Abstract
We study the paths of fluid particles in velocity fields modelling
rigidly rotating
velocity fields that occur in the concentric Taylor problem. We set up velocity
fields
using the model of Davey, DiPrima & Stuart (1968) based on small-gap
asymptotics.
This allows a numerical study of the Lagrangian properties of steady flow
patterns in
a rotating frame. The spiral and Taylor vortex modes are integrable, implying
that in
these cases almost all particle paths are confined to two-dimensional surfaces
in the
fluid. For the case of Taylor vortices the motion on these surfaces is
quasi-periodic,
whereas for spirals the particles propagate up or down the cylinder on
these surfaces.The non-axisymmetric modes we consider are wavy vortices, spirals, ribbons and
twisted Taylor vortices. All of these flows have the property that they are
steady flows
when examined in a rotating frame of reference. For all non-axisymmetric modes
with the exception of spirals, we observe the existence of regions of chaotic mixing
within the fluid. We discuss mixing of the fluid by these flows with
reference to the
pattern of stagnation points and some of the periodic trajectories within
the fluid and on the boundary.
Publisher
Cambridge University Press (CUP)
Subject
Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics
Cited by
31 articles.
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