Upper ocean diapycnal mixing in the northwestern Weddell Sea

被引:27
|
作者
Muench, RD
Padman, L
Howard, SL
Fahrbach, E
机构
[1] Earth & Space Res, Seattle, WA 98102 USA
[2] Alfred Wegener Inst Polar & Marine Res, D-27515 Bremerhaven, Germany
基金
美国国家科学基金会;
关键词
D O I
10.1016/S0967-0645(02)00162-5
中图分类号
P7 [海洋学];
学科分类号
0707 ;
摘要
Vertical profiles of ocean temperature, salinity, dissolved oxygen concentration, and currents were obtained during austral winter 1997 from a region extending from the northeastern Antarctic Peninsula to the South Orkney Plateau in the northern Weddell Sea. From these data we estimate the spatial variation of shear-driven turbulent mixing and the mean diapycnal diffusivity (K-v) in the main pycnocline. We conclude that the mean upper ocean beat flux in the northwestern Weddell Sea is in the range 2-10Wm(-2). The ocean tide provides a significant fraction of the oceanic kinetic energy in the region: tidal current speeds at the shelf break can approach 50 cm s(-1) compared with mean flows of similar to5-10 cm s(-1). We show that the conversion rate of barotropic to baroclinic semidiurnal tidal energy along the South Scotia Ridge, as a pathway for energy flux to the turbulent microscale, is consistent with the data-based estimates of K,. Baroclinic tides from the ridge can penetrate into the northern Weddell Sea and may explain observed significant velocity shears in the central Powell Basin, hundreds of kilometers from significant topographic features. (C) 2002 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:4843 / 4861
页数:19
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