In total, three sets of MPAS forecasts were produced. Two MPAS forecasts used the same physics configuration as HRRR and RRFS with varying initial conditions: MPAS-RT-NSSL (initialized from RRFS) and MPAS-HT-NSSL (initialized from HRRR). Varying the initial conditions this way enables a fair test of model core performance without the potential implications of initial condition bias. Additionally, to test the hypothesis that forecasted thunderstorm property differences between the NSSL and Thompson microphysics schemes when used in WRF remain similar in MPAS, an additional MPAS forecast was produced using HRRR initial conditions and NSSL microphysics (MPAS-HN-NSSL).
We will present preliminary (this is likely to be a multi-year, ongoing effort) forecasting skill analysis along with storm object properties. Two-dimensional kernel density estimates (KDE) of surrogate severe reports (i.e., updraft helicity) probability will be compared to observed severe reports to assess severe storm forecasting skill. Accumulated forecast precipitation will be compared against Stage 4 observed precipitation to compute forecast bias ratios for various precipitation rate thresholds. This analysis is important as the current largest weakness of the FV3-based RRFS is significant overprediction of precipitation, particularly for larger amounts/rates. Storm objects will be identified, classified, and tracked using the iterative storm segmentation and classification technique developed by Potvin et al. (2022). Object properties such as area, strength, depth, and various shape parameters will be compared against environmental parameters using 2-D KDEs to assess how these relationships (e.g., storm depth vs. MUCAPE) change across model cores and microphysical parameterizations. These relationships will also be compared against those associated with observed storm objects from Multi-Radar / Multi-Sensor (MRMS) composite reflectivity products.

