the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Strategies for Regional Modelling of Surface Mass Balance at the Monte Sarmiento Massif, Tierra del Fuego
Abstract. This study investigates strategies for melt model calibration in the Monte Sarmiento Massif (MSM), Tierra del Fuego, with the goal to achieve realistic simulations of the regional surface mass balance (SMB). Applied calibration strategies range from a local single-glacier calibration to a regional calibration with the inclusion of a snowdrift parametrization. We apply four SMB models of different complexity. This way, we examine the model transferability in space, the benefit of regional mass change observations and the advantage of increasing the complexity level regarding included processes. Measurements include ablation and ice thickness observations at Schiaparelli Glacier as well as elevation changes and flow velocity from satellite data for the entire study site. Performance of simulated SMB is validated against geodetic mass changes and stake observations of surface melting. Results show that transferring SMB models in space is a challenge, and common practices can produce distinctly biased estimates. Model performance can be significantly improved by the use of remotely sensed regional observations. Furthermore, we have shown that snowdrift does play an important role for the SMB in the Cordillera Darwin, where strong and consistent winds prevail. The massif-wide average annual SMB between 2000 and 2022 falls between -0.25 and -0.07 m w.e. yr-1, depending on the applied model. SMB is mainly controlled by surface melting and snowfall. The model intercomparison does not indicate one obviously best-suited model for SMB simulations in the MSM.
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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
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Supplement
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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
(4600 KB) - Metadata XML
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Supplement
(1807 KB) - BibTeX
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Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2022-1036', Enrico Mattea, 30 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-1036/egusphere-2022-1036-RC1-supplement.pdf
- AC1: 'Reply on RC1', Franziska Temme, 13 Feb 2023
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RC2: 'Comment on egusphere-2022-1036', David Rounce, 11 Dec 2022
- AC2: 'Reply on RC2', Franziska Temme, 13 Feb 2023
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2022-1036', Enrico Mattea, 30 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-1036/egusphere-2022-1036-RC1-supplement.pdf
- AC1: 'Reply on RC1', Franziska Temme, 13 Feb 2023
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RC2: 'Comment on egusphere-2022-1036', David Rounce, 11 Dec 2022
- AC2: 'Reply on RC2', Franziska Temme, 13 Feb 2023
Peer review completion
Journal article(s) based on this preprint
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David Farías-Barahona
Thorsten Seehaus
Ricardo Jaña
Jorge Arigony-Neto
Inti Gonzalez
Anselm Arndt
Tobias Sauter
Christoph Schneider
Johannes Jakob Fürst
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(4600 KB) - Metadata XML
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Supplement
(1807 KB) - BibTeX
- EndNote
- Final revised paper