A physical–statistical recipe for representation of small-scale oceanic turbulent mixing in climate models

IF 2.8 Q2 MECHANICS Flow (Cambridge, England) Pub Date : 2022-08-22 DOI:10.1017/flo.2022.16
A. Mashayek, B. Cael, L. Cimoli, M. Alford, C. Caulfield
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引用次数: 3

Abstract

Abstract It is well established that small-scale cross-density (diapycnal) turbulent mixing induced by breaking of overturns in the interior of the ocean plays a significant role in sustaining the deep ocean circulation and in regulating tracer budgets such as those of heat, carbon and nutrients. There has been significant progress in the fluid mechanical understanding of the physics of breaking internal waves. Connection of the microphysics of such turbulence to the larger scale dynamics, however, is significantly underdeveloped. We offer a hybrid theoretical–statistical approach, informed by observations, to make such a link. By doing so, we define a bulk flux coefficient, $\varGamma _B$, which represents the partitioning of energy available to an ‘ocean box’ (such as a grid cell of a coarse resolution climate model), from winds, tides, and other sources, into mixing and dissipation. Here, $\varGamma _B$ depends on both the statistical distribution of turbulent patches and the flux coefficient associated with individual patches, $\varGamma _i$. We rely on recent parametrizations of $\varGamma _i$ and the seeming universal characteristics of statistics of turbulent patches to infer $\varGamma _B$, which is the essential quantity for representation of turbulent diffusivity in climate models. By applying our approach to climatology and global tidal estimates, we show that, on a basin scale, energetic mixing zones exhibit moderately efficient mixing that induces significant vertical density fluxes, while quiet zones (with small background turbulence levels), although highly efficient in mixing, exhibit minimal vertical fluxes. The transition between the less energetic to more energetic zones marks regions of intense upwelling and downwelling of deep waters. We suggest that such upwelling and downwelling may be stronger than previously estimated, which in turn has direct implications for the closure of the deep branch of the ocean meridional overturning circulation as well as for the associated tracer budgets.
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气候模型中表示小规模海洋湍流混合的物理-统计配方
摘要海洋内部倾覆破碎引起的小尺度交叉密度湍流混合在维持深海环流和调节热量、碳和养分等示踪剂收支方面发挥着重要作用。对破碎内波的物理性质的流体力学理解已经取得了重大进展。然而,这种湍流的微观物理学与更大尺度动力学的联系还很不发达。我们提供了一种混合的理论-统计方法,通过观察来建立这种联系。通过这样做,我们定义了一个体积通量系数$\varGamma _B$,它表示“海洋箱”(如粗分辨率气候模式的网格单元)从风、潮汐和其他来源获得的能量分配为混合和耗散。这里,$\varGamma _B$取决于湍流斑块的统计分布和与单个斑块相关的通量系数$\varGamma _i$。我们依靠最近的参数化$\varGamma _i$和湍流斑块统计的看似普遍的特征来推断$\varGamma _B$,这是表征气候模式中湍流扩散率的基本量。通过将我们的方法应用于气候学和全球潮汐估计,我们表明,在盆地尺度上,能量混合区表现出中等效率的混合,引起显著的垂直密度通量,而安静区(具有小背景湍流水平)虽然混合效率很高,但表现出最小的垂直通量。能量较低的区域和能量较高的区域之间的过渡标志着深水的强烈上升流和下升流。我们认为,这种上升流和下升流可能比以前估计的更强,这反过来对海洋经向翻转环流的深部分支的关闭以及相关的示踪剂预算有直接影响。
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2.40
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