IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
M. Kurgansky, T. Seelig, M. Klein, A. Will, U. Harlander
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引用次数: 2

摘要

在一个旋转圆柱环空的实验室实验中,我们发现了一个顺流射流,它与一个纵向振动的内直圆柱壁面相邻。在这里,壁面的振动被实现为内气缸旋转速率的时谐调制。外圆柱体壁和底盖和顶盖以恒定的角速度旋转。我们研究的主要目的是有助于定性和定量地理解在旋转壁面流动中经常遇到的振荡但离心稳定的垂直边界层中存在的非线性。我们考虑的问题在某种意义上是对以前的工作的补充,这些工作专注于振荡的Ekman层,而忽略了垂直的Stokes - Stewartson层。本文提出了一个简单的解析模型,该模型能够根据内柱边界层动力学的非线性特性来预测新出现的渐进式近壁射流的大小和空间结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Mean flow generation due to longitudinal librations of sidewalls of a rotating annulus
Laboratory experiments with a rotating cylindrical annulus are reported that reveal a prograde jet, which is adjacent to a (longitudinally) librating inner straight cylindrical wall. Here, wall libration is realised as a time-harmonic modulation of the inner cylinder's rotation rate. The outer cylindrical wall and bottom and top lids rotate with constant angular velocity. The main purpose of our study is to contribute to a qualitative and quantitative understanding of non-linearities that are present in oscillating, but centrifugally stable, vertical boundary layers frequently encountered in rotating wall-bounded flows. We consider a problem that is in a sense complementary to that of previous works that focused on oscillating Ekman layers but neglected the vertical Stokes−Stewartson layers. A simple analytical model is proposed that is able to predict the magnitude and spatial structure of the emerging prograde near-wall jet in terms of nonlinearity inherent in the inner cylinder's boundary layer dynamics.
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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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