We examine the effects of changing size distributions (i.e., intercept parameter) and densities of graupel and hail in the WRF model for simulated supercells using an idealized sounding based on previous research. The impacts of changing microphysical parameters are documented for environments with varying buoyancy, utilizing several available single-moment microphysics schemes. Specifically, we investigate the development and evolution of storm updrafts early in the numerical simulations as a function of individual buoyancy terms within the WRF model.
Preliminary results suggest a sensitivity of vertical motion on choice of the size distribution and density of graupel and hail. We hypothesize that these differences are attributed to enhancements in latent heating for particle size distributions that describe numerous, smaller graupel particles with overall more surface area that maximizes freezing. Understanding upscale impacts of graupel and hail parameterizations on supercell structure and intensity may elucidate under what environmental conditions microphysics matter most in numerical simulations of these storms.