Beaufort Gyre Isopycnal Structure Produces a Steady Mesoscale Eddy Field Modulated by Sea Ice Drag

IF 3.4 2区 地球科学 Q1 OCEANOGRAPHY
Hassan Mason, K. Shafer Smith
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Abstract

The Beaufort Gyre (BG) mean state is set by a balance between surface wind stress, sea ice, and subsurface eddy transport. This study addresses the existence and generation of the eddies. We show that underice baroclinic instability of the observed BG mean state produces an eddy field that is both consistent with observations and sufficient to maintain the mean state. We use high-resolution simulations forced by the BG mean state to spin up a steady eddy field. The model includes a representation of sea ice with active rheology but inactive thermodynamics. Each simulation is initialized with different sea ice concentrations that remain constant throughout each integration, thus imparting varying amounts of surface drag. We find that these simulations are characterized by two regimes: a static ice regime with strong surface drag and a motile ice regime with low surface drag. Simulations in the motile ice simulations exhibit high eddy energy with near-surface maximum eddy velocities of about 30 $30\,$ cm s−1 and eddy diffusivities of about 4000 $4000\,$ m2 s−1. Eddy energy is lower in the static ice regime but nevertheless maintains significant strength at the halocline depth (150 m) with eddy velocity maxima exceeding 10 $10\,$ cm s−1. Eddy diffusivity under static ice ( O 1000 $\mathcal{O}\left(1000\,\right.$ m2 s−1)) peaks just below the surface and decays with depth, which is consistent with the upper end of previous analyses. This work both suggests the presence of locally generated halocline-intensified eddies and provides insight into the future behavior of the BG as we slowly transition to an ice-free Arctic.

Abstract Image

波弗特环流等平结构在海冰阻力调制下产生稳定的中尺度涡旋场
波弗特环流(BG)的平均状态是由地面风应力、海冰和地下涡旋输送三者之间的平衡决定的。本研究探讨了涡旋的存在和产生。我们发现观测到的冰下斜压不稳定的BG平均状态产生了一个涡场,该涡场既与观测一致,又足以维持平均状态。我们使用高分辨率模拟,迫使BG平均状态旋转一个稳定的涡流场。该模型包括具有活跃流变学但不具有活跃热力学的海冰的表示。每个模拟初始化时都使用不同的海冰浓度,这些浓度在每次整合过程中保持不变,从而产生不同的表面阻力。我们发现这些模拟具有两种状态:具有强表面阻力的静态冰状态和具有低表面阻力的运动冰状态。在移动冰模拟中显示出高涡能,近地表最大涡速度约为30 $30\,$ cm s - 1,涡扩散系数约为4000 $4000\,$ m2 s - 1。静冰状态下涡旋能量较低,但在盐斜深度(150 m)处仍保持显著强度,涡旋速度最大值超过10 $10\,$ cm s - 1。静态冰下的涡流扩散率(O 1000 $\mathcal{O}\left(1000\,\right)。$ m2 s−1))在表面以下达到峰值,并随深度衰减,这与先前分析的上端一致。这项工作既表明了局部产生的盐温增强涡流的存在,也为我们慢慢过渡到无冰北极时BG的未来行为提供了洞见。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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