Turbulence and Diapycnal Mixing in Drake Passage

被引:100
|
作者
Laurent, L. St. [1 ]
Garabato, A. C. Naveira [2 ]
Ledwell, J. R. [3 ]
Thurnherr, A. M. [4 ]
Toole, J. M. [1 ]
Watson, A. J. [5 ]
机构
[1] Woods Hole Oceanog Inst, Dept Phys Oceanog, Woods Hole, MA 02543 USA
[2] Univ Southampton, Natl Oceanog Ctr, Southampton, Hants, England
[3] Woods Hole Oceanog Inst, Dept Appl Ocean Phys & Engn, Woods Hole, MA 02543 USA
[4] Lamont Doherty Earth Observ, Div Ocean & Climate Phys, Palisades, NY USA
[5] Univ E Anglia, Sch Environm Sci, Norwich NR4 7TJ, Norfolk, England
基金
美国国家科学基金会; 英国自然环境研究理事会;
关键词
TRACER-RELEASE EXPERIMENT; SOUTHERN-OCEAN; SPATIAL VARIABILITY; HAWAIIAN RIDGE; ABYSSAL OCEAN; TIDAL ENERGY; TOPOGRAPHY; DISSIPATION; PROFILES; TIDES;
D O I
10.1175/JPO-D-12-027.1
中图分类号
P7 [海洋学];
学科分类号
0707 ;
摘要
Direct measurements of turbulence levels in the Drake Passage region of the Southern Ocean show a marked enhancement over the Phoenix Ridge. At this site, the Antarctic Circumpolar Current (ACC) is constricted in its flow between the southern tip of South America and the northern tip of the Antarctic Peninsula. Observed turbulent kinetic energy dissipation rates are enhanced in the regions corresponding to the ACC frontal zones where strong flow reaches the bottom. In these areas, turbulent dissipation levels reach 10(-8) W kg(-1) at abyssal and middepths. The mixing enhancement in the frontal regions is sufficient to elevate the diapycnal turbulent diffusivity acting in the deep water above the axis of the ridge to 1 x 10(-4) m(2) s(-1). This level is an order of magnitude larger than the mixing levels observed upstream in the ACC above smoother bathymetry. Outside of the frontal regions, dissipation rates are O(10(-10)) W kg(-1), comparable to the background levels of turbulence found throughout most mid-and low-latitude regions of the global ocean.
引用
收藏
页码:2143 / 2152
页数:10
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