• Sorted by Date • Sorted by Last Name of First Author •
Wu, Tianhao, Li, Bofeng, and Ge, Haibo, 2026. Neural network–based clock bias prediction for low earth orbit satellites with a reconstruction fine–tuning mechanism. Satellite Navigation, 7(1):28, doi:10.1186/s43020-026-00215-x.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2026SatNa...7...28W,
author = {{Wu}, Tianhao and {Li}, Bofeng and {Ge}, Haibo},
title = "{Neural network-based clock bias prediction for low earth orbit satellites with a reconstruction fine-tuning mechanism}",
journal = {Satellite Navigation},
keywords = {Low Earth Orbit (LEO), Satellite Clock Bias (SCB) prediction, Neural network, Informer, Information and Computing Sciences, Artificial Intelligence and Image Processing},
year = 2026,
month = sep,
volume = {7},
number = {1},
eid = {28},
pages = {28},
abstract = "{Accurate prediction of Satellite Clock Bias (SCB) for Low Earth Orbit
(LEO) satellites is critical for real-time LEO-enhanced Global
Navigation Satellite System (LeGNSS) applications. However, the
inherent instability of LEO onboard oscillators results in
complex SCB variations that are difficult for conventional
prediction models to capture. While deep learning methods offer
a promising alternative, their effectiveness can be limited by
two key issues: the pronounced high-order trends in LEO SCB,
which are not completely removed by the conventional single
differencing; and the potential biased error accumulation that
occurs when reconstructing predictions from the differenced
domain. To address these challenges, we propose a novel neural
network-based framework featuring two key innovations: (1)
advanced differencing strategies---single-differencing with
segment-wise standardization and direct double-differencing---to
suppress high-order trends without performing external fitting,
thereby preserving prediction independence; and (2) a
reconstruction fine-tuning mechanism to explicitly mitigate
directional error accumulation. Validated with Gravity Recovery
and Climate Experiment Follow-On (GRACE-FO) data, the fine-
tuning mechanism reduces overall prediction errors by 6\%--16\%
with reconstruction biases mitigated. Compared to the
conventional spectrum analysis model, the proposed framework
improves overall prediction accuracy by approximately 90\% and
94\% for the 60 min and the 10 min prediction horizons,
respectively. Specifically, for the prediction length of 60 min,
the prediction errors for the GRACE-FO C and D satellites
decrease to 0.84 ns and 1.42 ns, respectively; for the
prediction length of 10 min, they decrease to 0.10 ns and 0.15
ns, respectively. These results indicate the framework's
potential for high-precision real-time applications from the
inference-efficiency perspective.}",
doi = {10.1186/s43020-026-00215-x},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026SatNa...7...28W},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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