A series of general circulation model experiments using Global Environ
mental and Ecological Simulation of Interactive Systems (GENESIS) were
executed to evaluate the sensitivity of simulated mid-Cretaceous clim
ate to smalt perturbations in ocean heat transport. Three experiments
were performed: (1) mixed layer ocean with no ocean heat transport, ZE
ROQ, (2) ocean heat transport specified as required for GENESIS to bes
t match modern observations, ONEQ, and (3) doubled ocean heat transpor
t, TWOQ. The ONEQ experiment represents an ocean heat transport which
is actually about 15% of the values given by Carissimo et al. (1985) f
rom modern observations. As a sensitivity experiment these model simul
ations represent a doubling of the role of the ocean. However, relativ
e to the observations, they represent small perturbations to the total
poleward heat transport in the model. With the exception of the tropi
cs, no major changes in the structure of the general circulation of th
e atmosphere resulted from the modification of the ocean heat transpor
t. However, relatively small increases in ocean heat transport resulte
d in a number of significant differences between simulations, includin
g tropical. cooling, polar warming, weakened equator-to-pole surface t
emperature gradients, weakened midlatitude jets, decreased land-sea pr
essure contrast, and decreased midlatitude storminess. The experiments
indicate that changes in ocean heat transport which are well within t
he realm of possibility for Earth history can have significant climati
c impact. Although ocean heat transport may be a significant factor in
explaining Cretaceous polar warmth, the changes specified in these ex
periments alone are not sufficient to explain the polar warmth of the
Cretaceous.