Eddy saturation in a reduced two-level model of the atmosphere

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2021-07-13 DOI:10.1080/03091929.2021.1990912
Melanie Kobras, M. Ambaum, V. Lucarini
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引用次数: 1

Abstract

Eddy saturation describes the nonlinear mechanism in geophysical flows whereby, when average conditions are considered, direct forcing of the zonal flow increases the eddy kinetic energy, while the energy associated with the zonal flow does not increase. Here, we present a minimal baroclinic model that exhibits complete eddy saturation. Starting from Phillips' classical quasi-geostrophic two-level model on the beta channel of the mid-latitudes, we derive a reduced order model comprising of six ordinary differential equations including parameterised eddies. This model features two physically realisable steady state solutions, one a purely zonal flow and one where, additionally, finite eddy motions are present. As the baroclinic forcing in the form of diabatic heating is increased, the zonal solution loses stability and the eddy solution becomes attracting. After this bifurcation, the zonal components of the solution are independent of the baroclinic forcing, and the excess of heat in the low latitudes is efficiently transported northwards by finite eddies, in the spirit of baroclinic adjustment.
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简化的两层大气模式中的涡旋饱和
涡旋饱和描述了地球物理流动中的非线性机制,即当考虑平均条件时,纬向流的直接强迫增加了涡旋动能,而与纬向流相关的能量不增加。在这里,我们提出了一个最小斜压模型,显示完全涡饱和。本文从Phillips在中纬度β通道上的经典准地转两能级模型出发,推导了包含参数化涡流的六个常微分方程的降阶模型。该模型具有两种物理上可实现的稳态解,一种是纯纬向流,另一种是另外存在有限涡动。随着非绝热加热形式的斜压强迫的增加,纬向溶液失去稳定性,涡流溶液变得有吸引力。在此分岔后,解的纬向分量不受斜压强迫的影响,低纬度地区的多余热量在斜压调整的精神下被有限涡流有效地向北输送。
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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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