CAN INCREASED POLEWARD OCEANIC HEAT-FLUX EXPLAIN THE WARM CRETACEOUS CLIMATE

The poleward transport of heat in the mid-Cretaceous (100 Ma) is exami ned using an idealized coupled ocean-atmosphere model. The oceanic com ponent consists of two zonally averaged basins representing the proto- Pacific and proto-Indian oceans and models the dynamics of the meridio nal thermohaline circulation. The atmospheric component is a simple en ergy and moisture balance model which includes the diffusive meridiona l transport of sensible heat and moisture. The ocean model is spun up with a variety of plausible Cretaceous surface temperature and salinit y profiles, and a consistent atmosphere is objectively derived based o n the resultant sea surface temperature and the surface heat and fresh water fluxes. The coupled model does not exhibit climate drift. Multip le equilibria of the coupled model are found that break the initial sy mmetry of the ocean circulation; several of these equilibria have one- cell (northern or southern sinking) thermohaline circulation patterns. Two main classes of circulation are found: circulations where the den sest water is relatively cool and is formed at the polar latitudes and circulations where the densest water is warm, but quite saline, and t he strongest sinking occurs at the tropics. In all cases, significant amounts of warm, saline bottom water are formed in the proto-Indian ba sin which modify the deepwater characteristics in the larger (proto-Pa cific) basin. Temperatures in the deep ocean are warm, 10 degrees-17 d egrees C, in agreement with benthic foraminiferal oxygen isotope data. The poleward transport of heat in the modeled Cretaceous oceans is la rger than in some comparable models of the present day thermohaline ci rculation and significantly larger than estimates of similar processes in the present-day ocean. It is consistently larger in the polar sink ing cases when compared with that seen in the tropical sinking cases, but this represents an increase of only 10%. The largest increase over present-day model transports is in the atmospheric latent heat transp ort, where an increased hydrological cycle (especially in the tropical sinking cases) contributes up to an extra 1 PW of poleward heat trans port. Better constraints on the oceanic deepwater circulation during t his period are necessary before the meridional circulation can be unam biguously described.