In order to perform as complete a test as possible of the available physical parameterizations, we began with an experiment that utilized WSM 6-class microphysics, CAM long wave and shortwave radiation (Collins et al. 2004), Kain-Fritsch cumulus (Kain 2004), YSU PBL (Hong et al. 2006), and the NOAH LSM (Chen and Dudhia 2001), which we then designated as the control run (CTRL). From this, we varied each of the physics types in turn, for each type cycling through the available options and producing a time series for each option.