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Enhanced upward heat transport at deep submesoscale ocean fronts

Siegelman, Lia and Klein, Patrice and Rivière, Pascal and Thompson, Andrew F. and Torres, Hector S. and Flexas, Mar and Menemenlis, Dimitris (2020) Enhanced upward heat transport at deep submesoscale ocean fronts. Nature Geoscience, 13 (1). pp. 50-55. ISSN 1752-0894.

[img] PDF (Supplementary Discussion Figs. 1 and 2) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 1 - Weakly turbulent and southern eddy edge areas) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 2 - Lateral gradient of buoyancy and Richardson number in the strongly turbulent area) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 3 - Map of finite size Lyapunov exponents) - Supplemental Material
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[img] PDF (Extended Data Fig. 4 - Finite size Lyapunov exponents and horizontal gradient of buoyancy, vertical velocities and vertical heat transport at 300 m) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 5 - Daily averaged vertical velocities and vertical heat transport from the high-resolution numerical simulation) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 6 - Averaged vertical heat transport from the high-resolution numerical simulation) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 7 - Domain averaged vertical heat transport from the high-resolution numerical simulation) - Supplemental Material
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[img] Image (JPEG) (Extended Data Fig. 8 - Distance between two dives and angle between the seal’s trajectory and the fronts) - Supplemental Material
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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.

Item Type:Article
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URLURL TypeDescription ReadCube access
Siegelman, Lia0000-0003-3330-082X
Klein, Patrice0000-0002-3089-3896
Rivière, Pascal0000-0002-4705-2700
Thompson, Andrew F.0000-0003-0322-4811
Torres, Hector S.0000-0003-2098-8012
Flexas, Mar0000-0002-0617-3004
Menemenlis, Dimitris0000-0001-9940-8409
Additional Information:© 2019 Springer Nature Limited. Received 18 June 2019; Accepted 16 October 2019; Published 02 December 2019. We thank K. Richards for his insightful comments, F. d’Ovidio for providing the code to compute FSLE. The elephant seal work was supported as part of the SNO-MEMO and by the CNES-TOSCA project Elephant seals as Oceanographic Samplers of submesoscale features led by C. Guinet with support of the French Polar Institute (programmes 109 and 1201). This research was carried out, in part, at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). High-end computing resources for the numerical simulation were provided by the NASA Advanced Supercomputing Division at the Ames Research Center. This work was partly funded by the CNES (OSTST-OSIW) and the Laboratoire d’Excellence LabexMER (ANR-10-LABX-19). L.S. is a NASA-JVSRP affiliate and is supported by a joint CNES-Région Bretagne doctoral grant. P.K. is supported by the NASA-CNES SWOT mission and a NASA Senior NPP Fellowship. A.F.T. is supported by the David and Lucille Packard Foundation and NASA grant NNX16AG42G. M.F. is supported by NASA grant NNX15AG42G. Data availability: The marine mammal data were collected and made freely available by the International MEOP Consortium and the national programs that contribute to it, and is available at The Ssalto/Duacs altimeter products were produced and distributed by the Copernicus Marine and Environment Monitoring Service with support from CNES, and is available at Author Contributions: L.S. and P.K. conceived the experiments, analysed the results and wrote the manuscript. D.M. and H.S.T. ran the numerical simulations. H.S.T. helped with analysing the regional simulation. L.S., P.K., P.R., A.F.T., H.S.T. and M.F. reviewed the manuscript. The authors declare no competing interests.
Funding AgencyGrant Number
Centre National d'Études Spatiales (CNES)UNSPECIFIED
Agence Nationale pour la Recherche (ANR)ANR-10-LABX-19
David and Lucille Packard FoundationUNSPECIFIED
Subject Keywords:Physical oceanography
Issue or Number:1
Record Number:CaltechAUTHORS:20191003-111504890
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Official Citation:Siegelman, L., Klein, P., Rivière, P. et al. Enhanced upward heat transport at deep submesoscale ocean fronts. Nat. Geosci. 13, 50–55 (2020) doi:10.1038/s41561-019-0489-1
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99047
Deposited By: George Porter
Deposited On:02 Dec 2019 18:27
Last Modified:08 Jan 2020 17:15

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