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首页> 外文期刊>Journal of Physical Oceanography >Response of the Southern Ocean to the Southern Annular Mode: Interannual Variability and Multidecadal Trend
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Response of the Southern Ocean to the Southern Annular Mode: Interannual Variability and Multidecadal Trend

机译:南大洋对南环空模式的响应:年际变化和年代际趋势

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摘要

The authors evaluate the response of the Southern Ocean to the variability and multidecadal trend of the southern annular mode (SAM) from 1972 to 2001 in a global eddy-permitting model of the DRAKKAR project. The transport of the Antarctic Circumpolar Current (ACC) is correlated with the SAM at interannual time scales but exhibits a drift because of the thermodynamic adjustment of the model (the ACC transport decreases because of a low renewal rate of dense waters around Antarctica). The interannual variability of the eddy kinetic energy (EKE) and the ACC transport are uncorrelated, but the EKE decreases like the ACC transport over the three decades, even though meridional eddy fluxes of heat and buoyancy remain stable. The contribution of oceanic eddies to meridional transports is an important issue because a growth of the poleward eddy transport could, in theory, oppose the increase of the mean overturning circulation forced by the SAM. In the authors' model, the total meridional circulation at 50°S is well correlated with the SAM index (and the Ekman transport) at interannual time scales, and both increase over three decades between 1972 and 2001. However, given the long-term drift, no SAM-linked trend in the eddy contribution to the meridional overturning circulation is detectable. The increase of the meridional overturning is due to the time-mean component and is compensated by an increased buoyancy gain at the surface. The authors emphasize that the meridional circulation does not vary in a simple relationship with the zonal circulation. The model solution points out that the zonal circulation and the eddy kinetic energy are governed by different mechanisms according to the time scale considered (interannual or decadal).
机译:作者在DRAKKAR项目的全球涡流允许模型中,评估了1972年至2001年南大洋对南环状模式(SAM)的变异性和年代际趋势的响应。在年际尺度上,南极绕极流(ACC)的传输与SAM相关,但由于模型的热力学调整而表现出漂移(由于南极周围稠密水的更新率低,ACC的传输减少了)。涡动能(EKE)的年际变化与ACC的运输无关,但即使在子午线的热量和浮力通量保持稳定的情况下,EKE在过去的三十年中也像ACC的运输一样下降。海洋涡流对子午输运的贡献是一个重要的问题,因为从理论上说,极涡流的增长可能会反对由SAM推动的平均翻转环流的增加。在作者的模型中,在年际尺度上,50°S时的总子午环流与SAM指数(和Ekman运移)具有很好的相关性,并且在1972年至2001年的三个十年中都增加了。漂移,涡旋对子午俯仰环流的贡献没有与SAM相关的趋势。经向翻转的增加是由于时间平均分量引起的,并通过增加表面的浮力增益得到补偿。作者强调,子午环流与纬向环流没有简单的关系。模型解决方案指出,纬线环流和涡动能根据所考虑的时间尺度(年际或年代际)受不同机制控制。

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  • 来源
    《Journal of Physical Oceanography》 |2010年第7期|P.1659-1668|共10页
  • 作者单位

    Laboratoire de Physique des Oceans, CNRS-IRD-IFREMER-UBO, UMR 6523, IFREMER, BP 70, 29280 Plouzane, France LEGI, CNRS-UJF-INPG, Grenoble, France;

    rnLEGI, CNRS-UJF-INPG, Grenoble, France;

    LEGI, CNRS-UJF-INPG, Grenoble, France;

    rnNational Oceanography Centre, Southampton, Southampton, United Kingdom;

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