4.7 Article

The Impact of New Accelerometer Transplant Data (ACH) on GRACE Follow-On Along-Orbit Inter-Satellite Laser Ranging Observations and Monthly Time-Variable Gravity and Mascon Solutions

Journal

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1029/2023JB026740

Keywords

GRACE Follow-On; non-gravitational accelerations; accelerometer transplant; time-variable gravity; mass change; laser ranging interferometer

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GRACE-D accelerometer data has shown significant bias jumps since one month after the launch of the GRACE Follow-On (GRACE-FO) satellites in May 2018, rendering them unusable for correcting GRACE-FO products. The GRACE-FO Science Data System (SDS) addressed this issue by replacing the problematic GRACE-D data with that of GRACE-C. Recently, an updated transplant method was implemented, which has improved GRACE-FO measurements at various levels, resulting in more accurate time-variable gravity and mass change observations.
GRACE-D accelerometer data show significant bias jumps since one month after the launch of the GRACE Follow-On (GRACE-FO) satellites in May 2018, making them inapplicable for correcting GRACE-FO products for non-gravitational accelerations. The GRACE-FO Science Data System (SDS) compensated this issue by transplanting the GRACE-C accelerometer data toward that of GRACE-D. Recently, GRACE-FO SDS implemented an updated transplant method, used in the latest release of GRACE-FO data. Here, we examine the impact of updated accelerometer transplant data (ACH) on GRACE-FO measurements at all levels: (a) Level-1B inter-satellite laser ranging residuals measured along satellite orbit, (b) Level-2 time-variable gravity solutions from all SDS centers (JPL, CSR, and GFZ), and (c) Level-3 mascon solutions. We show that inter-satellite laser ranging residuals are modified at low frequencies below 1 mHz, affecting the along-orbit analysis of large-scale time-variable gravity signals. When mapped into monthly Level-2 spherical harmonic coefficients of geopotential, the low-frequency change in inter-satellite ranging residuals leads to substantial improvement of coefficients associated with resonant orders (i.e., 15, 30, 45, etc.) and C-30. We also present an improved SLR-derived C-30 which significantly improves the agreement with updated GRACE-FO C-30 at seasonal and interannual timescales. Moreover, we demonstrate the noise reduction in mass change estimates from new GRACE-FO Level-2 data over oceans, Greenland, and Antarctica for all SDS solutions. GRACE-FO mascon solutions show a moderate change in the updated release. Our comprehensive analyses demonstrate high-quality estimates of non-gravitational accelerations by the updated transplant method, resulting in more accurate GRACE-FO time-variable gravity and mass change observations.

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