Convection is initiated by inserting randomly-perturbed warm bubbles in the boundary layer where cells are indicated by radar reflectivity. The ensemble members therefore require some spin up time, which allows for some comparison of precipitation initiation in the various microphysics schemes. Comparison of time-height reflectivity innovations (RMS and mean) reveal differences in microphysical behaviors, such as speed of precipitation generation and fall speed of precipitation hydrometeors. For example, the single-moment warm-rain (i.e., no ice phase) Kessler-type schemes tend to generate precipitation (and radar echo) more rapidly and thus tend to have lower initial reflectivity innovations. On the other hand, the addition of ice or number concentration provides greater diversity in fall speed and better mean innovations at middle to high altitudes at later times. Ice and number concentration also seem to help maintain higher ensemble spread, which is important for effective data assimilation.
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