Abstract
The flow in a rotating cylinder driven by the differential rotation
of its top endwall
is studied by numerically solving the time-dependent axisymmetric Navier–Stokes
equations. When the differential rotation is small, the flow is well described
in
terms of similarity solutions of individual rotating disks of infinite
radius. For larger
differential rotations, whether the top is co-rotating or counter-rotating
results in
qualitatively distinct behaviour. For counter-rotation, the boundary layer
on the top
endwall separates, forming a free shear layer and this results in a global
coupling
between the boundary layer flows on the various walls and a global departure
from
the similarity flows. At large Reynolds numbers, this shear layer becomes
unstable.
For a co-rotating top, there is a qualitative change in the flow depending
on whether
the top rotates faster or slower than the rest of the cylinder. When the
top rotates
faster, so does the bulk of the interior fluid, and the sidewall boundary
layer region
where the fluid adjusts to the slower rotation rate of the cylinder is
centrifugally
unstable. The secondary induced meridional flow is also potentially unstable
in this
region. This is manifested by the inflectional radial profiles of the vertical
velocity
and azimuthal vorticity in this region. At large Reynolds numbers, the
instability of
the sidewall layer results in roll waves propagating downwards.
Publisher
Cambridge University Press (CUP)
Subject
Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics
Cited by
47 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献