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  • 1
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 3 (1991), S. 2758-2776 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The motion of small spherical solid particles is simulated numerically in a homogeneous turbulent gas shear flow generated by the large eddy simulation for two different mean shear rates (Γ), 12.9 sec−1 and 44 sec−1, which correspond to two different flow regimes. The results include a detailed study of the effect of the particle's inertia and the particle's free-fall velocity in still fluid (vd) on the particle dispersion and settling velocities. Let 〈YiYj〉 be the displacement tensor of the particles, where subscripts 1, 2, and 3 refer to the streamwise, the upward, and the spanwise directions, respectively. For the case with Γ=12.9 sec−1, the turbulence intensity of the flow decreases as time (t) increases and approaches an essentially constant value. It was found that 〈Y21〉∝t3, 〈Y22〉∝t, and 〈Y23〉∝t essentially when Γt=3–5, which agrees with the asymptotic behavior of the previous theoretical result for the fluid point dispersion in a stationary sheared turbulence. For the case with Γ=44 sec−1, the turbulence intensity of the flow increases with time monotonically. It was found that 〈Y21〉∝t4, 〈Y1Y2〉∝t3, 〈Y22〉∝t2, and 〈Y23〉∝t2 for large values of Γt. For both cases with different Γ's, a particle falling in the direction perpendicular to the mean flow is found to approach an asymptotic state and the relative velocity between the particle and the fluid reaches a constant value. A particle leads the fluid in the streamwise direction but falls less rapidly in sheared turbulence than that in still fluid. It is also found that the magnitudes of the relative velocity components between the particle and the fluid in a turbulent shear flow are less than those in a corresponding laminar Couette flow.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 2 (1990), S. 63-75 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Detailed numerical simulation has been carried out for fully developed laminar flow through a circular straight pipe with radius a, which is rotating with constant speed Ω about an axis perpendicular to its own axis. The flow is symmetric about a plane containing the pipe axis with its normal parallel to the rotation axis. There are four types of flow regime that result from the various effects of the secondary flow on the main stream via the convection and Coriolis term. When RΩ≤10 and RΩG≤100, the axial velocity profile is essentially axisymmetric and parabolic. Here RΩ=Ωa2/ν and G=G*a3/(ρν2), where G* is the reduced axial pressure gradient driving the flow, ρ is the fluid density, and ν is the kinematic viscosity. When RΩ〈0.85(RΩG)1/3 and RΩG〉100, the axial velocity profile is skewed toward the pressure side with one maximum occurring on the symmetric plane. When RΩ〉1.26(RΩG)2/5 and RΩ〉10, the axial velocity shows a dumbell-like profile with the "dumbell'' center coinciding with the pipe axis and the "dumbell'' axis perpendicular to the symmetric plane. When 0.85(RΩG)1/3≤RΩ≤1.26(RΩG)2/5 and RΩG〉100, the axial velocity profile is skewed toward the pressure size but with two maxima, occurring symmetrically on both sides of the symmetric plane. The present calculation bridges most of the previous asymptotic analyses and provides a correlation formula for the friction factor ratio between the rotating and stationary pipe flow for most of the laminar regime of engineering interest.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 6 (1994), S. 1972-1982 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Some measurements have been obtained for the axial velocity of the fully developed laminar flow in a circular straight pipe with radius a, which is rotating with constant angular speed Ω about an axis perpendicular to its own axis. A diode laser LDA system was mounted together with a circulating pipe flow system on a rotating table for the experiment. According to previous analyses and calculations, there exist four types of axial velocity distributions that result from the various effects of the secondary flow on the main stream via the convection and Coriolis effect for different values of R( = wm'a/ν) and RΩ(=Ωa2/ν), where wm' is the mean axial velocity and ν is the kinematic viscosity of the fluid. The present study provides experimental validation for the previous theoretical and numerical analyses. Experiments have also been carried out for studying the asymptotic nature of the slow flow in a rapidly rotating pipe (RΩ(very-much-greater-than)1 and RΩ(very-much-greater-than)R) and the rapid flow in a slowly rotating pipe (RRΩ(very-much-greater-than)1 and R(very-much-greater-than)RΩ).
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 3 (1991), S. 2571-2586 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The motion of small spherical solid particles are simulated numerically in a decaying homogeneous isotropic turbulent gas flow field generated by the large eddy simulation. By comparing with the previous experimental and theoretical studies, the present method is found to be a successful tool to generate the properties of the particle motion involving the second-order statistics, such as the mean-square displacement, the dispersion coefficient, and the root-mean-square velocity fluctuation. The present results are complementary to the experimental data and include a detailed study of the effects of the flow turbulence, the particle's inertia, and the particle's free-fall velocity in a still fluid on the particle dispersion and turbulence intensity. By performing particle simulation in the flow fields generated with different values of the coefficient in the subgrid model and with different sizes of the calculation domain, it is found that the particle motion is indeed controlled mainly by the large eddies, and there are only minor contributions of the high wave number components of the flow field to the particle motion. Also included in the results is the effect of the turbulence decay on the long time particle dispersion. It is found that the peak value of the dispersion coefficient during the turbulence decay can be correlated with the large-scale Reynolds number and the velocity ratio between the particle's free-fall velocity and the root-mean-square velocity fluctuation of the fluid. Simulation also shows that the particle's settling velocity in turbulence is greater than that in a still fluid.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 5 (1993), S. 2405-2429 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Rigorous analysis shows that the spin synchronous mode fluid motion inside a nutation fluid damper on board of a spinning satellite can be modeled as an incompressible, laminar pulsatile flow in a circular straight pipe. The pipe rotates with constant angular velocity ω(underbar) about an axis perpendicular to its own axis. The distance between the rotation axis and the pipe axis is much greater than a, the pipe's radius. The flow is driven by a three-dimensional harmonic oscillation of the pipe wall with frequency Ω and amplitude w'0, and is governed by three-dimensionless parameters: RΩ(=Ωa2/ν), Δ(=ω/Ω), and A( = w'0/Ωa), where ν is the kinematic viscosity of the fluid. Both the asymptotic analysis and the numerical calculation have been carried out for RΩ=0.1–1000 and Δ=0–2 under A(very-much-less-than)1. It is found that the rotating effect increases the energy dissipation significantly in comparison with the result of the pulsatile straight pipe flow in an inertia frame (the previous theory for the nutation damper). For Δ=1.5, the energy dissipation in a rotating pipe flow is 5.43 times that in a "stationary'' pipe flow for large RΩ, which agrees with the previous experiment. A steady stream is induced by the convective effect for finite values of A. Such steady motion is consisted of axial counter flows together with pairs of counter-rotating vortices in the cross-sectional plane.
    Type of Medium: Electronic Resource
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  • 6
    Publication Date: 2014-03-17
    Print ISSN: 0003-6951
    Electronic ISSN: 1077-3118
    Topics: Physics
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  • 7
    Publication Date: 2009-12-21
    Print ISSN: 0003-6951
    Electronic ISSN: 1077-3118
    Topics: Physics
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  • 8
    Publication Date: 2006-10-16
    Print ISSN: 0003-6951
    Electronic ISSN: 1077-3118
    Topics: Physics
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  • 9
    Publication Date: 2006-10-30
    Print ISSN: 0003-6951
    Electronic ISSN: 1077-3118
    Topics: Physics
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  • 10
    Publication Date: 2010-06-28
    Print ISSN: 0003-6951
    Electronic ISSN: 1077-3118
    Topics: Physics
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