Impact of a fresh-core mesoscale eddy in modulating oceanic response to a Madden-Julian Oscillation

IF 2.3 3区 地球科学 Q2 OCEANOGRAPHY Deep-sea Research Part Ii-topical Studies in Oceanography Pub Date : 2024-06-11 DOI:10.1016/j.dsr2.2024.105396
Marina V.C. Azaneu , Adrian J. Matthews , Karen J. Heywood , Rob A. Hall , Dariusz B. Baranowski
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Abstract

Theories of ocean–atmosphere interaction during a Madden–Julian Oscillation (MJO) are generally based on a thermodynamic model with surface fluxes dictating changes in sea surface temperature. Evidence from a two month ocean glider deployment in early 2019 in the southeast Indian Ocean suggests the impact of mesoscale dynamics on upper-ocean stratification likely affects ocean–atmosphere interaction at MJO scales. Until mid-February, local surface fluxes consistent with a convectively suppressed MJO phase drove near-surface ocean evolution. With the advection of a fresh-core eddy to the glider location in late February, ocean dynamics then becomes an additional driver of this evolution by modulating local stratification and generating a barrier layer of ≈12 m thickness for 10 days. One-dimensional modelling experiments based on the ocean and atmospheric conditions experienced during our sampling period show that the ocean subsurface structure within the eddy induce changes in SST of physical significance for ocean-atmosphere interaction. Moreover, results also suggest that the presence of a thick eddy-induced barrier layer during the MJO suppressed phase modulates the magnitude of temperature anomalies forced by surface fluxes during the following enhanced MJO phase. As eddies are abundant in this area, their dynamics must be considered to correctly represent SST variability for MJO modelling.

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新鲜核心中尺度涡流在调节海洋对马登-朱利安涛动的响应方面的影响
马登-朱利安涛动(MJO)期间海洋-大气相互作用的理论通常基于热力学模型,即海面通量决定海面温度的变化。2019 年初在印度洋东南部部署的两个月海洋滑翔机提供的证据表明,中尺度动力学对上层海洋分层的影响可能会影响到 MJO 尺度的海洋-大气相互作用。直到 2 月中旬,与对流抑制的 MJO 相一致的局地表层通量推动了近表层海洋的演变。二月下旬,随着一个新鲜核心涡流被吸附到滑翔机所在位置,海洋动力学通过调节局部分层和生成厚度≈12 米的阻挡层,成为这种演变的额外驱动力,持续了 10 天。根据取样期间的海洋和大气条件进行的一维模拟实验表明,漩涡内的海洋次表层结构引起了海温的变化,对海洋-大气相互作用具有重要的物理意义。此外,研究结果还表明,在 MJO 受抑制的阶段,漩涡引起的厚阻挡层的存在会调节在随后的 MJO 增强阶段由地表通量引起的温度异常的幅度。由于该地区存在大量涡,因此必须考虑它们的动态变化,以便在模拟 MJO 时正确反映 SST 的变化。
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来源期刊
CiteScore
6.40
自引率
16.70%
发文量
115
审稿时长
3 months
期刊介绍: Deep-Sea Research Part II: Topical Studies in Oceanography publishes topical issues from the many international and interdisciplinary projects which are undertaken in oceanography. Besides these special issues from projects, the journal publishes collections of papers presented at conferences. The special issues regularly have electronic annexes of non-text material (numerical data, images, images, video, etc.) which are published with the special issues in ScienceDirect. Deep-Sea Research Part II was split off as a separate journal devoted to topical issues in 1993. Its companion journal Deep-Sea Research Part I: Oceanographic Research Papers, publishes the regular research papers in this area.
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