the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Increasing numerical stability of mountain valley glacier simulations: implementation and testing of free-surface stabilization in Elmer/Ice
Abstract. This paper concerns a numerical stabilization method for free-surface ice flow called the free-surface stabilization algorithm (FSSA). In the current study, the FSSA is implemented into the numerical ice-flow software Elmer/Ice and tested on synthetic two-dimensional (2D) glaciers, as well as on the real-world glacier of Midtre Lovénbreen, Svalbard. For the synthetic 2D cases it is found that the FSSA method increases the largest stable time-step size at least by a factor of ten for the case of a gently sloping ice surface (3°), and by at least a factor of five for cases of moderately to steeply inclined surfaces (6° to 12°) . Furthermore, the FSSA method increases the overall accuracy for all surface slopes. The largest stable time-step size is found to be smallest for the case of a low sloping surface, despite having overall smaller velocities. For Midtre Lovénbreen the FSSA method doubles the largest stable time-step size, however, the accuracy is in this case slightly lowered in the deeper parts of the glacier, while it increases near edges. The implication is that the non-FSSA method might be more accurate at predicting glacier thinning, while the FSSA method is more suitable for predicting future glacier extent. A possible application of the larger time-step sizes allowed for by the FSSA is for spin-up simulations, where relatively fast changing climate data can be incorporated on short time scales, while the slowly changing velocity field is updated over larger time scales.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
(1777 KB)
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2023-1507', Anonymous Referee #1, 14 Sep 2023
- AC1: 'Reply on RC1', Andre Löfgren, 18 Dec 2023
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AC3: 'Reply on RC1', Andre Löfgren, 18 Dec 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1507/egusphere-2023-1507-AC3-supplement.pdf
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RC2: 'Comment on egusphere-2023-1507', Anonymous Referee #2, 15 Nov 2023
- AC2: 'Reply on RC2', Andre Löfgren, 18 Dec 2023
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2023-1507', Anonymous Referee #1, 14 Sep 2023
- AC1: 'Reply on RC1', Andre Löfgren, 18 Dec 2023
-
AC3: 'Reply on RC1', Andre Löfgren, 18 Dec 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1507/egusphere-2023-1507-AC3-supplement.pdf
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RC2: 'Comment on egusphere-2023-1507', Anonymous Referee #2, 15 Nov 2023
- AC2: 'Reply on RC2', Andre Löfgren, 18 Dec 2023
Peer review completion
Journal article(s) based on this preprint
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Thomas Zwinger
Peter Råback
Christian Helanow
Josefin Ahlkrona
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(1777 KB) - Metadata XML