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.
Competing interests: Josefin Ahlkrona is a member of the editorial board of The Cryosphere.
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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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
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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.
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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
-
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.
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