静止欧拉流的几何稳定性

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-05-03 DOI:10.1080/03091929.2019.1680660
Chen Sun
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引用次数: 0

摘要

几何稳定性理论是作为结构稳定性在物理空间中的类比而发展起来的。如果两个定常流具有相同的流线图样,且速度令人满意,则称它们在几何上相等。如果存在具有水平变化F的几何等价解,则欧拉方程的平稳解是非唯一的,在这种情况下,其几何结构是稳定的,并且允许非比例速度变化。没有这样一个等价解的欧拉流是唯一的和几何上不稳定的。伪平面流动分析表明,只有等速流动,特别是直线射流和垂直排列的圆涡,才具有几何稳定性。具有封闭流线的稳定流动只有垂直排列的圆涡,这为涡旋排列和轴对称现象提供了稳定性解释。利用一系列多项式和非多项式欧拉解验证了拟平面理想流的一般不稳定性。二次解表明压力场具有动态多重性,不能作为几何分析的代表。
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Geometric stability of stationary Euler flows
ABSTRACT Geometric stability theory is developed as an analogue of structural stability in physical space. Two steady flows are said to be geometrically equivalent if they have the same streamline pattern with velocities satisfying . A stationary solution to the Euler equations is non-unique if there exists a geometrically equivalent solution with horizontally varying F, in which case its geometric structure is stable and permits non-proportional velocity change. An Euler flow without such an equivalent solution is unique and geometrically unstable. Analysis of pseudo-plane flows shows that only constant-speed flows, specifically straightline jet and vertical-aligned circular vortex, are geometrically stable. The only stable flow with closed streamlines is vertical-aligned circular vortex, which provides a stability explanation for the phenomenon of vortex alignment and axisymmetrisation. A series of polynomial and nonpolynomial Euler solutions is used to validate the generic instability of pseudo-plane ideal flows. The quadratic solutions indicate that the pressure field has dynamic multiplicity and cannot be used as a proxy for geometric analysis.
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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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