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Effect of GIA models with 3D composite mantle viscosity on GRACE mass balance estimates for Antarctica

van der Wal, Wouter; Whitehouse, Pippa L.; Schrama, E.J.O.

Effect of GIA models with 3D composite mantle viscosity on GRACE mass balance estimates for Antarctica Thumbnail


Authors

Wouter van der Wal

E.J.O. Schrama



Abstract

Seismic data indicate that there are large viscosity variations in the mantle beneath Antarctica. Consideration of such variations would affect predictions of models of Glacial Isostatic Adjustment (GIA), which are used to correct satellite measurements of ice mass change. However, most GIA models used for that purpose have assumed the mantle to be uniformly stratified in terms of viscosity. The goal of this study is to estimate the effect of lateral variations in viscosity on Antarctic mass balance estimates derived from the Gravity Recovery and Climate Experiment (GRACE) data. To this end, recently-developed global GIA models based on lateral variations in mantle temperature are tuned to fit constraints in the northern hemisphere and then compared to GPS-derived uplift rates in Antarctica. We find that these models can provide a better fit to GPS uplift rates in Antarctica than existing GIA models with a radially-varying (1D) rheology. When 3D viscosity models in combination with specific ice loading histories are used to correct GRACE measurements, mass loss in Antarctica is smaller than previously found for the same ice loading histories and their preferred 1D viscosity profiles. The variation in mass balance estimates arising from using different plausible realizations of 3D viscosity amounts to 20 Gt/yr for the ICE-5G ice model and 16 Gt/yr for the W12a ice model; these values are larger than the GRACE measurement error, but smaller than the variation arising from unknown ice history. While there exist 1D Earth models that can reproduce the total mass balance estimates derived using 3D Earth models, the spatial pattern of gravity rates can be significantly affected by 3D viscosity in a way that cannot be reproduced by GIA models with 1D viscosity. As an example, models with 1D viscosity always predict maximum gravity rates in the Ross Sea for the ICE-5G ice model, however, for one of the three preferred 3D models the maximum (for the same ice model) is found near the Weddell Sea. This demonstrates that 3D variations in viscosity affect the sensitivity of present-day uplift and gravity rates to changes in the timing of the ice history. In particular, low viscosities (View the MathML source) found in West Antarctica make the mantle very sensitive to recent changes in ice thickness.

Citation

van der Wal, W., Whitehouse, P. L., & Schrama, E. (2015). Effect of GIA models with 3D composite mantle viscosity on GRACE mass balance estimates for Antarctica. Earth and Planetary Science Letters, 414, 134-143. https://doi.org/10.1016/j.epsl.2015.01.001

Journal Article Type Article
Acceptance Date Jan 1, 2015
Online Publication Date Jan 28, 2015
Publication Date Mar 15, 2015
Deposit Date Jan 6, 2015
Publicly Available Date Jan 15, 2015
Journal Earth and Planetary Science Letters
Print ISSN 0012-821X
Publisher Elsevier
Peer Reviewed Peer Reviewed
Volume 414
Pages 134-143
DOI https://doi.org/10.1016/j.epsl.2015.01.001
Keywords Glacial rebound, Mantle rheology, Viscosity, Time-variable gravity, GRACE, Antarctica.

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