Our findings indicate that the WRF model well represents the thermodynamic conditions, as well as SBC timing and intensity. However, for the associated convective cells, WRF overestimates the 30-dBZ echo top height (ETH), cell area, and maximum radar reflectivity compared to radar observations. This overestimation is primarily due to under-resolved entrainment processes and an overestimated cell merging frequency. Furthermore, the model exhibits a deficiency in simulating congestus clouds, showing a more rapid transition from shallow to deep convection compared to observed behavior. Moreover, sounding observations indicate a moister environment preceding convective clouds with merging events, which are linked to stronger, deeper, and wider clouds. Conversely, in simulations, the merging process does not produce higher or longer-lived cells, as many cases already exhibit high ETH (>10 km) before merging, where updrafts can no longer increase.
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