A high-resolution, quasi-geostrophic numerical model is utilized to ex
amine two-layer baroclinic flow in a cylinder. Particular attention is
given to the role of horizontal shear of the basic state induced by v
iscosity near the cylinder wall, and to the desymmetrization brought a
bout by the cylindrical geometry, in the transition to baroclinic chao
s. Solutions are computed for both f-plane and beta-plane situations,
and the results are compared to previous laboratory experiments. Agree
ment in the former case is found to be good, although the onset of cha
os occurs at slightly lower forcing in the laboratory when its basic f
low is prograde, and at higher forcing amplitude when the experimental
basic azimuthal currents are retrograde. This suggests that the modes
t discrepancies may be attributable to computationally neglected ageos
trophic effects in the interior fluid and Ekman boundary layers. When
beta not equal 0, the numerical and laboratory results are in excellen
t agreement. The computational simulations indicate that the viscous s
idewall boundary layer plays a pivotal role in the dynamics. Moreover,
in contrast to previous studies performed in a periodic, rectilinear
channel, the route to chaos is largely temporal and involves relativel
y few spatial modes. The reduction in symmetries upon going from f-pla
ne channel to either f-plane or beta-plane cylinder models leads to fe
wer secondary instabilities and fewer spatial modes that are active in
the dynamics.