{"title":"Eddy acceleration and decay driven by internal tides","authors":"Callum J. Shakespeare","doi":"10.1175/jpo-d-23-0127.1","DOIUrl":null,"url":null,"abstract":"Abstract Recent observations and numerical simulations have demonstrated the potential for significant interactions between mesoscale eddies and smaller-scale tidally generated internal waves — also known as internal tides. Here we develop a simple theoretical model that predicts the one-way upscale transfer of energy from internal tides to mesoscale eddies through a critical level mechanism. We find that — in the presence of a critical level — the internal tide energy flux into an eddy is partitioned according to the wave frequency Ω and local inertial frequency f : a fraction of 1 – f /Ω is transferred to the eddy kinetic energy while the remainder is viscously dissipated or supports mixing. These predictions are validated by comparison with a suite of numerical simulations. The simulations further show that the wave-driven energisation of the eddies also accelerates the onset of hydrodynamical instabilities and the break down of the eddies, thereby increasing eddy kinetic energy, but reducing eddy lifetimes. Our estimates suggest that in regions of the ocean with both significant eddy fields and internal tides—such as parts of the Gulf Stream and Antarctic Circumpolar Current—the critical level effect could drive a ∼10% per month increase in the kinetic energy of a typical eddy. Our results provide a basis for parameterising internal tide-eddy interactions in global ocean models where they are currently unrepresented.","PeriodicalId":56115,"journal":{"name":"Journal of Physical Oceanography","volume":"6 1","pages":"0"},"PeriodicalIF":2.8000,"publicationDate":"2023-10-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Physical Oceanography","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1175/jpo-d-23-0127.1","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"OCEANOGRAPHY","Score":null,"Total":0}
引用次数: 0
Abstract
Abstract Recent observations and numerical simulations have demonstrated the potential for significant interactions between mesoscale eddies and smaller-scale tidally generated internal waves — also known as internal tides. Here we develop a simple theoretical model that predicts the one-way upscale transfer of energy from internal tides to mesoscale eddies through a critical level mechanism. We find that — in the presence of a critical level — the internal tide energy flux into an eddy is partitioned according to the wave frequency Ω and local inertial frequency f : a fraction of 1 – f /Ω is transferred to the eddy kinetic energy while the remainder is viscously dissipated or supports mixing. These predictions are validated by comparison with a suite of numerical simulations. The simulations further show that the wave-driven energisation of the eddies also accelerates the onset of hydrodynamical instabilities and the break down of the eddies, thereby increasing eddy kinetic energy, but reducing eddy lifetimes. Our estimates suggest that in regions of the ocean with both significant eddy fields and internal tides—such as parts of the Gulf Stream and Antarctic Circumpolar Current—the critical level effect could drive a ∼10% per month increase in the kinetic energy of a typical eddy. Our results provide a basis for parameterising internal tide-eddy interactions in global ocean models where they are currently unrepresented.
最近的观测和数值模拟表明,中尺度涡旋和较小尺度潮汐产生的内波(也称为内潮)之间可能存在显著的相互作用。在这里,我们建立了一个简单的理论模型,预测能量通过一个临界水平机制从内部潮汐向中尺度漩涡的单向高级转移。我们发现,在存在临界水平时,进入涡流的内部潮汐能量通量根据波频率Ω和局部惯性频率f进行了划分:1 - f /Ω的一小部分被转移到涡流动能中,而其余部分则被粘性耗散或支持混合。这些预测通过与一系列数值模拟的比较得到了验证。模拟进一步表明,波浪驱动的涡流能量也加速了流体动力不稳定性的发生和涡流的破裂,从而增加了涡流动能,但减少了涡流寿命。我们的估计表明,在具有显著涡旋场和内部潮汐的海洋区域,如墨西哥湾流和南极环极流的部分地区,临界水平效应可以使典型涡旋的动能每月增加约10%。我们的研究结果为参数化全球海洋模型中的内部潮汐-涡流相互作用提供了基础,而这些模型目前还没有得到代表。
期刊介绍:
The Journal of Physical Oceanography (JPO) (ISSN: 0022-3670; eISSN: 1520-0485) publishes research related to the physics of the ocean and to processes operating at its boundaries. Observational, theoretical, and modeling studies are all welcome, especially those that focus on elucidating specific physical processes. Papers that investigate interactions with other components of the Earth system (e.g., ocean–atmosphere, physical–biological, and physical–chemical interactions) as well as studies of other fluid systems (e.g., lakes and laboratory tanks) are also invited, as long as their focus is on understanding the ocean or its role in the Earth system.