Ocean 2D eddy energy fluxes from small mesoscale processes with SWOT

IF 4.1 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES
Elisa Carli, Rosemary Morrow, Oscar Vergara, Robin Chevrier, Lionel Renault
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Abstract

Abstract. We investigate ocean dynamics at different scales in the Agulhas Current system, a region of important interocean exchange of heat and energy. While ocean observations and some of the most advanced climate models capture the larger mesoscale dynamics (> 100 km), the smaller-scale fronts and eddies are underrepresented. The recently launched NASA–CNES Surface Water and Ocean Topography (SWOT) wide-swath altimeter mission observes the smaller ocean geostrophic scales down to 15 km in wavelength globally. Here we will analyse different eddy diagnostics in the Agulhas Current region and quantify the contributions from the larger mesoscales observable today and the smaller scales to be observed with SWOT. Surface geostrophic diagnostics of eddy kinetic energy, strain, and energy cascades are estimated from modelled sea surface height (SSH) fields of the Massachusetts Institute of Technology general circulation model (MITgcm) latitude–longitude polar cap (LLC4320) simulation subsampled at 1/10∘. In this region, the smaller scales (<150 km) have a strong signature on the horizontal geostrophic strain rate and for all eddy diagnostics in the Western Boundary Current and along the meandering Agulhas Extension. We investigate the horizontal cascade of energy using a coarse-graining technique, and we observe that the wavelength range where the inverse cascade occurs is biased towards larger mesoscale wavelengths with today’s altimetric sampling. We also calculate the projected sampling of the eddy diagnostics under the SWOT swaths built with the NASA–CNES simulator to include the satellite position and realistic noise. For the swaths, a neural network noise mitigation method is implemented to reduce the residual SWOT random error before calculating eddy diagnostics. In terms of SSH, observable wavelengths of 15 to 20 km are retrieved after neural network noise mitigation, as opposed to wavelengths larger than 40 km before the noise reduction.
基于SWOT的小中尺度过程海洋二维涡旋能量通量
摘要我们研究了阿古拉斯海流系统在不同尺度上的海洋动力学,这是一个重要的海洋间热量和能量交换区域。虽然海洋观测和一些最先进的气候模式捕捉到了更大的中尺度动力学(>100公里),较小尺度的锋面和涡流较少。最近发射的NASA-CNES地表水和海洋地形(SWOT)宽波段高度计任务在全球范围内观测到较小的海洋地转尺度,波长降至15公里。在这里,我们将分析阿古拉斯海流地区的不同涡旋诊断,并量化今天可观察到的较大中尺度和用SWOT观察到的较小尺度的贡献。根据麻省理工学院一般环流模式(MITgcm)模拟的海面高度(SSH)场,在1/10°下采样纬度-经纬度极帽(LLC4320),估算了涡旋动能、应变和能量级联的地表地转诊断。在该地区,较小尺度(<150 km)对水平地转应变率和西边界流和蜿蜒的阿古拉斯伸展带的所有涡动诊断都有很强的特征。我们使用粗粒化技术研究了能量的水平级联,我们观察到,在今天的测高采样中,发生逆级联的波长范围偏向于较大的中尺度波长。我们还计算了在NASA-CNES模拟器构建的SWOT图下涡流诊断的投影采样,以包括卫星位置和实际噪声。在计算涡旋诊断前,采用神经网络降噪方法降低SWOT随机误差。就SSH而言,在神经网络降噪之后,可观测波长为15至20公里,而在降噪之前,可观测波长大于40公里。
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来源期刊
Ocean Science
Ocean Science 地学-海洋学
CiteScore
5.90
自引率
6.20%
发文量
78
审稿时长
6-12 weeks
期刊介绍: Ocean Science (OS) is a not-for-profit international open-access scientific journal dedicated to the publication and discussion of research articles, short communications, and review papers on all aspects of ocean science: experimental, theoretical, and laboratory. The primary objective is to publish a very high-quality scientific journal with free Internet-based access for researchers and other interested people throughout the world. Electronic submission of articles is used to keep publication costs to a minimum. The costs will be covered by a moderate per-page charge paid by the authors. The peer-review process also makes use of the Internet. It includes an 8-week online discussion period with the original submitted manuscript and all comments. If accepted, the final revised paper will be published online. Ocean Science covers the following fields: ocean physics (i.e. ocean structure, circulation, tides, and internal waves); ocean chemistry; biological oceanography; air–sea interactions; ocean models – physical, chemical, biological, and biochemical; coastal and shelf edge processes; paleooceanography.
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