To study how the precipitation processes evolve through time, we use a clustering technique to identify the front at each hour of the simulation based on dense clusters of points where convergence and virtual potential temperature exceed certain thresholds. Although an imperfect technique, the general front is trackable through time, enabling statistics of the surrounding environmental and microphysical characteristics. In terms of dynamical processes, there is a slight relationship between the low-level shear strength and the hourly rain accumulations behind the front, but the relationship with the cold pool propagation speed is weak. We hypothesize that this discrepancy occurs since the propagation of the front is not solely controlled by thunderstorm-cold pool dynamics. At short time scales, high graupel mixing ratios are often associated with high rain mixing ratios. This relationship is somewhat problematic given that overestimation of graupel by microphysical schemes is a known problem in tropical precipitation modeling. On longer time scales and in terms of the rainfall distribution, low-level integrated moisture flux exhibits a strong correlation with the total hourly rain accumulations near the front. Finally, we compare the simulated microphysical structure with operational polarimetric radar data; this comparison allows us to assess the realism of the microphysical structures from the numerical simulation.
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