国际极地年(IPY)对南极大地参考框架的前景进行了展望,其中重点介绍了我国对构建南极大地参考框架的贡献。  相似文献   

基于扩展EL的大地测量报表系统     

陈正生  吕志平  李昌贵  王鹏 《四川测绘》2010,33(4):159-161

通过分析现有大地测量数据报表格式中存在的问题，以基于XML的大地测量数据接口文档为数据模型，建立了以Word文档为模板的EL引擎，使用户能够方便地对大地测量报表模板的样式和内容进行动态控制和修改，实现了数据库管理系统与报表系统、报表格式和数据内容的解耦，增加了报表的灵活性和扩展性。  相似文献   

Numerical simulations of a Mars geodesy network experiment: Effect of orbiter angular momentum desaturation on Mars' rotation estimation     

P. Rosenblatt  J.C. Marty  J.P. Barriot  V. Dehant 《Planetary and Space Science》2004,52(11):965-975

The scientific objectives of a geodetic experiment based on a network of landers, such as NEIGE (NEtlander Ionosphere and Geodesy Experiment) are to improve the current knowledge of Mars' interior and atmosphere dynamics. Such a network science experiment allows monitoring the motions of the Martian rotation axis with a precision of a few centimeters (or milli-arc-seconds (mas)) over annual and sub-annual periods. Thereto, besides radio tracking of a Mars orbiter from the Earth, radio Doppler shifts between this orbiter and several landers at the planet's surface will be performed. From the analysis of these radio Doppler data, it is possible to reconstruct the orbiter motion and Mars' orientation in space. The errors on the orbit determination (position and velocity of the orbiter) have an impact on the geodetic parameters determination from the Doppler shifts and must be removed from the signal in order to achieve a high enough accuracy. In this paper, we perform numerical simulations of the two Doppler signals involved in such an experiment to estimate the impact of the spacecraft angular momentum desaturations on the determination of Mars' orientation variations. The attitude control of the orbiter needs such desaturation maneuvers regularly repeated. They produce velocity variations that must be taken into account when determining the orbit. For our simulations, we use a priori models of the Martian rotation and introduce the spacecraft velocity variations induced by each desaturation event. By a least-squares adjustment of the simulated Doppler signals, we then estimate the orbiter velocity variations and the parameters of the Mars' rotation model. We show that these velocity variations are ill resolved when the spacecraft is not tracked, therefore requiring a near-continuous tracking from the Earth to accurately determine the orbit. In such conditions we show that only 15- of lander-orbiter tracking per week allows recovering Mars' orientation parameters with a precision of a few mas over a period of 1 Martian year.  相似文献   

Position and velocity perturbations for the determination of geopotential from space geodetic measurements   总被引：10，自引：0，他引：10  

Peiliang Xu 《Celestial Mechanics and Dynamical Astronomy》2008,100(3):231-249

Although space geodetic observing systems have been advanced recently to such a revolutionary level that low Earth Orbiting (LEO) satellites can now be tracked almost continuously and at the unprecedented high accuracy, none of the three basic methods for mapping the Earth’s gravity field, namely, Kaula linear perturbation, the numerical integration method and the orbit energy-based method, could meet the demand of these challenging data. Some theoretical effort has been made in order to establish comparable mathematical modellings for these measurements, notably by Mayer-Gürr et al. (J Geod 78:462–480, 2005). Although the numerical integration method has been routinely used to produce models of the Earth’s gravity field, for example, from recent satellite gravity missions CHAMP and GRACE, the modelling error of the method increases with the increase of the length of an arc. In order to best exploit the almost continuity and unprecedented high accuracy provided by modern space observing technology for the determination of the Earth’s gravity field, we propose using measured orbits as approximate values and derive the corresponding coordinate and velocity perturbations. The perturbations derived are quasi-linear, linear and of second-order approximation. Unlike conventional perturbation techniques which are only valid in the vicinity of reference mean values, our coordinate and velocity perturbations are mathematically valid uniformly through a whole orbital arc of any length. In particular, the derived coordinate and velocity perturbations are free of singularity due to the critical inclination and resonance inherent in the solution of artificial satellite motion by using various types of orbital elements. We then transform the coordinate and velocity perturbations into those of the six Keplerian orbital elements. For completeness, we also briefly outline how to use the derived coordinate and velocity perturbations to establish observation equations of space geodetic measurements for the determination of geopotential.  相似文献   

流动卫星激光测距技术在中国的发展     

秦宽  魏二虎  严韦 《测绘科学》2007,32(2):169-171

SLR(卫星激光测距)技术是一项应用广泛的空间大地测量技术,本文在介绍其测距原理的基础上,通过与GPS、VLBI技术进行对比,分析了其实现手段和所能达到的精度;根据SLR应用现状提出了在国内建立SLR流动站的思路;并对SLR技术的未来发展作了展望。  相似文献   

Geodetic and geological evidence of active tectonics in south-western Sicily (Italy)     

《Journal of Geodynamics》2014

Integrated geological, geodetic and marine geophysical data provide evidence of active deformation in south-western Sicily, in an area spatially coincident with the macroseismic zone of the destructive 1968 Belice earthquake sequence. Even though the sequence represents the strongest seismic event recorded in Western Sicily in historical times, focal solutions provided by different authors are inconclusive on possible faulting mechanism, which ranges from thrusting to transpression, and the seismogenic source is still undefined. Interferometric (DInSAR) observations reveal a differential ground motion on a SW–NE alignment between Campobello di Mazara and Castelvetrano (CCA), located just west of the maximum macroseismic sector. In addition, new GPS campaign-mode data acquired across the CCA alignment documents NW–SE contractional strain accumulation. Morphostructural analysis allowed to associate the alignment detected through geodetic measurements with a topographic offset of Pleistocene marine sediments. The on-land data were complemented by new high-resolution marine geophysical surveys, which indicate recent contraction on the offshore extension of the CCA alignment. The discovery of archaeological remains displaced by a thrust fault associated with the alignment provided the first likely surface evidence of coseismic and/or aseismic deformation related to a seismogenic source in the area. Results of the integrated study supports the contention that oblique thrusting and folding in response to NW–SE oriented contraction is still active. Although we are not able to associate the CCA alignment to the 1968 seismic sequence or to the historical earthquakes that destroyed the ancient Greek city of Selinunte, located on the nearby coastline, our result must be incorporated in the seismic hazard evaluation of this densely populated area of Sicily.  相似文献   

Revealing Mars’ deep interior: Future geodesy missions using radio links between landers, orbiters, and the Earth     

V. Dehant  S. Le Maistre 《Planetary and Space Science》2011,59(10):1069-1081

In the frame of a comparison between Earth, Venus, and Mars, a vision on future geodesy missions to Mars is discussed with particular focus on furthering our understanding of the interior, rotation, and orientation of this terrestrial planet. We explain how radioscience instruments can be used to observe the rotation and orientation and therewith to study the deep interior of Mars and its global atmosphere dynamics. Transponders in X-band and Ka-band are proposed with radio links between a lander or a rover and an orbiter around Mars and/or directly to the Earth. The radio budget links are studied in the frame of possible mission constraints and simulations are performed, which show that important information on the interior of Mars can be obtained from the radioscience data. From the observation of Mars’ orientation in space and of tidal effects on a spacecraft orbiting around Mars we show that it is possible for instance to constrain the dimension and composition of the core, the percentage of light element within the core, and to determine the presence of a pressure-induced mineral-phase transition at the bottom of the mantle.  相似文献   

基于PCWin98经济网络分布式动力大地测量学数据库的设计与实现   总被引：1，自引：1，他引：0  

罗少聪 《地球物理学进展》2000,15(4):97-103

分析了动力大地测量学数据的结构和应用特点,结构现有网络和计算机软硬件状况,兼顾使用者的计算机水平和建库的人物力条件,得出了建立地测量学科数据库的思路和方案,建成基于Ｗｉｎ９８经济网络分布式动力大地测量学数据库。基于Ｗｉｎ９８经济网络、以资源共享方式集成的数据库系统开发环境有很大的在线数据存储能力、灵活分散式的数据库实现模式和调用功能。实现了以往大型计算机才能完成的系统。目前,系统平时能满足一般需要,必要时完成大型复杂任务。已拥有中国及其邻区原始气象数据、全球平均气压数据、超导观测数据、中国邻区重力场数据、地球自转及其有关数据、海潮模型、重力模型、软件等子库,容量达数十千兆,为科研提供快捷的数据服务。为目前普遍使用的区域网用户提供一种可行的科学数据库实现模式。  相似文献   

方差分量估计理论及其在整体大地测量中的应用     

王兴涛 《测绘学院学报》1990,(1)

本文探讨了整体大地测量平差中的方差分量估计问题,给出了自适应最小二乘配置;不仅较好地解决了各类观测量权比的确定问题,而且能够确定信号的方差因子。此外,文章还对如何更好地确定局部地区扰动位及其泛函的协方差函数作了讨论;最后通过对一个实测网进行了整体平差,并与经典平差结果进行了比较。  相似文献   

Accuracy assessment of the National Geodetic Survey’s OPUS-RS utility   总被引：1，自引：1，他引：0  

Charles R. Schwarz  Richard A. Snay  Tomás Soler 《GPS Solutions》2009,13(2):119-132

OPUS-RS is a rapid static form of the National Geodetic Survey’s On-line Positioning User Service (OPUS). Like OPUS, OPUS-RS accepts a user’s GPS tracking data and uses corresponding data from the U.S. Continuously Operating Reference Station (CORS) network to compute the 3-D positional coordinates of the user’s data-collection point called the rover. OPUS-RS uses a new processing engine, called RSGPS, which can generate coordinates with an accuracy of a few centimeters for data sets spanning as little as 15 min of time. OPUS-RS achieves such results by interpolating (or extrapolating) the atmospheric delays, measured at several CORS located within 250 km of the rover, to predict the atmospheric delays experienced at the rover. Consequently, standard errors of computed coordinates depend highly on the local geometry of the CORS network and on the distances between the rover and the local CORS. We introduce a unitless parameter called the interpolative dilution of precision (IDOP) to quantify the local geometry of the CORS network relative to the rover, and we quantify the standard errors of the coordinates, obtained via OPUS-RS, by using functions of the form here α and β are empirically determined constants, and RMSD is the root-mean-square distance between the rover and the individual CORS involved in the OPUS-RS computations. We found that α = 6.7 ± 0.7 cm and β = 0.15 ± 0.03 ppm in the vertical dimension and α = 1.8 ± 0.2 cm and β = 0.05 ± 0.01 ppm in either the east–west or north–south dimension.  相似文献