Ellipsoidal Correction in GRACE Surface Mass Change Estimation

Abstract

AbstractThe Earth's shape is much closer to an ellipsoid than a sphere. The commonly used spherical approximation in mass change inversion is expected to cause bias by the spherical harmonic (SH) solutions from Gravity Recovery and Climate Experiment (GRACE), especially in high‐latitude regions where significant present‐day ice losses occur. This bias, or ellipsoidal correction, reaches up to 8% from the evaluation by simulations based on synthetic mass change rate models. Further evaluation using 14 plus years of GRACE monthly SH solutions (from April 2002 to December 2016) indicates that the ellipsoidal correction is also noticeable in the total mass change time series over polar regions. Before and after the ellipsoidal correction, the estimated linear rates from mass change time series differ by 4.3%, 4.7%, 5.2%, 5.7%, and 6.6% for five selected regions over Greenland, Antarctic Peninsula, Amundsen Sea Embayment, Alaska glacier, and Svalbard Islands, respectively. Although with amplitudes likely below the current GRACE's uncertainty level, these differences are consistently negative over the five regions. This indicates that the spherical approximation leads to systematic underestimation for polar mass change rates. Thus, the ellipsoidal correction needs to be considered for more precise mass recovery with GRACE SH solutions. It also depends on spatial scales of mass change signals (the smaller the spatial scale, the larger the correction). To more reliably estimate high‐latitude surface mass changes by GRACE SH solutions, the ellipsoidal correction is recommended, especially for ice‐loss signals over polar regions.