Preprints
https://doi.org/10.5194/egusphere-2025-3942
https://doi.org/10.5194/egusphere-2025-3942
28 Aug 2025
 | 28 Aug 2025
Status: this preprint is open for discussion and under review for The Cryosphere (TC).

Evolution of the Antarctic Ice Sheet from 2000–2300 and beyond: model sensitivity and uncertainty analysis using MPAS-Albany Land Ice

Trevor R. Hillebrand, Matthew J. Hoffman, Holly K. Han, Mauro Perego, Alexander O. Hager, Andrew Nolan, Xylar Asay-Davis, Stephen F. Price, Jerry Watkins, and Max Carlson

Abstract. We present a description of the Antarctic Ice Sheet model configuration submitted to the ISMIP6-Antarctica-2300 experiment using the MPAS-Albany Land Ice model, along with three new sets of simulations: (1) a set of extended simulations to 2500 for three forced experiments and to 2775 for the control experiment; (2) a sensitivity analysis of our model configuration to parameters controlling basal sliding and sub-shelf melt, and to model structural choices including the choice of the energy and stress balances; and (3) a 72-member ensemble run on graphics processing units (GPUs) and analysis of variance to determine the primary sources of uncertainty in our ice-sheet model projections. Our extended simulations predict rapid retreat beginning after 2300 for SSP1-2.6 forcing and after 2500 for present-day (control) forcing, primarily in the Amundsen Sea Embayment. Our parameter sensitivity experiments reveal only moderate sensitivity to the value of the sub-shelf melt parameter, ranging from the 5th to 95th percentile values. The Amundsen Sea Embayment region displays a strongly non-linear dependence of mass loss on the sliding law, with no discernible relationship between the sliding law exponent and the mass loss by 2300, while the sectors feeding the Ross and Filchner-Ronne ice shelves exhibit more mass loss with a more-plastic sliding law and vice versa. Our model fidelity sensitivity experiments indicate a modest sensitivity to the choice of stress balance approximation and a very strong sensitivity to thermomechanical coupling versus an uncoupled configuration. Our 72-member ensemble and analysis of variance show that the uncertainty in long-term projections is dominated by the choice of Earth system model forcing and the presence or absence of hydrofracture forcing, rather than uncertainty in sliding and sub-shelf melt parameters. We hypothesize that initial condition uncertainty could account for much of the inter-model spread in the ISMIP6 ensembles.

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Trevor R. Hillebrand, Matthew J. Hoffman, Holly K. Han, Mauro Perego, Alexander O. Hager, Andrew Nolan, Xylar Asay-Davis, Stephen F. Price, Jerry Watkins, and Max Carlson

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Trevor R. Hillebrand, Matthew J. Hoffman, Holly K. Han, Mauro Perego, Alexander O. Hager, Andrew Nolan, Xylar Asay-Davis, Stephen F. Price, Jerry Watkins, and Max Carlson

Data sets

MPAS- Albany Land Ice simulations of the Antarctic Ice Sheet through 2300: Exp02–05 flux fields T. Hillebrand et al. https://doi.org/10.5281/zenodo.16803637

MPAS- Albany Land Ice simulations of the Antarctic Ice Sheet through 2300: Exp02–05 state fields T. Hillebrand et al. https://doi.org/10.5281/zenodo.16798097

MPAS- Albany Land Ice simulations of the Antarctic Ice Sheet through 2300: Exp11–14 flux fields T. Hillebrand et al. https://doi.org/10.5281/zenodo.16805185

MPAS- Albany Land Ice simulations of the Antarctic Ice Sheet through 2300: Exp11–14 state fields T. Hillebrand et al. https://doi.org/10.5281/zenodo.16805033

MPAS-Albany Land Ice simulations of the Antarctic Ice Sheet through 2300: time series T. Hillebrand et al. https://doi.org/10.5281/zenodo.16805241

Model code and software

Energy Exascale Earth System Model E3SM Team https://doi.org/10.5281/zenodo.16809723

Interactive computing environment

mali-ismip6-ais-2300-anova analysis scripts Matthew Hoffman https://doi.org/10.5281/zenodo.16813658

Trevor R. Hillebrand, Matthew J. Hoffman, Holly K. Han, Mauro Perego, Alexander O. Hager, Andrew Nolan, Xylar Asay-Davis, Stephen F. Price, Jerry Watkins, and Max Carlson

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Short summary
We present new simulations that complement our contribution to the ISMIP6-Antarctica-2300 ensemble. We find significant mass loss after 2300 under both low-emissions and present-day forcing. Thermal evolution is extremely important, with fixed temperature yielding up to twice as much mass loss as simulations with evolving temperature. External forcing uncertainty dominates the ensemble spread after 2050. Initial condition uncertainty could explain the inter-model spread in the ISMIP6 ensembles.
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