Abstract

Past redistributions of the Earth’s mass resulting from the Earth’s viscoelastic response to the cycle of deglaciation and glaciation reflect the process known as glacial isostatic adjustment (GIA). GPS data are effective at constraining GIA velocities, provided that these data are accurate, have adequate spatial coverage, and account for competing geophysical processes, including the elastic loading of ice/snow ablation/accumulation. GPS solutions are significantly affected by common mode errors (CMEs) and the choice of optimal noise model, and they are contaminated by other geophysical signals due primarily to the Earth’s elastic response. Here, independent component analysis is used to remove the CMEs, and the Akaike information criterion is used to determine the optimal noise model for 79 GPS stations in Antarctica, primarily distributed across West Antarctica and the Antarctic Peninsula. Next, a high-resolution surface mass variation model is used to correct for elastic deformation. Finally, we use the improved GPS solution to assess the accuracy of seven contemporary GIA forward models in Antarctica. The results show that the maximal GPS crustal displacement velocity deviations reach 4.0 mm yr−1, and the mean variation is 0.4 mm yr−1 after removing CMEs and implementing the noise analysis. All GIA model-predicted velocities are found to systematically underestimate the GPS-observed velocities in the Amundsen Sea Embayment. Additionally, the GPS vertical velocities on the North Antarctic Peninsula are larger than those on the South Antarctic Peninsula, and most of the forward models underestimate the GIA impact on the Antarctic Peninsula.

Highlights

  • Glacial isostatic adjustment (GIA) is a process by which the solid Earth viscoelastically responds to the cycle of glaciation and deglaciation

  • The results clearly reveal that the scattering in the filtered time series is effectively reduced by the independent component analysis (ICA) filter, as the mean root mean square (RMS) decreases from 6.41 to 4.46 mm; the maximum reduction in the RMS value is

  • To determine the optimal noise model (ONM) for Antarctica, we evaluated 5 noise models supplied by Hector [42], namely, white noise (WN) + power law (PL), WN + random walk noise (RW), WN + flicker noise (FN), WN + FN + RW, and WN + RW + GGM, to analyze the 79 Global Positioning System (GPS) station time series based on the Akaike criterion (AIC)

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Summary

Introduction

Glacial isostatic adjustment (GIA) is a process by which the solid Earth viscoelastically responds to the cycle of glaciation and deglaciation. GIA-induced Earth surface velocities can be computed using forward or assimilated global GIA models, the results of which 4.0/). To estimate changes in surface mass (for example, ice sheet mass), GIA signals must be deduced from satellite gravity signals [7]. GIA is the largest error source at present, hindering the use of Gravity Recovery And Climate Experiment (GRACE/GRACE-FO) satellite gravimetry data to estimate the large-scale Antarctic ice sheet mass balance [6,8]. Geodetic data-driven regionally inverted models, e.g., GIA models generated by assimilating GRACE, Global Positioning System (GPS), and other geodetic data or combining GRACE and satellite (laser) altimetry (ICESat) data, have been used [9,10,11,12] to correct for the effects of GIA on GRACE data

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