High mixing rates in the abyssal Southern Ocean

被引:91
作者
Heywood, KJ [1 ]
Garabato, ACN
Stevens, DP
机构
[1] Univ E Anglia, Sch Environm Sci, Norwich NR4 7TJ, Norfolk, England
[2] Univ E Anglia, Sch Math, Norwich NR4 7TJ, Norfolk, England
基金
澳大利亚研究理事会; 英国自然环境研究理事会;
关键词
D O I
10.1038/4151011a
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Mixing of water masses from the deep ocean to the layers above can be estimated from considerations of continuity in the global ocean overturning circulation(1-3). But averaged over ocean basins, diffusivity has been observed to be too small(4-12) to account for the global upward flux of water, and high mixing intensities have only been found in the restricted areas close to sills and narrow gaps(10,11,13-15). Here we present observations from the Scotia Sea, a deep ocean basin between the Antarctic peninsula and the tip of South America, showing a high intensity of mixing that is unprecedented over such a large area. Using a budget calculation over the whole basin, we find a diffusivity of (39 +/- 10) x 10(4) m(2) s(-1), averaged over an area of 7 x 10(5) km(2). The Scotia Sea is a basin with a rough topography(16), situated just east of the Drake passage where the strong flow of the Antarctic Circumpolar Current is constricted in width. The high basin-wide mixing intensity in this area of the Southern Ocean may help resolve the question of where the abyssal water masses are mixed towards the surface.
引用
收藏
页码:1011 / 1014
页数:4
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