Inter-frequency code bias handling and estimation for multi-frequency BeiDou-3/Galileo uncombined precise point positioning

被引:3
|
作者
Cao, Xinyun [1 ,2 ,3 ]
Shen, Fei [1 ,2 ,3 ]
Ge, Yulong [4 ]
Liu, Chao [5 ]
Zhang, Shoujian [6 ]
机构
[1] Nanjing Normal Univ, Sch Geog, Nanjing 210023, Peoples R China
[2] Nanjing Normal Univ, Minist Educ, Key Lab Virtual Geog Environm, Nanjing 210023, Peoples R China
[3] Jiangsu Ctr Collaborat Innovat Geog Informat Reso, Nanjing 210023, Peoples R China
[4] Nanjing Normal Univ, Sch Marine Sci & Engn, Nanjing 210023, Peoples R China
[5] Hebei Univ Engn, Sch Min & Geomat, Handan 056038, Peoples R China
[6] Wuhan Univ, Sch Geodesy & Geomat, Wuhan 430079, Peoples R China
基金
中国国家自然科学基金;
关键词
uncombined precise point positioning; multi-frequency signals; differential code biases; ionospheric constraint; inter-frequency code biases; MULTI-GNSS; LINEAR-COMBINATIONS; CYCLE SLIP; PPP;
D O I
10.1088/1361-6501/ac3198
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
The development of a global navigation satellite system (GNSS) with multi-frequency signals brings new opportunities for providing high-quality positioning, navigation and timing (PNT) services. Proper inter-frequency code bias (IFB) handling is a prerequisite for multi-frequency uncombined precise point positioning (UC-PPP) to ensure reliable and accurate PNT services. This work focuses on analyzing the mathematical representation of estimated parameters, as well as the relationship between different multi-frequency UC-PPP models, caused by whether to correct the inter-frequency satellite differential code bias (DCB) or the external ionosphere. Multi-GNSS experiment (MGEX) network stations tracking Galileo E1/E5a/E5b/E6/E5ab and BeiDou-3 (BDS-3) B1I/B3I/B1C/B2a signals were used to investigate the positioning performance and parameter estimations of three multi-frequency UC-PPP models. The results show that the loosely constrained ionosphere will make the estimated ionosphere and DCB/IFB parameters unable to effectively separate due to their high linear dependence. The 3D positioning accuracy of UC-PPP using Galileo five-frequency, BDS-3 four-frequency and Galileo/BDS-3 multi-frequency signals in static mode is 1.76, 2.36 and 1.39 cm, while the corresponding accuracy in kinematic mode is 6.40, 7.08 and 4.16 cm, respectively. The consistency of Galileo IFBs with respect to the MGEX DCB files is rather good, and the probability of deviations within 0.3 ns is 96.58%. Compared to Galileo, the agreement of the BDS-3 IFBs with respect to the reference values is worse, with 92.69% of them within 1 ns.
引用
收藏
页数:15
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