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Rapid ambiguity resolution over medium-to-long baselines based on GPS/BDS multi-frequency observables

机译:基于GPS / BDS多频可观测值的中至长基线的快速歧义解决

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摘要

Medium-long baseline RTK positioning generally needs a long initial time to find an accurate position due to non-negligible atmospheric delay residual. In order to shorten the initial or re-convergence time, a rapid phase ambiguity resolution method is employed based on GPS/BDS multi-frequency observables in this paper. This method is realized by two steps. First, double-differenced un-combined observables (i.e., L1/L2 and B1/B2/B3 observables) are used to obtain a float solution with atmospheric delay estimated as random walk parameter by using Kalman filter. This model enables an easy and consistent implementation for different systems and different frequency observables and can readily be extended to use more satellite navigation systems (e.g., Galileo, QZSS). Additional prior constraints for atmospheric information can be quickly added as well, because atmospheric delay is parameterized. Second, in order to fix ambiguity rapidly and reliably, ambiguities are divided into three types (extra-wide-lane (EWL), wide-lane (WL) and narrow-lane (NL)) according to their wavelengths and are to be fixed sequentially by using the LAMBDA method. Several baselines ranging from 61 km to 232 km collected by Trimble and Panda receivers are used to validate the method. The results illustrate that it only takes approximately 1, 2 and 6 epochs (30 s intervals) to fix EWL, WL and NL ambiguities, respectively. More epochs' observables are needed to fix WL and NL ambiguity around local time 14:00 than other time mainly due to more active ionosphere activity. As for the re-convergence time, the simulated results show that 90% of epochs can be fixed within 2 epochs by using prior atmospheric delay information obtained from previously 5 min. Finally, as for positioning accuracy, meter, decimeter and centimeter level positioning results are obtained according to different ambiguity resolution performances, i.e., EWL, WL and NL fixed solutions.
机译:由于不可忽略的大气延迟残留,中等长的基准RTK定位通常需要很长的初始时间才能找到准确的位置。为了缩短初始或重新收敛的时间,本文采用了基于GPS / BDS多频观测的快速相位模糊度解析方法。该方法通过两个步骤实现。首先,通过使用卡尔曼滤波器,使用双差未组合可观测值(即L1 / L2和B1 / B2 / B3可观测值)来获得具有大气延迟的浮点解,该浮点解被估计为随机游走参数。该模型可为不同的系统和不同的可观测频率提供简单,一致的实现,并且可以轻松扩展以使用更多的卫星导航系统(例如Galileo,QZSS)。由于大气延迟是参数化的,因此还可以快速添加对大气信息的其他现有约束。其次,为了快速,可靠地消除歧义,根据其波长将歧义分为三种类型(超宽车道(EWL),宽车道(WL)和窄车道(NL))并加以固定。依次使用LAMBDA方法。 Trimble和Panda接收器收集的从61 km到232 km的几个基线被用来验证该方法。结果表明,分别只需要大约1个,2个和6个时期(30 s间隔)即可解决EWL,WL和NL的歧义。与当地时间相比,在当地时间14:00左右需要更多时段的观测值来解决WL和NL的歧义,这主要是由于电离层活动更为活跃。至于再收敛时间,仿真结果表明,通过使用从前5分钟获得的先前大气延迟信息,可以将90%的纪元固定在2个纪元内。最后,关于定位精度,根据不同的歧义分辨率性能,即EWL,WL和NL固定解,获得了米,分米和厘米级的定位结果。

著录项

  • 来源
    《Advances in space research》 |2017年第3期|794-803|共10页
  • 作者单位

    GNSS Research Center, Wuhan University, 129 Luoyu Road, Wuhan, Hubei 430079, China;

    GNSS Research Center, Wuhan University, 129 Luoyu Road, Wuhan, Hubei 430079, China ,Collaborative Innovation Centre for Geospatial Technology, 129 Luoyu Road, Wuhan, Hubei 430079, China;

    School of Geodesy and Geomatics, Wuhan University, 129 Luoyu Road, Wuhan, Hubei 430079, China ,Collaborative Innovation Centre for Geospatial Technology, 129 Luoyu Road, Wuhan, Hubei 430079, China;

    GNSS Research Center, Wuhan University, 129 Luoyu Road, Wuhan, Hubei 430079, China;

    GNSS Research Center, Wuhan University, 129 Luoyu Road, Wuhan, Hubei 430079, China;

    Collaborative Innovation Centre for Geospatial Technology, 129 Luoyu Road, Wuhan, Hubei 430079, China ,Department of Surveying Engineering, Guangdong University of Technology, 100 Waihuan Xi Road, Guangzhou, China;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    GPS/BDS; Medium-long baseline; Rapid ambiguity resolution; Multi-frequency observables;

    机译:GPS / BDS;中长基线;快速的歧义解决;多频观测;
  • 入库时间 2022-08-17 13:18:52

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