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Modelling of partially-resolved oceanic symmetric instability

dc.creatorBachman, Scott Daniel
dc.creatorTaylor, John Ryan
dc.date.accessioned2018-11-24T23:17:53Z
dc.date.available2014-11-06T15:53:25Z
dc.date.available2018-11-24T23:17:53Z
dc.date.issued2014-08-04
dc.identifierhttps://www.repository.cam.ac.uk/handle/1810/246308
dc.identifier.urihttp://repository.aust.edu.ng/xmlui/handle/123456789/3183
dc.description.abstractA series of idealized numerical models have been developed to investigate the effects of partially resolved symmetric instability (SI) in oceanic general circulation models. An analysis of the energetics of symmetric instability is used to argue that the mixed layer can be at least partially restratified even when some SI modes are absent due to either large horizontal viscosity or coarse model resolution. Linear stability analysis reveals that in the idealized models the amount of restratification can be predicted as a function of the grid spacing and viscosity. The models themselves are used to demonstrate these predictions and reveal three possible outcomes in steady-state: (1) incomplete restratification due to viscosity, (2) incomplete restratification due to resolution, and (3) excessive restratification due to anisotropy of the viscosity. The third outcome occurs even on a high-resolution isotropic grid and in two separate numerical models, and thus appears to be a sort of robust numerical feature. The three outcomes are used to recommend criteria that a successful SI parameterization should satisfy.
dc.languageen
dc.publisherElsevier
dc.publisherOcean Modelling
dc.rightshttp://creativecommons.org/licenses/by/2.0/uk/
dc.rightsAttribution 2.0 UK: England & Wales
dc.titleModelling of partially-resolved oceanic symmetric instability
dc.typeArticle


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