重力场不均匀性对地转流扰动的影响:三维解析模型

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-05-27 DOI:10.1080/03091929.2020.1762080
L. Ingel, A. A. Makosko
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引用次数: 2

摘要

研究了由重力场空间不均匀性引入背景地转流的线性平稳扰动的理论问题。本文首次考虑了三维解析模型。我们的结果表明,重力场的不均匀性可以导致大面积大气流速度场的有序扰动。我们的三维模型使我们能够理解和分析这种扰动产生的一些最简单的机制和模式,并做出一些估计。速度水平分量的扰动幅值可以达到浮力频率乘以大地水准面偏差幅值的数量级。这一结果与先前对由重力场不均匀性引起的一种截然不同的扰动机制的估计一致。
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Geostrophic flow disturbances influenced by inhomogeneities of gravity field: 3D analytical model
A theoretical problem on linear stationary disturbances introduced by spatial inhomogeneities of gravity field into the background geostrophic flow of the stratified rotating medium (atmosphere) is considered. For the first time, the three-dimensional analytical model is considered. Our results imply that inhomogeneities of the gravity field can lead to ordered perturbations of the velocity field of atmospheric currents in large areas. Our three-dimensional model allows us to understand and analyse some of the simplest mechanisms and patterns of generation of such disturbances and to make some estimates. The amplitude of the disturbances for the velocity horizontal components can reach values of the order of buoyancy frequency multiplied by the amplitude of deviations of the geoid. This result agrees with the estimates obtained previously for a substantially different disturbances mechanism caused by gravity field inhomogeneities.
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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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