Responses of Pine Island and Thwaites glaciers to melt and sliding parameterizations ...
Pine Island and Thwaites glaciers are the two largest contributors to sea level rise from Antarctica. Here we examine the influence of basal friction and melt in determining projected losses. We examine both Weertman and Coulomb friction laws with explicit weakening as the ice thins to flotation, wh...
| Main Authors: | , , |
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| Format: | Dataset |
| Language: | English |
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Dryad
2024
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| Subjects: | |
| Online Access: | https://dx.doi.org/10.5061/dryad.7sqv9s50x https://datadryad.org/stash/dataset/doi:10.5061/dryad.7sqv9s50x |
| Summary: | Pine Island and Thwaites glaciers are the two largest contributors to sea level rise from Antarctica. Here we examine the influence of basal friction and melt in determining projected losses. We examine both Weertman and Coulomb friction laws with explicit weakening as the ice thins to flotation, which many friction laws include implicitly via the effective pressure. We find relatively small differences with the choice of friction law (Weertman or Coulomb) but find losses are highly sensitive to the rate at which the basal traction is reduced as the area above the grounding line thins. Consistent with earlier work on Pine Island Glacier, we find sea level contributions from both glaciers vary linearly with the melt volume averaged over time and space, with little influence from the spatial or temporal distribution of melt. Based on recent estimates of melt from other studies, our work simulations suggest that melt-driven combined sea-level rise contribution from both glaciers is unlikely to exceed 10 cm by ... : # Responses of Pine Island and Thwaites glaciers to melt and sliding parameterizations [https://doi.org/10.5061/dryad.7sqv9s50x](https://doi.org/10.5061/dryad.7sqv9s50x) ## Sharing/Access information This archive contains data related to a paper currently in revision at the Cryosphere: [https://egusphere.copernicus.org/preprints/2024/egusphere-2023-2929/](https://egusphere.copernicus.org/preprints/2024/egusphere-2023-2929/) Icepack/firedrake ([https://icepack.github.io/](https://icepack.github.io/)) must be installed and the firedrake environment must be activated. The forward and inverse code is at [https://github.com/fastice/icesheetModels](https://github.com/fastice/icesheetModels) It will require: [https://github.com/fastice/modelfunc](https://github.com/fastice/modelfunc) The results are in the following 7 directories (each with a README with further detail not given here) **forwardModel:** With directories and a script to run the forward model **forwardModelInputs**: The SMB file needed or the forward ... |
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