湍流边界层中不可压缩流体流动的相干结构动力学

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2023-01-02 DOI:10.1080/03091929.2023.2175822
R. S. Selim
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引用次数: 0

摘要

我们考虑了波的非线性相互作用系统来识别共振三联频的离散簇,并根据共振条件对它们进行了分类。本文研究了湍流边界层中不可压缩流体流动的相干结构。离散波湍流在单模近似下具有弱非线性相互作用模的特征。在多尺度分析框架下,定义了多重三波共振情况下振幅方程的相干部分。用切比雪夫配点法求解Orr-Sommerfeld方程的谱问题,根据这些振幅的色散关系确定共振条件。研究了这些振幅的频谱特征,以确定多重三波共振的条件。此条件也适用于由共享共模的三和弦组成的谐振团,其中所有三和弦都满足谐振条件。相干振幅用常微分方程的自治系统动态表示。注意到单三元组和一簇三元组的不可积系统,其中给定系统中的相互作用系数不具有相同的复相。所得到的动力系统允许一些不变量,类似于经典的曼利-罗不变量,但性质不同。其中一个不变量被称为能量不变量流形,它表示动力系统的模的平方振幅的和,这个不变量被归一化以在单位球上定义。因此,采用Birkhoff-Khinchin理论计算二次谐波和次谐波振幅的时间平均值。此外,本文还着重研究了用随机初始条件下的龙格-库塔方法求解动力系统简单结构和复杂结构的数值解。在权因子的不同符号下研究了动力系统的解,其中该系统的有界解在正号和负号下都可以找到。然而,在另一个动力系统的研究中,爆炸不稳定性仅在一个权重因子的负号处被注意到,其中所有的研究案例都与波矢量的选择有关。将随机初始条件应用于简单和复杂动力系统,研究系统解的行为。动力系统内部不同三元组的耦合导致了混沌乱流状态。
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Dynamics of the coherent structure for incompressible fluid flow in turbulent boundary layers
We consider the nonlinear interaction system of waves to identify discrete clusters of resonant triads, which are classified on the basis of the resonance condition. This study is conducted to investigate the coherent structure of incompressible fluid flow in the turbulent boundary layer. The discrete wave turbulence is characterised by weakly nonlinear interaction modes for amplitude Tollmien Schlichting in a single-mode approximation. Within the framework of multiple-scale analysis, the coherent part of the amplitude equation is defined in the case of multiple three-wave resonance. The resonance condition is defined from the dispersion relation of these amplitudes, which are determined from solving the spectral problem of Orr–Sommerfeld equation by the Chebyshev collocation method. The spectral characteristics of these amplitudes are investigated to define the condition of multiple three-wave resonance. This condition is also defined for a resonant cluster made out of triads sharing a common mode, where all triads satisfy the resonance condition. The coherent amplitudes are represented dynamically by an autonomous system of ordinary differential equations. Non-integrable system of a single triad and a cluster of triads is noted, where the interaction coefficients in the given system do not have the same complex phase. The obtained dynamical system admits a number of invariants, similar to the classical Manley–Rowe invariants but of a different nature. One of these invariants is called the energy invariant manifold that represents the sum of modules square amplitudes of the dynamical system, this invariant is normalised to be defined on the unit sphere. Therefore, Birkhoff–Khinchin theory is applied to calculate the time average of square harmonic and sub harmonic amplitudes. Moreover, this paper is also focused on studying the numerical solutions of both simple and complex structure of the dynamical system by using Runge–Kutta method with random initial conditions. The solution of the dynamical system is examined at different signs of the weight factors, where the bounded solutions of this system are found at both positive and negative signs. However, in another study of a dynamical system, an explosive instability is noted at a negative sign for only one of the weight factors, where all study cases are related to the choice of wave vectors. The random initial conditions are applied to both simple and complex dynamical system to study the behaviour of system solutions. The coupling different triads within the dynamical system lead to chaotic turbulence regime.
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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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