The instability patterns in the flow between counter-rotating disks (radius to height ratio R/h from 3.8 to 20.9) are investigated experimentally by means of visualization and Particle Image Velocimetry. We restrict ourselves to the situation where the boundary layers remain stable, focusing on the shear layer instability that occurs only in the counter-rotating regime. The associated pattern is a combination of a circular chain of vortices, as observed by Lopez et al. (2002) at low aspect ratio, surrounded by a set of spiral arms, first described by Gauthier et al. (2002) in the case of high aspect ratio. Stability curve and critical modes are measured for the whole range of aspect ratios. From the measurement of a local Reynold...
This dissertation concerns experimental work on the instability and transition of the rotating-disk ...
The flow above an infinite rotating disk is an example of 3D boundary-layers where crossflow instabi...
Hydrodynamic simulations have been used to study accretion disks consisting of counterrotating compo...
International audienceThe instability patterns in the flow between counter-rotating disks (radius to...
International audienceThe shear layer instability in the flow between two counter-rotating disks enc...
The flow between two rotating disks (radius to heigh ratio of 20.9), enclosed by a rotating cylinder...
International audienceThe rotating-disk boundary layer is generally considered as an example of a fl...
International audienceWe study the first bifurcation in the axisymmetric flow between two exactly co...
We consider the convective instability of stationary and traveling modes within the boundary layer o...
National audienceThe present work considers the turbulent Von Kármán flow generated by two coaxial c...
The stability of the flow due to a rotating disk is considered for non-Newtonian fluids, specificall...
International audienceThis paper proposes a resolution to the conundrum of the roles of convective a...
AbstractThe stability of the flow due to a rotating disk is considered for non-Newtonian fluids, spe...
The major objective is to explore any visible differences of the flow field with wall curvature of t...
This paper proposes a resolution to the conundrum of the roles of convective and absolute instabili...
This dissertation concerns experimental work on the instability and transition of the rotating-disk ...
The flow above an infinite rotating disk is an example of 3D boundary-layers where crossflow instabi...
Hydrodynamic simulations have been used to study accretion disks consisting of counterrotating compo...
International audienceThe instability patterns in the flow between counter-rotating disks (radius to...
International audienceThe shear layer instability in the flow between two counter-rotating disks enc...
The flow between two rotating disks (radius to heigh ratio of 20.9), enclosed by a rotating cylinder...
International audienceThe rotating-disk boundary layer is generally considered as an example of a fl...
International audienceWe study the first bifurcation in the axisymmetric flow between two exactly co...
We consider the convective instability of stationary and traveling modes within the boundary layer o...
National audienceThe present work considers the turbulent Von Kármán flow generated by two coaxial c...
The stability of the flow due to a rotating disk is considered for non-Newtonian fluids, specificall...
International audienceThis paper proposes a resolution to the conundrum of the roles of convective a...
AbstractThe stability of the flow due to a rotating disk is considered for non-Newtonian fluids, spe...
The major objective is to explore any visible differences of the flow field with wall curvature of t...
This paper proposes a resolution to the conundrum of the roles of convective and absolute instabili...
This dissertation concerns experimental work on the instability and transition of the rotating-disk ...
The flow above an infinite rotating disk is an example of 3D boundary-layers where crossflow instabi...
Hydrodynamic simulations have been used to study accretion disks consisting of counterrotating compo...