scholarly journals Asymptotic turbulent friction in 2D rough-walled flows

2021 ◽  
Vol 7 (5) ◽  
pp. eabc6234
Author(s):  
Alexandre Vilquin ◽  
Julie Jagielka ◽  
Simeon Djambov ◽  
Hugo Herouard ◽  
Patrick Fisher ◽  
...  

The friction f is the property of wall-bounded flows that sets the pumping cost of a pipeline, the draining capacity of a river, and other variables of practical relevance. For highly turbulent rough-walled pipe flows, f depends solely on the roughness length scale r, and the f − r relation may be expressed by the Strickler empirical scaling f ∝ r1/3. Here, we show experimentally that for soap film flows that are the two-dimensional (2D) equivalent of highly turbulent rough-walled pipe flows, f ∝ r and the f − r relation is not the same in 2D as in 3D. Our findings are beyond the purview of the standard theory of friction but consistent with a competing theory in which f is linked to the turbulent spectrum via the spectral exponent α: In 3D, α = 5/3 and the theory yields f ∝ r1/3; in 2D, α = 3 and the theory yields f ∝ r.


2009 ◽  
Vol 79 (6) ◽  
Author(s):  
Nicholas Guttenberg ◽  
Nigel Goldenfeld


1999 ◽  
Vol 11 (8) ◽  
pp. 2167-2177 ◽  
Author(s):  
P. Vorobieff ◽  
M. Rivera ◽  
R. E. Ecke
Keyword(s):  


2014 ◽  
Vol 26 (5) ◽  
pp. 055105 ◽  
Author(s):  
M. K. Rivera ◽  
H. Aluie ◽  
R. E. Ecke


Author(s):  
David Lovett ◽  
John Tilley
Keyword(s):  


2003 ◽  
Vol 259 (5) ◽  
pp. 1011-1036 ◽  
Author(s):  
A.E. VARDY ◽  
J.M.B. BROWN


1997 ◽  
Vol 9 (9) ◽  
pp. S2-S2 ◽  
Author(s):  
P. D. Weidman ◽  
V. O. Afenchenko ◽  
A. B. Ezersky ◽  
S. V. Kiyashko ◽  
M. I. Rabinovich


2017 ◽  
Vol 815 ◽  
pp. 77-116 ◽  
Author(s):  
S. Viroulet ◽  
J. L. Baker ◽  
A. N. Edwards ◽  
C. G. Johnson ◽  
C. Gjaltema ◽  
...  

Geophysical granular flows, such as avalanches, debris flows, lahars and pyroclastic flows, are always strongly influenced by the basal topography that they flow over. In particular, localised bumps or obstacles can generate rapid changes in the flow thickness and velocity, or shock waves, which dissipate significant amounts of energy. Understanding how a granular material is affected by the underlying topography is therefore crucial for hazard mitigation purposes, for example to improve the design of deflecting or catching dams for snow avalanches. Moreover, the interactions with solid boundaries can also have important applications in industrial processes. In this paper, small-scale experiments are performed to investigate the flow of a granular avalanche over a two-dimensional smooth symmetrical bump. The experiments show that, depending on the initial conditions, two different steady-state regimes can be observed: either the formation of a detached jet downstream of the bump, or a shock upstream of it. The transition between the two cases can be controlled by adding varying amounts of erodible particles in front of the obstacle. A depth-averaged terrain-following avalanche theory that is formulated in curvilinear coordinates is used to model the system. The results show good agreement with the experiments for both regimes. For the case of a shock, time-dependent numerical simulations of the full system show the evolution to the equilibrium state, as well as the deposition of particles upstream of the bump when the inflow ceases. The terrain-following theory is compared to a standard depth-averaged avalanche model in an aligned Cartesian coordinate system. For this very sensitive problem, it is shown that the steady-shock regime is captured significantly better by the terrain-following avalanche model, and that the standard theory is unable to predict the take-off point of the jet. To retain the practical simplicity of using Cartesian coordinates, but have the improved predictive power of the terrain-following model, a coordinate mapping is used to transform the terrain-following equations from curvilinear to Cartesian coordinates. The terrain-following model, in Cartesian coordinates, makes identical predictions to the original curvilinear formulation, but is much simpler to implement.



2001 ◽  
Vol 442 ◽  
pp. 387-409 ◽  
Author(s):  
JEAN-MARC CHOMAZ

Nearly two decades ago, Couder (1981) and Gharib & Derango (1989) used soap films to perform classical hydrodynamics experiments on two-dimensional flows. Recently soap films have received renewed interest and experimental investigations published in the past few years call for a proper analysis of soap film dynamics. In the present paper, we derive the leading-order approximation for the dynamics of a flat soap film under the sole assumption that the typical length scale of the flow parallel to the film surface is large compared to the film thickness. The evolution equations governing the leading-order film thickness, two-dimensional velocities (locally averaged across the film thickness), average surfactant concentration in the interstitial liquid, and surface surfactant concentration are given and compared to similar results from the literature. Then we show that a sufficient condition for the film velocity distribution to comply with the Navier–Stokes equations is that the typical flow velocity be small compared to the Marangoni elastic wave velocity. In that case the thickness variations are slaved to the velocity field in a very specific way that seems consistent with recent experimental observations. When fluid velocities are of the order of the elastic wave speed, we show that the dynamics are generally very specific to a soap film except if the fluid viscosity and the surfactant solubility are neglected. In that case, the compressible Euler equations are recovered and the soap film behaves like a two-dimensional gas with an unusual ratio of specific heat capacities equal to unity.



1998 ◽  
Vol 10 (2) ◽  
pp. 390-399 ◽  
Author(s):  
V. O. Afenchenko ◽  
A. B. Ezersky ◽  
S. V. Kiyashko ◽  
M. I. Rabinovich ◽  
P. D. Weidman


Fractals ◽  
2002 ◽  
Vol 10 (03) ◽  
pp. 253-264 ◽  
Author(s):  
D. SACHS ◽  
S. LOVEJOY ◽  
D. SCHERTZER

The cloud radiances and atmospheric dynamics are strongly nonlinearly coupled, the observed scaling of the former from 1 km to planetary scales is prima facae evidence for scale invariant dynamics. In contrast, the scaling properties of radiances at scales <1 km have not been well studied (contradictory claims have been made) and if a characteristic vertical cloud thickness existed, it could break the scaling of the horizontal radiances. In order to settle this issue, we use ground-based photography to study the cloud radiance field through the range scales where breaks in scaling have been reported (30 m to 500 m). Over the entire range 1 m to 1 km the two-dimensional (2D) energy spectrum (E(k)) of 38 clouds was found to accurately follow the scaling form E(k)≈ k-β where k is a wave number and β is the spectral exponent. This indirectly shows that there is no characteristic vertical cloud thickness, and that "radiative smoothing" of cloud structures occurs at all scales. We also quantitatively characterize the type of (multifractal) scaling showing that the main difference between transmitted and reflected radiance fields is the (scale-by-scale) non-conservation parameter H. These findings lend support to the unified scaling model of the atmosphere which postulates a single anisotropic scaling regime from planetary down to dissipation scales.



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