EGU25-2002, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-2002
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 29 Apr, 14:55–15:05 (CEST)
 
Room K2
Real-time LEO satellite precise orbit and clock determination for augmenting GNSS: Strategies and Challenges
Kan Wang1,2,3, Wei Xie1,2, Beixi Chen1,2,3, Jiawei Liu1,2,3, Meifang Wu1,2,3, Ahmed El-Mowafy4, and Xuhai Yang1,2,3
Kan Wang et al.
  • 1National Time Service Center, Chinese Academy of Sciences, Xi’an, China
  • 2Key Laboratory of Time Reference and Applications, Chinese Academy of Sciences, Xi’an, China
  • 3University of Chinese Academy of Sciences, Beijing, China
  • 4chool of Earth and Planetary Sciences, Curtin University, Perth, Australia

To realize the various benefits brought by Low Earth Orbit (LEO) satellites in single-receiver high-precision GNSS-based Positioning Navigation and Timing (PNT) services, LEO satellite orbits and clocks need to be processed and delivered to users in real-time with precision of a few centimeters. While post-processing of cm-level LEO satellite orbits and clocks can be widely achieved, real-time processing faces various Challenges. When the number of LEO satellites increases, the observation data downlinked to the processing center may experience large and complicated discontinuities and incompleteness depending on the downlinking strategies. Even with the observations downlinked in real-time, the LEO satellite clock precision tends to be very sensitive to the continuity and quality of the GNSS real-time products. This study first introduces the procedure for ground-based cm-level real-time LEO satellite Precise Orbit Determination (POD), including near-real-time POD, short-term prediction, and ephemeris fitting/broadcasting. Next, the short-term predicted orbits and long-term predicted clocks of LEO satellites are introduced and properly constrained in filter-based real-time LEO satellite clock determination to achieve a precision of about 0.2 ns. Strategies to deal with sub-optimal observation data and GNSS products are explained. With the proposed methods, a Signal-In-Space Ranging Error at sub-dm to 1 dm can be achieved in practice. 

How to cite: Wang, K., Xie, W., Chen, B., Liu, J., Wu, M., El-Mowafy, A., and Yang, X.: Real-time LEO satellite precise orbit and clock determination for augmenting GNSS: Strategies and Challenges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2002, https://doi.org/10.5194/egusphere-egu25-2002, 2025.