Abstract:
Numerical solutions of the unstable, growing modes are found for the two-layer inviscid
quasigeostrophic equations in a meridional channel. A steady mean flow in
the N-S direction is imposed in the upper layer, and it is assumed that changes in
planetary vorticity following this mean flow are balanced by the input of vorticity
from an imposed wind stress curl. Thus in the two-layer system, the vertical shear, in
thermal wind balance, is associated with an interface slope which provides a gradient
of potential vorticity (PV) in the x-direction, of equal magnitude and opposite sign
in the two layers. In the y-direction the PV gradient has the value of planetary beta,
β in both layers.
The unstable modes of this system exhibit a boundary-layer structure across the
channel. They are intensified in the west. The growth rates of the unstable modes are
of the same order as the zonal case, however the range of wavenumber and shear for
which instability is possible is larger. Established cutoff criteria for the equal-layer
zonal case are not applicable, and no analogous criteria has yet been found. Growing
modes are found even for very weakly sheared flows, and this suggests that baroclinic
instability may represent a more significant source of mid-ocean eddy energy than
previously believed.
