Chaotic mixing processes and transport barriers around the wintertime strat
ospheric polar vortex are investigated with an idealized barotropic model,
previously used by Ishioka and Yoden. A barotropically unstable jet is forc
ed in order to obtain a fluctuating polar vortex. A flow with quasiperiodic
time dependence and an aperiodic flow with similar behavior are investigat
ed using several Lagrangian methods.
A typical chaotic mixing process is observed in the quasiperiodic flow, res
ulting in effective mixing inside and outside of the polar vortex. The mixi
ng regions are on the critical latitudes of several planetary waves that gr
ow through barotropic instability. Poincare sections give accurate location
s of chaotic mixing regions, and transport barriers are identified as the e
dges of invariant torus regimes. In addition to the transport barriers asso
ciated with strong potential vorticity gradients, another type of transport
barrier exists, which is not related to the steep potential vorticity grad
ient.
Chaotic mixing is dominant also in the aperiodic flow. Comparing with the q
uasiperiodic flow, an aperiodic flow with the same wave energy has a higher
average Lyapunov exponent. This arises because the area involved in chaoti
c zones increases. The evolution of the correlation function is also more t
ypical of a chaotic zone. Isolated regions are found near the center of the
polar vortex, which can be explained by the invariant tori in the Poincare
sections of the quasiperiodic flow. Implications of the results for the ob
served "4-day wave'' in the upper stratosphere are discussed.