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首页> 外文期刊>Journal of Geodesy >Multi-GNSS orbit determination using satellite laser ranging
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Multi-GNSS orbit determination using satellite laser ranging

机译:使用卫星激光测距的多GNSS轨道确定

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摘要

Galileo, BeiDou, QZSS, and NavIC are emerging global navigation satellite systems (GNSSs) and regional navigation satellite systems all of which are equipped with laser retroreflector arrays for range measurements. This paper summarizes the GNSS-intensive tracking campaigns conducted by the International Laser Ranging Service and provides results from multi-GNSS orbit determination using solely SLR observations. We consider the whole constellation of GLONASS, all active Galileo, four BeiDou satellites: 1 MEO, 3 IGSO, and one QZSS. We analyze the influence of the number of SLR observations on the quality of the 3-day multi-GNSS orbit solution. About 60 SLR observations are needed for obtaining MEO orbits of sufficient quality with the root mean square (RMS) of 3 cm for the radial component when compared to microwave-based orbits. From the analysis of a minimum number of tracking stations, when considering the 3-day arcs, 5 SLR stations do not provide a sufficient geometry of observations. The solution obtained using ten stations is characterized with RMS of 4, 9, and 18 cm in the radial, along-track, and cross-track direction, respectively, for MEO satellites. We also investigate the impact of the length of orbital arc on the quality of SLR-derived orbits. Hence, 5- and 7-day arcs constitute the best solution, whereas 3-day arcs are of inferior quality due to an insufficient number of SLR observations and 9-day arcs deteriorate the along-track component. The median RMS from the comparison between 7-day orbital arcs determined using SLR data with microwave-based orbits assumes values in the range of 3-4, 11-16, and 15-27 cm in radial, along-track, and cross-track, respectively, for MEO satellites. BeiDou IGSO and QZSS are characterized by RMS values higher by a factor of 8 and 24, respectively, than MEO orbits.
机译:伽利略(Galileo),北斗(BeiDou),QZSS和NavIC是新兴的全球导航卫星系统(GNSS)和区域导航卫星系统,所有这些系统都配备了用于距离测量的激光后向反射器阵列。本文总结了国际激光测距服务局开展的GNSS密集跟踪活动,并提供了仅使用SLR观测值进行多GNSS轨道确定的结果。我们考虑了整个GLONASS星座,所有活跃的伽利略卫星,四颗北斗卫星:1颗MEO,3颗IGSO和1颗QZSS。我们分析了SLR观测次数对3天多GNSS轨道解决方案质量的影响。与基于微波的轨道相比,为了获得足够质量的MEO轨道,径向分量的均方根(RMS)为3 cm,大约需要进行60次SLR观测。从最少数量的跟踪站的分析来看,当考虑3天的弧线时,5个SLR站不能提供足够的观测几何形状。使用十个站点获得的解决方案的特征是,对于MEO卫星,其径向,沿轨道和跨轨道方向的RMS分别为4、9和18 cm。我们还研究了轨道弧长对SLR衍生轨道质量的影响。因此,5天和7天弧线是最好的解决方案,而3天弧线由于SLR观测次数不足而质量较差,而9天弧线则使沿航迹分量变差。使用SLR数据与基于微波的轨道确定的7天轨道弧之间的比较得出的RMS中值,假设径向,沿轨道和交叉方向的值分别在3-4、11-16和15-27 cm范围内分别跟踪MEO卫星。北斗IGSO和QZSS的特征在于RMS值分别比MEO轨道高8到24倍。

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