On the Ambiguity of Oceanic Eddy Polarity

IF 3.3 2区 地球科学 Q1 OCEANOGRAPHY
Ge Chen, Xiaoyan Chen
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Abstract

Polarity is a fundamental feature of oceanic eddies, which defines many aspects of its hydrodynamics and thermodynamics. Polarity ambiguity is a challenging and sometimes puzzling issue for the classification of eddies and analysis of their dynamics. Here, we propose a new methodology combining drifter-measured currents and temperatures to evaluate the validity of altimeter-derived eddy polarity. Different from previous schemes based purely on assessing oceanic temperature ambiguity of eddies from either satellite or Argo observations, our approach integrates the concurrent vector flow and surface temperature measured by drifters riding on altimeter-tracked eddies. The idea is to examine the consistency between the rotation of drifter trajectory and the spinning of eddy motion on the assumption that the looping and circulating directions are identical for a normal eddy and otherwise for an “ambiguous” or “abnormal” one. For a special class of radial drifter trajectory with respect to the eddy centroid, the temperature trend along its path is used to judge its polarity, that is, warmer toward the core for a normal anticyclonic eddy and colder for cyclonic. Our results reveal that many eddies previously classified as “abnormal” are in fact dynamically or thermally ambiguous due to distortions in their upper-layer structures rather than being genuinely misclassified by altimeter. After excluding such ambiguous cases, only ∼3% of eddies show polarity inconsistency in both aspects. These findings suggest that altimeter-derived eddy polarity is highly reliable, and that combining a multi-parameter, Lagrangian-informed approach offers more accurate interpretations of eddy structures by distinguishing intrinsic anomalies from superficial distortions.

Abstract Image

论海洋涡旋极性的模糊性
极性是海洋涡旋的一个基本特征,它决定了海洋涡旋流体力学和热力学的许多方面。极性模糊是涡流分类和涡流动力学分析的一个难题。在这里,我们提出了一种结合漂移测量电流和温度的新方法来评估高度计导出的涡极性的有效性。与以往单纯基于卫星或Argo观测结果评估海洋涡旋温度模糊度的方案不同,我们的方法整合了由乘坐高度计跟踪的涡旋的漂流者测量的同步矢量流和表面温度。这个想法是在假设正常涡流和“模糊”或“异常”涡流的循环和循环方向相同的情况下,检查漂移轨迹的旋转和涡流运动的旋转之间的一致性。对于一类特殊的相对于涡旋质心的径向漂移轨迹,利用其路径上的温度趋势来判断其极性,即正常反气旋涡旋向中心偏暖,气旋涡旋向中心偏冷。我们的研究结果表明,许多以前被归类为“异常”的涡旋实际上是由于其上层结构的扭曲而在动态或热上模糊不清,而不是真正被高度计错误分类。在排除这种模棱两可的情况后,只有~ 3%的涡流在两个方面都表现出极性不一致。这些发现表明,高度计导出的涡旋极性是高度可靠的,结合多参数、拉格朗日信息方法,通过区分内在异常和表面扭曲,可以更准确地解释涡旋结构。
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来源期刊
Journal of Geophysical Research-Oceans
Journal of Geophysical Research-Oceans Earth and Planetary Sciences-Oceanography
CiteScore
7.00
自引率
13.90%
发文量
429
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