The Drake Passage opening from an experimental fluid dynamics point of view.


Journal

Scientific reports
ISSN: 2045-2322
Titre abrégé: Sci Rep
Pays: England
ID NLM: 101563288

Informations de publication

Date de publication:
07 Oct 2021
Historique:
received: 26 02 2021
accepted: 09 09 2021
entrez: 8 10 2021
pubmed: 9 10 2021
medline: 9 10 2021
Statut: epublish

Résumé

Pronounced global cooling around the Eocene-Oligocene transition (EOT) was a pivotal event in Earth's climate history, controversially associated with the opening of the Drake Passage. Using a physical laboratory model we revisit the fluid dynamics of this marked reorganization of ocean circulation. Here we show, seemingly contradicting paleoclimate records, that in our experiments opening the pathway yields higher values of mean water surface temperature than the "closed" configuration. This mismatch points to the importance of the role ice albedo feedback plays in the investigated EOT-like transition, a component that is not captured in the laboratory model. Our conclusion is supported by numerical simulations performed in a global climate model (GCM) of intermediate complexity, where both "closed" and "open" configurations were explored, with and without active sea ice dynamics. The GCM results indicate that sea surface temperatures would change in the opposite direction following an opening event in the two sea ice dynamics settings, and the results are therefore consistent both with the laboratory experiment (slight warming after opening) and the paleoclimatic data (pronounced cooling after opening). It follows that in the hypothetical case of an initially ice-free Antarctica the continent could have become even warmer after the opening, a scenario not indicated by paleotemperature reconstructions.

Identifiants

pubmed: 34620925
doi: 10.1038/s41598-021-99123-0
pii: 10.1038/s41598-021-99123-0
pmc: PMC8497466
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

19951

Informations de copyright

© 2021. The Author(s).

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Auteurs

Miklós Vincze (M)

von Kármán Laboratory of Environmental Flows, Eötvös Loránd University, Budapest, 1117, Hungary. mvincze@general.elte.hu.
MTA-ELTE Theoretical Physics Research Group, Budapest, 1117, Hungary. mvincze@general.elte.hu.

Tamás Bozóki (T)

von Kármán Laboratory of Environmental Flows, Eötvös Loránd University, Budapest, 1117, Hungary.
Doctoral School of Environmental Sciences, University of Szeged, Szeged, 6720, Hungary.
Institute of Earth Physics and Space Science (ELKH EPSS), Sopron, 9400, Hungary.

Mátyás Herein (M)

MTA-ELTE Theoretical Physics Research Group, Budapest, 1117, Hungary.
Institute for Theoretical Physics, Eötvös Loránd University, Budapest, 1117, Hungary.

Ion Dan Borcia (ID)

Department of Statistical Physics and Nonlinear Dynamics, Brandenburg University of Technology Cottbus-Senftenberg, Cottbus, 03046, Germany.

Uwe Harlander (U)

Department of Aerodynamics and Fluid Mechanics, Brandenburg University of Technology Cottbus-Senftenberg, Cottbus, 03046, Germany.

Attila Horicsányi (A)

von Kármán Laboratory of Environmental Flows, Eötvös Loránd University, Budapest, 1117, Hungary.

Anita Nyerges (A)

Department of Geology, Eötvös Loránd University, Budapest, 1117, Hungary.
MTA-MTM-ELTE Research Group for Paleontology, 1431, Budapest, Hungary.

Costanza Rodda (C)

Laboratoire des Ecoulements Géophysiques et Industriels, Université Grenoble Alpes, CNRS, Grenoble-INP, 38000, Grenoble, France.

András Pál (A)

Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH), 1121, Budapest, Hungary.

József Pálfy (J)

Department of Geology, Eötvös Loránd University, Budapest, 1117, Hungary.
MTA-MTM-ELTE Research Group for Paleontology, 1431, Budapest, Hungary.

Classifications MeSH