A comparison of different solutions for the dynamic smagorinsky model applied in a GCM

dc.bibliographicCitation.firstPage249eng
dc.bibliographicCitation.issue3eng
dc.bibliographicCitation.journalTitleMeteorologische Zeitschrifteng
dc.bibliographicCitation.volume27eng
dc.contributor.authorSchaefer-Rolffs, U.
dc.date.accessioned2020-11-25T14:52:43Z
dc.date.available2020-11-25T14:52:43Z
dc.date.issued2018
dc.description.abstractA discussion of different approaches and solutions of the basic tensor equation within the Dynamic Smagorinsky Model (DSM) suitable for General Circulation Models (GCM) is presented. Particular interest is dedicated to the relationship between various approaches (i.e., the specific formulation of the tensor equation), namely a least-square approach, a time lag approach, and a simple tensor contraction approach, and the impact of the specific solution (i.e., how to solve the equation) on the Smagorinsky parameter c2S . In addition to the standard solutions, clipped solutions, absolute solutions, and tensor norm solutions are examined. The numerical results are based on calculations from a general circulation model, where the different approaches are applied to provide the turbulent horizontal momentum diffusion. Here, they are examined with focus on two issues: 1) At the beginning of the simulations, the different choices for the tensor equation result in different values for the locally distributed and zonally averaged values of the Smagorinsky parameter. These values show that for the standard solutions almost half of the values of c2S are negative, in accordance with known results from isotropic turbulence and leads to unstable simulations. In addition, the tensor norm is related to the absolute solution via the Cauchy-Schwarz inequality. 2) As the simulations proceed, the differences of the Smagorinsky parameter values diminish except for the tensor norm solutions while evolving to a stationary state in a process of self-organization such that they form a group with values comparable to isotropic three-dimensional simulations. In summary, the least-squares and time lag approaches provide reasonable results, while the simple contraction approach fluctuates more. For the solutions, it is discussed whether the clipped or the tensor norm solution is more reasonable. © 2018 The authors.eng
dc.description.fondsLeibniz_Fonds
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://doi.org/10.34657/4639
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/6010
dc.language.isoengeng
dc.publisherStuttgart : Bornträgereng
dc.relation.doihttps://doi.org/10.1127/metz/2018/0885
dc.relation.issn0941-2948
dc.rights.licenseCC BY-NC 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by-nc/4.0/eng
dc.subject.ddc550eng
dc.subject.otherMomentum diffusioneng
dc.subject.otherSubgrid-scale modellingeng
dc.subject.otherTurbulence modellingeng
dc.titleA comparison of different solutions for the dynamic smagorinsky model applied in a GCMeng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorIAPeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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