The importance of snow albedo for ice sheet evolution over the last glacial cycle

The surface energy and mass balance of ice sheets strongly depends on the amount of solar radiation absorbed at the surface, which is mainly controlled by the albedo of snow and ice. Here, using an Earth system model of intermediate complexity, we explore the role played by surface albedo for the si...

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Main Authors: Willeit, Matteo, Ganopolski, Andrey
Format: Article in Journal/Newspaper
Language:English
Published: München : European Geopyhsical Union 2018
Subjects:
550
Online Access:https://doi.org/10.34657/1337
https://oa.tib.eu/renate/handle/123456789/655
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spelling ftleibnizopen:oai:oai.leibnizopen.de:QtJDfYoBNQPDO7WIgGWC 2023-10-09T21:52:23+02:00 The importance of snow albedo for ice sheet evolution over the last glacial cycle Willeit, Matteo Ganopolski, Andrey 2018 application/pdf https://doi.org/10.34657/1337 https://oa.tib.eu/renate/handle/123456789/655 eng eng München : European Geopyhsical Union CC BY 4.0 Unported https://creativecommons.org/licenses/by/4.0/ Climate of the Past, Volume 14, Issue 5, Page 697-707 albedo climate modeling deglaciation glacier mass balance ice sheet Last Glacial Northern Hemisphere optical property snow solar radiation surface energy 550 article Text 2018 ftleibnizopen https://doi.org/10.34657/1337 2023-09-10T23:17:03Z The surface energy and mass balance of ice sheets strongly depends on the amount of solar radiation absorbed at the surface, which is mainly controlled by the albedo of snow and ice. Here, using an Earth system model of intermediate complexity, we explore the role played by surface albedo for the simulation of glacial cycles. We show that the evolution of the Northern Hemisphere ice sheets over the last glacial cycle is very sensitive to the representation of snow albedo in the model. It is well known that the albedo of snow depends strongly on snow grain size and the content of light-absorbing impurities. Excluding either the snow aging effect or the dust darkening effect on snow albedo leads to an excessive ice build-up during glacial times and consequently to a failure in simulating deglaciation. While the effect of snow grain growth on snow albedo is well constrained, the albedo reduction due to the presence of dust in snow is much more uncertain because the light-absorbing properties of dust vary widely as a function of dust mineral composition. We also show that assuming slightly different optical properties of dust leads to very different ice sheet and climate evolutions in the model. Conversely, ice sheet evolution is less sensitive to the choice of ice albedo in the model. We conclude that a proper representation of snow albedo is a fundamental prerequisite for a successful simulation of glacial cycles. publishedVersion Article in Journal/Newspaper Ice Sheet LeibnizOpen (The Leibniz Association)
institution Open Polar
collection LeibnizOpen (The Leibniz Association)
op_collection_id ftleibnizopen
language English
topic albedo
climate modeling
deglaciation
glacier mass balance
ice sheet
Last Glacial
Northern Hemisphere
optical property
snow
solar radiation
surface energy
550
spellingShingle albedo
climate modeling
deglaciation
glacier mass balance
ice sheet
Last Glacial
Northern Hemisphere
optical property
snow
solar radiation
surface energy
550
Willeit, Matteo
Ganopolski, Andrey
The importance of snow albedo for ice sheet evolution over the last glacial cycle
topic_facet albedo
climate modeling
deglaciation
glacier mass balance
ice sheet
Last Glacial
Northern Hemisphere
optical property
snow
solar radiation
surface energy
550
description The surface energy and mass balance of ice sheets strongly depends on the amount of solar radiation absorbed at the surface, which is mainly controlled by the albedo of snow and ice. Here, using an Earth system model of intermediate complexity, we explore the role played by surface albedo for the simulation of glacial cycles. We show that the evolution of the Northern Hemisphere ice sheets over the last glacial cycle is very sensitive to the representation of snow albedo in the model. It is well known that the albedo of snow depends strongly on snow grain size and the content of light-absorbing impurities. Excluding either the snow aging effect or the dust darkening effect on snow albedo leads to an excessive ice build-up during glacial times and consequently to a failure in simulating deglaciation. While the effect of snow grain growth on snow albedo is well constrained, the albedo reduction due to the presence of dust in snow is much more uncertain because the light-absorbing properties of dust vary widely as a function of dust mineral composition. We also show that assuming slightly different optical properties of dust leads to very different ice sheet and climate evolutions in the model. Conversely, ice sheet evolution is less sensitive to the choice of ice albedo in the model. We conclude that a proper representation of snow albedo is a fundamental prerequisite for a successful simulation of glacial cycles. publishedVersion
format Article in Journal/Newspaper
author Willeit, Matteo
Ganopolski, Andrey
author_facet Willeit, Matteo
Ganopolski, Andrey
author_sort Willeit, Matteo
title The importance of snow albedo for ice sheet evolution over the last glacial cycle
title_short The importance of snow albedo for ice sheet evolution over the last glacial cycle
title_full The importance of snow albedo for ice sheet evolution over the last glacial cycle
title_fullStr The importance of snow albedo for ice sheet evolution over the last glacial cycle
title_full_unstemmed The importance of snow albedo for ice sheet evolution over the last glacial cycle
title_sort importance of snow albedo for ice sheet evolution over the last glacial cycle
publisher München : European Geopyhsical Union
publishDate 2018
url https://doi.org/10.34657/1337
https://oa.tib.eu/renate/handle/123456789/655
genre Ice Sheet
genre_facet Ice Sheet
op_source Climate of the Past, Volume 14, Issue 5, Page 697-707
op_rights CC BY 4.0 Unported
https://creativecommons.org/licenses/by/4.0/
op_doi https://doi.org/10.34657/1337
_version_ 1779315543535255552