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...

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Main Authors: Joughin, Ian, Shapero, Daniel, Dutrieux, Pierre
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2024
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-2929
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spelling ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00070910 2024-02-11T09:58:12+01:00 Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations Joughin, Ian Shapero, Daniel Dutrieux, Pierre 2024-01 electronic https://doi.org/10.5194/egusphere-2023-2929 https://noa.gwlb.de/receive/cop_mods_00070910 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00069235/egusphere-2023-2929.pdf https://egusphere.copernicus.org/preprints/2024/egusphere-2023-2929/egusphere-2023-2929.pdf eng eng Copernicus Publications https://doi.org/10.5194/egusphere-2023-2929 https://noa.gwlb.de/receive/cop_mods_00070910 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00069235/egusphere-2023-2929.pdf https://egusphere.copernicus.org/preprints/2024/egusphere-2023-2929/egusphere-2023-2929.pdf https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2024 ftnonlinearchiv https://doi.org/10.5194/egusphere-2023-2929 2024-01-15T00:22:45Z 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 2200. We do not include other factors, such as ice shelf breakup that might increase loss, nor factors such as increased accumulation and isostatic uplift that may mitigate loss. Article in Journal/Newspaper Antarc* Antarctica Ice Shelf Pine Island Pine Island Glacier Niedersächsisches Online-Archiv NOA Pine Island Glacier ENVELOPE(-101.000,-101.000,-75.000,-75.000) Weertman ENVELOPE(-67.753,-67.753,-66.972,-66.972)
institution Open Polar
collection Niedersächsisches Online-Archiv NOA
op_collection_id ftnonlinearchiv
language English
topic article
Verlagsveröffentlichung
spellingShingle article
Verlagsveröffentlichung
Joughin, Ian
Shapero, Daniel
Dutrieux, Pierre
Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations
topic_facet article
Verlagsveröffentlichung
description 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 2200. We do not include other factors, such as ice shelf breakup that might increase loss, nor factors such as increased accumulation and isostatic uplift that may mitigate loss.
format Article in Journal/Newspaper
author Joughin, Ian
Shapero, Daniel
Dutrieux, Pierre
author_facet Joughin, Ian
Shapero, Daniel
Dutrieux, Pierre
author_sort Joughin, Ian
title Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations
title_short Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations
title_full Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations
title_fullStr Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations
title_full_unstemmed Responses of Pine Island and Thwaites Glaciers to Melt and Sliding Parameterizations
title_sort responses of pine island and thwaites glaciers to melt and sliding parameterizations
publisher Copernicus Publications
publishDate 2024
url https://doi.org/10.5194/egusphere-2023-2929
https://noa.gwlb.de/receive/cop_mods_00070910
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00069235/egusphere-2023-2929.pdf
https://egusphere.copernicus.org/preprints/2024/egusphere-2023-2929/egusphere-2023-2929.pdf
long_lat ENVELOPE(-101.000,-101.000,-75.000,-75.000)
ENVELOPE(-67.753,-67.753,-66.972,-66.972)
geographic Pine Island Glacier
Weertman
geographic_facet Pine Island Glacier
Weertman
genre Antarc*
Antarctica
Ice Shelf
Pine Island
Pine Island Glacier
genre_facet Antarc*
Antarctica
Ice Shelf
Pine Island
Pine Island Glacier
op_relation https://doi.org/10.5194/egusphere-2023-2929
https://noa.gwlb.de/receive/cop_mods_00070910
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00069235/egusphere-2023-2929.pdf
https://egusphere.copernicus.org/preprints/2024/egusphere-2023-2929/egusphere-2023-2929.pdf
op_rights https://creativecommons.org/licenses/by/4.0/
uneingeschränkt
info:eu-repo/semantics/openAccess
op_doi https://doi.org/10.5194/egusphere-2023-2929
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