Angular momentum transfer in direct numerical simulations of a laboratory model of a tropical cyclone

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2022-05-04 DOI:10.1080/03091929.2022.2066659
A. Evgrafova, A. Sukhanovskii
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引用次数: 2

Abstract

ABSTRACT Numerical simulations of a laboratory model of a tropical cyclone are carried out for different rotation rates. Particular attention is paid to the non-stationary stage of intensive cyclonic vortex formation. The transfer of angular momentum plays a key role in the formation of cyclonic and anticyclonic flows; therefore, a detailed analysis of the redistribution and variation of angular momentum is given. The time evolution of angular momentum fluxes and total angular momentum strongly depend on the rotation rate. It is shown that intensive cyclonic motion with velocity exceeding initial values substantially (ten or more times) is a result of accumulation in the centre of a small fraction of global angular momentum of a fluid layer (from 0.25% at fast rotation to 2% at slow rotation). The integral angular momentum of the anticyclonic flow is significantly larger than that of the cyclonic flow, mainly because of the relatively large fluid volume of the anticyclonic flow. Another important result is that the rotating fluid layer very quickly adapts to new boundary conditions (heating and cooling). Approximately two rotation periods are required to reach a quasi-stationary state. The application of the obtained results to the evolution of real tropical cyclones is discussed.
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热带气旋实验室模式直接数值模拟中的角动量传递
本文对一个热带气旋实验室模型进行了不同旋转速率下的数值模拟。特别注意了强气旋涡旋形成的非平稳阶段。角动量的传递在气旋和反气旋流的形成中起着关键作用;因此,详细分析了角动量的重分布和变化。角动量通量和总角动量的时间演化强烈依赖于旋转速率。结果表明,速度大大超过初始值(10倍或更多)的强烈气旋运动是流体层整体角动量的一小部分(从快旋转时的0.25%到慢旋转时的2%)在中心积聚的结果。反气旋流的积分角动量明显大于气旋流,这主要是由于反气旋流的流体体积相对较大。另一个重要的结果是,旋转的流体层非常迅速地适应新的边界条件(加热和冷却)。大约需要两个旋转周期才能达到准静止状态。讨论了所得结果在实际热带气旋演化中的应用。
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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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