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dc.contributor.authorEfstathiou, GA
dc.date.accessioned2023-03-17T09:10:18Z
dc.date.issued2023-06-01
dc.date.updated2023-03-16T07:48:15Z
dc.description.abstractA scale-dependent dynamic Smagorinsky model is implemented in the Met Office/NERC cloud model (MONC) using two averaging flavours, along Lagrangian pathlines and local moving averages. The dynamic approaches were compared against the conventional Smagorinsky-Lilly scheme in simulating the diurnal cycle of shallow cumulus convection. The simulations spanned from the LES to the near-grey-zone and grey-zone resolutions and revealed the adaptability of the dynamic model across the scales and different stability regimes. The dynamic model can produce a scale and stability dependent profile of the subfilter turbulence length-scale across the chosen resolution range. At grey-zone resolutions the adaptive length scales can better represent the early pre-cloud boundary layer leading to temperature and moisture profiles closer to the LES compared to the standard Smagorinsky. As a result the initialisation and general representation of the cloud field in the dynamic model is in good agreement with the LES. In contrast, the standard Smagorinsky produces a less well-mixed boundary-layer which fails to ventilate moisture from the boundary layer resulting in the delayed spin-up of the cloud layer. Moreover, strong down-gradient diffusion controls the turbulent transport of scalars in the cloud layer. However, the dynamic approaches rely on the resolved field to account for non-local transports, leading to over-energetic structures when the boundary layer is fully developed and the Lagrangian model is used. Introducing the local averaging version of the model or adopting a new Lagrangian time scale provides stronger dissipation without significantly affecting model behaviour.en_GB
dc.description.sponsorshipNatural Environment Research Council (NERC)en_GB
dc.identifier.citationVol. 80 (6), pp. 1519–1545en_GB
dc.identifier.doi10.1175/JAS-D-22-0132.1
dc.identifier.grantnumberNE/T011351/1en_GB
dc.identifier.urihttp://hdl.handle.net/10871/132699
dc.identifierORCID: 0000-0003-3469-8729 (Efstathiou, Georgios)
dc.language.isoen_USen_GB
dc.publisherAmerican Meteorological Societyen_GB
dc.relation.urlhttps://doi.org/10.24378/exe.4604en_GB
dc.rights© 2023 American Meteorological Society. Open access. This article is licensed under a Creative Commons Attribution 4.0 license (http://creativecommons.org/licenses/by/4.0/).
dc.titleDynamic subgrid turbulence modeling for shallow cumulus convection simulations beyond LES resolutions (article)en_GB
dc.typeArticleen_GB
dc.date.available2023-03-17T09:10:18Z
dc.identifier.issn0022-4928
dc.descriptionThis is the final version. Available on open access from the American Meteorological Society via the DOI in this recorden_GB
dc.descriptionThe dataset associated with this article is available in ORE at: https://doi.org/10.24378/exe.4604en_GB
dc.identifier.eissn1520-0469
dc.identifier.journalJournal of the Atmospheric Sciencesen_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2023-03-13
dcterms.dateSubmitted2022-06-07
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2023-03-13
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2023-03-17T09:06:21Z
refterms.versionFCDAM
refterms.dateFOA2023-06-01T14:15:59Z
refterms.panelBen_GB


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© 2023 American Meteorological Society. Open access. This article is licensed under a Creative Commons Attribution 4.0 license (http://creativecommons.org/licenses/by/4.0/).
Except where otherwise noted, this item's licence is described as © 2023 American Meteorological Society. Open access. This article is licensed under a Creative Commons Attribution 4.0 license (http://creativecommons.org/licenses/by/4.0/).