Analyses of storm-relative winds reveal familiar features, including near-logarithmic wind speed profiles below low-level jets (Franklin et al. 2003; Powell et al. 2003); strong, frictionally-driven near-surface inflow layers that penetrate the eyewall region (Montgomery et al. 2006; Zhang et al. 2011, 2013); and outward sloping of the eyewall with height (Stern and Nolan 2009; Hazelton et al. 2013; Stern et al. 2014). These kinematic analyses also depict differences between composite groups, seen most notably in the horizontal and vertical extent of the low-level jet, near-surface inflow maxima, and the radial profile of tangential wind. Composited thermodynamic fields depict the warm-core nature of hurricanes, nearly moist adiabatic conditions outside of the eye and above the frictional inflow layer, and the reservoir of moist static energy in the low-level hurricane eye.
We discuss the role of surface turbulent fluxes in establishing apparent profiles of entropy (dry and moist) and momentum in the near-surface inflow, and the implications of these processes in hurricane intensity change. We supplement our observational findings using preliminary results from a 7-day simulation of Hurricane Irma using the Advanced Research Weather Research and Forecasting model (WRF-ARW; Skamarock et al. 2008), which we use to examine the air-sea processes occurring in the simulated hurricane boundary layer.