Enhanced upward heat transport at deep submesoscale ocean fronts
International audience The ocean is the largest solar energy collector on Earth. The amount of heat it can store is modulated by its complex circulation, which spans a broad range of spatial scales, from metres to thousands of kilometres. In the classical paradigm, fine oceanic scales, less than 20...
Published in: | Nature Geoscience |
---|---|
Main Authors: | , , , , , , |
Other Authors: | , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2020
|
Subjects: | |
Online Access: | https://hal.science/hal-02933393 https://hal.science/hal-02933393/document https://hal.science/hal-02933393/file/Siegelman_etal_NG_2020.pdf https://doi.org/10.1038/s41561-019-0489-1 |
id |
ftinsu:oai:HAL:hal-02933393v1 |
---|---|
record_format |
openpolar |
institution |
Open Polar |
collection |
Institut national des sciences de l'Univers: HAL-INSU |
op_collection_id |
ftinsu |
language |
English |
topic |
SIZE LYAPUNOV EXPONENTS BAROCLINIC INSTABILITY SEA MESOSCALE ALTIMETRY RESTRATIFICATION ACL [SDV.MP]Life Sciences [q-bio]/Microbiology and Parasitology [SDE.BE]Environmental Sciences/Biodiversity and Ecology |
spellingShingle |
SIZE LYAPUNOV EXPONENTS BAROCLINIC INSTABILITY SEA MESOSCALE ALTIMETRY RESTRATIFICATION ACL [SDV.MP]Life Sciences [q-bio]/Microbiology and Parasitology [SDE.BE]Environmental Sciences/Biodiversity and Ecology Siegelman, Lia Klein, Patrice Riviere, Pascal Thompson, Andrew F. Torres, Hector S. Flexas, Mar Menemenlis, Dimitris Enhanced upward heat transport at deep submesoscale ocean fronts |
topic_facet |
SIZE LYAPUNOV EXPONENTS BAROCLINIC INSTABILITY SEA MESOSCALE ALTIMETRY RESTRATIFICATION ACL [SDV.MP]Life Sciences [q-bio]/Microbiology and Parasitology [SDE.BE]Environmental Sciences/Biodiversity and Ecology |
description |
International audience The ocean is the largest solar energy collector on Earth. The amount of heat it can store is modulated by its complex circulation, which spans a broad range of spatial scales, from metres to thousands of kilometres. In the classical paradigm, fine oceanic scales, less than 20 km in size, are thought to drive a significant downward heat transport from the surface to the ocean interior, which increases oceanic heat uptake. Here we use a combination of satellite and in situ observations in the Antarctic Circumpolar Current to diagnose oceanic vertical heat transport. The results explicitly demonstrate how deep-reaching submesoscale fronts, with a size smaller than 20 km, are generated by mesoscale eddies of size 50-300 km. In contrast to the classical paradigm, these submesoscale fronts are shown to drive an anomalous upward heat transport from the ocean interior back to the surface that is larger than other contributions to vertical heat transport and of comparable magnitude to air-sea fluxes. This effect can remarkably alter the oceanic heat uptake and will be strongest in eddy-rich regions, such as the Antarctic Circumpolar Current, the Kuroshio Extension and the Gulf Stream, all of which are key players in the climate system. |
author2 |
Department of Environmental Science and Engineering Pasadena (ESE) California Institute of Technology (CALTECH) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) Laboratoire des Sciences de l'Environnement Marin (LEMAR) (LEMAR) Institut de Recherche pour le Développement (IRD)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Université de Brest (UBO)-Institut Universitaire Européen de la Mer (IUEM) Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS) Laboratoire d'Océanographie Physique et Spatiale (LOPS) Institut de Recherche pour le Développement (IRD)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS) SNO-MEMO CNES-TOSCA project Laboratoire d'Excellence LabexMER ANR-10-LABX-19 CNES-Region Bretagne doctoral grant NASA-CNES SWOT mission NASA Senior NPP Fellowship David and Lucille Packard FoundationThe David and Lucile Packard Foundation NASANational Aeronautics and Space Administration (NASA) NNX16AG42G, NNX15AG42G French Polar Institute 109, 1201 National Aeronautics and Space Administration (NASA)National Aeronautics and Space Administration (NASA) CNES (OSTST-OSIW) ANR-10-LABX-0019,LabexMER,LabexMER Marine Excellence Research: a changing ocean(2010) |
format |
Article in Journal/Newspaper |
author |
Siegelman, Lia Klein, Patrice Riviere, Pascal Thompson, Andrew F. Torres, Hector S. Flexas, Mar Menemenlis, Dimitris |
author_facet |
Siegelman, Lia Klein, Patrice Riviere, Pascal Thompson, Andrew F. Torres, Hector S. Flexas, Mar Menemenlis, Dimitris |
author_sort |
Siegelman, Lia |
title |
Enhanced upward heat transport at deep submesoscale ocean fronts |
title_short |
Enhanced upward heat transport at deep submesoscale ocean fronts |
title_full |
Enhanced upward heat transport at deep submesoscale ocean fronts |
title_fullStr |
Enhanced upward heat transport at deep submesoscale ocean fronts |
title_full_unstemmed |
Enhanced upward heat transport at deep submesoscale ocean fronts |
title_sort |
enhanced upward heat transport at deep submesoscale ocean fronts |
publisher |
HAL CCSD |
publishDate |
2020 |
url |
https://hal.science/hal-02933393 https://hal.science/hal-02933393/document https://hal.science/hal-02933393/file/Siegelman_etal_NG_2020.pdf https://doi.org/10.1038/s41561-019-0489-1 |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
ISSN: 1752-0894 Nature Geoscience https://hal.science/hal-02933393 Nature Geoscience, 2020, 13 (1), pp.50-+. ⟨10.1038/s41561-019-0489-1⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1038/s41561-019-0489-1 hal-02933393 https://hal.science/hal-02933393 https://hal.science/hal-02933393/document https://hal.science/hal-02933393/file/Siegelman_etal_NG_2020.pdf doi:10.1038/s41561-019-0489-1 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1038/s41561-019-0489-1 |
container_title |
Nature Geoscience |
container_volume |
13 |
container_issue |
1 |
container_start_page |
50 |
op_container_end_page |
55 |
_version_ |
1796300305257725952 |
spelling |
ftinsu:oai:HAL:hal-02933393v1 2024-04-14T08:03:58+00:00 Enhanced upward heat transport at deep submesoscale ocean fronts Siegelman, Lia Klein, Patrice Riviere, Pascal Thompson, Andrew F. Torres, Hector S. Flexas, Mar Menemenlis, Dimitris Department of Environmental Science and Engineering Pasadena (ESE) California Institute of Technology (CALTECH) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) Laboratoire des Sciences de l'Environnement Marin (LEMAR) (LEMAR) Institut de Recherche pour le Développement (IRD)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Université de Brest (UBO)-Institut Universitaire Européen de la Mer (IUEM) Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS) Laboratoire d'Océanographie Physique et Spatiale (LOPS) Institut de Recherche pour le Développement (IRD)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS) SNO-MEMO CNES-TOSCA project Laboratoire d'Excellence LabexMER ANR-10-LABX-19 CNES-Region Bretagne doctoral grant NASA-CNES SWOT mission NASA Senior NPP Fellowship David and Lucille Packard FoundationThe David and Lucile Packard Foundation NASANational Aeronautics and Space Administration (NASA) NNX16AG42G, NNX15AG42G French Polar Institute 109, 1201 National Aeronautics and Space Administration (NASA)National Aeronautics and Space Administration (NASA) CNES (OSTST-OSIW) ANR-10-LABX-0019,LabexMER,LabexMER Marine Excellence Research: a changing ocean(2010) 2020-01 https://hal.science/hal-02933393 https://hal.science/hal-02933393/document https://hal.science/hal-02933393/file/Siegelman_etal_NG_2020.pdf https://doi.org/10.1038/s41561-019-0489-1 en eng HAL CCSD Nature Publishing Group info:eu-repo/semantics/altIdentifier/doi/10.1038/s41561-019-0489-1 hal-02933393 https://hal.science/hal-02933393 https://hal.science/hal-02933393/document https://hal.science/hal-02933393/file/Siegelman_etal_NG_2020.pdf doi:10.1038/s41561-019-0489-1 info:eu-repo/semantics/OpenAccess ISSN: 1752-0894 Nature Geoscience https://hal.science/hal-02933393 Nature Geoscience, 2020, 13 (1), pp.50-+. ⟨10.1038/s41561-019-0489-1⟩ SIZE LYAPUNOV EXPONENTS BAROCLINIC INSTABILITY SEA MESOSCALE ALTIMETRY RESTRATIFICATION ACL [SDV.MP]Life Sciences [q-bio]/Microbiology and Parasitology [SDE.BE]Environmental Sciences/Biodiversity and Ecology info:eu-repo/semantics/article Journal articles 2020 ftinsu https://doi.org/10.1038/s41561-019-0489-1 2024-03-21T17:18:41Z International audience The ocean is the largest solar energy collector on Earth. The amount of heat it can store is modulated by its complex circulation, which spans a broad range of spatial scales, from metres to thousands of kilometres. In the classical paradigm, fine oceanic scales, less than 20 km in size, are thought to drive a significant downward heat transport from the surface to the ocean interior, which increases oceanic heat uptake. Here we use a combination of satellite and in situ observations in the Antarctic Circumpolar Current to diagnose oceanic vertical heat transport. The results explicitly demonstrate how deep-reaching submesoscale fronts, with a size smaller than 20 km, are generated by mesoscale eddies of size 50-300 km. In contrast to the classical paradigm, these submesoscale fronts are shown to drive an anomalous upward heat transport from the ocean interior back to the surface that is larger than other contributions to vertical heat transport and of comparable magnitude to air-sea fluxes. This effect can remarkably alter the oceanic heat uptake and will be strongest in eddy-rich regions, such as the Antarctic Circumpolar Current, the Kuroshio Extension and the Gulf Stream, all of which are key players in the climate system. Article in Journal/Newspaper Antarc* Antarctic Institut national des sciences de l'Univers: HAL-INSU Antarctic The Antarctic Nature Geoscience 13 1 50 55 |