Abstract
A unique microphysical structure of rainfall is observed by the surface laser optical Particle Size and Velocity (Parsivel) disdrometers on 25 April 2011 during Midlatitude Continental Convective Clouds Experiment (MC3E). According to the systematic differences in rainfall rate and bulk effective droplet radius, the sampling data can be divided into two groups; the rainfall mostly from the deep convective clouds has relatively high rainfall rate and large bulk effective droplet radius, whereas the reverse is true for the rainfall from the shallow wrm clouds. The Weather Research and Forecasting model coupled with spectral bin microphysics (WRF‐SBM) successfully reproduces the two distinct modes in the observed rainfall microphysical structure. The results show that the up‐to‐date model can demonstrate how the cloud physics and the weather condition on the day are involved in forming the unique rainfall characteristic.
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