Of particular interest was the APBL structure detected by the GPS sondes dropped in Bonnie's eyewall. Here, the vertically averaged flow was removed from the observed wind profile to show the perturbation wind field. The perturbation wind vectors (typically 10 m s-1) indicate a clear upward anticyclonic spiralling of the winds with height. There is also considerable structure in these profiles which perhaps implies baroclinicity in the wind perturbations since the height-averaged wind was removed. These wind profiles are markedly similar to oceanic current profiles where energy propagates downward from a wind-forced OPBL (Shay et al. 1998). Given this wind vector rotation theory predicts upward propagation of group velocity and hence energy flux from the near-surface layer through the APBL. The equivalent potential temperatures (i.e. thetae) are about 360° K in the area of maximum heat loss in the upper ocean. Although the correspondence is not necessarily one-to-one, along-track variations of thetae are apparently correlated to these upper ocean heat content changes. This result suggests more of a positive feedback from the ocean to the atmosphere rather that differs from previously held notions that the oceans only provide negative feedback. These profiles and their relationship to the atmospheric and oceanic environments represent a unique opportunity to examine their relative importance on both tropical cyclone structure and intensity variations.