been used as a model of stellar and planetary accretion disks. The apparatus has a cylinder
radius ratio of. Flow super-rotation, an angular velocity greater than those of both cylinders,
is observed in the sub-rotating regime. The velocity profiles give lower bounds for the
torques required to rotate the inner cylinder that are larger than the torques for the case of
laminar Taylor–Couette flow. The quasi-Keplerian profiles are composed of a well-mixed …