大型高精度GNSS基线向量网并行抗差估计     

崔阳  吕志平  张友阳  李林阳 《测绘学报》2015,44(5):495-502

针对大型GNSS基线向量网的特点,在改进的相关观测抗差估计RECO方案的基础上采用并行计算技术进行相关抗差估计的并行计算(简称"并行抗差估计"),并给出了可行的解算步骤。通过算例分析,验证了大型GNSS基线向量网的并行相关抗差估计,不仅有效抑制了观测异常对参数估值的影响,而且显著提高了计算效率。  相似文献   

Impact of different sampling rates on precise point positioning performance using online processing service     

Serdar Erol  Reha Metin Alkan  ?.Murat Ozulu  Veli Il?i 《地球空间信息科学学报》2021,24(2):302-312

In this study, the effect of different sampling rates (i.e. observation recording interval) on the Precise Point Positioning (PPP) solutions in terms of accuracy was investigated. For this purpose, a field test was carried out in ?orum province, Turkey, on 11 September 2019. Within this context, a Geodetic Point (GP) was established and precisely coordinated. A static GNSS measurement was occupied on the GP for about 4-hour time at 0.10 second (s)/10 Hz measurement intervals with the Trimble R10 geodetic grade GNSS receiver. The original observation file was converted to RINEX format and then decimated into the different data sampling rates as 0.2 s, 0.5 s, 1 s, 5 s, 10 s, 30 s, 60 s, and 120 s. All these RINEX observation files were submitted to the Canadian Spatial Reference System-Precise Point Positioning (CSRS-PPP) online processing service the day after the data collection date by choosing both static and kinematic processing options. In this way, PPP-derived static coordinates, and the kinematic coordinates of each measurement epoch were calculated. The PPP-derived coordinates obtained from each decimated sampling intervals were compared to known coordinates of the GP for northing, easting, 2D position, and height components. According to the static and kinematic processing results, high data sampling rates did not change the PPP solutions in terms of accuracy when compared to the results obtained using lower sampling rates. The results of this study imply that it was not necessary to collect GNSS data with high-rate intervals for many surveying projects requiring cm-level accuracy.  相似文献   

iGMAS全球电离层TEC格网产品精度分析     

李涌涛  马洪磊  李建文  师一帅  米科峰  朱璇 《测绘科学》2021,46(2):7-14,41

为了分析与评估国际GNSS监测评估系统(iGMAS)全球电离层TEC格网产品精度,该文基于iGMAS及IGS各电离层分析中心发布的全球电离层TEC格网产品,进行了精度比较分析,结果表明:iGMAS与IGS、CODE、JPL、ESOC、UPC等IGS电离层工作组发布的全球电离层TEC格网产品,在全球、不同纬度带和欧洲等不同区域均表现出较高的一致性和强相关性,互差为0~2.0 TECU;JPL分析中心GIM的内符合精度约为2.5 TECU,iGMAS、IGS、CODE、ESOC和UPC等分析中心GIM的内符合精度均小于1.5 TECU;在2~8 TECU的精度范围内,iGMAS全球电离层TEC格网产品的精度总体与IGS、CODE、JPL、ESOC、UPC等IGS电离层工作组的精度相当。  相似文献   

利用FY-3C折射率对大气边界层高度的反演与分析     

朱洲宗  徐晓华  罗佳 《武汉大学学报(信息科学版)》2021,(3)

2013年中国发射了首颗进行全球导航卫星系统(global navigation satellite system,GNSS)掩星观测的气象卫星风云3号C星(Fengyun-3C,FY-3C),且已发布自2014年6月以来的FY-3C掩星大气产品,但目前还未见将其应用于大气边界层的相关研究。首次尝试利用FY-3C折射率产品确定边界层高度并进一步进行空间分布分析。结果表明,在小波协方差变换法基础上,进行尖锐度约束,能够确定FY-3C掩星低层大气折射率廓线中可能存在的突变,反演边界层高度。所得到的2015―2018年各年边界层高度全球分布在不同纬度及海洋和陆地上的差异基本体现了边界层与地表气候及地形的关系,但FY-3C折射率产品在低层大气的精度和垂直分辨率相对较低。因此,反演成功率总体上较低,反演结果对边界层高度空间分布细节特征的呈现仍有待提升。  相似文献   

GNSS控制网方案优化与数据处理分析     

刘平利  乔天荣  张永杰  张鸿祥 《地理空间信息》2021,19(1):106-108

GNSS布设平面控制网已在工程项目中得到广泛应用。获得满意的平差结果的前提条件为:①高质量的基线数据;②约束GNSS控制网的已知点精度足够高,使得GNSS控制网的整体精度不受已知点约束而有明显改变;③优化的平差方案;④科学严密的平差模型。通过对某项目GNSS控制网的布设进行优化设计,并利用不同软件对观测数据进行处理分析,总结了GNSS控制网方案优化与数据处理的有效方法。  相似文献   

青藏高原地区大气加权平均温度模型的构建     

石灵璠  王萍  黄良珂 《测绘通报》2021,(4):52-59

加权平均温度（T_m）是将天顶湿延迟转换为大气可降水量的关键参数,针对青藏高原地区海拔高、地形起伏大、水汽高度分布复杂的特点,本文利用2010—2014年GGOS Atmosphere T_m格网数据和地表高程数据建立T_m垂直递减率函数,进而建立一种顾及T_m垂直递减率变化的适合青藏高原地区的新模型（QTm模型）。此外,利用2015年青藏高原地区14个探空站和GGOS Atmosphere T_m格网数据评估模型精度和适用性。试验结果表明,与GGOS Atmosphere T_m相比,QTm模型的年均Bias和RMSE分别为0.29和2.49 K,相对于GPT2w-1和GPT2w-5模型,RMSE分别提升了38.97%、67.06%;与探空数据相比,QTm模型的年均Bias和RMSE分别为0.16和2.90 K,相对于GPT2w-1和GPT2w-5模型分别提升了31.12%、39.46%。新模型的构建为青藏高原地区提供了可靠的T_m值,进而提供实时、高精度GNSS水汽信息。  相似文献   

大型GNSS观测网的并行计算     

吕志平  许国昌  陈正生  崔阳  李林阳  邝英才 《测绘科学技术学报》2021,38(1):1-8

CGCS2000精化及其全球拓展需要采用最新的模型,处理长期积累的大型GNSS观测网数据,大型GNSS网联合、快速和协同解算是空间基准精化、维持与服务的重要技术方向。在大数据技术背景下,以并行计算、云计算为代表的高性能计算技术逐渐成为大规模数据处理的首选方法。针对海量、多源、异构GNSS数据在解算处理与平差分析等方面面临的挑战,阐述了大型GNSS观测网质量控制并行计算、非差模型并行解算、双差模型并行解算、高维模糊度并行搜索固定等方法。介绍了可同时处理上千个观测站的大型GNSS观测网并行计算软件GNSSer,开展了CGCS2000精化计算的试验与验证。构建了一套适合并行计算的大型GNSS观测网解算方法,实现了CGCS2000精化及其全球拓展的多节点协同并行计算的创新。  相似文献   

利用徕卡GS18仪器进行高精度RTK定位试验与分析     

伍吉仓  李玉婷 《测绘通报》2019,(4):155-158

目前，GNSS和IMU（惯性测量单元）传感器融合领域的快速发展，给高精度RTK定位带来了新的机遇。传统倾斜补偿的解决方案大多是使用磁力计和INS（惯性导航系统），对电磁干扰十分敏感并且需要现场校准，倾斜补偿的角度范围通常限制在15°；以内。为了克服上述的缺点，徕卡GS18 GPS倾斜机使用基于工业级别微电子机械传感器MEMS的IMU来补偿测杆倾斜情况的位置改正。本文通过试验检验了徕卡GS18仪器在大角度倾斜和不同复杂环境下的定位精度，结果表明GS18倾斜机能较好实现倾斜补偿，在有信号遮挡等场景下仍能获得厘米级定位精度。  相似文献   

Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo     

Tan Bao-lin  Cheng Jun  Tan Cheng-ming  Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.  相似文献   

月球交会对接VLBI差分时延研究          下载免费PDF全文

郑鑫  刘庆会  吴亚军  马俊武  邓涛 《天文学报》2020,61(3):22

中国探月3期任务中,月球交会对接技术是任务成功的重要保障.利用嫦娥3号(CE03)绕月飞行的VLBI (Very Long Baseline Interferometry)时延数据,模拟仿真绕月交会对接过程中,同波束VLBI观测模式下,差分群时延的变化情况.仿真结果显示,在远程导引段,轨道器和上升组合体轨道距离保持100 km,持续半小时,差分群时延很好地反映了两者的轨道信息,可以用于定轨定位;自主控制段,上升组合体靠近轨道器,在轨道距离从5 km减小到20 m过程中,上升组合体加速追赶轨道器时,差分群时延快速趋近于0,上升组合体减速远离轨道器时,差分群时延绝对值快速变大.最后,利用嫦娥3号奔月段同时发射两个DOR (Differential One-Ranging)信号的VLBI时延数据,计算差分相时延,初步展示了月球交会对接过程中同波束VLBI差分相时延的误差情况.  相似文献