213 research outputs found

    Turbulence drag modulation by dispersed droplets in Taylor-Couette flow: the effects of the dispersed phase viscosity

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    The dispersed phase in turbulence can vary from almost inviscid fluid to highly viscous fluid. By changing the viscosity of the dispersed droplet phase, we experimentally investigate how the deformability of dispersed droplets affects the global transport quantity of the turbulent emulsion. Different kinds of silicone oil are employed to result in the viscosity ratio, ζ\zeta, ranging from 0.530.53 to 8.028.02. The droplet volume fraction, ϕ\phi, is varied from 0\% to 10\% with a spacing of 2\%. The global transport quantity, quantified by the normalized friction coefficient cf,ϕ/cf,ϕ=0c_{f,\phi}/c_{f,\phi=0}, shows a weak dependence on the turbulent intensity due to the vanishing finite-size effect of the droplets. The interesting fact is that, with increasing ζ\zeta, the cf,ϕ/cf,ϕ=0c_{f,\phi}/c_{f,\phi=0} first increases and then saturates to a plateau value which is similar to that of the rigid particle suspension. By performing image analysis, this drag modification is interpreted from the aspect of droplet deformability, which is responsible for the breakup and coalescence effect of the droplets. The statistics of the droplet size distribution show that, with increasing ζ\zeta, the stabilizing effect induced by interfacial tension comes to be substantial and the pure inertial breakup process becomes dominant. The measurement of the droplet distribution along the radial direction of the system shows a bulk-clustering effect, which can be attributed to the non-negligible coalescence effect of the droplet. It is found that the droplet coalescence effect could be suppressed as the ζ\zeta increases, thereby affecting the contribution of interfacial tension to the total stress, and accounting for the observed emulsion rheology.Comment: 17 pages, 8 figure

    Accelerations of large inertial particles in turbulence

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    Understanding the dynamics of material objects advected by turbulent flows is a long standing question in fluid dynamics. In this perspective article we focus on the characterization of the statistical properties of non-interacting finite-sized massive spherical particles advected by a vigorous turbulent flow. We study the fluctuations and temporal correlations of particle accelerations and explore their behaviours with respect to both the particle size and the particle mass density by means of fully-resolved numerical simulations. We observe that the measured trends can not be interpreted as the simple multiplicative combination of the two dominant effects: the spatial filtering of fluid accelerations and the added-mass-adjusted fluid-to-particle density ratio. We argue that other hydrodynamical forces or effects (e.g. preferential flow sampling) have still a significant role even at the largest particle sizes, which are here of the order of the integral scale of turbulence.Comment: 7 pages, 4 figure

    From Rayleigh-B\'enard convection to porous-media convection: how porosity affects heat transfer and flow structure

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    We perform a numerical study of the heat transfer and flow structure of Rayleigh-B\'enard (RB) convection in (in most cases regular) porous media, which are comprised of circular, solid obstacles located on a square lattice. This study is focused on the role of porosity Ï•\phi in the flow properties during the transition process from the traditional RB convection with Ï•=1\phi=1 (so no obstacles included) to Darcy-type porous-media convection with Ï•\phi approaching 0. Simulations are carried out in a cell with unity aspect ratio, for the Rayleigh number RaRa from 10510^5 to 101010^{10} and varying porosities Ï•\phi, at a fixed Prandtl number Pr=4.3Pr=4.3, and we restrict ourselves to the two dimensional case. For fixed RaRa, the Nusselt number NuNu is found to vary non-monotonously as a function of Ï•\phi; namely, with decreasing Ï•\phi, it first increases, before it decreases for Ï•\phi approaching 0. The non-monotonous behaviour of Nu(Ï•)Nu(\phi) originates from two competing effects of the porous structure on the heat transfer. On the one hand, the flow coherence is enhanced in the porous media, which is beneficial for the heat transfer. On the other hand, the convection is slowed down by the enhanced resistance due to the porous structure, leading to heat transfer reduction. For fixed Ï•\phi, depending on RaRa, two different heat transfer regimes are identified, with different effective power-law behaviours of NuNu vs RaRa, namely, a steep one for low RaRa when viscosity dominates, and the standard classical one for large RaRa. The scaling crossover occurs when the thermal boundary layer thickness and the pore scale are comparable. The influences of the porous structure on the temperature and velocity fluctuations, convective heat flux, and energy dissipation rates are analysed, further demonstrating the competing effects of the porous structure to enhance or reduce the heat transfer
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