TROPICAL CYCLONES

 

The schematic below summarizes our previous research on tropical cyclones in vertical wind shear (in collaboration with M. T. Montgomery, NPS, Monterey, CA, USA; Riemer et al. 2010, Riemer and Montgomery 2011, Riemer et al. 2013). Click here for more details.

          

Left panel: Dynamic and kinematic consequence of the shear interaction. The shear-forced tropical-cyclone vortex may achieve a left-of-shear tilt equilibrium due to Asymmetric Balance dynamics. The outer vortex (dashed contours indicate positive vorticity anomaly) exhibits a much larger tilt than the eyewall (solid cylinder). Shear-induced, storm-relative flow distorts the high-entropy storm‘s „moist envelope“ (red colors) leading to a highly asymmetric distribution such that high-entropy air at low levels coincides with the positive vorticity anomaly due to vortex tilt. 
Right panel: Consequences for distribution of convection, precipitation, and downdrafts. Convection is forced in the high-vorticity, high-entropy region to the right of the shear vector and ascends on a helical path within the primary rain band (long black arrow). Precipitation falls into unsaturated air below and ensuing downdrafts (blue arrows) bring low-entropy air into the frictional inflow layer (blue shading). This low-entropy air enters the eyewall updrafts effectively diluting the tropical cyclone‘s power machine.

Currently, I am interested in the Lagrangian description of „ventilation“, i.e. the intrusion of low-entropy air from the environment into the inner-core convection. Intrusion is most significant in vertically-sheared storms and these storms exhibit distinct asymmetric structure.

In a first study (Riemer and Laliberte, 2015, JAS), we examined trajectories calculated for the shear experiments of Riemer et al. (2010). Examination in physical (e.g. radius-height) space does not appear to provide a clear picture for two reasons: 1) Asymmetric storm structure makes radius as a coordinate rather ambiguous, and 2) geometric height (or pressure-based vertical coordinates) provide no clear distinction between the frictional boundary layer, the outflow layer, and the free troposphere. We find the examination of trajectories in thermodynamic (entropy-temperature) space to be very helpful. This framework relates to the axisymmetric, steady-state Potential Intensity theory and its recent extension to ventilated storms by Tang and Emanuel (2010,2012). We suggest that the mass flux in entropy-temperature space as a key diagnostic. Using this diagnostic, different ventilation pathways can be described quantitatively.