Preprints
https://doi.org/10.5194/egusphere-2026-4041
https://doi.org/10.5194/egusphere-2026-4041
15 Jul 2026
 | 15 Jul 2026
Status: this preprint is open for discussion and under review for The Cryosphere (TC).

An accurate present-day model of the Antarctic ice sheet is necessary but insufficient for an accurate projection of its future evolution

Constantijn J. Berends, Jorge A. Bernales, Erwin Lambert, and Roderik S. W. van de Wal

Abstract. Accelerated retreat of the Antarctic ice sheet (AIS) dominates both the magnitude of, and the uncertainty in, high-end sea-level projections. One frequently cited caveat in the computational models used to create these projections is that many of them poorly represent the observed present-day state of the AIS. Following the thought that a model should accurately represent the present before it can be expected to accurately represent the future, there have been discussions in the ice-sheet modelling community to weight or even exclude individual models from ensemble studies based on how well they reproduce present-day observations.

In this study, we create a wide ensemble of realisations of the AIS with a numerical ice-sheet model under different parametric assumptions, utilising inverse methods to ensure every realisation reproduces snapshot observations of the present-day geometry, velocity, and thinning rates of the AIS to a degree that is comparable with the most recent ISMIP6 ensemble. These model realisations project anything between −0.3 m and +1.5 m of sea-level contribution (SLC) by 2300, with the sea-level rate at that time varying from −0.7 to +9.7 mm/yr. There is no clear relation between the degree to which these model realisations reproduce snapshot observations of the present-day AIS, and the amount of SLC they project. The main factors contributing to the wide variance in projected SLC are the sliding law and the distribution of slipperiness of the subglacial bed. Since these quantities are typically derived by inversion from observations of the ice flow, they can only be known as accurately as other processes affecting the flow, such as subglacial hydrology, ice damage, and calving. The resulting compensating errors are known to affect the modelled present-day state of the ice sheet differently than its response to future climate change, explaining why models with a nearly identical initial state can produce such different SLC projections. This implies that weighting or excluding models from ensemble studies based only on their agreement with snapshot observations of the present-day ice sheet might not be a wise choice. Instead, comparing to temporal observations, and to novel observations of the ice sheet’s sub-surface, might be more helpful to reduce the uncertainty in Antarctica’s future contribution to sea-level rise.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Constantijn J. Berends, Jorge A. Bernales, Erwin Lambert, and Roderik S. W. van de Wal

Status: open (until 26 Aug 2026)

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Constantijn J. Berends, Jorge A. Bernales, Erwin Lambert, and Roderik S. W. van de Wal
Constantijn J. Berends, Jorge A. Bernales, Erwin Lambert, and Roderik S. W. van de Wal

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Short summary
Computer models of the Antarctic ice sheet can project how much it will melt in response to climate change. That depends on the properties of the rock and the water beneath the ice, about which we know very little. That means the amount of sea-level in the future is very uncertain. Techniques to reduce that uncertainty do not always work as well as expected. We must get actual measurements of the bottom of the ice to improve our understanding of the ice sheet, and our knowledge of its future.
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