共查询到19条相似文献，搜索用时 140 毫秒
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高精度三维坐标控制网是进行空间大尺寸精密坐标测量的基础,在对大尺寸机构和大型设备的安装、调试、监测过程中发挥着至关重要的作用。现阶段,激光测距的精度可达微米级,因此,利用激光测距可建立高精度的三维控制网。与边角网中点位精度受测角和测距精度两者的影响不同,三维测边网中点位精度仅受测距误差的影响。为了建立全局的精密三维控制网,文中基于激光测距建立了三维测边网整体平差模型,解算出测站点与定向点坐标,并利用Levenberg-Marquardt(LM)优化算法根据距离前方交会原理对三维网进行优化。经实验验证,优化算法提高了定向点的精度。 相似文献
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星载激光测距精度是影响激光测高仪几何检校与处理精度的主要来源之一.针对由全波形星载激光模拟信号经数字化处理后的量化误差带来的激光测距提取精度不高、稳定性低的问题,本文提出一种全波形星载激光测距误差抑制的滑动窗口高斯拟合算法.该方法利用滑动窗口剔除波峰附近似噪声点,并基于高斯曲线拟合优化波形峰值,从而精化激光测距值.然后以高分七号国产星载激光测高仪为试验对象,利用冰面、内陆湖面和平坦陆地地表进行激光高程相对和绝对精度对比验证.结果表明,相对于一般峰值方法,本文算法使得激光测距精度提升了7.5 cm;基于本文方法提取的测距值,计算的激光高程相对精度提升4.2 cm;利用机载LiDAR点云数据验证,高程绝对精度提升了4.5 cm;充分说明本文方法可作为有效减少星载激光测距随机误差的一种方法,为高分七号卫星亚米级高程测量精度处理提供了不可或缺的基础. 相似文献
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现在,激光测卫与测月已达到进行地球动力学研究所需的精度。本文从激光测距系统的主要硬部件、环境影响对测距精度的限制以及数据处理等方面,论述激光测距的现状及发展趋势。 相似文献
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利用脉冲激光测量地面站至人造卫星（装有后向反射器）的距离是六十年代中期出现的新技术，是目前观测人卫最准确的手段。它大大超过了跟踪照相机和其它无线电方法的精度。经过十多年的努力，人卫照相机的最高精度仅达到1″（角秒）左右，对于2000公里远的卫星，相应的位置误差为10米。由于大气折射等因素的影响，要得到较大的改进，希望甚微。而人卫激光测距采用了新的测量原理，不用测量卫星的方位，而是测量其距离，这种方法受大气的影响小。由于光速在大气中变慢所引起的误差，可以根据测站的气象资料作精确改正，在地平高度10°以上，改正的误差有可能小于1厘米。因此，人卫测距技术比较容易获得2—3米的精度。 相似文献
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《测绘科学》2020,(5)
针对北斗卫星导航系统空间信号测距误差能否满足公开服务性能需求的问题,该文顾及卫星轨道误差和卫星钟误差影响的北斗卫星导航系统空间信号测距误差评估方法,利用MGEX提供的北斗广播星历和GFZ提供的事后精密星历,对2018年1月北斗卫星的广播星历误差、轨道误差和空间信号测距误差进行了短期分析评估。结果表明,所有北斗卫星在评估期内的空间信号测距误差精度为2.11 m,满足北斗系统公开服务空间信号性能需求。其中,MEO卫星空间信号测距误差精度最高,为1.43 m,GEO卫星精度最差,为2.62 m;所有卫星的空间信号测距误差总体上优于2.5 m,空间信号测距误差呈1 d周期变化;在变化趋势上,MEO空间信号测距误差变化比较稳定,而GEO和IGSO存在一定的跳变情况。 相似文献
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针对超宽带测距误差大影响定位精度以及传统精度评定方案不能准确反映定位区域误差问题,该文基于RBF神经网络的UWB测距模型提高测距精度,针对室内狭长楼道环境特点,分析UWB基站组网优化方案下的四基站布设与五基站布设精度.分析表明,在相同定位区域,五基站布设方法有效抑制了四基站布设时中间区域最大PDOP值.在测距误差经过改正后,UWB基站组网优化方案更准确反映测区精度.相同精度要求下,采用基站优化布设方案基站覆盖范围更广,可用于应急场景快速定位.基于不等精度加权DOP值的UWB基站组网优化方案,在考虑测距误差后能够准确反映UWB基站布设区域定位精度. 相似文献
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激光在天空对地观测中的应用 总被引：1，自引：0，他引：1
1960年7月世界上第一台激光器问世后，激光测距迅速兴起，不管是地面激光测距，还是激光测卫和激光测月，都为大地测量学的发展作出了重大贡献；特别是激光测卫测月成果，为我们深化对地球动态效应的认识，揭示地球的奥秘，提供了许多重要的科学数据，本文综析了值得注视的下列新近发展。.在IGEX-98国际大联测中，求定GLONASS卫星的激光轨道与微波轨道之差；.评定PRN05/06号GPS卫星星历的精度；.检核Topex/Poseidon海洋测高卫星用GPS定轨的测量误差，.用机载激光测深系统测量海水的浓度；.用EOS-ALT星载激光测距/测高系统测量地球动态参数。 相似文献
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从全球国际地球参考框架（International Terrestrial Reference Frame，ITRF）的建立、维护与发展，卫星测高、卫星重力等的发展及应用，全球卫星导航系统（Global Navigation Satellite System，GNSS）、卫星激光测距（Satellite Laser Ranging，SLR）、甚长基线干涉测量（very Long Baseline Interferometry，VLBI）、卫星多普勒定轨定位（Doppler Orbitography by Radiopositioning Integrated on Satellite，DORIS）的融合应用，海洋测绘和室内定位的发展等几个方面综述了大地测量学及卫星导航定位技术的最新进展，并提出中国2000国家大地坐标系与自主卫星导航系统的主要应用及发展目标。 相似文献
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卫星激光测距（satellite laser ranging,SLR）作为一种完全独立于微波测量的测距方法,为GNSS（global navigation satellite system）广播星历精度评估提供了独立的外部检核手段。基于2013年4月~2014年7月的北斗卫星SLR数据,对北斗卫星导航系统正式提供服务后的广播星历精度进行了评估,推导了北斗地球静止轨道卫星激光残差近似表达式,分析了不同姿态模式下北斗倾斜地球同步轨道卫星、中圆地球轨道卫星激光残差特性。检核结果表明了参与国际激光联测的北斗卫星C01星广播星历精度为0.97 m、C08星为0.43 m、C10星为0.41 m、C11星为0.41 m。 相似文献
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Additional results are presented concerning a study that consider improvements over present Earth Rotation Parameter (ERP) determination methods by directly combining observations from various space geodetic systems in one adjustment. Earlier
results are extended, showing that in addition to slight improvements in accuracy substantial (a factor of three or more)
improvements in precision and significant reductions in correlations between various parameters can be obtained (by combining
Lunar Laser Ranging (LLR), Satellite Laser Ranging (SLR) to Lageos, and Very Long Baseline Interferometry (VLBI) data in one adjustment) as compared to results from individual systems. Smaller improvements are also seen over the weighted
means of the individual system results. Although data transmission would not be significantly reduced, negligible additional
computer time would be required if (standardized) normal equations were available from individual solutions. Suggestions for
future work and implications for the new International Earth Rotation Service (IERS) are also presented. 相似文献
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A new computer-aided design (CAD) program called Falcon 3.0 has been created to simulate and evaluate receiver designs. This
CAD tool aims to solve tasks at the design stage of navigation receivers that operate with signals from Navigational Satellite
Time and Ranging (NAVSTAR) and Global Navigational Satellite System (GLONASS). Specific tasks include:
· Defining the receiver frequency plan (frequencies of oscillators and filters that guarantee accuracy of the receiver)
· Specifying parameters for the digital processing of received signal
· Computing interpath and interchannel biases
· Computing statistical characteristics of correlation signals I, Q, dl, and dQ
· Calculating noise and multipath errors of measurements
· Determeining energy losses
This CAD tool has been used in the design of receivers such as Javad Positioning Systems (JPS) Legacy, Regency, Odyssey, and
Eurocard and in the prediction of their accuracy. It has been shown that experimental and predicted data agree well. ? 2000
John Wiley & Sons, Inc. 相似文献
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GIOVE-B is one of two test satellites for the future European Global Navigation Satellite System Galileo. The Cooperative Network for GIOVE Observation (CONGO) is a global tracking network of GIOVE-capable receivers established by Deutsches Zentrum für Luft- und Raumfahrt (DLR) and Bundesamt für Kartographie und Geodäsie (BKG). This network provides the basis for the precise orbit determination of the GIOVE-B satellite for the time period 29 June till 27 October 2009 with a modified version of the Bernese GPS Software. Different arc lengths and sets of orbit parameters were tested. These tests showed that the full set of nine radiation pressure parameters resulted in a better performance than the reduced set of five parameters. An internal precision of about one to two decimeters could be demonstrated for the central day of 5-day solutions. The orbit predictions have a precision of about 1 m for a prediction period of 24 h. External validations with Satellite Laser Ranging (SLR) show residuals on the level of 12 cm. The accuracy of the final orbits is expected to be on the few decimeter level. 相似文献
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It has been widely known that the use of two-frequency Satellite Laser Ranging (SLR) system is limited by stringent precision
requirements of the range measurements and the proper atmospheric model. Owing to the stringent requirements, this SLR system
is impractical for the current requirement of SLR measurements within the framework of global geodetic observing system (GGOS).
If in the future this stringent requirement could be met, this SLR system would be an attractive tool to reduce atmospheric
propagation effects of SLR and would be of great benefit for the next generation of GGOS design. To anticipate possible future
developments of the two-frequency SLR systems, we have developed a new atmospheric correction formula for the two-frequency
SLR measurements. The new formula eliminates the total atmospheric density effect including its gradient and provides two
terms to calculate the curvature effect and the water vapor distribution effect. While the curvature effect can be calculated
by an accurate model, the required information about the water vapor distribution along the propagation path can be calculated
using previous developments of optical delay modeling or alternatively using results from microwave measurements. Theoretical
simulations using the two-frequency systems of the Graz and TIGO-Concepción stations shows that the new formula completely
reduces all propagation effects at any elevation angle above 3° with an accuracy better than 1 mm. However, the required precision
for the difference of the two-frequency SLR measurements, i.e. better than 45 μm for a single epoch, exceeds the capability
of the current state of the art SLR systems. 相似文献
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Accurate geocentric three dimensional positioning is of great importance for various geodetic and oceanographic applications.
While relative positioning accuracy of a few centimeters has become a reality using Very Long Baseline Interferometry (VLBI), the uncertainty in the offset of the adopted coordinate system origin from the geocenter is still believed to be of the
order of one meter. Satellite Laser Ranging (SLR) is capable of determining this offset to better than10 cm, though, because of the limited number of satellites, this requires a long arc of data. The Global Positioning System (GPS) measurements provide a powerful alternative for an accurate determination of this origin offset in relatively short period
of time. Two strategies are discussed, the first utilizes the precise relative positions predetermined byVLBI, where as the second establishes a reference frame by holding only one of the tracking sites longitude fixed. Covariance
analysis studies indicate that geocentric positioning to an accuracy of a few centimeters can be achieved with just one day
of preciseGPS pseudorange and carrier phase data. 相似文献