Abstract
Recently, \(C_{30}\) coefficients of time-variable gravity field models from GRACE and GRACE-Follow On (GRACE/GRACE-FO) are reported to contain larger uncertainties when only one of the two onboard accelerometers is fully functional, which mainly concerns the GRACE-FO period and the final stage of the GRACE period. Using these problematic coefficients leads to incorrect mass change (rate) estimates, especially over Antarctic Ice-Sheet (AIS), and a replacement with those from satellite laser ranging (SLR) is currently recommended. In this study, we aim to discuss the possibility of improving the \(C_{30}\) coefficients by extending the GRACE-OBP approach that has previously been applied to the estimation of geocenter motion and variations in the Earth’s dynamic oblateness. Such an approach mainly relies on GRACE/GRACE-FO level 2 products and an ocean bottom pressure model, and it produces compatible coefficients with the GRACE/GRACE-FO product labeled as GSM. With a numerical experiment, we demonstrate the effectiveness of the proposed approach and identify the optimal implementation parameter setup. The resulting \(C_{30}\) coefficient time series is generally consistent with those based on SLR and the original solutions from the GRACE dual-accelerometer period, but with differences in the annual amplitude estimates. Then, we obtain \(C_{30}\) coefficients based on real data and check the AIS mass change time series with and without replacing the original ones with our solution. Our \(C_{30}\) solution ensures consistent linear trend estimates for the dual- and single-accelerometer periods.
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Data availability
GRACE/GRACE-FO level 2 data are publicly available from the ICGEM website (http://icgem.gfz-potsdam.de/home). The GSFC SLR \(C_{30}\) coefficients (TN-14) are taken from https://podaac-tools.jpl.nasa.gov/drive/files/GeodeticsGravity/gracefo/docs/TN-14_C30_C20_GSFC_SLR.txt. The CSR SLR \(C_{30}\) coefficients are extracted from http://download.csr.utexas.edu/pub/slr/degree_5/CSR_Monthly_5x5_Gravity_Harmonics.txt. The IGG SLR solution is available at http://icgem.gfz-potsdam.de/series/04_SLR/IGG_SLR_HYBRID. The updated ESM can be accessed at https://isdc.gfz-potsdam.de/esmdata/esaesm/. The A12 GIA model is provided by Geruo A through personal communications. The Caron17 GIA model can be downloaded from https://vesl.jpl.nasa.gov/solid-earth/gia/ and the Peltier18 GIA model can be taken from https://www.atmosp.physics.utoronto.ca/~peltier/data.php. The resulting \(C_{30}\) coefficients of this study for CSR, GFZ and JPL GRACE/GRACE-FO level 2 data are available in the supplementary materials. \(C_{30}\) time series based on the GRACE-OBP approach using other data center’s TVG models are available upon requests.
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Acknowledgements
We thank our editors and three anonymous reviewers for their insightful comments which greatly improved the quality of the manuscript. We thank Riccardo Riva from Delft University of Technology for carefully revising the manuscript as well as constructive suggestions and insightful comments. This study is supported by the National Natural Science Foundation of China (grant 42171426 and 41904009) and open project from Key Lab of Spatial Data Mining and Information Sharing, Ministry of Education (grant 2022LSDMIS06). We estimate AIS mass change time series using a dedicated tool package provided by Wei Feng (Feng 2019). All the figures are prepared by the Generic Mapping Tools (Wessel et al. 2019).
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YS and XG conceived the idea and designed all the experiments; YS, YL, and XG performed the research and analyzed the data; YS and XG wrote the paper; JG revised the paper; all authors reviewed and commented on the paper.
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Sun, Y., Li, Y., Guo, X. et al. Estimating \(C_{30}\) coefficients for GRACE/GRACE-FO time-variable gravity field models using the GRACE-OBP approach. J Geod 97, 20 (2023). https://doi.org/10.1007/s00190-023-01707-3
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DOI: https://doi.org/10.1007/s00190-023-01707-3