A control simulation is conducted using the WRF v4.2.2 model with a 1-km resolution innermost domain centered over the WINTRE-MIX study region. An HRRR-like model configuration is adopted with the Thompson aerosol-aware microphysics scheme and the MYNN planetary boundary layer (PBL) scheme. The control simulation performs well in simulating the transition from rain to FZRA but shows a delay in the transition from FZRA to IP. Analysis of microphysical process rates reveals that the rain-collecting-ice process might play an important role in the production of IP when the melting layer is relatively deep. A sensitivity test using the MYJ PBL scheme is about 2 °C colder in the sub-freezing layer around the DOW-US-P site and activates the SIP at an earlier time, leading to an earlier formation of ice pellets via the rain-collecting-ice process and an improvement in the transition from FZRA to IP. A second sensitivity test adds an additional source for the SIP process, which enhances the local production of cloud ice at the DOW-CAN-S site. As a result, the transition from FZRA to IP occurs at an earlier time and is closer to the manual observations. These results suggest that both the occurrence time and intensity of the SIP process within the subfreezing layer might modulate the transition from FZRA to IP, motivating the need for an accurate representation of SIP in numerical models used to forecast p-type in winter storms.
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