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Jun 2012

Volume 24, Issue 6, Articles (06xxxx)

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Phys. Fluids 24, 063302 (2012); http://dx.doi.org/10.1063/1.4729453 (18 pages)

Wenbo Tang, Brent Knutson, Alex Mahalov, and Reneta Dimitrova
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Finite Rossby radius effects on vortex motion near a gap

R. S. Nilawar, E. R. Johnson, and N. R. McDonald

Phys. Fluids 24, 066601 (2012); http://dx.doi.org/10.1063/1.4721432 (18 pages) | Cited 1 time

Online Publication Date: 5 June 2012

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This work investigates the effect of the Rossby radius of deformation on the motion of a vortex near a gap in an infinitely long barrier. A key parameter determining the behaviour of the vortex is a, the ratio of the Rossby radius of deformation to the width of the gap. Assuming quasi-geostrophic dynamics for a single-layer, reduced-gravity fluid, an integral equation is derived whose solution gives the velocity at any point in the fluid. The integral equation is solved numerically and the velocity field is integrated to give the trajectories of point vortices. Combined with the method of contour dynamics, the method can be used to compute the evolution of finite area patches of constant vorticity. The trajectories of point vortices and vortex patches are compared. The patches are initially circular and the centroids of those vortex patches that remain close to circular follow the trajectory and speed of their equivalent point vortices when appropriately normalised. The critical point vortex trajectory (the separatrix) which divides vortices that leap across the gap and those that pass through, is computed for various a. Decreasing the Rossby radius of deformation increases the tendency of vortices to pass through the gap. The effect of various background flows on both point vortex and vortex patch motion is also described.
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47.32.cb Vortex interactions
47.60.-i Flow phenomena in quasi-one-dimensional systems
02.30.Rz Integral equations
02.60.Nm Integral and integrodifferential equations

Structure and stability of the finite-area von Kármán street

Paolo Luzzatto-Fegiz and Charles H. K. Williamson

Phys. Fluids 24, 066602 (2012); http://dx.doi.org/10.1063/1.4724307 (25 pages) | Cited 2 times

Online Publication Date: 8 June 2012

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By using a recently developed numerical method, we explore in detail the possible inviscid equilibrium flows for a Kármán street comprising uniform, large-area vortices. In order to determine stability, we make use of an energy-based stability argument (originally proposed by Lord Kelvin), whose previous implementation had been unsuccessful in determining stability for the Kármán street [P. G. Saffman and J. C. Schatzman, “Stability of a vortex street of finite vortices,” J. Fluid Mech. 117, 171–186 (1982)10.1017/S0022112082001578]. We discuss in detail the issues affecting this interpretation of Kelvin's ideas, and show that this energy-based argument cannot detect subharmonic instabilities. To find superharmonic instabilities, we employ a recently introduced approach, which constitutes a reliable implementation of Kelvin's stability ideas [P. Luzzatto-Fegiz and C. H. K. Williamson, “Stability of conservative flows and new steady fluid solutions from bifurcation diagrams exploiting a variational argument,” Phys. Rev. Lett. 104, 044504 (2010)10.1103/PhysRevLett.104.044504]. For periodic flows, this leads us to organize solutions into families with fixed impulse I, and to construct diagrams involving the flow energy E and horizontal spacing (i.e., wavelength) L. Families of large-I vortex streets exhibit a turning point in L, and terminate with “cat's eyes” vortices (as also suggested by previous investigators). However, for low-I streets, the solution families display a multitude of turning points (leading to multiple possible streets, for given L), and terminate with teardrop-shaped vortices. This is radically different from previous suggestions in the literature. These two qualitatively different limiting states are connected by a special street, whereby vortices from opposite rows touch, such that each vortex boundary exhibits three corners. Furthermore, by following the family of I = 0 streets to small L, we gain access to a large, hitherto unexplored flow regime, involving streets with L significantly smaller than previously believed possible. To elucidate in detail the possible solution regimes, we introduce a map of spacing L, versus impulse I, which we construct by numerically computing a large number of steady vortex configurations. For each constant-impulse family of steady vortices, our stability approach also reveals a single superharmonic bifurcation, leading to new families of vortex streets, which exhibit lower symmetry.
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47.32.cd Vortex stability and breakdown
02.60.-x Numerical approximation and analysis
47.20.Ky Nonlinearity, bifurcation, and symmetry breaking
47.32.ck Vortex streets

Role of fluid density in shaping eruption currents driven by frontal particle blow-out

C. S. Carroll, B. Turnbull, and M. Y. Louge

Phys. Fluids 24, 066603 (2012); http://dx.doi.org/10.1063/1.4725538 (20 pages) | Cited 1 time

Online Publication Date: 8 June 2012

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We study the role of suspension density in eruption currents, a regime of gravity-driven flow that is sustained by massive, localized blow-out of particles acting as a steady source of heavier fluid injected into a uniform flow at high Reynolds number. Inspired by the potential flow solution of Saffman and Yuen [“Finite-amplitude interfacial waves in the presence of a current,” J. Fluid Mech. 123, 459–476 (1982)10.1017/S0022112082003152], we show that the relative density difference between the two fluids swells the size of the current's head without changing its shape, while inducing a velocity jump at the interface. We test this inviscid theory against inviscid and large-eddy-simulations. We also conduct experiments in a water flume, where a line source of fluorescent brines of various densities is injected in a cross-stream and visualized with a narrow sheet of light. Simulations and experiments reveal that, with isotropic velocity distribution on a finite source, eruption currents expand further and develop interface oscillations, but the inviscid theory still captures relative swelling induced by density. We compare predictions to the static pressure data of McElwaine and Turnbull [“Air pressure data from the Vallee de la Sionne avalanches of 2004,” J. Geophys. Res. 110, F03010, doi:10.1029/2004JF000237 (2005)] in powder snow avalanches.
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47.57.E- Suspensions
47.27.Jv High-Reynolds-number turbulence
47.27.ep Large-eddy simulations
47.80.Jk Flow visualization and imaging
47.55.Kf Particle-laden flows
47.35.Bb Gravity waves

On the necessary conditions for bursts of convection within the rapidly rotating cylindrical annulus

Robert J. Teed, Chris A. Jones, and Rainer Hollerbach

Phys. Fluids 24, 066604 (2012); http://dx.doi.org/10.1063/1.4711398 (21 pages) | Cited 1 time

Online Publication Date: 8 June 2012

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Zonal flows are often found in rotating convective systems. Not only are these jet-flows driven by the convection, they can also have a profound effect on the nature of the convection. In this work the cylindrical annulus geometry is exploited in order to perform nonlinear simulations seeking to produce strong zonal flows and multiple jets. The parameter regime is extended to Prandtl numbers that are not unity. Multiple jets are found to be spaced according to a Rhines scaling based on the zonal flow speed, not the convective velocity speed. Under certain conditions the nonlinear convection appears in quasi-periodic bursts. A mean field stability analysis is performed around a basic state containing both the zonal flow and the mean temperature gradient found from the nonlinear simulations. The convective growth rates are found to fluctuate with both of these mean quantities suggesting that both are necessary in order for the bursting phenomenon to occur.
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47.32.Ef Rotating and swirling flows
47.20.-k Flow instabilities
47.10.-g General theory in fluid dynamics
05.40.-a Fluctuation phenomena, random processes, noise, and Brownian motion

Light attenuation experiments on double diffusive plumes and fountains

Bruce R. Sutherland, Brace Lee, and Joseph K. Ansong

Phys. Fluids 24, 066605 (2012); http://dx.doi.org/10.1063/1.4730431 (20 pages)

Online Publication Date: 29 June 2012

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By adapting the method of light attenuation to the study of axisymmetric disturbances, we examine the structure of forced plumes and fountains whose buoyancy is set by salinity and/or temperature differences between the turbulent flow and the otherwise stationary ambient. The attenuation measurements are used to infer the statistically steady-state density as a function of radius and height. These compare well with in situ measurements of density taken from a conductivity-temperature probe that repeatedly traversed the centreline of the plume. The theory for forced plumes also agrees well with the centreline density profile. The radial structure of plumes and fountains near the source is found to correspond well to a Gaussian profile, although the standard deviation is found to increase moderately faster with height than spreading rates reported in the existing literature. This is attributed in part to averaging biases resulting from light attenuating through transient eddies. In most experiments, hot and salty fountains reached a steady state height consistent with existing semi-empirical theories for fountains with just one diffusive component. However, if the density of the hot and salty fluid near the source is close to, but moderately larger than, that of the ambient, over time, the fountain is observed to increase progressively in height. This occurs presumably as a consequence of heat diffusion at the top of the fountain making the ambient above it increasingly buoyant relative to the negative buoyancy associated with less diffusive salt.
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47.27.tb Turbulent diffusion
47.80.-v Instrumentation and measurement methods in fluid dynamics
68.08.Bc Wetting
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