scispace - formally typeset
Journal ArticleDOI

Terminal velocity of porous spheres

TLDR
In this paper, the authors experimentally measured the terminal velocity of porous spheres for a Reynolds number range of 0.2 to 120 and found that the porous sphere terminal velocity was less affected by the container walls than for the case of an impermeable sphere.
Abstract
Terminal velocity of porous spheres was experimentally measured for a Reynolds number range of 0.2 to 120 for a normalized sphere radius, β = R/R of 15.6 to 33, where R and k are the sphere radius and permeability, respectively. The drag coefficient for 15 < β < 33 was found to be CD = 24Ω/Re [1 + 0.1315 Re(0.82 - 0.05w)] for 0.1 < Re ≤ 7 and CD = 24Ω/Re [1 + 0.0853 Re(1.093 - 0.105w)] for 7 < Re < 120 with w = log10Re where Re is the sphere Reynolds number and Ω=2β2 [1 - (tanh β/β)] / 2β2 + 3[1 - tanh β/β)] At high Reynolds numbers, it was found that the porous sphere terminal velocity was less affected by the container walls than for the case of an impermeable sphere. However, at very low Reynolds numbers, the wall effects were found to be similar for both the permeable and the impermeable spheres. On a mesure experimentalement la vitesse de chute libre de spheres poreuses, pour des nombres de Reynolds variant entre 0.2 et 120, et pour un rayon normalise de sphere( β = R/k) de 15.6 a 33; R et k sont respectivement le rayon et la permeabilite de la sphere. On a trouve que le coefficient de frottement, dans le cas ou 15 < β < 33, etait: CD = 24Ω/Re [1 + 0.1315 Re(0.82 - 0.05 w)] lorsque 0.1 < Re ≤ 7 et CD = 24Ω/Re [1 + 0.0853 Re(1.093-0.105 w)] lorsque 7 < Re < 120 w = log10ReRe est le nombre de Reynolds de la sphere et Ω = 2β2 [1 - (tanh β/β)]/2β2 + 3[1 - (tanh β/β)] On a trouve que, pour des nombres de Reynolds eleves, la vitesse limite de la sphere poreuse etait moins affectee par les parois du contenant que lorsqil agissait d'une sphere impermeable; toutefois, pour des nombres de Reynolds faibles, les effets des parois etaient les měmes, dans le cas de spheres permeables et impermeables.

read more

Citations
More filters
Journal ArticleDOI

Association of sinking organic matter with various types of mineral ballast in the deep sea: Implications for the rain ratio

TL;DR: In this paper, the authors show that most of the organic carbon rain in the deep sea is carried by calcium carbonate, because it is denser than opal and more abundant than terrigenous material.
Journal ArticleDOI

In situ settling behavior of marine snow1

TL;DR: The settling velocities of undisturbed macroscopic aggregates known as marine snow were measured with SCUBA in surface waters off southern California and analyzed as a function of aggregate size, mass, and density as discussed by the authors.
Journal ArticleDOI

Settling Velocities of Fractal Aggregates

TL;DR: In this paper, the authors demonstrate that the settling velocity models based on impermeable spheres do not accurately relate aggregate size, porosity and settling velocity for highly porous fractal aggregates.
Journal ArticleDOI

Momentum transport at a fluid–porous interface

TL;DR: In this article, the momentum balance at the interface between a liquid and a porous substrate is investigated for a configuration with forced flow parallel to the interface, where an heterogeneous continuously varying transition layer between the two outer bulk regions is introduced.
Journal ArticleDOI

Fluidization of biomass particles: A review of experimental multiphase flow aspects

TL;DR: In this article, a review of recent research on the hydrodynamics and mixing of biomass particles in fluidized beds is presented, where the authors have characterized the relevant flow characteristics of the biomass particles and investigated measures that could assist in resolving flow issues.
References
More filters
Journal ArticleDOI

Creeping flow relative to permeable spheres

TL;DR: In this paper, several possible solutions to the problem of creeping flow relative to an isolated permeable sphere are discussed and compared quantitatively, and the most satisfactory solutions are based upon Brinkman's extension of Darcy's Law.
Journal ArticleDOI

Numerical study of steady flow past spheroids

TL;DR: In this article, numerical methods have been used to investigate the steady incompressible flow past oblate and prolate spheroids for Reynolds numbers up to 100, and the ratio of minor to major axis of the spheroid investigated were 0·9, 0·5 and 0·2, together with 1·0, which represents the limiting case of a sphere.
Related Papers (5)