Preprints
https://doi.org/10.22541/essoar.170158288.87102456/v2
https://doi.org/10.22541/essoar.170158288.87102456/v2
25 Mar 2025
 | 25 Mar 2025
Status: this preprint is open for discussion and under review for Ocean Science (OS).

Insights Into Mesoscale Eddy Dynamics: A Three-Dimensional Perspective on Potential Density Anomalies

Yan Barabinot, Sabrina Speich, and Xavier Carton

Abstract. Mesoscale eddies are fundamental components of global ocean circulation. In situ observations and Lagrangian analyses have shown that most eddies are materially coherent, transporting a water mass within their core that differs from the surrounding environment. Additionally, laboratory experiments indicate that eddies locally modify stratification in accordance with thermal wind balance, regardless of whether they trap a water mass. These two mechanisms drive, respectively, spiciness mode anomalies and heaving mode anomalies associated with mesoscale eddies. In this study, aiming to quantitatively assess the physical processes governing mesoscale eddy dynamics, we introduce a novel theoretical decomposition of the potential density field within eddy cores to account for both effects. This framework is applied to six anticyclonic eddies sampled during the EUREC4A-OA, METEOR 124, and Physindien 2011 oceanographic campaigns. Unlike previous studies, we evaluate not only the amplitude of these anomalies but also their vertical structure. Our results confirm that heaving mode anomalies dominate the total density anomaly. However, in contrast to previous assumptions, we demonstrate that their vertical structure is dictated by the local background stratification and often follows a nearly Gaussian profile. Meanwhile, spiciness anomalies provide only a second-order contribution to the total potential density anomaly, rendering them negligible in most dynamical processes governing mesoscale eddies. By bridging experimental results with observational eddy datasets, this study refines our understanding of mesoscale eddy vertical structure, offering a more accurate predictive framework for their shape and role in oceanic property transport.

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Yan Barabinot, Sabrina Speich, and Xavier Carton

Status: open (until 20 May 2025)

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Yan Barabinot, Sabrina Speich, and Xavier Carton

Data sets

Concatenated Temperature, Salinity, and Velocity measurements from EUREC4A_OA/ATOMIC Pierre L'Hégaret et al. https://doi.org/10.17882/92071

AtlantOS data products from multibeam EM122 data: METEOR cruise M124 (Atlantic) Anne-Cathrin Wölfl and Martin Schade https://doi.org/10.1594/PANGAEA.902947

Physical oceanography during METEOR cruise M124 Johannes Karstensen and Gerd Krahmann https://doi.org/10.1594/PANGAEA.863015

Raw multibeam EM122 data: METEOR cruise M124 (SE Atlantic) Johannes Karstensen and Anne-Cathrin Wölfl https://doi.org/10.1594/PANGAEA.869740

Physindien 2011 Seasoar measurements Pierre L'Hégaret and Xavier Carton https://doi.org/10.17882/77351

Yan Barabinot, Sabrina Speich, and Xavier Carton

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Short summary
Mesoscale eddies, characterized by rotating currents, are ubiquitous in the ocean. However, their three-dimensional structure remains poorly observed and analyzed, with transport estimates often relying on approximations. To better quantify their shape, we propose a new theoretical framework based on geophysical fluid dynamics and apply it to field observations.
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