Wednesday, 6 June 2001: 1:40 PM
The oceanic thermohaline circulation is forced by horizontally
differential heat and water fluxes, primarily those that arise on the
planetary scale. Its dynamical behavior exhibits some regimes of
great delicacy with respect to the forcing, associated with
transitions between multiple equilibria, and others with intrinsic
oscillations, due to instabilities of the mean circulation and
finite-amplitude limit cycles. Furthermore, its oscillations are
easily excited by atmospheric interannual variability, and there is a
potentially significant feedback onto the climate associated with
anomoalous advection of the upper-ocean temperature in the boundary
region between the subtropical and subpolar gyres.
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