Flows in horizontal thermohaline convection with differential diffusion

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2021-03-02 DOI:10.1080/03091929.2021.1888375
J. A. Whitehead
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Abstract

Oceanographers use the term “differential diffusion” to express a greater value of bulk turbulent diffusivity of temperature within the ocean than the value of bulk diffusivity of salinity, the ratio quantified by Lewis number. Investigation of horizontal thermohaline convection at Prandtl number 1 and infinity over the range reveals a variety of new flow patterns. The chamber has a linearly changing temperature T and salinity S along the top extending from the cold, fresh “polar” end to the hot, salty “tropics” end. It has an aspect ratio of 8 and sides and bottom are insulated and impermeable. Five transition flow patterns occur with little hysteresis for a fixed salinity Rayleigh number Ras of order 105 as Rayleigh number Ra changes from 3.2 × 106 down to 1. They are: 1. A steady T-cell with sinking at the cold end flowing into a bottom flow that feeds up into a top thermal boundary layer. 2. Salty blobs in the boundary layer that amplify and move from the hot to cold end. Each cold end arrival triggers a sudden increase in overturning velocity. 3. A “stripes” pattern where top to bottom cells (alternating T and S cells) move toward the cold end. 4. An S-cell that is a mirror image of the T-cell near the top along with small T-cells lying at the bottom that move toward the cold end 5. A steady S-cell. Each pattern has a distinct volumetric signature in a T-S diagram. Ranges of Ra with various patterns are sizeable at Ras=7.5 × 105 if Le >4/3 but insensitive to Pr. Balanced convection at Ra = Ras >106 adopts a large unsteady supercell containing smaller T and S cells. Exact ranges of the supercell are unknown. Since differential diffusion produces a large collection of flows compared to thermal convection alone, it might produce unexpected new results if added into numerical models of the ocean.
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具有微分扩散的水平温盐对流中的流动
海洋学家使用“差分扩散”一词来表示海洋内温度的体积湍流扩散系数大于盐度的体积扩散系数,后者是由刘易斯数量化的比率。在普朗特数1和无穷远处对水平温盐对流的研究揭示了多种新的流动模式。这个腔室的温度T和盐度S沿顶部呈线性变化,从寒冷、新鲜的“极地”一端延伸到炎热、咸的“热带”一端。它的长宽比为8,侧面和底部是绝缘和不透水的。在固定盐度条件下,瑞利数Ra为105阶时,瑞利数Ra从3.2 × 106降至1,出现了5种过渡流型,滞后性很小。它们是:1;一个稳定的t细胞,在冷端下沉,流入底部,流入顶部热边界层。2. 边界层中的含盐斑点放大并从热端向冷端移动。每次冷端到达都会引起倾覆速度的突然增加。3.从上到下的细胞(T细胞和S细胞交替)向冷端移动的“条纹”模式。4. 一种s细胞,它是靠近顶部的t细胞的镜像,位于底部的小t细胞向冷端移动。一个稳定的s型电池。每种模式在T-S图中都有不同的体积特征。在Ra =7.5 × 105处,当Le >4/3时,Ra的变化范围较大,但对Pr不敏感。在Ra = Ras >106处,平衡对流采用包含较小T胞和S胞的大型非定常超级单体。超级单体的确切范围尚不清楚。由于与单独的热对流相比,微分扩散产生了大量的流动,如果将其添加到海洋的数值模型中,可能会产生意想不到的新结果。
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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