Improved undifferenced ambiguity resolution for LEO precise orbit determination

被引:3
|
作者
Gao, Geng [1 ]
Zhang, Shoujian [1 ]
Zou, Xiancai [1 ]
Kuang, Kaifa [2 ]
Yu, Nan [3 ]
机构
[1] Wuhan Univ, Sch Geodesy & Geomat, Wuhan 430000, Peoples R China
[2] Beijing Univ Civil Engn & Architecture, Beijing 102616, Peoples R China
[3] China Univ Geosci, Hubei Key Lab Marine Geol Resources, Wuhan 430074, Peoples R China
基金
中国国家自然科学基金;
关键词
Precise orbit determination; Undifferenced ambiguity resolution; Single-difference ambiguity resolution; Clock modeling; GRACE Follow-on; MODELING TECHNIQUES; GRAVITY-FIELD; SATELLITE;
D O I
10.1016/j.asr.2023.04.035
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Ambiguity resolution (AR) is critical for enhancing the orbit accuracy in precise orbit determination (POD) for low earth orbit (LEO) satellites. While orbit estimation using single-difference (SD) AR has been widely researched, the investigation of orbit estimation using undifferenced (UD) AR for LEO satellites is limited due to time-varying hardware biases at the LEO receiver end. To address this deficiency, we propose an improved UD AR method for LEO satellite orbit determination. The method employs the optimal integer datum ambiguity for a 1-day observation arc, and the random-walk clock model is utilized to transfer the integer ambiguity datum to the other epochs, which enables the arc-wise ambiguities to regain the integer property within the time frame. To validate the effectiveness of our improved method, numerical experiments are conducted. Moreover, we assess the performance of the random-walk clock model for a spaceborne ultra-stable oscillator (USO). The high frequency stability of the USO establishes the satisfactory requirements for this study. Both in the kinematic and dynamic modes, the AR success rates of our improved method are - 2% higher than that of the current SD AR method, and the orbit results indicate a slight improvement. The 3-Dimensional (3D) root-mean-squares (RMS) of the orbit differences between JPL precise science orbits (PSO) and our orbits are reduced by up to 4% and 5% for kinematic and dynamic orbits, respectively. The subtle benefit is also proven by K-band ranging (KBR) system validations. In the case of the Gravity Recovery and Climate Experiment Follow-on (GFO) satellites, the results indicate that the effect of our improved UD AR can be equivalent to that of SD AR. Our improved UD AR method can be a good alternative for its superior ability to generate hardware delay at the LEO receiver end. & COPY; 2023 COSPAR. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:1518 / 1527
页数:10
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