Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports

The degree to which total meridional heat transport is sensitive to the details of its atmospheric and oceanic components is explored. A coupled atmosphere, ocean, and sea ice model of an aquaplanet is employed to simulate very different climates—some with polar ice caps, some without—even though th...

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Published in:Journal of the Atmospheric Sciences
Main Authors: Enderton, Daniel, Marshall, John C
Other Authors: Massachusetts Institute of Technology. Department of Earth and Planetary Sciences, Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences, MIT Energy Initiative, Marshall, John C.
Format: Article in Journal/Newspaper
Language:English
Published: American Meteorological Society 2007
Subjects:
Online Access:http://hdl.handle.net/1721.1/52333
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spelling ftmit:oai:dspace.mit.edu:1721.1/52333 2024-04-21T08:11:27+00:00 Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports Enderton, Daniel Marshall, John C Massachusetts Institute of Technology. Department of Earth and Planetary Sciences Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences MIT Energy Initiative Marshall, John C. Enderton, Daniel 2007-11 application/pdf http://hdl.handle.net/1721.1/52333 en_US eng American Meteorological Society http://dx.doi.org/10.1175/2008JAS2680.1 Journal of the Atmospheric Sciences 0022-4928 http://hdl.handle.net/1721.1/52333 Enderton, Daniel, and John Marshall. “Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports.” Journal of the Atmospheric Sciences (2009): 1593-1611. © 2010 American Meteorological Society orcid:0000-0001-9230-3591 Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. American Meteorological Society Article http://purl.org/eprint/type/JournalArticle 2007 ftmit https://doi.org/10.1175/2008JAS2680.1 2024-03-27T15:02:15Z The degree to which total meridional heat transport is sensitive to the details of its atmospheric and oceanic components is explored. A coupled atmosphere, ocean, and sea ice model of an aquaplanet is employed to simulate very different climates—some with polar ice caps, some without—even though they are driven by the same incoming solar flux. Differences arise due to varying geometrical constraints on ocean circulation influencing its ability to transport heat meridionally. Without complex land configurations, the results prove easier to diagnose and compare to theory and simple models and, hence, provide a useful test bed for ideas about heat transport and its partition within the climate system. In particular, the results are discussed in the context of a 1978 study by Stone, who argued that for a planet with Earth’s astronomical parameters and rotation rate, the total meridional heat transport would be independent of the detailed dynamical processes responsible for that transport and depend primarily on the distribution of incoming solar radiation and the mean planetary albedo. The authors find that in warm climates in which there is no ice, Stone’s result is a useful guide. In cold climates with significant polar ice caps, however, meridional gradients in albedo significantly affect the absorption of solar radiation and need to be included in any detailed calculation or discussion of total heat transport. Since the meridional extent of polar ice caps is sensitive to details of atmospheric and oceanic circulation, these cannot be ignored. Finally, what has been learned is applied to a study of the total heat transport estimated from the Earth Radiation Budget Experiment (ERBE) data. MIT Climate Modeling Initiative National Science Foundation Article in Journal/Newspaper Sea ice DSpace@MIT (Massachusetts Institute of Technology) Journal of the Atmospheric Sciences 66 6 1593 1611
institution Open Polar
collection DSpace@MIT (Massachusetts Institute of Technology)
op_collection_id ftmit
language English
description The degree to which total meridional heat transport is sensitive to the details of its atmospheric and oceanic components is explored. A coupled atmosphere, ocean, and sea ice model of an aquaplanet is employed to simulate very different climates—some with polar ice caps, some without—even though they are driven by the same incoming solar flux. Differences arise due to varying geometrical constraints on ocean circulation influencing its ability to transport heat meridionally. Without complex land configurations, the results prove easier to diagnose and compare to theory and simple models and, hence, provide a useful test bed for ideas about heat transport and its partition within the climate system. In particular, the results are discussed in the context of a 1978 study by Stone, who argued that for a planet with Earth’s astronomical parameters and rotation rate, the total meridional heat transport would be independent of the detailed dynamical processes responsible for that transport and depend primarily on the distribution of incoming solar radiation and the mean planetary albedo. The authors find that in warm climates in which there is no ice, Stone’s result is a useful guide. In cold climates with significant polar ice caps, however, meridional gradients in albedo significantly affect the absorption of solar radiation and need to be included in any detailed calculation or discussion of total heat transport. Since the meridional extent of polar ice caps is sensitive to details of atmospheric and oceanic circulation, these cannot be ignored. Finally, what has been learned is applied to a study of the total heat transport estimated from the Earth Radiation Budget Experiment (ERBE) data. MIT Climate Modeling Initiative National Science Foundation
author2 Massachusetts Institute of Technology. Department of Earth and Planetary Sciences
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
MIT Energy Initiative
Marshall, John C.
Enderton, Daniel
format Article in Journal/Newspaper
author Enderton, Daniel
Marshall, John C
spellingShingle Enderton, Daniel
Marshall, John C
Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports
author_facet Enderton, Daniel
Marshall, John C
author_sort Enderton, Daniel
title Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports
title_short Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports
title_full Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports
title_fullStr Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports
title_full_unstemmed Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports
title_sort explorations of atmosphere–ocean–ice climates on an aquaplanet and their meridional energy transports
publisher American Meteorological Society
publishDate 2007
url http://hdl.handle.net/1721.1/52333
genre Sea ice
genre_facet Sea ice
op_source American Meteorological Society
op_relation http://dx.doi.org/10.1175/2008JAS2680.1
Journal of the Atmospheric Sciences
0022-4928
http://hdl.handle.net/1721.1/52333
Enderton, Daniel, and John Marshall. “Explorations of Atmosphere–Ocean–Ice Climates on an Aquaplanet and Their Meridional Energy Transports.” Journal of the Atmospheric Sciences (2009): 1593-1611. © 2010 American Meteorological Society
orcid:0000-0001-9230-3591
op_rights Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
op_doi https://doi.org/10.1175/2008JAS2680.1
container_title Journal of the Atmospheric Sciences
container_volume 66
container_issue 6
container_start_page 1593
op_container_end_page 1611
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