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An Improved BeiDou-2 Satellite-Induced Code Bias Estimation Method

机译:改进的北斗二号卫星诱发码偏估计方法

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摘要

Different from GPS, GLONASS, GALILEO and BeiDou-3, it is confirmed that the code multipath bias (CMB), which originate from the satellite end and can be over 1 m, are commonly found in the code observations of BeiDou-2 (BDS) IGSO and MEO satellites. In order to mitigate their adverse effects on absolute precise applications which use the code measurements, we propose in this paper an improved correction model to estimate the CMB. Different from the traditional model which considering the correction values are orbit-type dependent (estimating two sets of values for IGSO and MEO, respectively) and modeling the CMB as a piecewise linear function with a elevation node separation of 10°, we estimate the corrections for each BDS IGSO + MEO satellite on one hand, and a denser elevation node separation of 5° is used to model the CMB variations on the other hand. Currently, the institutions such as IGS-MGEX operate over 120 stations which providing the daily BDS observations. These large amounts of data provide adequate support to refine the CMB estimation satellite by satellite in our improved model. One month BDS observations from MGEX are used for assessing the performance of the improved CMB model by means of precise point positioning (PPP). Experimental results show that for the satellites on the same orbit type, obvious differences can be found in the CMB at the same node and frequency. Results show that the new correction model can improve the wide-lane (WL) ambiguity usage rate for WL fractional cycle bias estimation, shorten the WL and narrow-lane (NL) time to first fix (TTFF) in PPP ambiguity resolution (AR) as well as improve the PPP positioning accuracy. With our improved correction model, the usage of WL ambiguity is increased from 94.1% to 96.0%, the WL and NL TTFF of PPP AR is shorten from 10.6 to 9.3 min, 67.9 to 63.3 min, respectively, compared with the traditional correction model. In addition, both the traditional and improved CMB model have a better performance in these aspects compared with the model which does not account for the CMB correction.
机译:与GPS,GLONASS,GALILEO和BeiDou-3不同,已经确认,北斗2号(BDS)的代码观测结果中普遍存在源自卫星端且可能超过1 m的代码多径偏置(CMB)。 )IGSO和MEO卫星。为了减轻它们对使用代码测量的绝对精确应用程序的不利影响,我们在本文中提出了一种改进的校正模型来估计CMB。与传统模型不同,传统模型考虑校正值取决于轨道类型(分别估计两组IGSO和MEO值)并将CMB建模为仰角节点间隔为10°的分段线性函数,我们估算校正值一方面,对于每个BDS IGSO + MEO卫星,另一方面,使用5°的更密集的高程节点间距来建模CMB变化。目前,IGS-MGEX等机构运营着超过120个台站,这些台站每天提供BDS观测。这些大量数据为我们改进模型中的逐个卫星完善CMB估算卫星提供了足够的支持。来自MGEX的一个月BDS观测值用于通过精确点定位(PPP)评估改进的CMB模型的性能。实验结果表明,对于相同轨道类型的卫星,在相同节点和频率的CMB中可以发现明显的差异。结果表明,新的校正模型可以提高WL分数周期偏差估计的宽车道(WL)歧义使用率,缩短PPP歧义分辨率(AR)的WL和窄道(NL)首次修复时间(TTFF)以及提高PPP定位精度。与传统的校正模型相比,通过改进的校正模型,WL模糊度的使用率从94.1%增加到96.0%,PPP AR的WL和NL TTFF分别从10.6分钟缩短到9.3分钟,从67.9分钟缩短到63.3分钟。此外,与不考虑CMB校正的模型相比,传统和改进的CMB模型在这些方面均具有更好的性能。

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