Transition to chaos in the wake of a rolling sphere
Identifieur interne : 001268 ( PascalFrancis/Corpus ); précédent : 001267; suivant : 001269Transition to chaos in the wake of a rolling sphere
Auteurs : A. Rao ; P.-Y. Passaggia ; H. Bolnot ; M. C. Thompson ; T. Leweke ; K. HouriganSource :
- Journal of Fluid Mechanics [ 0022-1120 ] ; 2012.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
The wake of a sphere rolling along a wall at low Reynolds number is investigated numerically and experimentally. Two successive transitions are identified in this flow, as the Reynolds number is increased. The first leads to the periodic shedding of planar symmetric hairpin vortices. The second and previously unknown transition involves a loss of planar symmetry and a low-frequency lateral oscillation of the wake, exhibiting a surprising 7:3 resonance with the hairpin vortex shedding. The two transitions are characterized by dye visualizations and quantitative information obtained from numerical simulations, such as force coefficients and wake frequencies (Strouhal numbers). Both transitions are found to be supercritical. Further increasing the Reynolds number, the flow becomes progressively more disorganized and chaotic. Overall, the transition sequence for the rolling sphere is closer to the one for a non-rotating sphere in a free stream than to that of a non-rotating sphere close to a wall.
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Format Inist (serveur)
NO : | PASCAL 12-0264427 INIST |
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ET : | Transition to chaos in the wake of a rolling sphere |
AU : | RAO (A.); PASSAGGIA (P.-Y.); BOLNOT (H.); THOMPSON (M. C.); LEWEKE (T.); HOURIGAN (K.) |
AF : | Fluids Laboratory for Aeronautical and Industrial Research (FLAIR), Department of Mechanical and Aerospace Engineering, Monash University/Melbourne, VIC 3800/Australie (1 aut., 4 aut., 6 aut.); Institut de Recherche sur les Phenomenes Hors-Équilibre (IRPHE), CNRS/Aix-Marseille Universite/13384 Marseille/France (2 aut., 3 aut., 5 aut.); Division of Biological Engineering, Monash University/Melbourne, VIC 3800/Australie (6 aut.) |
DT : | Publication en série; Niveau analytique |
SO : | Journal of Fluid Mechanics; ISSN 0022-1120; Coden JFLSA7; Royaume-Uni; Da. 2012; Vol. 695; Pp. 135-148; Bibl. 1 p.1/4 |
LA : | Anglais |
EA : | The wake of a sphere rolling along a wall at low Reynolds number is investigated numerically and experimentally. Two successive transitions are identified in this flow, as the Reynolds number is increased. The first leads to the periodic shedding of planar symmetric hairpin vortices. The second and previously unknown transition involves a loss of planar symmetry and a low-frequency lateral oscillation of the wake, exhibiting a surprising 7:3 resonance with the hairpin vortex shedding. The two transitions are characterized by dye visualizations and quantitative information obtained from numerical simulations, such as force coefficients and wake frequencies (Strouhal numbers). Both transitions are found to be supercritical. Further increasing the Reynolds number, the flow becomes progressively more disorganized and chaotic. Overall, the transition sequence for the rolling sphere is closer to the one for a non-rotating sphere in a free stream than to that of a non-rotating sphere close to a wall. |
CC : | 001B40G32F; 001B40G52 |
FD : | Ecoulement tourbillonnaire; Détachement tourbillonnaire; Système chaotique; Sillage; Simulation numérique; Etude expérimentale; Roulement; Sphère; 4732F; 4752 |
ED : | Vortex flow; Vortex shedding; Chaotic systems; Wakes; Digital simulation; Experimental study; Rolling (mechanics); Spheres |
SD : | Desprendimiento vorticial; Rodadura |
LO : | INIST-5180.354000509322280060 |
ID : | 12-0264427 |
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Pascal:12-0264427Le document en format XML
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<front><div type="abstract" xml:lang="en">The wake of a sphere rolling along a wall at low Reynolds number is investigated numerically and experimentally. Two successive transitions are identified in this flow, as the Reynolds number is increased. The first leads to the periodic shedding of planar symmetric hairpin vortices. The second and previously unknown transition involves a loss of planar symmetry and a low-frequency lateral oscillation of the wake, exhibiting a surprising 7:3 resonance with the hairpin vortex shedding. The two transitions are characterized by dye visualizations and quantitative information obtained from numerical simulations, such as force coefficients and wake frequencies (Strouhal numbers). Both transitions are found to be supercritical. Further increasing the Reynolds number, the flow becomes progressively more disorganized and chaotic. Overall, the transition sequence for the rolling sphere is closer to the one for a non-rotating sphere in a free stream than to that of a non-rotating sphere close to a wall.</div>
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<ET>Transition to chaos in the wake of a rolling sphere</ET>
<AU>RAO (A.); PASSAGGIA (P.-Y.); BOLNOT (H.); THOMPSON (M. C.); LEWEKE (T.); HOURIGAN (K.)</AU>
<AF>Fluids Laboratory for Aeronautical and Industrial Research (FLAIR), Department of Mechanical and Aerospace Engineering, Monash University/Melbourne, VIC 3800/Australie (1 aut., 4 aut., 6 aut.); Institut de Recherche sur les Phenomenes Hors-Équilibre (IRPHE), CNRS/Aix-Marseille Universite/13384 Marseille/France (2 aut., 3 aut., 5 aut.); Division of Biological Engineering, Monash University/Melbourne, VIC 3800/Australie (6 aut.)</AF>
<DT>Publication en série; Niveau analytique</DT>
<SO>Journal of Fluid Mechanics; ISSN 0022-1120; Coden JFLSA7; Royaume-Uni; Da. 2012; Vol. 695; Pp. 135-148; Bibl. 1 p.1/4</SO>
<LA>Anglais</LA>
<EA>The wake of a sphere rolling along a wall at low Reynolds number is investigated numerically and experimentally. Two successive transitions are identified in this flow, as the Reynolds number is increased. The first leads to the periodic shedding of planar symmetric hairpin vortices. The second and previously unknown transition involves a loss of planar symmetry and a low-frequency lateral oscillation of the wake, exhibiting a surprising 7:3 resonance with the hairpin vortex shedding. The two transitions are characterized by dye visualizations and quantitative information obtained from numerical simulations, such as force coefficients and wake frequencies (Strouhal numbers). Both transitions are found to be supercritical. Further increasing the Reynolds number, the flow becomes progressively more disorganized and chaotic. Overall, the transition sequence for the rolling sphere is closer to the one for a non-rotating sphere in a free stream than to that of a non-rotating sphere close to a wall.</EA>
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