Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone

The mixed layer (ML) hosts an intense submesoscale turbulence playing a pivotal role for energy transfers. Representation of ML turbulence from observations and models, partly, relies on the knowledge of its spatio-temporal scales. Here, we physically-inform the need of high spatio-temporal resoluti...

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Main Authors: Tedesco, P., Mashayek, A., Naveira-Garabato, A., Caulfield, C.
Format: Conference Object
Language:English
Published: 2023
Subjects:
Online Access:https://gfzpublic.gfz-potsdam.de/pubman/item/item_5017822
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spelling ftgfzpotsdam:oai:gfzpublic.gfz-potsdam.de:item_5017822 2023-08-27T04:09:11+02:00 Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone Tedesco, P. Mashayek, A. Naveira-Garabato, A. Caulfield, C. 2023 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5017822 eng eng info:eu-repo/semantics/altIdentifier/doi/10.57757/IUGG23-1778 https://gfzpublic.gfz-potsdam.de/pubman/item/item_5017822 XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG) info:eu-repo/semantics/conferenceObject 2023 ftgfzpotsdam https://doi.org/10.57757/IUGG23-1778 2023-08-06T23:41:22Z The mixed layer (ML) hosts an intense submesoscale turbulence playing a pivotal role for energy transfers. Representation of ML turbulence from observations and models, partly, relies on the knowledge of its spatio-temporal scales. Here, we physically-inform the need of high spatio-temporal resolutions (L ~ 1km; T ~1 hour) to accurately infer the ML turbulence. Based on a numerical simulation of the Drake Passage in winter, we combine a Lagrangian filtering and a Helmholtz decomposition to decompose motions (LPF: low vs. HPF: high frequency) and their dynamical components (rotational vs. divergent). The ML hosts a 'zoo' of motions including: energetics, primarily rotational, submesoscale currents (LPF) and less energetics internal-gravity waves (HPF), such as rotational inertial waves, divergent lee waves and an internal-wave continuum. The contributions of motions to kinetic energy transfers are driven by their partitioning into dynamical components and spatio-temporal scales. Purely rotational motions realise an inverse cascade and coupled rotational-divergent motions realise a forward cascade. Submesoscale currents are largely rotational and primarily realise an inverse cascade. Internal-gravity waves, roughly equipartitioned between rotational and divergent components, realise an inverse and forward cascade of close magnitudes when coupled to submesoscale currents. All motions spread up to small spatio-temporal scales (L < 10 km; T< 6 hours) and these ranges significantly contribute to the inverse (≥ 30 %) and forward (80 — 95 %) cascades. Our results show that all classes of motions should be represented at high spatio-temporal resolutions to comprehensively infer winter ML turbulence, which has implications for study strategies. Conference Object Drake Passage GFZpublic (German Research Centre for Geosciences, Helmholtz-Zentrum Potsdam) Drake Passage
institution Open Polar
collection GFZpublic (German Research Centre for Geosciences, Helmholtz-Zentrum Potsdam)
op_collection_id ftgfzpotsdam
language English
description The mixed layer (ML) hosts an intense submesoscale turbulence playing a pivotal role for energy transfers. Representation of ML turbulence from observations and models, partly, relies on the knowledge of its spatio-temporal scales. Here, we physically-inform the need of high spatio-temporal resolutions (L ~ 1km; T ~1 hour) to accurately infer the ML turbulence. Based on a numerical simulation of the Drake Passage in winter, we combine a Lagrangian filtering and a Helmholtz decomposition to decompose motions (LPF: low vs. HPF: high frequency) and their dynamical components (rotational vs. divergent). The ML hosts a 'zoo' of motions including: energetics, primarily rotational, submesoscale currents (LPF) and less energetics internal-gravity waves (HPF), such as rotational inertial waves, divergent lee waves and an internal-wave continuum. The contributions of motions to kinetic energy transfers are driven by their partitioning into dynamical components and spatio-temporal scales. Purely rotational motions realise an inverse cascade and coupled rotational-divergent motions realise a forward cascade. Submesoscale currents are largely rotational and primarily realise an inverse cascade. Internal-gravity waves, roughly equipartitioned between rotational and divergent components, realise an inverse and forward cascade of close magnitudes when coupled to submesoscale currents. All motions spread up to small spatio-temporal scales (L < 10 km; T< 6 hours) and these ranges significantly contribute to the inverse (≥ 30 %) and forward (80 — 95 %) cascades. Our results show that all classes of motions should be represented at high spatio-temporal resolutions to comprehensively infer winter ML turbulence, which has implications for study strategies.
format Conference Object
author Tedesco, P.
Mashayek, A.
Naveira-Garabato, A.
Caulfield, C.
spellingShingle Tedesco, P.
Mashayek, A.
Naveira-Garabato, A.
Caulfield, C.
Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
author_facet Tedesco, P.
Mashayek, A.
Naveira-Garabato, A.
Caulfield, C.
author_sort Tedesco, P.
title Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
title_short Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
title_full Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
title_fullStr Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
title_full_unstemmed Spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
title_sort spatio-temporal characteristics of winter mixed layer turbulence in an energetic oceanic zone
publishDate 2023
url https://gfzpublic.gfz-potsdam.de/pubman/item/item_5017822
geographic Drake Passage
geographic_facet Drake Passage
genre Drake Passage
genre_facet Drake Passage
op_source XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
op_relation info:eu-repo/semantics/altIdentifier/doi/10.57757/IUGG23-1778
https://gfzpublic.gfz-potsdam.de/pubman/item/item_5017822
op_doi https://doi.org/10.57757/IUGG23-1778
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