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Shen, Zhengyuan, Cai, Lin, Wang, Hongmin, and Zhou, Zebing, 2025. Enhancing the Estimation Precision of C$_20$ Through Revised GRACE Follow on Accelerometer Response Model to Thrusters. Journal of Geophysical Research (Solid Earth), 130(12):e2025JB031121, doi:10.1029/2025JB031121.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2025JGRB..13031121S,
author = {{Shen}, Zhengyuan and {Cai}, Lin and {Wang}, Hongmin and {Zhou}, Zebing},
title = "{Enhancing the Estimation Precision of C$_{20}$ Through Revised GRACE Follow on Accelerometer Response Model to Thrusters}",
journal = {Journal of Geophysical Research (Solid Earth)},
keywords = {accelerometer, cold-gas thruster, C$_{20}$ coefficient, data processing, GRACE-FO},
year = 2025,
month = dec,
volume = {130},
number = {12},
eid = {e2025JB031121},
pages = {e2025JB031121},
abstract = "{As the largest component of Earth's time-variable gravity field,
${C}_{20}$ is crucial for understanding regional mass
variability and climate changes. However, the ${C}_{20}$
estimated by Gravity Recovery and Climate Experiment Follow-On
(GRACE-FO) is currently unreliable and has been replaced by
values derived from the satellite laser ranging (SLR) to ensure
the proper scientific application of GRACE-FO data products.
Yet, exploring the reasons for the bias in the ${C}_{20}$
estimates has been of great interest, as there is always a
concern about the inconsistency between the SLR and GRACE
solutions. This study investigates the impact of accelerometer
(ACC) data processing methods on the accuracy of ${C}_{20}$
estimation by examining the anomalous response characteristics
of the GRACE-FO ACC to the thruster. Firstly, using the
statistical analysis method, we identify a correlation between
the anomalous response caused by the Roll thrusters and the ACC
range mode. From this basis, we make a conjecture about the
mechanism of anomalous response generation, and a new thruster
firing physical model based on statistical results is proposed
to replace the anomalous response and optimize the current ACC
data processing flow. From the results of the gravity field
recovery, the corrected ACC data improve the accuracy of the
estimation of ${C}_{20}$. After multiple months of estimation,
the estimate RMSD ${C}_{20}$ between the new ACC product and the
TN-14 solutions was $1.16\times 1{0}^{-10}$, better than the
precision of the estimate of the reference solutions. Finally,
we discuss the correlation between this ACC processing method
and the accuracy of ${C}_{20}$ estimation.}",
doi = {10.1029/2025JB031121},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025JGRB..13031121S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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