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Long-term behavior and statistical characterization of BeiDou signal-in-space errors

机译:北斗信号空间误差的长期行为及统计表征

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摘要

We derive orbit and clock errors for BeiDou satellites from March 1, 2013, to September 30, 2016 by comparing broadcast ephemerides with the precise ephemerides produced by Wuhan University. The broadcast ephemerides are pre-processed to filter out the "data-logging" errors, and a robust estimation is subsequently implemented for removing the time-varying common timescale bias between the broadcast and precise clocks. To obtain the nominal SISEs (Signal-In-Space Errors), the SIS (Signal-In-Space) outliers are excluded according to the standard of SIS integrity. The long-term satellite clock behavior reveals that for GEO, IGSO and MEO satellites, each category of satellites has its inter-category clock consistency, and the clocks of MEO as well as the clocks of IGSO satellites have better inter-category consistency than that of GEO satellites. Between different categories, GEO satellite clocks have been more divergent from IGSO satellite clocks since May 2014. The larger orbit errors, resulting in approximately 1-2 m orbit-only UREs (User Range Errors), periodically occur for all satellites every half year when the satellites are in eclipse period. For the GEO and IGSO satellites, several larger orbit errors may be caused by the effect of satellite maneuvering, resulting in 2-3 m orbit-only UREs. Most satellite clocks have a nonzero mean, and all MEO satellite clocks have a positive mean of approximately 1.0 m, whereas the IGSO satellite clocks have a negative mean at the same level. For the GEO satellites, the various means indicate that the clocks are divergent from one to another. The clock standard deviation of 1 m is achieved by all satellites except for C03. Near-zero means are obtained in along-track, cross-track and radial errors for the IGSO and MEO satellites but not for the GEO satellites. The average RMSs (Root Mean Square) of approximately 0.8, 1.7 and 2.0 m are obtained for the orbit-only UREs, global-average UREs and worst-UREs, respectively, for the constellation as a whole. The RMSs of clock errors for GEO, IGSO and MEO are 1.8, 1.4 and 1.3 m, respectively. Due to a nearly-static observation geometry, the GEO satellites always have the worst SISE performance, and as a result, they degrade the overall SISE statistical characterization. The analysis of URE and broadcast URA (User Range Accuracy) indicates that the broadcast URA of 2.0 m throughout is slightly optimistic. The unchanging URA of 2.0 m may not be able to describe adequately the accuracy of UREs. Instead, the upper-bound URA of 2.4 m is recommended to users. The cross-correlation analysis results show that there is a significant positive correlation between along-track errors and radial errors, whereas radial errors are not evidently correlated to clock errors as they are with GPS.
机译:我们从2013年3月1日到2016年3月1日到2016年9月30日,通过比较武汉大学生产的精确短暂杂志,从2016年3月1日起北斗卫星的轨道和时钟错误。预处理广播的单次杂化以滤除“数据记录”错误,随后实现稳健的估计以消除广播和精确时钟之间的时变常见时间尺度偏差。为了获得标称智能(空中空间错误),根据SIS完整性的标准排除SIS(信号 - 空间)异常值。长期卫星时钟行为表明,对于Geo,Igso和Meo卫星,每个类别的卫星都有其类别的类别时钟一致性,以及MEO的时钟以及IGSO卫星的时钟具有比该类别更好的类别的一致性地理卫星。自2014年5月以来,不同类别之间的Geo卫星时钟从Igso卫星时钟更加分开。轨道较大的轨道误差,导致每半年的所有卫星定期出现大约1-2米的轨道ures(用户范围错误)卫星在日食期间。对于Geo和Igso卫星,几个较大的轨道误差可能是由卫星机动的影响引起的,导致2-3米轨道掉ures。大多数卫星时钟都有一个非零平均值,所有Meo卫星时钟具有大约1.0米的正均值,而Igso卫星时钟具有相同水平的负平均值。对于Geo卫星,各种手段表明时钟从一个到另一个时钟都是不同的。除C03之外,所有卫星都可以实现1米的时钟标准偏差。沿着轨道,交叉轨道和IGSO和MEO卫星的横轨和径向误差,但不是用于Geo卫星的近零的方法。对于仅作为整体的星座,仅针对仅用于轨道的ures,全局平均ures和最差的ures获得约0.8,1.7和2.0μm的平均RMS(均方根)。 Geo,Igso和Meo的时钟误差的RMS分别为1.8,1.4和1.3米。由于近乎静态的观察几何形状,地理卫星始终具有最糟糕的性能,因此,它们降低了整体大观统计表征。对URE和广播URA(用户范围精度)的分析表明整个2.0米的广播URA略有乐观。 2.0米的不变URA可能无法充分描述ures的准确性。相反,向用户建议使用2.4米的上限URA。互相关分析结果表明,沿着轨道误差和径向误差之间存在显着的正相关,而径向误差并不明显与时钟误差相关,因为它们具有GPS。

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