TY - JOUR
T1 - Taylor-Couette turbulence at radius ratio η = 0.5
T2 - Scaling, ow structures and plumes
AU - van der Veen, Roeland C.A.
AU - Huisman, Sander G.
AU - Merbold, Sebastian
AU - Harlander, Uwe
AU - Egbers, Christoph
AU - Lohse, Detlef
AU - Sun, Chao
N1 - Publisher Copyright:
© 2016 Cambridge University Press.
PY - 2016/7/25
Y1 - 2016/7/25
N2 - Using high-resolution particle image velocimetry, we measure velocity profiles, the wind Reynolds number and characteristics of turbulent plumes in Taylor-Couette flow for a radius ratio of 0.5 and Taylor number of up to 6.2×109. The extracted angular velocity profiles follow a log law more closely than the azimuthal velocity profiles due to the strong curvature of this η =0.5 set-up. The scaling of the wind Reynolds number with the Taylor number agrees with the theoretically predicted 3/7 scaling for the classical turbulent regime, which is much more pronounced than for the wellexplored η =0.71 case, for which the ultimate regime sets in at much lower Taylor number. By measuring at varying axial positions, roll structures are found for counterrotation while no clear coherent structures are seen for pure inner cylinder rotation. In addition, turbulent plumes coming from the inner and outer cylinders are investigated. For pure inner cylinder rotation, the plumes in the radial velocity move away from the inner cylinder, while the plumes in the azimuthal velocity mainly move away from the outer cylinder. For counter-rotation, the mean radial flow in the roll structures strongly affects the direction and intensity of the turbulent plumes. Furthermore, it is experimentally confirmed that, in regions where plumes are emitted, boundary layer profiles with a logarithmic signature are created.
AB - Using high-resolution particle image velocimetry, we measure velocity profiles, the wind Reynolds number and characteristics of turbulent plumes in Taylor-Couette flow for a radius ratio of 0.5 and Taylor number of up to 6.2×109. The extracted angular velocity profiles follow a log law more closely than the azimuthal velocity profiles due to the strong curvature of this η =0.5 set-up. The scaling of the wind Reynolds number with the Taylor number agrees with the theoretically predicted 3/7 scaling for the classical turbulent regime, which is much more pronounced than for the wellexplored η =0.71 case, for which the ultimate regime sets in at much lower Taylor number. By measuring at varying axial positions, roll structures are found for counterrotation while no clear coherent structures are seen for pure inner cylinder rotation. In addition, turbulent plumes coming from the inner and outer cylinders are investigated. For pure inner cylinder rotation, the plumes in the radial velocity move away from the inner cylinder, while the plumes in the azimuthal velocity mainly move away from the outer cylinder. For counter-rotation, the mean radial flow in the roll structures strongly affects the direction and intensity of the turbulent plumes. Furthermore, it is experimentally confirmed that, in regions where plumes are emitted, boundary layer profiles with a logarithmic signature are created.
KW - Taylor-Couette flow
KW - Turbulent boundary layers
KW - Turbulent flows
KW - 2023 OA procedure
UR - http://www.scopus.com/inward/record.url?scp=84976334302&partnerID=8YFLogxK
U2 - 10.1017/jfm.2016.352
DO - 10.1017/jfm.2016.352
M3 - Article
SN - 0022-1120
VL - 799
SP - 334
EP - 351
JO - Journal of fluid mechanics
JF - Journal of fluid mechanics
ER -