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    Turbulence and Diapycnal Mixing in Drake Passage

    Source: Journal of Physical Oceanography:;2012:;Volume( 042 ):;issue: 012::page 2143
    Author:
    St. Laurent, L.
    ,
    Naveira Garabato, A. C.
    ,
    Ledwell, J. R.
    ,
    Thurnherr, A. M.
    ,
    Toole, J. M.
    ,
    Watson, A. J.
    DOI: 10.1175/JPO-D-12-027.1
    Publisher: American Meteorological Society
    Abstract: irect 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 ? 10?4 m2 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.
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      Turbulence and Diapycnal Mixing in Drake Passage

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    contributor authorSt. Laurent, L.
    contributor authorNaveira Garabato, A. C.
    contributor authorLedwell, J. R.
    contributor authorThurnherr, A. M.
    contributor authorToole, J. M.
    contributor authorWatson, A. J.
    date accessioned2017-06-09T17:19:49Z
    date available2017-06-09T17:19:49Z
    date copyright2012/12/01
    date issued2012
    identifier issn0022-3670
    identifier otherams-83293.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4226502
    description abstractirect 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 ? 10?4 m2 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.
    publisherAmerican Meteorological Society
    titleTurbulence and Diapycnal Mixing in Drake Passage
    typeJournal Paper
    journal volume42
    journal issue12
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/JPO-D-12-027.1
    journal fristpage2143
    journal lastpage2152
    treeJournal of Physical Oceanography:;2012:;Volume( 042 ):;issue: 012
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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