A unique aspect of the Megi observations was that most eyewall sondes were deployed in pairs closely spaced in time (< 1-min time separation). The dropsonde pairs showed dramatically different boundary layer structures which were remarkably consistent in different storm quadrants with one sonde showing relatively weak boundary layer wind shear and its partner showing extreme wind shear, a result due in part, to very different sonde trajectories within the eyewall. The high wind-shear partner sonde exhibited highest winds near the top of the mixed layer on order of 90-100 m/s, and were associated with surface winds on order of 60-70 m/s. The weak wind shear partner exhibited top of the mixed layer winds of order of 90-95 m/s while strongest surface winds were on order of 80-85 m/s. A well-defined surface layer extending to 50-100 m exhibited constant potential temperature (theta) as well as constant radial and tangential winds. This constant wind with height layer resulted in higher near-surface winds than would be suggested by the boundary-layer log law. Unusual high-theta layers were observed above the surface layer and within the supposedly well-mixed layer. We speculate that the phenomena responsible for the unusual variations in the eyewall boundary layer structure may be associated with micro-vortices embedded within the eyewall.
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