大地测量学与导航

星蚀期北斗卫星轨道性能分析--SLR检核结果

  • 彭汉兵 ,
  • 杨元喜 ,
  • 王刚 ,
  • 何海波
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  • 1. 信息工程大学地理空间信息学院, 河南 郑州 450001;
    2. 西安测绘研究所地理空间工程国家重点实验室, 陕西 西安 710054;
    3. 北京卫星导航中心, 北京 100094
彭汉兵(1991-),男,硕士生,研究方向为导航卫星精密定轨。E-mail:phb_xingzhewujiang@163.com

收稿日期: 2015-12-22

  修回日期: 2016-03-31

  网络出版日期: 2016-06-29

基金资助

国家自然科学基金(41020144004A;41374019;41474015);国家863计划(2013AA122501)

Performance Analysis of BDS Satellite Orbits during Eclipse Periods: Results of Satellite Laser Ranging Validation

  • PENG Hanbing ,
  • YANG Yuanxi ,
  • WANG Gang ,
  • HE Haibo
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  • 1. Institute of Geographical Spatial Information, Information Engineering University, Zhengzhou 450001, China;
    2. State Key Laboratory of Geo-information Engineering, Xi'an 710054, China;
    3. Beijing Satellite Navigation Center, Beijing 100094, China

Received date: 2015-12-22

  Revised date: 2016-03-31

  Online published: 2016-06-29

Supported by

The National Natural Science Foundation of China(Nos.41020144004A;41374019;41474015);The National High-tech Research and Development Program of China(863 Program)(No. 2013AA122501)

摘要

星蚀期北斗卫星的轨道性能是北斗卫星导航系统性能分析的重要部分。了解北斗卫星导航系统星历中星蚀期轨道的精度,不仅可为系统服务性能评估提供支持,还有助于了解星蚀期精密定轨中相关模型可能存在的问题,进而为精密定轨函数模型改进提供参考。本文基于2014年1月至2015年7月的卫星激光测距资料,重点分析了星蚀期对北斗不同类型卫星轨道的影响,同时也对北斗广播星历和精密星历中整体轨道径向精度进行检核。结果表明:星蚀期内(尤其是偏航机动期间),IGSO/MEO卫星的广播星历和精密星历轨道均存在明显的精度下降;广播星历轨道径向误差达1.5~2.0 m,精密星历轨道径向误差超过10.0 cm。但仅从轨道径向残差序列中难以发现星蚀期对GEO卫星轨道是否有显著影响。非星蚀期间,IGSO/MEO卫星和GEO卫星的广播星历轨道径向精度分别优于0.5 m和0.9 m。IGSO/MEO卫星的精密星历轨道径向精度优于10.0 cm,GEO卫星的轨道径向精度约50.0 cm,且存在40.0 cm左右的系统性偏差。

本文引用格式

彭汉兵 , 杨元喜 , 王刚 , 何海波 . 星蚀期北斗卫星轨道性能分析--SLR检核结果[J]. 测绘学报, 2016 , 45(6) : 639 -645 . DOI: 10.11947/j.AGCS.2016.20150637

Abstract

The performance of BeiDou satellite orbits during eclipse periods is an important part of the performance analysis of BeiDou Navigation Satellite System (BDS). Accuracy evaluation of satellite orbits in ephemeris of BDS during eclipse periods can provide support for the service performance assessment. It also helps to find possible deficiencies in the orbit modeling during eclipse periods, which may further contribute to the improvements of functional models for precise orbit determination. The effects of eclipse periods on the orbits of the three types of satellites of BDS are analyzed with the satellite laser ranging (SLR) observations ranging from January 2014 to July 2015. At the same time, the orbit radial accuracy of BDS broadcast and precise ephemeris are validated. The results show that, obvious orbit accuracy decrease can be observed in both broadcast and precise ephemeris for IGSO/MEO satellites during eclipse periods (especially the yaw-maneuver periods). And orbit radial errors of IGSO/MEO satellites in broadcast ephemeris reach 1.5~2.0 m, and exceed 10.0 cm for that in precise ephemeris. Performance decrease of the GEO satellite orbit during eclipse arcs can hardly be revealed by the orbit radial residual series. During non-eclipse periods, radial accuracy of IGSO/MEO and GEO satellite orbits in broadcast ephemeris are better than 0.5 m and 0.9 m respectively. The radial accuracy of IGSO/MEO satellite orbits in precise ephemeris are better than 10.0 cm and that of the GEO satellite is about 50.0 cm with a systematic bias of 40.0 cm around.

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