On the dynamics of an idealised bottom density current overflowing in a semi-enclosed basin: mesoscale and submesoscale eddies generation

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-04-08 DOI:10.1080/03091929.2020.1747058
Mathieu Morvan, X. Carton, P. L’Hégaret, Charly de Marez, Stéphanie Corréard, S. Louazel
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引用次数: 4

Abstract

The Red Sea Water enters the Gulf of Aden through the Strait of Bab El Mandeb as a density current. The Red Sea Water subsequently spreads into the Gulf of Aden under the influence of surface mesoscale eddies, which dominate the surface flow, of topographic features such as rift and capes, and of the monsoon regimes. The dynamics of a bottom density current overflowing in a semi-enclosed basin, as the Red Sea Water outflows in the Gulf of Aden, is investigated by performing idealised numerical simulations, at submesoscale resolution, in which we progressively add topographic and dynamical elements. The rift and cape play an important role, respectively, on the vertical and the horizontal mixing as well as baroclinic and barotropic instabilities undergone by the bottom density current. Mesoscale and submesoscale eddies are generated depending on the model configuration. In the presence of surface mesoscale eddies, the bottom density current water is mainly advected at their periphery. In winter, both mesoscale and submesoscale eddies are generated, while in summer only submesoscale eddies are present. Finally, to put our results based on idealised numerical simulations and Lagrangian experiments in perspective, we analyse the trajectories of three Argo floats, deployed in the Rift of Tadjurah. Clues of submesoscale eddies generation at capes are observed which is in agreement with our idealised numerical simulations.
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半封闭盆地中溢流的理想底密度动力学:中尺度和亚中尺度涡旋的产生
红海的水以密度流的形式通过曼德海峡进入亚丁湾。红海的水随后在地表中尺度涡流的影响下流入亚丁湾,这些涡流主导着地表水流,地形特征如裂谷和海角,以及季风的影响。在亚中尺度分辨率下,我们逐步添加地形和动力因素,通过理想化的数值模拟,研究了亚丁湾红海水流出时,半封闭盆地中底密度流溢出的动力学。裂谷和角分别对海底密度流的垂直和水平混合以及斜压和正压不稳定起着重要作用。中尺度和亚中尺度涡旋的产生取决于模式的配置。地表中尺度涡旋存在时,底密度流水主要在涡旋周边平流。冬季有中尺度和亚中尺度涡旋,夏季有亚中尺度涡旋。最后,为了让我们的结果基于理想化的数值模拟和拉格朗日实验,我们分析了部署在塔朱拉裂谷的三个Argo浮标的轨迹。在海角观测到亚中尺度涡旋产生的线索,这与我们的理想数值模拟结果一致。
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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