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Jan 2008

Volume 20, Issue 1, Articles (01xxxx)

Issue Cover Spotlight Figure

Phys. Fluids 20, 011301 (2008); http://dx.doi.org/10.1063/1.2832774 (4 pages)

John T. Scott

Physics of Fluids celebrates its 50th year in 2008.

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Announcement: The 2007 François Naftali Frenkiel Award for Fluid Mechanics

Phys. Fluids 20, 010201 (2008); http://dx.doi.org/10.1063/1.2809462 (2 pages)

Online Publication Date: 2 January 2008

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Abstract Unavailable
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01.10.Cr Announcements, news, and awards
47.00.00 Fluid dynamics
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Editorial: Fifty years of Physics of Fluids

John Kim and L. Gary Leal

Phys. Fluids 20, 010401 (2008); http://dx.doi.org/10.1063/1.2832366 (5 pages)

Online Publication Date: 31 January 2008

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Abstract Unavailable
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47.00.00 Fluid dynamics
01.30.-y Physics literature and publications
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Fifty years of Physics of Fluids

John T. Scott

Phys. Fluids 20, 011301 (2008); http://dx.doi.org/10.1063/1.2832774 (4 pages)

Online Publication Date: 31 January 2008

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Physics of Fluids celebrates its 50th anniversary with this issue. This brief history summarizes the launching of the journal in 1958 under its first editor François Frenkiel, who held the position for more than 20 years; reviews the next 16 years under the guidance of Andreas Acrivos, a fertile period during which the journal grew and spun off its sibling, Physics of Plasmas; and then reaches the current era under the present two editors.
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01.30.-y Physics literature and publications
47.00.00 Fluid dynamics
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Constrained subgrid-scale stress model for large eddy simulation

Yipeng Shi, Zuoli Xiao, and Shiyi Chen

Phys. Fluids 20, 011701 (2008); http://dx.doi.org/10.1063/1.2831134 (4 pages) | Cited 3 times

Online Publication Date: 22 January 2008

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In this letter, we propose to impose physical constraints in the dynamic procedure of the dynamic subgrid-scale (SGS) stress model in large eddy simulation, and to calculate the SGS model coefficients using a constrained variation. Numerical simulations of forced and decaying isotropic turbulence demonstrate that the constrained dynamic mixed model predicts the energy evolution and the SGS energy dissipation well. The constrained SGS model also shows a strong correlation with the real stress and is able to capture the energy backscatter, manifesting a desirable feature of combining the advantages of dynamics Smagorinsky and mixed models.
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67.25.dk Vortices and turbulence
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back to top Interfacial Flows

Instability of a vertical chemical front: Effect of viscosity and density varying with concentration

Subramanian Swernath and S. Pushpavanam

Phys. Fluids 20, 012101 (2008); http://dx.doi.org/10.1063/1.2829081 (10 pages) | Cited 5 times

Online Publication Date: 14 January 2008

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In this work we analyze the behavior of a chemical front in a vertical porous medium. A homogeneous autocatalytic reaction occurs in the liquid phase. The column is filled with a chemical species and the reaction is initiated at one end of the vertical column by instantaneously adding the product. The reaction occurs at the interface of the products and the reactants. This causes the reaction front to move down (up) when the product is added to the top (bottom). The front or interface demarcates the domain into two regions: one rich in the reactants and the other rich in products. In this work chemohydrodynamic instabilities are studied, when the density and viscosity of the reactants and products are different and concentration dependent. The dependency of these properties on concentration is explicitly considered. We assume the process to be isothermal and other properties such as diffusivity and permeability to be constant. A traveling wave of chemical concentration is generated in the upward direction (when the products are introduced at the bottom) as the product reacts at the interface. The stability of the interface is determined by the viscosity and density of the two fluids. A shooting method in combination with a Runge–Kutta fourth-order scheme is used for generating the base state of the traveling front. Here, the conditions at which an interfacial instability induced by the density gradients is stabilized due to the viscosity dependence on concentration are determined. Linear stability predictions are determined by inducing perturbations on the traveling wave base state and analyzing their evolution. The effect of various parameters on the stability of the flow was calculated and compared with the nonlinear simulations. The nonlinear problem is modeled using the stream-function, vorticity equations. These equations are solved using a second-order finite difference scheme in space and first-order forward difference scheme in time. The instability predicted from the linear stability analysis is validated with nonlinear simulations.
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47.20.Ib Instability of boundary layers; separation
82.30.Vy Homogeneous catalysis in solution, polymers and zeolites
47.56.+r Flows through porous media
47.11.Bc Finite difference methods
02.60.Lj Ordinary and partial differential equations; boundary value problems

On validation of turbulent mixing simulations for Rayleigh–Taylor instability

Hyunsun Lee, Hyeonseong Jin, Yan Yu, and James Glimm

Phys. Fluids 20, 012102 (2008); http://dx.doi.org/10.1063/1.2832775 (8 pages)

Online Publication Date: 24 January 2008

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The purpose of this paper is to analyze the validation achieved in recent simulations of Rayleigh–Taylor unstable mixing. The simulations are already in agreement with experiment; mesh refinement or insertion of a calibrated subgrid model for mass diffusion will serve to refine this validation and possibly shed light on the role of unobserved long wavelength perturbations in the initial data. In this paper we present evidence to suggest that a subgrid model will have a barely noticeable effect on the simulation. The analysis is of independent interest, as it connects a validated simulation to common studies of mixing properties. The average molecular mixing parameter θ for the ideal and immiscible simulations is zero at a grid block level, as is required by the exact microphysics of these simulations. Averaging of data over volumes of (4Δx)3 to (8Δx)3 yields a conventional value θ ∼ 0.8, suggesting that fluid entrainment in front tracked simulations produces a result similar to numerical mass diffusion in untracked simulations. The miscible simulations yield a nonzero θ ∼ 0.8 in agreement with experimental values. We find spectra in possible approximate agreement with the Kolmogorov theory. A characteristic upturn especially in the density fluctuation spectrum at high wave numbers suggests the need for a subgrid mass diffusion model, while the small size of the upturn and the analysis of θ suggest that the magnitude of the model will not be large. We study directly the appropriate settings for a subgrid diffusion coefficient, to be inserted into simulations modeling miscible experiments. This is our most definitive assessment of the role for a subgrid model. We find that a Smagorinsky-type subgrid mass diffusion model would have a diffusion coefficient at most about 0.15% of the value of the physical mass diffusion for the (mass diffusive) experiment studied.
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47.27.E- Turbulence simulation and modeling
47.51.+a Mixing
47.27.wj Turbulent mixing layers
47.20.-k Flow instabilities

Dispersion due to wall interactions in microfluidic separation systems

Subhra Datta and Sandip Ghosal

Phys. Fluids 20, 012103 (2008); http://dx.doi.org/10.1063/1.2828098 (14 pages) | Cited 9 times

Online Publication Date: 29 January 2008

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The transport of a solute in a straight microchannel of axially variable cross-sectional shape in the presence of an inhomogeneous flow field and an adsorption-desorption process on the wall is studied, motivated by applications to capillary electrophoresis and open-channel capillary electrochromatography. An asymptotic approach based on the long time limit is adopted that reduces the problem to the solution of a one-dimensional transport equation. The reduced model is integrated numerically to study the effects of inhomogeneous electro-osmotic flow and adsorption-desorption kinetics on solute migration and dispersion in a rectangular microchannel. The accuracy of the asymptotic equations is checked by the direct numerical solution of the original three-dimensional transport problem.
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82.80.-d Chemical analysis and related physical methods of analysis
07.10.Cm Micromechanical devices and systems
47.85.Np Fluidics
47.60.Dx Flows in ducts and channels
back to top Viscous and Non-Newtonian Flows

Microconfined equiviscous droplet deformation: Comparison of experimental and numerical results

Anja Vananroye, Pieter J. A. Janssen, Patrick D. Anderson, Peter Van Puyvelde, and Paula Moldenaers

Phys. Fluids 20, 013101 (2008); http://dx.doi.org/10.1063/1.2835312 (10 pages) | Cited 9 times

Online Publication Date: 29 January 2008

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The dynamics of confined droplets in shear flow is investigated using computational and experimental techniques for a viscosity ratio of unity. Numerical calculations, using a boundary integral method (BIM) in which the Green’s functions are modified to include wall effects, are quantitatively compared with the results of confined droplet experiments performed in a counter-rotating parallel plate device. For a viscosity ratio of unity, it is experimentally seen that confinement induces a sigmoidal droplet shape during shear flow. Contrary to other models, this modified BIM model is capable of predicting the correct droplet shape during startup and steady state. The model also predicts an increase in droplet deformation and more orientation toward the flow direction with increasing degree of confinement, which is all experimentally confirmed. For highly confined droplets, oscillatory behavior is seen upon startup of flow, characterized by an overshoot in droplet length followed by droplet retraction. Finally, in the case of a viscosity ratio of unity, a minor effect of confinement on the critical capillary number is observed both numerically and experimentally.
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47.55.D- Drops and bubbles
47.60.Dx Flows in ducts and channels
47.27.N- Wall-bounded shear flow turbulence
02.60.Nm Integral and integrodifferential equations
back to top Particulate, Multiphase, and Granular Flows

Dilute suspension flow with nanoparticle deposition in a representative nasal airway model

H. Shi, C. Kleinstreuer, and Z. Zhang

Phys. Fluids 20, 013301 (2008); http://dx.doi.org/10.1063/1.2833468 (23 pages) | Cited 6 times

Online Publication Date: 29 January 2008

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The human nasal cavities with an effective length of only 10 cm feature a wide array of basic flow phenomena because of their complex geometrics. Employing a realistic nasal airway model and demonstrating that laminar, quasisteady airflow can be assumed, dilute nanoparticle suspension flow and nanoparticle deposition are simulated and analyzed for 7.5 ⩽ Q ⩽ 20 L/min and 1 ⩽ dp ⩽ 150 nm. The understanding and quantitative assessment of mixture flow fields and local nanoparticle wall concentrations in nasal airways with a thin mucus layer are very important for estimating the health risks of inhaled toxic aerosols, determining proper drug-aerosol delivery to target sites such as the olfactory regions and developing algebraic transfer functions for overall nasal dose-response analyses. Employing a commercial software package with user-supplied programs, the validated computer modeling results can be summarized as follows: (i) Most of the air flows through the middle-to-low main passageways. Higher airflow rates result in stronger airflow in the olfactory region and relatively lower flow rates in the meatuses. (ii) Nanoparticle deposition in human nasal airways is significant for tiny nanoparticles, i.e., 1 ⩽ dp ⩽ 2 nm, which also represent some vapors. The smaller the nanoparticle size and the lower the flow rate, the higher are the total deposition efficiencies because of stronger diffusion and longer residence times. (iii) Nanoparticles with dp<5 nm flow preferentially through the middle-to-low main passageway along with the major portion of the airflow. For relatively large nanoparticles (dp ≥ 5 nm), due to the low diffusivities, fewer particles will deposit onto the wall leaving a much thinner nanoparticle gradient layer near the wall, i.e., such nanoparticles pass through the nasal cavities more uniformly with minor wall deposition. (iv) Secondary flows may enhance nanoparticle transport and deposition, especially in the meatuses by convecting nanoparticles into these particular regions. (v) For the olfactory region, an optimal particle size may exist due to the combined effects of nanoparticle transport and local deposition mechanisms. However, because of the low deposition flux and small surface area, the olfactory channels account for only very small total deposition values. (vi) A compact correlation for predicting nanoparticle deposition in human nasal airways has been developed.
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47.15.Rq Laminar flows in cavities, channels, ducts, and conduits
47.63.Ec Pulmonary fluid mechanics
47.11.-j Computational methods in fluid dynamics
47.57.E- Suspensions
47.55.Kf Particle-laden flows
44.25.+f Natural convection
back to top Instability and Transition

Turbulence suppression in channel flows by small amplitude transverse wall oscillations

Mihailo R. Jovanović

Phys. Fluids 20, 014101 (2008); http://dx.doi.org/10.1063/1.2824401 (11 pages) | Cited 4 times

Online Publication Date: 11 January 2008

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We model and analyze the influence of small amplitude transverse wall oscillations on the evolution of velocity perturbations in channel flows. We quantify the effect of stochastic outside disturbances on velocity perturbation energy and develop a framework for the optimal selection of transverse oscillation parameters for turbulence suppression. A perturbation analysis is used to demonstrate that depending on the wall oscillation frequency the energy of velocity perturbations can be increased or decreased compared to the uncontrolled flow. Our results elucidate the capability of properly designed oscillations to reduce receptivity of the linearized Navier-Stokes equations to stochastic disturbances, which entails decreased levels of variance in wall-bounded shear flows.
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47.15.Rq Laminar flows in cavities, channels, ducts, and conduits
47.27.nd Channel flow
47.85.ld Boundary layer control
47.10.ad Navier-Stokes equations

Tailored Taylor vortices

M. A. Sprague, P. D. Weidman, S. Macumber, and P. F. Fischer

Phys. Fluids 20, 014102 (2008); http://dx.doi.org/10.1063/1.2831493 (9 pages) | Cited 3 times

Online Publication Date: 18 January 2008

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The stability of circular Couette flow in discontinuous axisymmetric geometries is investigated using numerical simulations and physical experiments. By contouring the geometry of the inner cylinder, Taylor vortices can be made to appear in discrete sections along the length of the cylinder while adjoining sections remain stable. The disparate flows are connected by transition regions that arise from the stability of the axially nonuniform base flow state. The geometry of the inner cylinder can be tailored to produce the simultaneous onset of Taylor vortices of different wavelength in neighboring sections. In another variant, a stack of inner cylinders of common radius are made to rotate independently to produce adjacent regions of stable and unstable flow.
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47.20.-k Flow instabilities
47.32.cd Vortex stability and breakdown
back to top Turbulent Flows

The turbulence dissipation constant is not universal because of its universal dependence on large-scale flow topology

N. Mazellier and J. C. Vassilicos

Phys. Fluids 20, 015101 (2008); http://dx.doi.org/10.1063/1.2832778 (9 pages) | Cited 9 times

Online Publication Date: 23 January 2008

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The dimensionless dissipation rate constant Cϵ of homogeneous isotropic turbulence is such that Cϵ = f(log Reλ)Cs′3, where f(log Reλ) is a dimensionless function of log Reλ which tends to 0.26 (by extrapolation) in the limit where log Reλ⪢1 (as opposed to just Reλ⪢1) if the assumption is made that a finite such limit exists. The dimensionless number Cs reflects the number of large-scale eddies and is therefore nonuniversal. The nonuniversal asymptotic values of Cϵ stem, therefore, from its universal dependence on Cs. The Reynolds number dependence of Cϵ at values of log Reλ close to and not much larger than 1 is primarily governed by the slow growth (with Reynolds number) of the range of viscous scales of the turbulence. An eventual Reynolds number independence of Cϵ can be achieved, in principle, by an eventual balance between this slow growth and the increasing non-Gaussianity of the small scales. The turbulence is characterized by five length-scales in the following order of increasing magnitude: the Kolmogorov microscale η, the inner cutoff scale η*η(7.8+9.1 log Reλ), the Taylor microscale λ ∼ Reλ1/2η, the voids length scale λv ∼ Reλ1/3λ, and the integral length scale L ∼ Reλ2/3λv.
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47.27.Gs Isotropic turbulence; homogeneous turbulence

Large eddy simulation of magnetohydrodynamic turbulent duct flows

Hiromichi Kobayashi

Phys. Fluids 20, 015102 (2008); http://dx.doi.org/10.1063/1.2832779 (13 pages) | Cited 9 times

Online Publication Date: 25 January 2008

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Turbulent duct flows in a uniform magnetic field are examined at low magnetic Reynolds number. Large-eddy simulation is conducted to reveal a sidewall effect on the skin friction. The duct has a square cross section and entirely insulated walls. The duct flow has two kinds of boundary layers: Hartmann layer and sidewall layer. The Hartmann layer is located on the wall perpendicular to the magnetic field, while the sidewall layer exists on the wall parallel to the magnetic field. As the magnetic field increases in the range of turbulent flows, the Hartmann layer becomes thin because of the “Hartmann flattening”—a flattening effect of the flow by the Lorentz force. The sidewall layer, however, becomes thick because of the turbulence suppression until the laminarization takes place. When the Reynolds number, Re, based on the hydraulic diameter, molecular viscosity, and bulk velocity is 5 300, the Hartmann and sidewall layers are laminarized at the same Hartmann number that is proportional to the magnetic field. When the Hartmann layer is laminarized at Re = 29 000, the sidewall layer remains turbulence. This is due to a sidewall effect and is the condition that a local maximum takes place in the skin friction profile. When the sidewall layer is laminarized, the flow totally becomes laminar and the skin friction becomes minimum.
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47.65.-d Magnetohydrodynamics and electrohydrodynamics
47.27.ep Large-eddy simulations
47.27.nb Boundary layer turbulence
47.27.nf Flows in pipes and nozzles

Three-dimensional features of the turbulent flow through a planar sudden expansion

L. Casarsa and P. Giannattasio

Phys. Fluids 20, 015103 (2008); http://dx.doi.org/10.1063/1.2832780 (15 pages) | Cited 6 times

Online Publication Date: 28 January 2008

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An experimental investigation of the turbulent flow downstream of a planar sudden expansion has been performed by means of a 2D particle image velocimetry (PIV) technique. Flow fields at the Reynolds number of 104 have been measured in several mutually perpendicular planes of a channel having an expansion ratio of 3 and an aspect ratio of 10. As usual for large expansion ratios, the separated flow exhibits a strong asymmetry about the expansion axis and, consequently, very different reattachment lengths on the two side walls of the channel. The mean flow turns out to be substantially symmetric about the midspan plane and strong three-dimensional effects are observed in wide portions of the separation bubbles adjacent to the upper and lower walls. The reattachment lengths exhibit significant spanwise variations that are particularly pronounced in the longer reattachment line. Measurements performed in a single flow plane at Re = 4⋅104 show that the influence of the Reynolds number on the mean flow is not completely negligible in the considered variation range. Based on a careful analysis of the PIV data, a model of the three-dimensional mean flow structure in the separation bubbles has been conjectured and it is provided in the paper. The present investigation contributes to clarifying the controversial three-dimensional character of the turbulent flow in a planar sudden expansion and provides accurate and detailed reference data for numerical simulations.
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47.27.nd Channel flow
47.60.Dx Flows in ducts and channels
47.20.Ib Instability of boundary layers; separation
47.32.Ff Separated flows
47.55.D- Drops and bubbles
47.80.Jk Flow visualization and imaging
back to top Compressible Flows

Physical and computational aspects of shock waves over power-law leading edges

Wilson F. N. Santos

Phys. Fluids 20, 016101 (2008); http://dx.doi.org/10.1063/1.2831135 (11 pages) | Cited 2 times

Online Publication Date: 15 January 2008

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Computations using the direct simulation Monte Carlo (DSMC) method are presented for hypersonic flow on power-law shaped leading edges. The primary aim of this paper is to examine the geometry effect of such leading edges on the shock-wave structure. The sensitivity of the shock-wave shape, shock-wave thickness, and shock-wave standoff distance to shape variations of such leading edges is investigated by using a model that classifies the molecules in three distinct classes: (1) undisturbed freestream, (2) reflected from the boundary, and (3) scattered, i.e., molecules that had been indirectly affected by the presence of the leading edge. The analysis showed that, for power-law shaped leading edge with exponent between 2/3 and 1, the shock wave follows the body shape. It was found that, at the vicinity of the nose, the shock-wave power-law exponent is 1/2. Far from the nose, calculations showed that the shock-wave shape is in surprising qualitative agreement with that predicted by the hypersonic small disturbance theory for the flow conditions considered.
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47.40.Ki Supersonic and hypersonic flows
47.40.Nm Shock wave interactions and shock effects

Effective velocity for transport in heterogeneous compressible flows with mean drift

Sabine Attinger and Assyr Abdulle

Phys. Fluids 20, 016102 (2008); http://dx.doi.org/10.1063/1.2827584 (12 pages)

Online Publication Date: 23 January 2008

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Solving transport equations in heterogeneous flows might give rise to scale dependent transport behavior with effective large scale transport parameters differing from those found on smaller scales. For incompressible velocity fields, homogenization methods have proven to be powerful in describing the effective transport parameters. In this paper, we aim at studying the effective drift of transport problems in heterogeneous compressible flows. Such a study was done by Vergassola and Avellaneda in Physica D 106, 148 (1997) . There, it was shown that for static compressible flow without mean drift, impacts on the large scale drift do not occur. We will first discuss the impact of a mean drift and show that static compressible flow with mean drift can produce a heterogeneity driven large scale drift (or ballistic transport). For the case of Gaussian stationary random processes, we derive explicit results for the large scale drift. Moreover, we show that the large scale or effective drift depends on the small scale diffusion coefficients and thus on the molecular weights of the particles. This study could be applied to weight-based particle separation. Numerical simulations are presented to illustrate these phenomena.
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47.40.-x Compressible flows; shock waves

Enhancement in counterflow drag reduction by supersonic jet in high enthalpy flows

Vinayak Kulkarni and K. P. J. Reddy

Phys. Fluids 20, 016103 (2008); http://dx.doi.org/10.1063/1.2813042 (4 pages)

Online Publication Date: 23 January 2008

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Counterflow drag reduction by supersonic jet for a 60° apex angle blunt cone flying at hypersonic Mach number is investigated for two different flow enthalpies using conventional and free piston driven hypersonic shock tunnels. Enhancement in drag reduction has been observed with increase in freestream stagnation enthalpy. It is shown that the percentage of drag reduction goes up by a factor of 2 when the flow enthalpy increases by a factor of 2.5 for a given ratio of total pressure of supersonic jet and freestream flow.
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47.85.Gj Aerodynamics
47.40.Ki Supersonic and hypersonic flows
47.85.lb Drag reduction

Head-on collision of shock wave induced vortices with solid and perforated walls

K. Kontis, R. An, H. Zare-Behtash, and D. Kounadis

Phys. Fluids 20, 016104 (2008); http://dx.doi.org/10.1063/1.2837172 (17 pages) | Cited 9 times

Online Publication Date: 31 January 2008

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An experimental study has been conducted to examine the interaction of shock wave induced vortices with a flat plate and a perforated plate. The experiments were carried out using a 30 mm internal diameter shock-tube at Mach numbers 1.31, 1.49, and 1.61 under critical driver conditions. Air was used both in the driver and driven sections. High-speed schlieren photography was employed to study the flow development and the resulting interactions with the plates. Wall pressure measurements on both plates were also carried out in order to study the flow interactions quantitatively. The experimental results indicated that a region of strong flow development is generated near the wall surface, due to the flow interactions of reflected waves and oncoming induced vortices. This flow behavior causes the generation of multiple pressure fluctuations on the wall. In the case of the perforated plate, a weaker initial reflected wave is produced, which is followed by compression waves, due to the internal reflections within the plate. The transmitted wave is reduced in strength, compared to the initial incident shock wave.
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47.27.N- Wall-bounded shear flow turbulence
47.32.-y Vortex dynamics; rotating fluids
47.40.Nm Shock wave interactions and shock effects
back to top Geophysical Flows

Dynamo action in an annular array of helical vortices

R. Volk, P. Odier, and J.-F. Pinton

Phys. Fluids 20, 016601 (2008); http://dx.doi.org/10.1063/1.2830983 (12 pages) | Cited 1 time

Online Publication Date: 18 January 2008

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We numerically study the induction mechanisms generated from an array of helical motions distributed along a cylinder. Our flow is a very idealized geometry of the columnar structure that has been proposed for the convective motion inside the Earth’s core. Using an analytically prescribed flow, we apply a recently introduced iterative numerical scheme [ M. Bourgoin, P. Odier, J.-F. Pinton, and Y. Richard, Phys. Fluids 16, 2529 (2004) ] to solve the induction equation and analyze the flow response to externally applied fields with simple geometries (e.g., azimuthal, radial). Symmetry properties allow us to build selected induction modes whose interactions lead to dynamo mechanisms. Using an induction operator formalism, we show how dipole and quadrupole dynamos can be envisioned from such motions. The method identifies the main induction mechanisms that generate dynamo action in the selected geometry. Here, it emphasizes the competition between α-effect and field expulsion as well as the role of scale separation.
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91.25.Za Core processes
47.65.-d Magnetohydrodynamics and electrohydrodynamics
47.32.C- Vortex dynamics

Nonlinear adjustment of a front over escarpment

F. Bouchut, E. Scherer, and V. Zeitlin

Phys. Fluids 20, 016602 (2008); http://dx.doi.org/10.1063/1.2834731 (12 pages) | Cited 3 times

Online Publication Date: 29 January 2008

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We present the results of fully nonlinear numerical simulations of the geostrophic adjustment of a pressure front over topography, represented by an escarpment with a linear slope. The results of earlier simulations in the linear regime are confirmed and new essentially nonlinear effects are found. Topography influences both fast and slow components of motion. The fast unbalanced motion corresponds to inertia-gravity waves (IGW). The IGW emitted during initial stages of adjustment break and form the localized dissipation zones. Due to topography, the IGW activity is enhanced in certain directions. The slow balanced motion corresponds to topographic Rossby waves propagating along the escarpment. As shown, at large enough nonlinearities they may trap fluid/tracer and carry it on. There are indications that nonlinear topographic waves form a soliton train during the adjustment process. If the coastal line is added to the escarpment at the shallow side (continental shelf), secondary fronts related to the propagation of the coastal Kelvin waves appear.
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91.10.Jf Topography; geometric observations
back to top Others

Thermodiffusion in nanofluids under different gravity conditions

Raffaele Savino and Diego Paterna

Phys. Fluids 20, 017101 (2008); http://dx.doi.org/10.1063/1.2823561 (10 pages) | Cited 8 times

Online Publication Date: 8 January 2008

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A convective transport model is developed to study the role of thermal diffusion, or the Ludwig–Soret effect, in nanofluid systems with temperature gradients. The study deals with a fluid suspension of nanoparticles enclosed between two differentially heated horizontal, relatively closely spaced plates (Bénard configuration). An order-of-magnitude analysis is performed to identify the relevant parameters of the problem. Three-dimensional simulations are performed taking into account different conditions, including normal or microgravity conditions, gravity orientation, and positive or negative Soret effect. Different modes of convective instabilities are shown to be present in the system, which are associated with the gravity force and the density differences induced by concentration gradients. The characteristic flow patterns and instability developments are in agreement with the experimental findings obtained by independent investigators on colloidal suspensions. The onset of instabilities, their characteristic time scales, and flow patterns corresponding with different geometrical configurations, gravity levels, and gravity orientation are shown.
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47.57.eb Diffusion and aggregation
82.70.Kj Emulsions and suspensions
47.27.tb Turbulent diffusion
47.27.te Turbulent convective heat transfer
47.54.-r Pattern selection; pattern formation
47.20.-k Flow instabilities

Instabilities in the dynamics of neutrally buoyant particles

Themistoklis Sapsis and George Haller

Phys. Fluids 20, 017102 (2008); http://dx.doi.org/10.1063/1.2830328 (7 pages) | Cited 8 times

Online Publication Date: 15 January 2008

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The asymptotic dynamics of finite-size particles is governed by a slow manifold that is globally attracting for sufficiently small Stokes numbers. For neutrally buoyant particles (suspensions), the slow dynamics coincide with that of infinitesimally small particles, therefore the suspension dynamics should synchronize with Lagrangian particle motions. Paradoxically, recent studies observe a scattering of suspension dynamics along Lagrangian particle motions. Here we resolve this paradox by proving that despite its global attractivity, the slow manifold has domains that repel nearby passing trajectories. We derive an explicit analytic expression for these unstable domains; we also obtain a necessary condition for the global attractivity of the slow manifold. We illustrate our results on neutrally buoyant particle motion in a two-dimensional model of vortex shedding behind a cylinder in crossflow and on the three-dimensional steady Arnold–Beltrami–Childress flow.
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47.20.-k Flow instabilities
47.32.C- Vortex dynamics
47.55.Kf Particle-laden flows

Heat transfer in vacuum packaged microelectromechanical system devices

Chunpei Cai

Phys. Fluids 20, 017103 (2008); http://dx.doi.org/10.1063/1.2832777 (10 pages) | Cited 5 times

Online Publication Date: 17 January 2008

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This study analyzes heat transfer effects inside vacuum packaged microelectromechanical system (MEMS) devices. A packaged device is simplified as four plates forming a square cavity, the bottom plate represents a hot chip, while the other three plates are maintained at room temperature. For a highly rarefied free molecular internal gas flow scenario, the corresponding detailed density and temperature fields are analytically determined with a proposed speculation. This speculation indicates that for a steady free molecular gas flow inside a convex closure domain formed by walls maintained at different temperatures: (1) the velocity distribution functions for those molecules diffusely reflected at different walls and traveling away from them are Maxwellian with different number densities; (2) for each distribution, nimath is a constant, where ni is the number density for the group of reflected molecules, and Ti is the temperature for the ith plate. For a near continuum flow scenario, the governing energy equation degenerates to Laplace’s equation with several temperature-jump wall boundary conditions. This study also includes discussions and comparisons among analytical results, simulation results from the direct simulation Monte Carlo method, and results by solving the Navier–Stokes equations with proper wall boundary conditions. The approach used in this study is generally applicable to study internal flows and heat transfer effects in other vacuum packaged MEMS devices with different shapes.
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85.85.+j Micro- and nano-electromechanical systems (MEMS/NEMS) and devices
85.40.-e Microelectronics: LSI, VLSI, ULSI; integrated circuit fabrication technology

Numerical simulations of a cylinder wake under a strong axial magnetic field

Vincent Dousset and Alban Pothérat

Phys. Fluids 20, 017104 (2008); http://dx.doi.org/10.1063/1.2831153 (13 pages) | Cited 9 times

Online Publication Date: 23 January 2008

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We study the flow of a liquid metal in a square duct past a circular cylinder in a strong externally imposed magnetic field. In these conditions, the flow is quasi-two-dimensional, which allows us to model it using a two-dimensional (2D) model. We perform a parametric study by varying the two control parameters Re and Ha (Ha2 is the ratio of Lorentz to viscous forces) in the ranges [0…6000] and [0…2160], respectively. The flow is found to exhibit a sequence of four regimes. The first three regimes are similar to those of the non-magnetohydrodynamic (non-MHD) 2D circular wake, with transitions controlled by the friction parameter Re/Ha. The fourth one is characterized by vortices raising from boundary layer separations at the duct side walls, which strongly disturbs the Kármán vortex street. This provides the first explanation for the breakup of the 2D Kármán vortex street first observed experimentally by Frank, Barleon, and Müller [Phys. Fluids 13, 2287 (2001) ]. We also show that, for high values of Ha (Ha ≥ 1120), the transition to the fourth regime occurs for Re∝0.56Ha, and that it is accompanied by a sudden drop in the Strouhal number. In the first three regimes, we show that the drag coefficient and the length of the steady recirculation regions located behind the cylinder are controlled by the parameter Re/Ha4/5. Also, the free shear layer that separates the recirculation region from the free stream is similar to a free MHD parallel layer, with a thickness of the order of Ha−1/2 that is quite different to that of the non-MHD case, and therefore strongly influences the dynamics of this region. We also present one case at Re = 3×104 and Ha = 1120, where this layer undergoes an instability of the Kelvin–Helmholtz-type.
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47.20.Ib Instability of boundary layers; separation
47.32.Ff Separated flows
47.32.-y Vortex dynamics; rotating fluids
47.60.Dx Flows in ducts and channels
47.27.N- Wall-bounded shear flow turbulence

Modification and expansion of the generalized soft-sphere model to high temperature based on collision integrals

Jae Gang Kim, Oh Joon Kwon, and Chul Park

Phys. Fluids 20, 017105 (2008); http://dx.doi.org/10.1063/1.2832781 (14 pages) | Cited 2 times

Online Publication Date: 23 January 2008

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In the present study, modification and expansion of the collision parameters for the general soft-sphere model [ J. Fan, Phys. Fluids 12, 4399 (2002) ] were made for use in the direct simulation Monte Carlo calculation of hypersonic flows in the temperature range of 300–50 000 K. The collision integrals were expressed as a two-term function in a form of the inverse power of temperature, which was cast in terms of the soft-sphere scattering parameters and the four total cross-section parameters. Next, the most recent available data for the diffusion and viscosity collision integrals were collected and fitted into a function of temperature in the same form. By equating these expressions for the diffusion and viscosity collision integrals simultaneously, the five collision parameters were deduced as functions of species combinations. The resulting collision parameters for the general soft-sphere model were tabulated for 191 collision pairs involving 22 species. It was shown that the transport properties calculated by using the present collision parameters are much closer to experiments, theoretical data, and the values obtained by the ab initio calculations from quantum-mechanically derived potential energy surfaces than existing elastic collision models. The direct simulation Monte Carlo calculation of flow around a circular cylinder confirmed that discernible differences exist between the results based on the present study and those of the existing models.
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47.40.Ki Supersonic and hypersonic flows
47.11.-j Computational methods in fluid dynamics
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