Further studies are being made to determine the dependence of the results on the amplitude, radial and tangential scale of the asymmetric PV disturbance as well as its vertical structure. Contributions from the symmetric and asymmetric parts of the PV anomaly will be separated. In the course of the analysis a method has been developed for determining the vertical structure of a PV anomaly that is consistent with a diabatic source of arbitrary amplitude. An upper-level negative anomaly is induced above a lower-level positive one; the relative strengths of these anomalies depends on the thermal structure of the cyclone vortex. The upper-level anomaly tends to reduce the effect of the lower-level one on the evolution of the vortex. The cumulative effect of multiple convective "pulses" on the evolution of the vortex is being studied, as in Montgomery and Enagonio (1998) and Möller and Montgomery (1999), and the conditions under which the pulses are effective in intensifying the cyclone vortex are being evaluated.
As time permits, experiments will also be made with an imposed azimuthal-wavenumber one PV anomaly to establish the presence of an algebraically growing disturbance as elucidated by Nolan and Montgomery (1999). For these experiments minimal horizontal diffusion and maximum horizontal resolution will be used.
Experiments designed to evaluate these aspects of the problem are in progress and will be reported upon as available.