On the Role of Bottom Pressure Torques in Wind-Driven Gyres

被引:22
|
作者
Stewart, Andrew L. [1 ]
McWilliams, James C. [1 ]
Solodoch, Aviv [1 ]
机构
[1] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
Ocean dynamics; Pressure; Topographic effects; Wind stress; Isopycnal coordinates; Ocean models; SHALLOW-WATER EQUATIONS; POTENTIAL ENSTROPHY; IDEALIZED MODEL; FORM STRESS; LARGE-SCALE; OCEAN; FLOW; INSTABILITY; ENERGY; GENERATION;
D O I
10.1175/JPO-D-20-0147.1
中图分类号
P7 [海洋学];
学科分类号
0707 ;
摘要
Previous studies have concluded that the wind-input vorticity in ocean gyres is balanced by bottom pressure torques (BPT), when integrated over latitude bands. However, the BPT must vanish when integrated over any area enclosed by an isobath. This constraint raises ambiguities regarding the regions over which BPT should close the vorticity budget, and implies that BPT generated to balance a local wind stress curl necessitates the generation of a compensating, nonlocal BPT and thus nonlocal circulation. This study aims to clarify the role of BPT in wind-driven gyres using an idealized isopycnal model. Experiments performed with a single-signed wind stress curl in an enclosed, sloped basin reveal that BPT balances the winds only when integrated over latitude bands. Integrating over other, dynamically motivated definitions of the gyre, such as barotropic streamlines, yields a balance between wind stress curl and bottom frictional torques. This implies that bottom friction plays a nonnegligible role in structuring the gyre circulation. Nonlocal bottom pressure torques manifest in the form of along-slope pressure gradients associated with a weak basin-scale circulation, and are associated with a transition to a balance between wind stress and bottom friction around the coasts. Finally, a suite of perturbation experiments is used to investigate the dynamics of BPT. To predict the BPT, the authors extend a previous theory that describes propagation of surface pressure signals from the gyre interior toward the coast along planetary potential vorticity contours. This theory is shown to agree closely with the diagnosed contributions to the vorticity budget across the suite of model experiments.
引用
收藏
页码:1441 / 1464
页数:24
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