P11 Stochastic
Approaches Within a High Resolution Rapid Refresh Ensemble- Part I: Sensitivity
Testing
Jankov,
Isidora, Cooperative
Institute for Research in the Atmosphere (CIRA)/Affiliated with the National
Oceanic and Atmospheric Administration/Earth Systems Research Laboratory/Global
Systems Division (NOAA/ESRL/GSD), and the Developmental Testbed Center (DTC),
Judith Berner, National Center for
Atmospheric Research (NCAR), Jeff Beck, CIRA,
NOAA/ESRL/GSD, and DTC, Jamie Wolff, Michelle Harold, NCAR and DTC, Georg Grell, NOAA/ESRL/GSD,
Joseph B. Olson, Tatiana G. Smirnova, Cooperative
Institute for Research in Environmental Sciences (CIRES) and NOAA/ESRL/GSD,
John M. Brown, and Stanley G. Benjamin, NOAA/ESRL/GSD
A stochastic parameter perturbation (SPP) scheme
consisting of spatially and temporally varying perturbations of uncertain
parameters was implemented in the Grell-Freitas (GF) convective scheme, the
Mellor-Yamada-Nakanishi-Niino (MYNN) planetary boundary scheme and RUC land
surface model (LSM) scheme within the Rapid Refresh (RAP)/ High Resolution
Rapid Refresh (HRRR) physics suite. Ongoing efforts to implement SPP into
corresponding microphysics as well as radiation schemes are also underway.
Previous tests performed using the Rapid Refresh (RAP) ensemble with 13-km
grid spacing and stochastic perturbations within GF and MYNN schemes showed
that alone stochastic parameter perturbations generate insufficient spread.
However, when combined with other stochastic parameterization schemes, such
as the stochastic kinetic-energy backscatter (SKEB) scheme or the stochastic
perturbation of physics tendency scheme (SPPT), the stochastic ensemble
system has comparable forecast performance to a multi-physics ensemble. The
ensemble combining all three stochastic methods consistently produces the
best spread/skill ratio and generally outperforms the multi-physics ensemble.
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