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1

Tam, Christopher K. W., and Hongbin Ju. "Aerofoil tones at moderate Reynolds number." Journal of Fluid Mechanics 690 (December 1, 2011): 536–70. http://dx.doi.org/10.1017/jfm.2011.465.

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AbstractIt is known experimentally that an aerofoil immersed in a uniform stream at a moderate Reynolds number emits tones. However, there have been major differences in the experimental observations in the past. Some experiments reported the observation of multiple tones, with strong evidence that these tones are most probably generated by a feedback loop. There is also an experiment reporting the observation of a single tone with no tonal jump or other features associated with feedback. In spite of the obvious differences in the experimental observations published in the literature, it is noted that all the dominant tone frequencies measured in all the investigations are in agreement with an empirically derived Paterson formula. The objective of the present study is to perform a direct numerical simulation (DNS) of the flow and acoustic phenomenon to investigate the tone generation mechanism. When comparing with experimental studies, numerical simulations appear to have two important advantages. The first is that there is no background wind tunnel noise in numerical simulation. This avoids the signal-to-noise ratio problem inherent in wind tunnel experiments. In other words, it is possible to study tones emitted by a truly isolated aerofoil computationally. The second advantage is that DNS produces a full set of space–time data, which can be very useful in determining the tone generation processes. The present effort concentrates on the tones emitted by three NACA0012 aerofoils with a slightly rounded trailing edge but with different trailing edge thickness at zero degree angle of attack. At zero degree angle of attack, in the Reynolds number range of$2\ensuremath{\times} 1{0}^{5} $to$5\ensuremath{\times} 1{0}^{5} $, the boundary layer flow is attached nearly all the way to the trailing edge of the aerofoil. Unlike an aerofoil at an angle of attack, there is no separation bubble, no open flow separation. All the flow separation features tend to increase the complexity of the tone generation processes. The present goal is limited to finding the basic tone generation mechanism in the simplest flow configuration. Our DNS results show that, for the flow configuration under study, the aerofoil emits only a single tone. This is true for all three aerofoils over the entire Reynolds number range of the present study. In the literature, it is known that Kelvin–Helmholtz instabilities of free shear layers generally have a much higher spatial growth rate than that of the Tollmien–Schlichting boundary layer instabilities. A near-wake non-parallel flow instability analysis is performed. It is found that the tone frequencies are the same as the most amplified Kelvin–Helmholtz instability at the location where the wake has a minimum half-width. This suggests that near-wake instability is the energy source of aerofoil tones. However, flow instabilities at low subsonic Mach numbers generally do not cause strong tones. An investigation of how near-wake instability generates tones is carried out using the space–time data provided by numerical simulations. Our observations indicate that the dominant tone generation process is the interaction of the oscillatory motion of the near wake, driven by flow instability, with the trailing edge of the aerofoil. Secondary mechanisms involving unsteady near-wake motion and the formation of discrete vortices in regions further downstream are also observed.
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2

Bershadskii, A. G. "Turbulence singularities at moderate reynolds numbers." Journal of Engineering Physics 58, no. 6 (June 1990): 703–6. http://dx.doi.org/10.1007/bf00872720.

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3

KNAEPEN, B., S. KASSINOS, and D. CARATI. "Magnetohydrodynamic turbulence at moderate magnetic Reynolds number." Journal of Fluid Mechanics 513 (August 25, 2004): 199–220. http://dx.doi.org/10.1017/s0022112004000023.

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4

L’vov, Victor S., and Itamar Procaccia. "Extended universality in moderate-Reynolds-number flows." Physical Review E 49, no. 5 (May 1, 1994): 4044–51. http://dx.doi.org/10.1103/physreve.49.4044.

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5

Ruschak, Kenneth J., and Steven J. Weinstein. "Thin-Film Flow at Moderate Reynolds Number." Journal of Fluids Engineering 122, no. 4 (July 5, 2000): 774–78. http://dx.doi.org/10.1115/1.1319499.

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Viscous, laminar, gravitationally-driven flow of a thin film over a round-crested weir is analyzed for moderate Reynolds numbers. A previous analysis of this flow utilized a momentum integral approach with a semiparabolic velocity profile to obtain an equation for the film thickness (Ruschak, K. J., and Weinstein, S. J., 1999, “Viscous Thin-Film Flow Over a Round-Crested Weir,” ASME J. Fluids Eng., 121, pp. 673–677). In this work, a viscous boundary layer is introduced in the manner of Haugen (Haugen, R., 1968, “Laminar Flow Around a Vertical Wall,” ASME J. Appl. Mech. 35, pp. 631–633). As in the previous analysis of Ruschak and Weinstein, the approximate equations have a critical point that provides an internal boundary condition for a bounded solution. The complication of a boundary layer is found to have little effect on the thickness profile while introducing a weak singularity at its beginning. The thickness of the boundary layer grows rapidly, and there is little cumulative effect of the increased wall friction. Regardless of whether a boundary layer is incorporated, the approximate free-surface profiles are close to profiles from finite-element solutions of the Navier-Stokes equation. Similar results are obtained for the related problem of developing flow on a vertical wall (Cerro, R. L., and Whitaker, S., 1971, “Entrance Region Flows With a Free Surface: the Falling Liquid Film,” Chem. Eng. Sci., 26, pp. 785–798). Less accurate results are obtained for decelerating flow on a horizontal wall (Watson, E. J., 1964, “The Radial Spread of a Liquid Jet Over a Horizontal Plane,” J. Fluid Mech. 20, pp. 481–499) where the flow is not gravitationally driven. [S0098-2202(00)01904-0]
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6

Zamyshlyaev, A. A., and G. R. Shrager. "Fluid Flows past Spheroids at Moderate Reynolds Numbers." Fluid Dynamics 39, no. 3 (May 2004): 376–83. http://dx.doi.org/10.1023/b:flui.0000038556.08179.ea.

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7

Kotas, C. W., M. Yoda, and P. H. Rogers. "Visualizations of steady streaming at moderate Reynolds numbers." Physics of Fluids 18, no. 9 (September 2006): 091102. http://dx.doi.org/10.1063/1.2335902.

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8

Bandaru, Vinodh, Thomas Boeck, and Jörg Schumacher. "Hartmann duct flow at moderate magnetic Reynolds numbers." PAMM 16, no. 1 (October 2016): 577–78. http://dx.doi.org/10.1002/pamm.201610277.

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9

Smith, T. A., and Y. Ventikos. "Wing-tip vortex dynamics at moderate Reynolds numbers." Physics of Fluids 33, no. 3 (March 1, 2021): 035111. http://dx.doi.org/10.1063/5.0039492.

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10

HILL, REGHAN J., and DONALD L. KOCH. "Moderate-Reynolds-number flow in a wall-bounded porous medium." Journal of Fluid Mechanics 453 (February 25, 2002): 315–44. http://dx.doi.org/10.1017/s002211200100684x.

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The transition to unsteady flow and the dynamics of moderate-Reynolds-number flows in unbounded and wall-bounded periodic arrays of aligned cylinders are examined using lattice-Boltzmann simulations. The simulations are compared to experiments, which necessarily have bounding walls. With bounding walls, the transition to unsteady flow is accompanied by a loss of spatial periodicity, and the temporal fluctuations are chaotic at much smaller Reynolds numbers. The walls, therefore, affect the unsteady flows everywhere in the domain. Consistency between experiments and simulations is established by examining the wake lengths for steady flows and the fundamental frequencies at higher Reynolds numbers, both as a function of the Reynolds number. Simulations are used to examine the velocity fluctuations, flow topologies, and the fluctuating forces on the cylinders.
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11

BARRY, D. A., and J. Y. PARLANGE. "Recirculation within a fluid sphere at moderate Reynolds numbers." Journal of Fluid Mechanics 465 (August 25, 2002): 293–300. http://dx.doi.org/10.1017/s0022112002001167.

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Motion of a single fluid sphere is described by two theories, each characterized by different levels of Hill's vortex circulation within the sphere. An existing experimental data set giving measurements of vertical velocity along the major axis of the sphere is re-examined. Contrary to published discussions of that experiment, we find that the theory of Parlange agrees better with the laboratory data than that of Harper & Moore. This agreement supports the key difference between the two theories, i.e. that the fluid within the sphere is unlikely to have a singular (infinite) velocity as it moves upwards towards the stagnation region at the top of the sphere.
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12

Pirozzoli, Sergio, and Matteo Bernardini. "Turbulence in supersonic boundary layers at moderate Reynolds number." Journal of Fluid Mechanics 688 (October 21, 2011): 120–68. http://dx.doi.org/10.1017/jfm.2011.368.

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AbstractWe study the organization of turbulence in supersonic boundary layers through large-scale direct numerical simulations (DNS) at ${M}_{\infty } = 2$, and momentum-thickness Reynolds number up to ${\mathit{Re}}_{{\delta }_{2} } \approx 3900$ (corresponding to ${\mathit{Re}}_{\tau } \approx 1120$) which significantly extend the current envelope of DNS in the supersonic regime. The numerical strategy relies on high-order, non-dissipative discretization of the convective terms in the Navier–Stokes equations, and it implements a recycling/rescaling strategy to stimulate the inflow turbulence. Comparison of the velocity statistics up to fourth order shows nearly exact agreement with reference incompressible data, provided the momentum-thickness Reynolds number is matched, and provided the mean velocity and the velocity fluctuations are scaled to incorporate the effects of mean density variation, as postulated by Morkovin’s hypothesis. As also found in the incompressible regime, we observe quite a different behaviour of the second-order flow statistics at sufficiently large Reynolds number, most of which show the onset of a range with logarithmic variation, typical of ‘attached’ variables, whereas the wall-normal velocity exhibits a plateau away from the wall, which is typical of ‘detached’ variables. The modifications of the structure of the flow field that underlie this change of behaviour are highlighted through visualizations of the velocity and temperature fields, which substantiate the formation of large jet-like and wake-like motions in the outer part of the boundary layer. It is found that the typical size of the attached eddies roughly scales with the local mean velocity gradient, rather than being proportional to the wall distance, as happens for the wall-detached variables. The interactions of the large eddies in the outer layer with the near-wall region are quantified through a two-point amplitude modulation covariance, which characterizes the modulating action of energetic outer-layer eddies.
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13

Kitamura, T., K. Nagata, Y. Sakai, A. Sasoh, O. Terashima, H. Saito, and T. Harasaki. "On invariants in grid turbulence at moderate Reynolds numbers." Journal of Fluid Mechanics 738 (December 6, 2013): 378–406. http://dx.doi.org/10.1017/jfm.2013.595.

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AbstractThe decay characteristics and invariants of grid turbulence were investigated by means of laboratory experiments conducted in a wind tunnel. A turbulence-generating grid was installed at the entrance of the test section for generating nearly isotropic turbulence. Five grids (square bars of mesh sizes $M= 15$, 25 and 50 mm and cylindrical bars of mesh sizes $M= 10$ and 25 mm) were used. The solidity of all grids is $\sigma = 0. 36$. The instantaneous streamwise and vertical (cross-stream) velocities were measured by hot-wire anemometry. The mesh Reynolds numbers were adjusted to $R{e}_{M} = 6700$, 9600, 16 000 and 33 000. The Reynolds numbers based on the Taylor microscale $R{e}_{\lambda } $ in the decay region ranged from 27 to 112. In each case, the result shows that the decay exponent of turbulence intensity is close to the theoretical value of ${- }6/ 5$ (for the $M= 10~\mathrm{mm} $ grid, ${- }6(1+ p)/ 5\sim - 1. 32$) for Saffman turbulence. Here, $p$ is the power of the dimensionless energy dissipation coefficient, $A(t)\sim {t}^{p} $. Furthermore, each case shows that streamwise variations in the integral length scales, ${L}_{uu} $ and ${L}_{vv} $, and the Taylor microscale $\lambda $ grow according to ${L}_{uu} \sim 2{L}_{vv} \propto {(x/ M- {x}_{0} / M)}^{2/ 5} $ (for the $M= 10~\mathrm{mm} $ grid, ${L}_{uu} \propto {(x/ M- {x}_{0} / M)}^{2(1+ p)/ 5} \sim {(x/ M- {x}_{0} / M)}^{0. 44} $) and $\lambda \propto {(x/ M- {x}_{0} / M)}^{1/ 2} $, respectively, at $x/ M\gt 40{\unicode{x2013}} 60$ (depending on the experimental conditions, including grid geometry), where $x$ is the streamwise distance from the grid and ${x}_{0} $ is the virtual origin. We demonstrated that in the decay region of grid turbulence, ${ u}_{\mathit{rms}}^{2} { L}_{uu}^{3} $ and ${ v}_{\mathit{rms}}^{2} { L}_{vv}^{3} $, which correspond to Saffman’s integral, are constant for all grids and examined $R{e}_{M} $ values. However, ${ u}_{\mathit{rms}}^{2} { L}_{uu}^{5} $ and ${ v}_{\mathit{rms}}^{2} { L}_{vv}^{5} $, which correspond to Loitsianskii’s integral, and ${ u}_{\mathit{rms}}^{2} { L}_{uu}^{2} $ and ${ v}_{\mathit{rms}}^{2} { L}_{vv}^{2} $, which correspond to the complete self-similarity of energy spectrum and $\langle {\boldsymbol{u}}^{2} \rangle \sim {t}^{- 1} $, are not constant. Consequently, we conclude that grid turbulence is a type of Saffman turbulence for the examined $R{e}_{M} $ range of 6700–33 000 ($R{e}_{\lambda } = 27{\unicode{x2013}} 112$) regardless of grid geometry.
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14

Dasgupta, Ratul, and Gaurav Tomar. "Viscous Undular Hydraulic Jumps of Moderate Reynolds Number Flows." Procedia IUTAM 15 (2015): 300–304. http://dx.doi.org/10.1016/j.piutam.2015.04.042.

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15

Eldredge, Jeff D. "Numerical simulations of undulatory swimming at moderate Reynolds number." Bioinspiration & Biomimetics 1, no. 4 (December 1, 2006): S19—S24. http://dx.doi.org/10.1088/1748-3182/1/4/s03.

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16

JIMÉNEZ, JAVIER, SERGIO HOYAS, MARK P. SIMENS, and YOSHINORI MIZUNO. "Turbulent boundary layers and channels at moderate Reynolds numbers." Journal of Fluid Mechanics 657 (June 2, 2010): 335–60. http://dx.doi.org/10.1017/s0022112010001370.

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The behaviour of the velocity and pressure fluctuations in the outer layers of wall-bounded turbulent flows is analysed by comparing a new simulation of the zero-pressure-gradient boundary layer with older simulations of channels. The 99 % boundary-layer thickness is used as a reasonable analogue of the channel half-width, but the two flows are found to be too different for the analogy to be complete. In agreement with previous results, it is found that the fluctuations of the transverse velocities and of the pressure are stronger in the boundary layer, and this is traced to the pressure fluctuations induced in the outer intermittent layer by the differences between the potential and rotational flow regions. The same effect is also shown to be responsible for the stronger wake component of the mean velocity profile in external flows, whose increased energy production is the ultimate reason for the stronger fluctuations. Contrary to some previous results by our group, and by others, the streamwise velocity fluctuations are also found to be higher in boundary layers, although the effect is weaker. Within the limitations of the non-parallel nature of the boundary layer, the wall-parallel scales of all the fluctuations are similar in both the flows, suggesting that the scale-selection mechanism resides just below the intermittent region, y/δ = 0.3–0.5. This is also the location of the largest differences in the intensities, although the limited Reynolds number of the boundary-layer simulation (Reθ ≈ 2000) prevents firm conclusions on the scaling of this location. The statistics of the new boundary layer are available from http://torroja.dmt.upm.es/ftp/blayers/.
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17

Perot, J. B., and S. M. De Bruyn Kops. "Modeling turbulent dissipation at low and moderate Reynolds numbers." Journal of Turbulence 7 (January 2006): N69. http://dx.doi.org/10.1080/14685240600907310.

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18

Kheshgi, Haroon S. "Profile equations for film flows at moderate Reynolds numbers." AIChE Journal 35, no. 10 (October 1989): 1719–27. http://dx.doi.org/10.1002/aic.690351017.

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19

James, David F. "Flow in a converging channel at moderate reynolds numbers." AIChE Journal 37, no. 1 (January 1991): 59–64. http://dx.doi.org/10.1002/aic.690370105.

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20

Lubbersen, Y. S., M. A. I. Schutyser, and R. M. Boom. "Suspension separation with deterministic ratchets at moderate Reynolds numbers." Chemical Engineering Science 73 (May 2012): 314–20. http://dx.doi.org/10.1016/j.ces.2012.02.002.

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21

Iverson, Dylan, Matthieu Boudreau, Guy Dumas, and Peter Oshkai. "Boundary layer tripping on moderate Reynolds number oscillating foils." Journal of Fluids and Structures 86 (April 2019): 1–12. http://dx.doi.org/10.1016/j.jfluidstructs.2019.01.012.

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22

Erofeev, A. I., and V. P. Provotorov. "Properties of hypersonic separated flows at moderate reynolds numbers." Fluid Dynamics 35, no. 1 (January 2000): 108–16. http://dx.doi.org/10.1007/bf02698795.

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23

Yatsenko, V. P., and V. V. Alexandrov. "Measuring of the Magnus Force at Moderate Reynolds Numbers." International Journal of Fluid Mechanics Research 31, no. 5 (2004): 515–21. http://dx.doi.org/10.1615/interjfluidmechres.v31.i5.90.

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24

Cocetta, Francesco, Mike Gillard, Joanna Szmelter, and Piotr K. Smolarkiewicz. "Stratified flow past a sphere at moderate Reynolds numbers." Computers & Fluids 226 (August 2021): 104998. http://dx.doi.org/10.1016/j.compfluid.2021.104998.

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25

Sadikin, Azmahani, Nurul Akma Mohd Yunus, Kamil Abdullah, and Akmal Nizam Mohammed. "Numerical Study of Flow Past a Solid Sphere at Moderate Reynolds Number." Applied Mechanics and Materials 660 (October 2014): 674–78. http://dx.doi.org/10.4028/www.scientific.net/amm.660.674.

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The unsteady three dimensional flow simulation around sphere using numerical simulation computational fluid dynamic for moderate Reynolds Number between 20 ≤ Re ≤ 500 is presented. The aim of this work is to analyze the flow regimes around sphere and flow separation. Extensive comparisons were made between the present predicted results and available experimental and numerical investigations, and showed that they are in close agreement. The results show that the vortex shedding increases with the Reynolds number. The flow separates early when Reynolds number increases, therefore the separation angle is found to be smaller when high Reynolds number is present.
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26

Oliver, D. L. R., and J. N. Chung. "Flow about a fluid sphere at low to moderate Reynolds numbers." Journal of Fluid Mechanics 177 (April 1987): 1–18. http://dx.doi.org/10.1017/s002211208700082x.

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The steady-state equations of motion are solved for a fluid sphere translating in a quiescent medium. A semi-analytical series truncation method is employed in conjunction with a cubic finite-element scheme. The range of Reynolds numbers investigated is from 0.5 to 50. The range of viscosity ratios is from 0 (gas bubble) to 107 (solid sphere). The flow structure and the drag coefficients agree closely with the limited available experimental measurements and also compare favourably with published finite-difference solutions. The strength of the internal circulation was found to increase with increasing Reynolds number. The flow patterns and the drag coefficient show little variation with the interior Reynolds number. Based on the numerical results, predictive equations for drag coefficients are recommended for both moderate- and low-Reynolds-number flows.
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27

HILL, REGHAN J., DONALD L. KOCH, and ANTHONY J. C. LADD. "Moderate-Reynolds-number flows in ordered and random arrays of spheres." Journal of Fluid Mechanics 448 (November 26, 2001): 243–78. http://dx.doi.org/10.1017/s0022112001005936.

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Lattice-Boltzmann simulations are used to examine the effects of fluid inertia, at moderate Reynolds numbers, on flows in simple cubic, face-centred cubic and random arrays of spheres. The drag force on the spheres, and hence the permeability of the arrays, is calculated as a function of the Reynolds number at solid volume fractions up to the close-packed limits of the arrays. At Reynolds numbers up to O(102), the non-dimensional drag force has a more complex dependence on the Reynolds number and the solid volume fraction than suggested by the well-known Ergun correlation, particularly at solid volume fractions smaller than those that can be achieved in physical experiments. However, good agreement is found between the simulations and Ergun's correlation at solid volume fractions approaching the close-packed limit. For ordered arrays, the drag force is further complicated by its dependence on the direction of the flow relative to the axes of the arrays, even though in the absence of fluid inertia the permeability is isotropic. Visualizations of the flows are used to help interpret the numerical results. For random arrays, the transition to unsteady flow and the effect of moderate Reynolds numbers on hydrodynamic dispersion are discussed.
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28

ESMAEELI, ASGHAR, and GRÉTAR TRYGGVASON. "Direct numerical simulations of bubbly flows Part 2. Moderate Reynolds number arrays." Journal of Fluid Mechanics 385 (April 25, 1999): 325–58. http://dx.doi.org/10.1017/s0022112099004310.

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Direct numerical simulations of the motion of two- and three-dimensional finite Reynolds number buoyant bubbles in a periodic domain are presented. The full Navier–Stokes equations are solved by a finite difference/front tracking method that allows a fully deformable interface between the bubbles and the ambient fluid and the inclusion of surface tension. The rise Reynolds numbers are around 20–30 for the lowest volume fraction, but decrease as the volume fraction is increased. The rise of a regular array of bubbles, where the relative positions of the bubbles are fixed, is compared with the evolution of a freely evolving array. Generally, the freely evolving array rises slower than the regular one, in contrast to what has been found earlier for low Reynolds number arrays. The structure of the bubble distribution is examined and it is found that while the three-dimensional bubbles show a tendency to line up horizontally, the two-dimensional bubbles are nearly randomly distributed. The effect of the number of bubbles in each period is examined for the two-dimensional system and it is found that although the rise Reynolds number is nearly independent of the number of bubbles, the velocity fluctuations in the liquid (the Reynolds stresses) increase with the size of the system. While some aspects of the fully three-dimensional flows, such as the reduction in the rise velocity, are predicted by results for two-dimensional bubbles, the structure of the bubble distribution is not. The magnitude of the Reynolds stresses is also greatly over-predicted by the two-dimensional results.
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29

ZETTNER, C. M., and M. YODA. "Moderate-aspect-ratio elliptical cylinders in simple shear with inertia." Journal of Fluid Mechanics 442 (August 24, 2001): 241–66. http://dx.doi.org/10.1017/s0022112001005006.

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The effects of fluid inertia, geometry and flow confinement upon the dynamics of neutrally buoyant elliptical and non-elliptical cylinders over a wide range of aspect ratios in simple shear are studied experimentally for moderate shear-based Reynolds numbers Re. Unlike circular cylinders, elliptical cylinders of moderate aspect ratio cease to rotate, coming to rest at a nearly horizontal equilibrium orientation above a critical Reynolds number Recr (‘stationary behaviour’). Simple dynamics arguments are proposed to explain the effects of aspect ratio and flow confinement upon critical Reynolds number and particle dynamics. Experiments confirm results from previous numerical simulations that the normalized rotation period for Re < Recr (‘periodic behaviour’) is proportional to (Recr − Re)−0.5 for small Recr − Re. For periodic behaviour, maximum and minimum angular cylinder speeds both decrease, and period increases, as Recr − Re decreases. For stationary behaviour, the cylinder rotates until it achieves a nearly horizontal equilibrium orientation, which increases as the Reynolds number approaches the critical value. The experimental results are in good agreement with previous lattice-Boltzmann simulations for a 0.5 aspect ratio cylinder.Variation in angular speed over a rotation period decreases as aspect ratio increases, while Recr increases as flow confinement and aspect ratio increase. A non-elliptical cylinder of 0.33 aspect ratio also ceases to rotate above a certain Reynolds number. Although Recr is different from the corresponding elliptical case, the scaling of the normalized rotation period for this body as Recr → Re is identical to that for the elliptical cylinder, suggesting that this scaling is independent of particle shape (i.e. ‘universal’, as conjectured in previous numerical studies). The results also demonstrate that a variety of centrosymmetric bodies with aspect ratios below unity transition from periodic to stationary behaviour.
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30

Wu, J. S., and G. M. Faeth. "Sphere wakes at moderate Reynolds numbers in a turbulent environment." AIAA Journal 32, no. 3 (March 1994): 535–41. http://dx.doi.org/10.2514/3.12018.

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31

Mace, J. L., and T. C. Adamson. "Shock waves in transonic channel flows at moderate Reynolds numbers." AIAA Journal 24, no. 4 (April 1986): 591–98. http://dx.doi.org/10.2514/3.9312.

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32

Lapenna, P. E., and F. Creta. "Direct Numerical Simulation of Transcritical Jets at Moderate Reynolds Number." AIAA Journal 57, no. 6 (June 2019): 2254–63. http://dx.doi.org/10.2514/1.j058360.

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33

WHITE, BRIAN L., and HEIDI M. NEPF. "Scalar transport in random cylinder arrays at moderate Reynolds number." Journal of Fluid Mechanics 487 (June 25, 2003): 43–79. http://dx.doi.org/10.1017/s0022112003004579.

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34

Fonseca, F., and H. J. Herrmann. "Sedimentation of oblate ellipsoids at low and moderate Reynolds numbers." Physica A: Statistical Mechanics and its Applications 342, no. 3-4 (November 2004): 447–61. http://dx.doi.org/10.1016/j.physa.2004.05.043.

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35

Panides, E., and R. Chevray. "Vortex dynamics in a plane, moderate-Reynolds-number shear layer." Journal of Fluid Mechanics 214, no. -1 (May 1990): 411. http://dx.doi.org/10.1017/s0022112090000180.

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36

Uyttendaele, Marc A. J., and Robert L. Shambaugh. "The flow field of annular jets at moderate Reynolds numbers." Industrial & Engineering Chemistry Research 28, no. 11 (November 1989): 1735–40. http://dx.doi.org/10.1021/ie00095a027.

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37

Choi, Daehyun, and Hyungmin Park. "Flow around in-line sphere array at moderate Reynolds number." Physics of Fluids 30, no. 9 (September 2018): 097104. http://dx.doi.org/10.1063/1.5049734.

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38

Thompson, Charles, Kavitha Chandra, and Allan D. Pierce. "Acoustic streaming in a channel a moderate streaming Reynolds number." Journal of the Acoustical Society of America 144, no. 3 (September 2018): 1985. http://dx.doi.org/10.1121/1.5068667.

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39

Xiong, Xiangming, Jianjun Tao, Shiyi Chen, and Luca Brandt. "Turbulent bands in plane-Poiseuille flow at moderate Reynolds numbers." Physics of Fluids 27, no. 4 (April 2015): 041702. http://dx.doi.org/10.1063/1.4917173.

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40

Puga, Alejandro J., and John C. LaRue. "Normalized dissipation rate in a moderate Taylor Reynolds number flow." Journal of Fluid Mechanics 818 (March 29, 2017): 184–204. http://dx.doi.org/10.1017/jfm.2017.47.

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Time-resolved velocity measurements are obtained using a hot-wire in a nearly homogeneous and isotropic flow downstream of an active grid for a range of Taylor Reynolds numbers from$191$to$659$. It is found that the dimensionless dissipation rate,$C_{\unicode[STIX]{x1D716}}$, is nearly a constant for sufficiently high values of Taylor Reynolds number,$R_{\unicode[STIX]{x1D706},u_{q}}$, and is approximately equal to$0.87$. This value is approximately$5\,\%$less than the value reported by Boset al.(Phys. Fluids, vol. 19 (4), 2007, 045101), which is obtained using DNS/LES (direct numerical simulation combined with large eddy simulation) for decaying homogeneous and isotropic turbulence, and is in excellent agreement with the active grid experiment of Thormann & Meneveau (Phys. Fluids, vol. 26 (2), 2014, 025112.). The results presented herein show that deviation from isotropy may cause inconsistencies in the computation of$C_{\unicode[STIX]{x1D716}}$. As a result, it is suggested that the velocity scale be the square root of the turbulence kinetic energy. The integral length scale measurements obtained from the longitudinal velocity correlation are in close agreement with the integral length scale measured from the peak of the energy spectrum,$\unicode[STIX]{x1D705}E_{11}(\unicode[STIX]{x1D705})$, where$\unicode[STIX]{x1D705}$is the wavenumber and$E_{11}(\unicode[STIX]{x1D705})$is the one-dimensional power spectrum of the downstream velocity.
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41

Koch, Donald L. "Hydrodynamic diffusion in dilute sedimenting suspensions at moderate Reynolds numbers." Physics of Fluids A: Fluid Dynamics 5, no. 5 (May 1993): 1141–55. http://dx.doi.org/10.1063/1.858600.

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42

Shatskiy, Evgeny, and Evgeny Chinnov. "Thermocapillary rupture in falling liquid films at moderate Reynolds numbers." EPJ Web of Conferences 159 (2017): 00055. http://dx.doi.org/10.1051/epjconf/201715900055.

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43

Dargush, G. F., and P. K. Banerjee. "A time-dependent incompressible viscous BEM for moderate Reynolds numbers." International Journal for Numerical Methods in Engineering 31, no. 8 (June 1991): 1627–48. http://dx.doi.org/10.1002/nme.1620310812.

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44

Sreenivasan, K. R., A. Juneja, and A. K. Suri. "Scaling Properties of Circulation in Moderate-Reynolds-Number Turbulent Wakes." Physical Review Letters 75, no. 3 (July 17, 1995): 433–36. http://dx.doi.org/10.1103/physrevlett.75.433.

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45

Minakov, A. V., V. Ya Rudyak, A. A. Gavrilov, and A. A. Dekterev. "Mixing in a T-shaped micromixer at moderate Reynolds numbers." Thermophysics and Aeromechanics 19, no. 3 (September 2012): 385–95. http://dx.doi.org/10.1134/s0869864312030043.

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46

Thoroddsen, S. T. "Conditional sampling of dissipation in moderate Reynolds number grid turbulence." Physics of Fluids 8, no. 5 (May 1996): 1333–35. http://dx.doi.org/10.1063/1.868903.

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47

Thompson, Charles, Jairo Vanegas, Russell Perkins, Flore Norceide, Ivette Alvarez, and Kavitha Chandra. "Acoustic streaming in a channel a moderate streaming Reynolds number." Journal of the Acoustical Society of America 145, no. 3 (March 2019): 1817. http://dx.doi.org/10.1121/1.5101639.

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48

Kotelnikov, Alexei D., and David C. Montgomery. "Shock induced turbulence in composite materials at moderate Reynolds numbers." Physics of Fluids 10, no. 8 (August 1998): 2037–54. http://dx.doi.org/10.1063/1.869719.

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49

Valluri, Prashant, Omar K. Matar, Geoffrey F. Hewitt, and M. A. Mendes. "Thin film flow over structured packings at moderate Reynolds numbers." Chemical Engineering Science 60, no. 7 (April 2005): 1965–75. http://dx.doi.org/10.1016/j.ces.2004.12.008.

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50

Kim, Moon-Sang, Hae-Moon Jeon, and Yeong-Taek Lim. "Unsteady viscous flows past blunt bodies at moderate Reynolds numbers." Journal of Mechanical Science and Technology 22, no. 11 (November 2008): 2286–98. http://dx.doi.org/10.1007/s12206-008-0618-z.

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