A new framework for understanding the vertical structure of ocean gyres is
developed based on vertical fluxes of potential vorticity. The key ingredie
nt is an integral constraint that in a steady state prohibits a net flux of
potential vorticity through any closed contour of Bernoulli potential or d
ensity. Applied to an ocean gyre, the vertical fluxes of potential vorticit
y associated with advection, friction, and buoyancy forcing must therefore
balance in an integral sense.
In an anticyclonic subtropical gyre, the advective and frictional potential
vorticity fluxes are both directed downward, and buoyancy forcing is requi
red to provide the compensating upward potential vorticity flux. Three regi
mes are identified: 1) a surface "ventilated thermocline'' in which the upw
ard potential vorticity flux is provided by buoyancy forcing within the sur
face mixed layer, 2) a region of weak stratification- "mode water'' in whic
h all three components of the potential vorticity flux become vanishingly s
mall, and 3) an "internal boundary layer thermocline'' at the base of the g
yre where the upward potential vorticity flux is provided by the diapycnal
mixing. Within a cyclonic subpolar gyre, the advective and frictional poten
tial vorticity fluxes are directed upward and downward, respectively, and a
re thus able to balance without buoyancy forcing.
Geostrophic eddies provide an additional vertical potential vorticity flux
associated with slumping of isopycnals in baroclinic instability. Incorpora
ting the eddy potential vorticity flux into the integral constraint provide
s insights into the role of eddies in maintaining the Antarctic Circumpolar
Current and convective chimneys. The possible impact of eddies on the vert
ical structure of a wind-driven gyre is discussed.