Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet

The hysteresis behaviour of ice sheets arises because of the different thresholds for growth and decline of a continental-scale ice sheet depending on the initial conditions. In this study, the hysteresis effect of the early Cenozoic Antarctic ice sheet is investigated with an improved ice sheet-cli...

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Main Authors: Van Breedam, Jonas, Huybrechts, Philippe, Crucifix, Michel
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2023
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-399
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spelling ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00065495 2023-05-15T14:08:47+02:00 Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet Van Breedam, Jonas Huybrechts, Philippe Crucifix, Michel 2023-03 electronic https://doi.org/10.5194/egusphere-2023-399 https://noa.gwlb.de/receive/cop_mods_00065495 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00064016/egusphere-2023-399.pdf https://egusphere.copernicus.org/preprints/2023/egusphere-2023-399/egusphere-2023-399.pdf eng eng Copernicus Publications https://doi.org/10.5194/egusphere-2023-399 https://noa.gwlb.de/receive/cop_mods_00065495 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00064016/egusphere-2023-399.pdf https://egusphere.copernicus.org/preprints/2023/egusphere-2023-399/egusphere-2023-399.pdf https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2023 ftnonlinearchiv https://doi.org/10.5194/egusphere-2023-399 2023-03-20T00:15:10Z The hysteresis behaviour of ice sheets arises because of the different thresholds for growth and decline of a continental-scale ice sheet depending on the initial conditions. In this study, the hysteresis effect of the early Cenozoic Antarctic ice sheet is investigated with an improved ice sheet-climate coupling method that accurately captures the ice-albedo feedback. It is shown that the hysteresis effect of the early Cenozoic Antarctic ice sheet is about ~180 ppmv or between 3.5 °C and 5.5 °C, depending only weakly on the bedrock elevation dataset. Excluding the solid Earth feedback decreases the hysteresis effect significantly towards ~40 ppmv, because the transition to a glacial state can occur at a higher forcing. The rapid transition from a glacial to a deglacial state and oppositely from deglacial to glacial conditions is strongly enhanced by the ice-albedo feedback, in combination with the elevation – surface mass balance feedback. Variations in the orbital parameters show that extreme values of the orbital parameters are able to exceed the threshold in summer insolation to induce a (de)glaciation. It appears that the long-term eccentricity cycle has a large influence on the ice sheet growth and decline and is able to pace the ice sheet evolution for constant CO2 concentration close to the glaciation threshold. Article in Journal/Newspaper Antarc* Antarctic Ice Sheet Niedersächsisches Online-Archiv NOA Antarctic
institution Open Polar
collection Niedersächsisches Online-Archiv NOA
op_collection_id ftnonlinearchiv
language English
topic article
Verlagsveröffentlichung
spellingShingle article
Verlagsveröffentlichung
Van Breedam, Jonas
Huybrechts, Philippe
Crucifix, Michel
Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet
topic_facet article
Verlagsveröffentlichung
description The hysteresis behaviour of ice sheets arises because of the different thresholds for growth and decline of a continental-scale ice sheet depending on the initial conditions. In this study, the hysteresis effect of the early Cenozoic Antarctic ice sheet is investigated with an improved ice sheet-climate coupling method that accurately captures the ice-albedo feedback. It is shown that the hysteresis effect of the early Cenozoic Antarctic ice sheet is about ~180 ppmv or between 3.5 °C and 5.5 °C, depending only weakly on the bedrock elevation dataset. Excluding the solid Earth feedback decreases the hysteresis effect significantly towards ~40 ppmv, because the transition to a glacial state can occur at a higher forcing. The rapid transition from a glacial to a deglacial state and oppositely from deglacial to glacial conditions is strongly enhanced by the ice-albedo feedback, in combination with the elevation – surface mass balance feedback. Variations in the orbital parameters show that extreme values of the orbital parameters are able to exceed the threshold in summer insolation to induce a (de)glaciation. It appears that the long-term eccentricity cycle has a large influence on the ice sheet growth and decline and is able to pace the ice sheet evolution for constant CO2 concentration close to the glaciation threshold.
format Article in Journal/Newspaper
author Van Breedam, Jonas
Huybrechts, Philippe
Crucifix, Michel
author_facet Van Breedam, Jonas
Huybrechts, Philippe
Crucifix, Michel
author_sort Van Breedam, Jonas
title Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet
title_short Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet
title_full Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet
title_fullStr Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet
title_full_unstemmed Hysteresis and orbital pacing of the early Cenozoic Antarctic ice sheet
title_sort hysteresis and orbital pacing of the early cenozoic antarctic ice sheet
publisher Copernicus Publications
publishDate 2023
url https://doi.org/10.5194/egusphere-2023-399
https://noa.gwlb.de/receive/cop_mods_00065495
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00064016/egusphere-2023-399.pdf
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-399/egusphere-2023-399.pdf
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
Ice Sheet
genre_facet Antarc*
Antarctic
Ice Sheet
op_relation https://doi.org/10.5194/egusphere-2023-399
https://noa.gwlb.de/receive/cop_mods_00065495
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00064016/egusphere-2023-399.pdf
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-399/egusphere-2023-399.pdf
op_rights https://creativecommons.org/licenses/by/4.0/
uneingeschränkt
info:eu-repo/semantics/openAccess
op_doi https://doi.org/10.5194/egusphere-2023-399
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