The TC induced Rossby wavetrain is investigated in a 3-D high-resolution model. While a simulated TC moves northwestward in a resting environment due to the beta drift, its energy propagates southeastward, forming a synoptic-scale wavetrain with alternating regions of anticyclonic and cyclonic vorticity perturbations. The maximum intensity of the energy dispersion is found in the lower troposphere. Experiments with both explicit and mass-flux convective heating schemes show that cyclogenesis cannot occur in the Rossby wavetrain of a preexisting TC under the resting environment.
An anomaly baroclinic model was developed to understand the role of the mean monsoon flow on cyclogenesis. In the model a time-independent basic state similar to the WNP summer mean flow is specified. In the presence of such a mean flow, the model simulates TC formation in the wake of a pre-existing TC. Due to the influence of the mean flow, vortex-scale perturbations within the cyclonic circulation of the Rossby wavetrain are organized and intensified, leading to vortex-scale convection-circulation feedback. The simulated new TC has realistic dynamic and thermodynamic structures such as spiral rain bands, an upper-tropospheric warm core, and an eye wall. A vorticity budget is conducted to understand the cause of the PV generation, particularly in the earlier development stage when diabatic heating is relatively small.
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