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A SHEBA Intensive Observation Period program was designed to evaluate the hypothesis that rapid growth enhances ocean heat flux by simultaneously measuring turbulent fluxes under thin (0.5 m) and thick (2 m) ice during freezup in late Oct, 1997. Given straightforward application of a theory for heat and mass transport expounded by Yaglom and Kader, and given the temperature gradient observed in nearby ice of similar thickness, enhanced heat flux due to supercooling should have been readily observable, if present. Results were negative: observed friction velocity and heat flux were appreciably smaller in the growing internal boundary layer under the smooth, new ice surface than at the control (main) mast under thick ice. Interpretation of the present measurements is complicated by heterogeneity of the under-ice surface in the transition from old to new ice; nevertheless, it appears that the supercooling tendency in growing ice is relieved locally by uneven growth. From the point of view of upper ocean dynamics, this would not differ from uniform congelation growth.