Multi-GNSS Precise Point Positioning enhanced by the real navigation signals from CENTISPACETM LEO mission

精密点定位 全球定位系统 全球导航卫星系统应用 伽利略(卫星导航) 大地测量学 歧义消解 计算机科学 卫星 星座 遥感 趋同(经济学) 中地球轨道 格洛纳斯 定轨 GPS信号 卫星导航 实时计算 地理 辅助全球定位系统 电信 物理 航空航天工程 近地轨道 工程类 天文 经济增长 经济
作者
Shoujun Xu,Qianqian Yang,Xiaodong Du,Xingyu Xu,Qile Zhao,Long Yang,Yueping Qin,Jiming Guo
出处
期刊:Advances in Space Research [Elsevier BV]
标识
DOI:10.1016/j.asr.2024.01.017
摘要

The Low Earth Orbit (LEO) satellites can significantly reduce the convergence time of Precise Point Positioning (PPP), as the rapid motion of LEO satellites leads to the fast changes of the observation geometry. This helps to accelerate the separation of ambiguity as well as receiver’s positions. In this study, the real dual-frequency navigation signals of the CENTISPACETM ESAT1 satellite are used to enhance the Multi-GNSS Precise Point Positioning (PPP). The onboard GPS, Galileo and BDS-3 observations are used to derive the precise orbits of ESAT1, while the clock is determined based on the data from a ground network established by Wuhan University. With them, the impact of the ESAT1 on float PPP with single, dual, and three constellations (GPS-only, Galileo-only, BDS-3 only, GPS/Galileo, GPS/BDS-3, Galileo/BDS-3, and GPS/Galileo/BDS-3) is analyzed in terms of convergence time and positioning accuracy. The analysis reveals that the average convergence time in the east direction is reduced by 7.9, 2.4, 12.0, 2.0, 3.4, 2.6 and 1.3 min respectively. Additionally, the 3D accuracy improves around 3.2, 4.1, 5.8, 1.1, 0.3, 1.5 and 0.6 cm respectively. Furthermore, the contribution of ESAT1 observations for Mult-GNSS PPP with Ambiguity Resolution (PPP-AR) is also investigated. The average Time to First Fix (TTFF) of each solution can be reduced about 8.1, 5.2, 4.9, 1.3, 0.9, 1.1 and 0.4 min, respectively. Overall, the PPP and PPP-AR are benefited with LEO signals, in particularly for the single-system solutions, and the results demonstrate the promising contribution of LEO on high-accuracy positioning.

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