Sensitivity of global instability of spatially developing flow in weakly and fully nonlinear regimes

2008 ◽  
Vol 20 (7) ◽  
pp. 071703 ◽  
Author(s):  
Yongyun Hwang ◽  
Haecheon Choi
Keyword(s):  
Global Instability ◽  
Fully Nonlinear ◽  
Developing Flow ◽  
Nonlinear Regimes ◽  
Spatially Developing Flow

Global Instability in Fully Nonlinear Systems

1996 ◽  
Vol 77 (19) ◽  
pp. 4015-4018 ◽  
Author(s):  
A. Couairon ◽  
J. M. Chomaz
Keyword(s):  
Nonlinear Systems ◽  
Global Instability ◽  
Fully Nonlinear

Linear-eddy modelling of turbulent transport. Part 3. Mixing and differential molecular diffusion in round jets

1990 ◽  
Vol 216 ◽  
pp. 411-435 ◽  
Author(s):  
Alan R. Kerstein
Keyword(s):  
Molecular Diffusion ◽  
Turbulent Transport ◽  
Jet Mixing ◽  
Round Jets ◽  
Developing Flow ◽  
Planar Shear ◽  
Diffusion Effects ◽  
Linear Eddy Model ◽  
Spatially Developing Flow ◽  
Modelling Approach

The linear-eddy model of turbulent mixing represents a spatially developing flow by simulating the time development along a comoving transverse line. Along this line, scalar quantities evolve by molecular diffusion and by randomly occurring spatial rearrangements, representing turbulent convection. The modelling approach, previously applied to homogeneous turbulence and to planar shear layers, is generalized to axisymmetric flows. This formulation captures many features of jet mixing, including differential molecular diffusion effects. A novel experiment involving two unmixed species in the nozzle fluid is proposed and analysed.

Unstable Regions in Impulsively Started Pipe Entrance Flows Subjected to Infinitesimal Axisymmetric Disturbances

2003 ◽  
Author(s):  
E. A. Moss ◽  
A. H. Abbot
Keyword(s):  
Reynolds Number ◽  
Base Flow ◽  
Axial Distance ◽  
Flow Variable ◽  
Unconditionally Stable ◽  
Developing Flow ◽  
Displacement Thickness ◽  
Stability Data ◽  
Axisymmetric Disturbances ◽  
Spatially Developing Flow

This investigation presents computed base flow and stability data (axisymmetric disturbances) for impulsively started pipe entrance flows, and shows that at any given time, the displacement thickness (or any other flow variable) variation with axial distance is given by a varying portion which is accurately described by a steady, spatially developing flow, followed by a constant portion, described by the impulsively started parallel system. At the transition between these two systems is a small portion which is described by neither model. Arising from the inference that the latter region is sufficiently small to be neglected, variations in time and space of unstable regions in impulsively started pipe entrance flows were established, showing that (i) such flows are are unconditionally stable to infinitesimal axisymmetric disturbances for a Reynolds number of less than 23 350; (ii) for 38 770 > Re > 23 350, possible instability is confined to a maximum of 3.7% of the entire steady pipe entrance region; and (iii) for Re > 38 770, unstable regions may occur for finite time durations, over the entire length of the pipe.

scholarly journals Genesis and evolution of velocity gradients in near-field spatially developing turbulence

2017 ◽  
Vol 815 ◽  
pp. 295-332 ◽  
Author(s):  
I. Paul ◽  
G. Papadakis ◽  
J. C. Vassilicos
Keyword(s):  
Reynolds Number ◽  
Strain Rate ◽  
Velocity Gradient ◽  
Gradient Tensor ◽  
Velocity Gradient Tensor ◽  
Grid Element ◽  
Velocity Gradients ◽  
Developing Flow ◽  
Vorticity Vector ◽  
Spatially Developing Flow

This paper investigates the dynamics of velocity gradients for a spatially developing flow generated by a single square element of a fractal square grid at low inlet Reynolds number through direct numerical simulation. This square grid-element is also the fundamental block of a classical grid. The flow along the grid-element centreline is initially irrotational and becomes turbulent further downstream due to the lateral excursions of vortical turbulent wakes from the grid-element bars. We study the generation and evolution of the symmetric and anti-symmetric parts of the velocity gradient tensor for this spatially developing flow using the transport equations of mean strain product and mean enstrophy respectively. The choice of low inlet Reynolds number allows for fine spatial resolution and long simulations, both of which are conducive in balancing the budget equations of the above quantities. The budget analysis is carried out along the grid-element centreline and the bar centreline. The former is observed to consist of two subregions: one in the immediate lee of the grid-element which is dominated by irrotational strain, and one further downstream where both strain and vorticity coexist. In the demarcation area between these two subregions, where the turbulence is inhomogeneous and developing, the energy spectrum exhibits the best$-5/3$power-law slope. This is the same location where the experiments at much higher inlet Reynolds number show a well-defined$-5/3$spectrum over more than a decade of frequencies. Yet, the$Q{-}R$diagram, where$Q$and$R$are the second and third invariants of the velocity gradient tensor, remains undeveloped in the near-grid-element region, and both the intermediate and extensive strain-rate eigenvectors align with the vorticity vector. Along the grid-element centreline, the strain is the first velocity gradient quantity generated by the action of pressure Hessian. This strain is then transported downstream by fluctuations and strain self-amplification is activated a little later. Further downstream, vorticity from the bar wakes is brought towards the grid-element centreline, and, through the interaction with strain, leads to the production of enstrophy. The strain-rate tensor has a statistically axial stretching form in the production region, but a statistically biaxial stretching form in the decay region. The usual signatures of velocity gradients such as the shape of$Q{-}R$diagrams and the alignment of vorticity vector with the intermediate eigenvector are detected only in the decay region even though the local Reynolds number (based on the Taylor length scale) is only between 30 and 40.

Farfield extension of fully nonlinear nearfield ship waves

1999 ◽  
Author(s):  
Chi Yang ◽  
Rainald Lohner ◽  
Francis Noblesse
Keyword(s):  
Fully Nonlinear ◽  
Ship Waves
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