Filament Frontogenesis by Boundary Layer TurbulenceSource: Journal of Physical Oceanography:;2015:;Volume( 045 ):;issue: 008::page 1988Author:McWilliams, James C.
,
Gula, Jonathan
,
Molemaker, M. Jeroen
,
Renault, Lionel
,
Shchepetkin, Alexander F.
DOI: 10.1175/JPO-D-14-0211.1Publisher: American Meteorological Society
Abstract: submesoscale filament of dense water in the oceanic surface layer can undergo frontogenesis with a secondary circulation that has a surface horizontal convergence and downwelling in its center. This occurs either because of the mesoscale straining deformation or because of the surface boundary layer turbulence that causes vertical eddy momentum flux divergence or, more briefly, vertical momentum mixing. In the latter case the circulation approximately has a linear horizontal momentum balance among the baroclinic pressure gradient, Coriolis force, and vertical momentum mixing, that is, a turbulent thermal wind. The frontogenetic evolution induced by the turbulent mixing sharpens the transverse gradient of the longitudinal velocity (i.e., it increases the vertical vorticity) through convergent advection by the secondary circulation. In an approximate model based on the turbulent thermal wind, the central vorticity approaches a finite-time singularity, and in a more general hydrostatic model, the central vorticity and horizontal convergence are amplified by shrinking the transverse scale to near the model?s resolution limit within a short advective period on the order of a day.
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contributor author | McWilliams, James C. | |
contributor author | Gula, Jonathan | |
contributor author | Molemaker, M. Jeroen | |
contributor author | Renault, Lionel | |
contributor author | Shchepetkin, Alexander F. | |
date accessioned | 2017-06-09T17:21:09Z | |
date available | 2017-06-09T17:21:09Z | |
date copyright | 2015/08/01 | |
date issued | 2015 | |
identifier issn | 0022-3670 | |
identifier other | ams-83675.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4226926 | |
description abstract | submesoscale filament of dense water in the oceanic surface layer can undergo frontogenesis with a secondary circulation that has a surface horizontal convergence and downwelling in its center. This occurs either because of the mesoscale straining deformation or because of the surface boundary layer turbulence that causes vertical eddy momentum flux divergence or, more briefly, vertical momentum mixing. In the latter case the circulation approximately has a linear horizontal momentum balance among the baroclinic pressure gradient, Coriolis force, and vertical momentum mixing, that is, a turbulent thermal wind. The frontogenetic evolution induced by the turbulent mixing sharpens the transverse gradient of the longitudinal velocity (i.e., it increases the vertical vorticity) through convergent advection by the secondary circulation. In an approximate model based on the turbulent thermal wind, the central vorticity approaches a finite-time singularity, and in a more general hydrostatic model, the central vorticity and horizontal convergence are amplified by shrinking the transverse scale to near the model?s resolution limit within a short advective period on the order of a day. | |
publisher | American Meteorological Society | |
title | Filament Frontogenesis by Boundary Layer Turbulence | |
type | Journal Paper | |
journal volume | 45 | |
journal issue | 8 | |
journal title | Journal of Physical Oceanography | |
identifier doi | 10.1175/JPO-D-14-0211.1 | |
journal fristpage | 1988 | |
journal lastpage | 2005 | |
tree | Journal of Physical Oceanography:;2015:;Volume( 045 ):;issue: 008 | |
contenttype | Fulltext |