EGU26-5369, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-5369
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 07 May, 10:45–12:30 (CEST), Display time Thursday, 07 May, 08:30–12:30
 
Hall X2, X2.21
COST-G: Status and new developments
Ulrich Meyer1, Adrian Jaeggi1, Martin Lasser1, Christoph Dahle2, Frank Flechtner2, Felix Oehlinger3, Torsten Mayer-Guerr3, Jean-Michel Lemoine4, Igor Koch5, Hao Zhou6, Qiujie Chen7, and Wei Feng7
Ulrich Meyer et al.
  • 1University of Bern, Astronomical Institute (AIUB), Bern, Switzerland (ulrich.meyer@unibe.ch)
  • 2German Research Centre for Geosciences (GFZ), Munich, Germany
  • 3Graz University of Technology, Institute of Geodesy (IfG), Graz, Austria
  • 4Centre National d’Etudes Spatiales, Department of Terrestrial and Planetary Geodesy (GRGS), Toulouse, France
  • 5Leibniz University Hannover (LUH), Institute of Geodesy and Geoinformatics, Hannover, Germany
  • 6Huazhong University of Science and Technology (HUST), Institute of Geophysics, Wuhan, China
  • 7Tongji University, College of Surveying and Geo-informatics, Tongji, China

In June 2025, the RL02.1 GRACE and GRACE-FO time-series of monthly gravity fields, combined from the monthly solutions of 11 (GRACE), resp. 8 (GRACE-FO) different Analysis Centers (ACs) by the Combination Service for Time-variable Gravity fields (COST-G) has been published. Compared to the COST-G RL02 combination, presented at EGU 2025, the contributions of HUST and Tongji to the GRACE combination have been updated, with only minor impact on the combination. Meanwhile, the Tongji GRACE-FO solutions have passed the COST-G quality control and are included in the operational GRACE-FO combination, starting from July 2025. One month later, a new AIUB GRACE-FO RL03 became available, replacing AIUB-RL02 in the GRACE-FO combination from August 2025 on. Both changes led to significant noise reductions of the combined GRACE-FO gravity fields. To ensure consistency of the atmosphere and ocean dealiasing (AOD) models applied in the GRACE-FO data analysis, the new time-series, which already use AOD1B-RL07, have to be transformed back to AOD1B-RL06 prior to combination. A new COST-G release, including a switch to AOD1B-RL07, is foreseen, as soon as the GRACE-FO SDS RL07 time-series are available. Due to the realistic noise models applied by an increasing number of ACs, a combination on the normal equation instead of solution level may become feasible for this future COST-G release.

How to cite: Meyer, U., Jaeggi, A., Lasser, M., Dahle, C., Flechtner, F., Oehlinger, F., Mayer-Guerr, T., Lemoine, J.-M., Koch, I., Zhou, H., Chen, Q., and Feng, W.: COST-G: Status and new developments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5369, https://doi.org/10.5194/egusphere-egu26-5369, 2026.