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model ( Chen and Dudhia 2001 ). The Kain–Fritsch cumulus scheme ( Kain and Fritsch 1990 , 1993 ; Kain 2004 ) was used for the 12-km domain only, allowing convection to be explicitly resolved in the innermost two domains. For model microphysics, the Predicted Particle Property (P3) microphysics scheme ( Morrison and Milbrandt 2015 ) has been implemented, which is coupled with the Rapid Radiative Transfer Model for GCMs (RRTMG) longwave and shortwave radiation schemes ( Iacono et al. 2008 ). Several
model ( Chen and Dudhia 2001 ). The Kain–Fritsch cumulus scheme ( Kain and Fritsch 1990 , 1993 ; Kain 2004 ) was used for the 12-km domain only, allowing convection to be explicitly resolved in the innermost two domains. For model microphysics, the Predicted Particle Property (P3) microphysics scheme ( Morrison and Milbrandt 2015 ) has been implemented, which is coupled with the Rapid Radiative Transfer Model for GCMs (RRTMG) longwave and shortwave radiation schemes ( Iacono et al. 2008 ). Several
precipitation maximum during IOP2b. The simulation includes domains with 12-, 4-, and 1.3-km grid spacing [see Fig. 1 of Campbell and Steenburgh (2017) for nesting configuration and topography], 36 vertical levels with 8 levels at or below 1 km AGL, and a parameterization suite that includes the Rapid Radiative Transfer Model longwave radiation scheme ( Iacono et al. 2008 ), Dudhia shortwave radiation scheme ( Dudhia 1989 ), Noah land surface model ( Chen and Dudhia 2001 ), Yonsei University planetary
precipitation maximum during IOP2b. The simulation includes domains with 12-, 4-, and 1.3-km grid spacing [see Fig. 1 of Campbell and Steenburgh (2017) for nesting configuration and topography], 36 vertical levels with 8 levels at or below 1 km AGL, and a parameterization suite that includes the Rapid Radiative Transfer Model longwave radiation scheme ( Iacono et al. 2008 ), Dudhia shortwave radiation scheme ( Dudhia 1989 ), Noah land surface model ( Chen and Dudhia 2001 ), Yonsei University planetary
microphysical scheme ( Thompson et al. 2008 ) was utilized along with the Rapid Radiative Transfer Model for GCMs (RRTMG) longwave and shortwave radiation schemes ( Iacono et al. 2008 ), the Rapid Update Cycle (RUC) land surface model (LSM; Smirnova et al. 2016 ), the revised Pennsylvania State University–National Center for Atmospheric Research (PSU–NCAR) Mesoscale Model (MM5) Monin–Obukov surface-layer scheme ( Jiménez et al. 2012 ), and the new Shin–Hong ( Shin and Hong 2015 ) BL parameterization. No
microphysical scheme ( Thompson et al. 2008 ) was utilized along with the Rapid Radiative Transfer Model for GCMs (RRTMG) longwave and shortwave radiation schemes ( Iacono et al. 2008 ), the Rapid Update Cycle (RUC) land surface model (LSM; Smirnova et al. 2016 ), the revised Pennsylvania State University–National Center for Atmospheric Research (PSU–NCAR) Mesoscale Model (MM5) Monin–Obukov surface-layer scheme ( Jiménez et al. 2012 ), and the new Shin–Hong ( Shin and Hong 2015 ) BL parameterization. No
Dawson (2013) , McMillen and Steenburgh (2015a) , and Conrick et al. (2015) , the simulations presented in this paper use the Thompson cloud microphysics ( Thompson et al. 2008 ), Rapid Radiative Transfer Model longwave radiation ( Iacono et al. 2008 ), Dudhia shortwave radiation ( Dudhia 1989 ), Yonsei University planetary boundary layer ( Hong et al. 2006 ), revised MM5 surface layer ( Jiménez et al. 2012 ), and Noah land surface model ( Chen and Dudhia 2001 ) parameterizations. The Kain
Dawson (2013) , McMillen and Steenburgh (2015a) , and Conrick et al. (2015) , the simulations presented in this paper use the Thompson cloud microphysics ( Thompson et al. 2008 ), Rapid Radiative Transfer Model longwave radiation ( Iacono et al. 2008 ), Dudhia shortwave radiation ( Dudhia 1989 ), Yonsei University planetary boundary layer ( Hong et al. 2006 ), revised MM5 surface layer ( Jiménez et al. 2012 ), and Noah land surface model ( Chen and Dudhia 2001 ) parameterizations. The Kain
