EGU26-3237, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-3237
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Friday, 08 May, 11:20–11:30 (CEST)
 
Room K2
Geopotential Determination Using an Optical Link and a Cold-Atom Cesium Clock Aboard the ACES Mission
Abdelrahim Ruby1,2,3, WenBin Shen1,2, Ahmed Shaker3, Pengfei Zhang1, and Ziyu Shen4
Abdelrahim Ruby et al.
  • 1Time and Frequency Geodesy Center, School of Geodesy and Geomatics, Wuhan University, Wuhan 430079, China (wbshen@sgg.whu.edu.cn).
  • 2State Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan 430079, China
  • 3Geomatics Engineering Department, Faculty of Engineering at Shoubra, Benha University, Cairo 11629, Egypt
  • 4School of Resource, Environmental Science and Engineering, Hubei University of Science and Technology, Xianning, Hubei 437100, China

Relativistic geodesy exploits the gravitational redshift predicted by General Relativity (GR) to determine differences in the Earth’s gravitational potential (geopotential) through high-precision clock comparisons. Recent advances in optical atomic clocks and optical time-transfer techniques have achieved fractional frequency uncertainties at or below 10-18 , corresponding to a geopotential variation sensitivity of approximately 0.1m2s-2. This level of precision is sufficient to enable high-resolution chronometric leveling. Compared with conventional microwave time-transfer methods, optical links provide superior resilience to atmospheric perturbations, higher modulation bandwidths, and unambiguous time-transfer observables, making them particularly well suited for relativistic geodesy applications. Motivated by the European Laser Timing (ELT) experiment and the high-precision cesium cold-atom clock aboard the Atomic Clock Ensemble in Space (ACES) mission, characterized by a fractional frequency stability and accuracy of approximately 10-16, we propose and analyze a triple optical time-transfer model for determining the Earth’s geopotential. The model is formulated within a consistent relativistic framework based on post-Newtonian theory, which adequately supports atomic clock comparisons at the accuracy level of 10-18.

In the absence of actual ELT/ACES optical data and considering the limitations of current ground-based laser ranging stations, where heterogeneous time and frequency standards exhibit insufficient long-term stability for relativistic geodesy, a high-fidelity numerical simulation framework is developed. This framework incorporates representative ELT/ACES mission parameters, including a ground-based optical clock with a fractional frequency instability of 10⁻¹⁸. Simulation results show that approximately 70% of ELT/ACES mission passes yield geopotential bias estimates within (-0.180±0.846) m2s-2 relative to the reference value, corresponding to centimeter-level height sensitivity. These results demonstrate that optical time and frequency transfer links, when combined with state-of-the-art optical clocks, can support free-space measurement networks capable of global chronometric leveling. Such networks hold significant potential for the realization of a unified height reference system and for advancing high-precision geodetic applications. This study is supported by the National Natural Science Foundation of China (NSFC) (Grant Nos. 42388102, 42030105, and 42274011) and the Space Station Project (2020-228). National Gravitation Laboratory, Huazhong University of Science and Technology, Wuhan 430074, P.R. China.

How to cite: Ruby, A., Shen, W., Shaker, A., Zhang, P., and Shen, Z.: Geopotential Determination Using an Optical Link and a Cold-Atom Cesium Clock Aboard the ACES Mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3237, https://doi.org/10.5194/egusphere-egu26-3237, 2026.