首页> 外文期刊>Journal of Advances in Modeling Earth Systems >Ocean Kinetic Energy Backscatter Parametrization on Unstructured Grids: Impact on Global Eddy‐Permitting Simulations
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Ocean Kinetic Energy Backscatter Parametrization on Unstructured Grids: Impact on Global Eddy‐Permitting Simulations

机译:非结构化网格的海洋动能反向散射参数化:对全球涡流模拟的影响

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In this study we demonstrate the potential of a kinetic energy backscatter scheme for use in global ocean simulations. Ocean models commonly employ (bi)harmonic eddy viscosities causing excessive dissipation of kinetic energy in eddy‐permitting simulations. Overdissipation not only affects the smallest resolved scales but also the generation of eddies through baroclinic instabilities, impacting the entire wave number spectrum. The backscatter scheme returns part of this overdissipated energy back into the resolved flow. We employ backscatter in the FESOM2 multiresolution ocean model with a quasi‐uniform 1/4° mesh. In multidecadal ocean simulations, backscatter increases eddy activity by a factor 2 or more, moving the simulation closer to observational estimates of sea surface height variability. Moreover, mean sea surface height, temperature, and salinity biases are reduced. This amounts to a globally averaged bias reduction of around 10% for each field, which is even larger in the Antarctic Circumpolar Current. However, in some regions such as the coastal Kuroshio, backscatter leads to a slight overenergizing of the flow and, in the Antarctic, to an unrealistic reduction of sea ice. Some of the bias increases can be reduced by a retuning of the model, and we suggest related adjustments to the backscatter scheme. The backscatter simulation is about 2.5 times as expensive as a simulation without backscatter. Most of the increased cost is due to a halving of the time step to accommodate higher simulated velocities. Plain Language Summary The weather of the oceans is determined by so‐called mesoscale eddies, which carry a large portion of the kinetic energy of ocean currents. They are responsible for the transport of heat and dissolved substances; they can affect the large and fast mean currents of the ocean and interact strongly with the atmosphere above. However, these eddies are not well represented in current ocean and climate models. With this study, we apply a new method to better represent the effect of ocean weather in ocean models. We show that this leads to improvements of the simulation of ocean currents and their variability and reduces biases in ocean temperatures and salinity. While increasing the resolution of ocean models also helps to improve the representation of mesoscale eddies, such a resolution increase is computationally expensive. The new backscatter parametrization can help to save computational costs by allowing improved eddy simulations comparable to much higher resolution.
机译:在这项研究中,我们展示了在全球海洋模拟中使用的动能反散射方案的潜力。海洋模型通常采用(Bi)谐波涡粘度,导致涡旋允许模拟中的动能过度耗散。过度减少不仅影响最小的解决方案,还影响了通过曲金属稳定性产生的漩涡,影响整个波数谱。反向散射方案将该部分超越能量返回回已解决的流量。我们在FESOM2多分辨率海洋模型中使用反向散射,用准均匀1/4°网格。在多型海洋模拟中,反向散射将涡拍活动增加了2或更多的因素,使模拟更接近海面高度可变性的观察估计。此外,平均平均海表面高度,温度和盐度偏差减小。对于每个场的全局平均偏差约为10%,其在南极循环电流中甚至更大。然而,在沿海Kuroshio的一些地区,反向散射导致流动的略微过度过度,并且在南极地区的海冰减少不切实际。通过对模型的重新定期,可以减少一些偏差增加,我们建议对后散射方案相关的调整。反向散射仿真在没有反向散射的情况下昂贵约2.5倍。大多数增加的成本是由于减半,以适应更高的模拟速度。普通语言摘要海洋的天气由所谓的Mesoscale Eddies确定,该漩涡漩涡师将大部分是海洋电流的大部分动能。他们负责运输热量和溶解物质;它们可以影响海洋的大且快速平均电流,并在上面的大气中强烈地相互作用。然而,这些漩涡在当前的海洋和气候模型中没有很好地代表。通过这项研究,我们应用一种新方法以更好地代表海洋天气在海洋模型中的影响。我们表明,这导致了洋流模拟的改进及其变异性,并减少了海洋温度和盐度的偏差。虽然增加海洋模型的分辨率也有助于改善Messcale Eddies的代表性,但这种分辨率的增加是计算昂贵的。新的后散射参数化可以帮助通过允许改进的涡流模拟与更高的分辨率相当的涡流模拟来节省计算成本。

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