dc.creator | Bachman, Scott Daniel | |
dc.creator | Taylor, John Ryan | |
dc.date.accessioned | 2018-11-24T23:17:53Z | |
dc.date.available | 2014-11-06T15:53:25Z | |
dc.date.available | 2018-11-24T23:17:53Z | |
dc.date.issued | 2014-08-04 | |
dc.identifier | https://www.repository.cam.ac.uk/handle/1810/246308 | |
dc.identifier.uri | http://repository.aust.edu.ng/xmlui/handle/123456789/3183 | |
dc.description.abstract | A 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.language | en | |
dc.publisher | Elsevier | |
dc.publisher | Ocean Modelling | |
dc.rights | http://creativecommons.org/licenses/by/2.0/uk/ | |
dc.rights | Attribution 2.0 UK: England & Wales | |
dc.title | Modelling of partially-resolved oceanic symmetric instability | |
dc.type | Article | |