EGU24-7548, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-7548
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The COST-G GRACE RL02

Adrian Jaeggi1, Ulrich Meyer1, Martin Lasser1, Frank Flechtner2, Christoph Dahle2, Eva Boergens2, Torsten Mayer-Gürr3, Felix Öhlinger3, Jean-Michel Lemoine4, Stéphane Bourgogne5, Thorben Döhne6, Hao Zhou7, Jianjun Ran8, Qiujie Chen9, Changqing Wang10, and Wei Feng11
Adrian Jaeggi et al.
  • 1University of Bern, Astronomical Institute, Berne, Switzerland (adrian.jaeggi@aiub.unibe.ch)
  • 2German Research Centre for Geosciences, Germany
  • 3Graz University of Technology, Institute of Geodesy, Austria
  • 4Centre National d’Etudes Spatiales, Department of Terrestrial and Planetary Geodesy, France
  • 5Stellar Space Studies, France
  • 6Technical University of Dresden, Institute of Planetary Geodesy, Germany
  • 7Huazhong University of Science and Technology, Institute of Geophysics, China
  • 8Southern University of Science and Technology, Department of Earth and Space Sciences, China
  • 9Tongji University, College of Surveying and Geo-informatics, China
  • 10Chinese Academy of Sciences, Innovation Academy for Precision Measurement Science and Technology
  • 11Sun Yat-sen University, School of Geospatial Engineering and Science, China

In 2019 the Combination Service for Time-variable Gravity fields (COST-G) started its operation with the first release of combined monthly GRACE gravity field models. Meanwhile almost five years have passed, while new experience was gained with the operational combination of the monthly gravity field models of the successor mission GRACE-FO, which has triggered a review of the weighting scheme and consequently a second release of GRACE-FO models in 2023. Moreover, the COST-G consortium has been in close cooperation with new GRACE/GRACE-FO analysis centers from China since spring 2020, which recently provided time-series of unconstrained models, covering the whole GRACE period, as it is requested by the COST-G processing standards. After careful evaluation of all individual time-series the whole GRACE time-series has now been recombined based on the new weighting scheme and also taking into account the contributions of the new COST-G analysis centers APM-SYSU, HUST, SUSTech and Tongji. We present the COST-G GRACE RL02 and also show latest results of the operational GRACE-FO combination.

How to cite: Jaeggi, A., Meyer, U., Lasser, M., Flechtner, F., Dahle, C., Boergens, E., Mayer-Gürr, T., Öhlinger, F., Lemoine, J.-M., Bourgogne, S., Döhne, T., Zhou, H., Ran, J., Chen, Q., Wang, C., and Feng, W.: The COST-G GRACE RL02, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7548, https://doi.org/10.5194/egusphere-egu24-7548, 2024.