A dynamical stabilizer in the climate system: a mechanism suggested by a simple model

A simple zonally averaged hemispheric model of the climate system is constructed, based onenergy equations for two ocean basins separated at 30° latitude with the surface fluxes calculatedexplicitly. A combination of empirical input and theoretical calculation is used to determine anannual mean equilibrium climate for the model and to study its stability with respect to smallperturbations. The insolation, the mean albedos and the equilibrium temperatures for the twomodel zones are prescribed from observation. The principal agent of interaction between thezones is the vertically integrated poleward transport of atmospheric angular momentum acrosstheir common boundary. This is parameterized using an empirical formula derived from amultiyear atmospheric data set. The surface winds are derived from the angular momentumtransport assuming the atmosphere to be in a state of dynamic balance on the climatic timescalesof interest. A further assumption that the air–sea temperature difference and low level relativehumidity remain fixed at their mean observed values then allows the surface fluxes of latentand sensible heat to be calculated. Results from a radiative model, which show a positive lowertropospheric water vapour/infrared radiative feedback on SST perturbations in both zones, areused to calculate the net upward infrared radiative fluxes at the surface. In the model’s equilibriumclimate, the principal processes balancing the solar radiation absorbed at the surface areevaporation in the tropical zone and net infrared radiation in the extratropical zone. Thestability of small perturbations about the equilibrium is studied using a linearized form of theocean energy equations. Ice-albedo and cloud feedbacks are omitted and attention is focussedon the competing effects of the water vapour/infrared radiative feedback and the turbulentsurface flux and oceanic heat transport feedbacks associated with the angular momentum cycle.The perturbation equations involve inter-zone coupling and have coefficients dependent on thevalues of the equilibrium fluxes and the sensitivity of the angular momentum transport.Analytical solutions for the perturbations are obtained. These provide criteria for the stabilityof the equilibrium climate. If the evaporative feedback on SST perturbations is omitted, theequilibrium climate is unstable due to the influence of the water vapour/infrared radiativefeedback, which dominates over the effects of the sensible heat and ocean heat transport feedbacks.The inclusion of evaporation gives a negative feedback which is of sufficient strength tostabilize the system. The stabilizing mechanism involves wind and humidity factors in theevaporative fluxes that are of comparable magnitude. Both factors involve the angularmomentum transport. In including angular momentum and calculating the surface fluxes explicitly,the model presented here differs from the many simple climate models based on theBudyko–Sellers formulation. In that formulation, an atmospheric energy balance equation isused to eliminate surface fluxes in favour of top-of-the-atmosphere radiative fluxes and meridionalatmospheric energy transports. In the resulting models, infrared radiation appears as astabilizing influence on SST perturbations and the dynamical stabilizing mechanism found herecannot be identified. DOI: 10.1034/j.1600-0870.1999. t01-3-00002.x