Handout (10.1 MB)
We conducted numerous NEPTUNE simulations with different physics configurations and evaluated the forecast skill and numerical stability. We show that using a CCPP physics suite implemented with the Tiedtke convection parameterization performs statistically better than the same suite using the Grell-Freitas and simplified Arakawa and Schubert (SAS) parameterizations through comparisons with ERA-5 reanalyses and the NASA IMERG precipitation dataset. The new physics suite using the Tiedtke scheme is not particularly sensitive to changes in the vertical resolution and improves skill as the horizontal grid spacing is increased to 9 km on the globe. We also investigated the impact of subgrid scale cloud fraction from the planetary boundary layer and convection schemes on radiative heating and the impact of different cloud fraction parameterizations based on Xu-Randall and Thompson microphysics on forecast skill.
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