• Sorted by Date • Sorted by Last Name of First Author •
Li, Bofeng, Wu, Tianhao, and Ge, Haibo, 2025. Deep neural network based precise orbit prediction for low earth orbit (LEO) satellites. Journal of Geodesy, 99(9):75, doi:10.1007/s00190-025-01999-7.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2025JGeod..99...75L,
       author = {{Li}, Bofeng and {Wu}, Tianhao and {Ge}, Haibo},
        title = "{Deep neural network based precise orbit prediction for low earth orbit (LEO) satellites}",
      journal = {Journal of Geodesy},
     keywords = {Low earth orbit (LEO), Orbit prediction, Deep neural network (DNN), GNSS},
         year = 2025,
        month = sep,
       volume = {99},
       number = {9},
          eid = {75},
        pages = {75},
     abstract = "{High-accuracy orbits are the prerequisite for precise applications with
        all current Low Earth Orbit (LEO)-borne remote sensing and
        future LEO-enhanced GNSS (LeGNSS). Owing to the time latency
        mainly caused by the time consumption of computing precise orbit
        determination (POD), the predicted orbits of GNSS and LEOs are
        inevitably required for real-time applications. However, it is
        rather difficult to precisely predict the LEO orbits due to
        their perturbation complexity. In this paper, we propose a Deep
        Neural Network (DNN) based approach of precise LEO orbit
        prediction, where the errors of reduced-dynamic orbit prediction
        (RDOP) are further compensated by properly designing DNN-based
        Sequence-to-Sequence (Seq2Seq) structures. The GRACE Follow-On
        satellites are taken to numerically validate the efficiency of
        our method. The results show that with appropriate strategies,
        3D RMSEs of 6.9, 14.0 and 22.8 cm can be achieved by RDOP for
        half-, 1-, 2-h prediction arc. With the compensation of trained
        Seq2Seqs, the prediction accuracies can be significantly
        improved by 50{\textendash}80\% for all three directions, where
        the RMSEs of 5-min, half-hour, and 1-h are 0.6, 2.9, and 6.0 cm
        for 3D, respectively, and 0.4, 1.8, and 3.7 cm for OURE,
        respectively. Overall, the predicted orbits with accuracy of 5
        cm are achievable for the prediction arc as long as 50 min,
        which asserted the great potential of proposed DNN-based
        prediction approach in the high-accuracy LEO orbit prediction.}",
          doi = {10.1007/s00190-025-01999-7},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025JGeod..99...75L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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