The parameters epsilon and chi were observed to be lognormally distributed in the pycnocline. Two of the most popular microstructure models were found to give results which were consistent with the results obtained from the tracer. The Osborn-Cox model yielded a vertical eddy diffusivity for heat which was in agreement with that obtained from the tracer estimate (1.4 x 10^{-5} m^2/s for the fall and 2.54 x 10^{-5} m^2/s for the spring); the Osborn model yielded estimates of the vertical eddy diffusivity for density which were higher than those of either the tracer estimate or the Osborn-Cox estimate (3.14 x 10^{-5} m^2/s for the fall and 3.78 x 10^{-5} m^2/s for the spring). As a result of this, it is believed that the value of Gamma = 0.25 that is often used may be too high a value to be used in the pycnocline; furthermore, it is quite likely that Gamma is not even constant but depends upon the mixing conditions.
Jim Burke is now teaching physics at Riverview Rural High School in Sydney, Nova Scotia. He also serves on the provincial physics committee. He can be reached by e-mail at jfburke@syd.eastlink.ca.