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contributor authorMazloff, Matthew R.
contributor authorFerrari, Raffaele
contributor authorSchneider, Tapio
date accessioned2017-06-09T17:19:55Z
date available2017-06-09T17:19:55Z
date copyright2013/06/01
date issued2013
identifier issn0022-3670
identifier otherams-83321.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4226533
description abstracthe Southern Ocean (SO) limb of the meridional overturning circulation (MOC) is characterized by three vertically stacked cells, each with a transport of about 10 Sv (Sv ≡ 106 m3 s?1). The buoyancy transport in the SO is dominated by the upper and middle MOC cells, with the middle cell accounting for most of the buoyancy transport across the Antarctic Circumpolar Current. A Southern Ocean state estimate for the years 2005 and 2006 with ?° resolution is used to determine the forces balancing this MOC. Diagnosing the zonal momentum budget in density space allows an exact determination of the adiabatic and diapycnal components balancing the thickness-weighted (residual) meridional transport. It is found that, to lowest order, the transport consists of an eddy component, a directly wind-driven component, and a component in balance with mean pressure gradients. Nonvanishing time-mean pressure gradients arise because isopycnal layers intersect topography or the surface in a circumpolar integral, leading to a largely geostrophic MOC even in the latitude band of Drake Passage. It is the geostrophic water mass transport in the surface layer where isopycnals outcrop that accomplishes the poleward buoyancy transport.
publisherAmerican Meteorological Society
titleThe Force Balance of the Southern Ocean Meridional Overturning Circulation
typeJournal Paper
journal volume43
journal issue6
journal titleJournal of Physical Oceanography
identifier doi10.1175/JPO-D-12-069.1
journal fristpage1193
journal lastpage1208
treeJournal of Physical Oceanography:;2013:;Volume( 043 ):;issue: 006
contenttypeFulltext


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