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contributor authorEdwards, Neil R.
contributor authorWillmott, Andrew J.
contributor authorKillworth, Peter D.
date accessioned2017-06-09T14:52:59Z
date available2017-06-09T14:52:59Z
date copyright1998/05/01
date issued1998
identifier issn0022-3670
identifier otherams-28858.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4166020
description abstractA frictional geostrophic model is used to examine how the stability of the thermohaline circulation is affected by idealized topographic variations and the presence or absence of wind stress. If the flow exhibits collapses, the authors consider how topography and wind stress affect the ensuing oscillations. Large-scale slope up toward the north or the west can significantly destabilize the circulation by modifying the barotropic flow and reducing the depth of convection. Wind stress stabilizes the circulation by deepening the thermocline in the subtropical gyre. Wind driving can also radically reduce the period of oscillations by destabilizing the northern halocline in the collapsed phase. The overall period of the oscillation is usually governed by the time taken for diffusive warming to destabilize the deep ocean.
publisherAmerican Meteorological Society
titleOn the Role of Topography and Wind Stress on the Stability of the Thermohaline Circulation
typeJournal Paper
journal volume28
journal issue5
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(1998)028<0756:OTROTA>2.0.CO;2
journal fristpage756
journal lastpage778
treeJournal of Physical Oceanography:;1998:;Volume( 028 ):;issue: 005
contenttypeFulltext


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