Diagnosing Near-Surface Model Errors with Candidate Physics Parameterization Schemes for the Multiphysics Rapid Refresh Forecast System (RRFS) Ensemble during Winter over the Northeastern United States and Southern Great Plains

Author:

Hu Xiao-Ming12ORCID,Park Jun1,Supinie Timothy1,Snook Nathan A.12,Xue Ming12,Brewster Keith A.12,Brotzge Jerald3,Carley Jacob R.4

Affiliation:

1. a Center for Analysis and Prediction of Storms, University of Oklahoma, Norman, Oklahoma

2. b School of Meteorology, University of Oklahoma, Norman, Oklahoma

3. c New York State Mesonet, University at Albany, State University of New York, Albany, New York

4. d NOAA/NWS/NCEP/Environmental Modeling Center, NOAA National Centers for Environmental Prediction, College Park, Maryland

Abstract

Abstract During the winter of 2020/21 an ensemble of FV3-LAM forecasts was produced over the contiguous United States for the Winter Weather Experiment using five physics suites. These forecasts are evaluated with the goal of optimizing physics parameterizations within the future operational Rapid Refresh Forecast System (RRFS) in the Unified Forecast System (UFS) realm and for selecting suitable physics suites for a multiphysics RRFS ensemble. The five physics suites have different combinations of land surface models (LSMs), planetary boundary layer (PBL) parameterizations, and surface layer schemes, chosen from those used in current and possible future operational systems and likely to be supported in the operational UFS. Full-season evaluation reveals a persistent near-surface cold bias in the U.S. Northeast from one suite and a nighttime warm bias in the southern Great Plains in another suite, while other suites have smaller biases. A representative case is chosen to diagnose the cause for each of these biases using sensitivity simulations with different physics combinations or modified parameters and verified with additional mesonet observations. The cold bias in the Northeast is attributed to aspects of the Noah-MP LSM over snow cover, where Noah-MP simulates lower soil water content, and thus lower thermal conductivity than other LSMs, leading to less upward ground heat flux during nighttime and consequently lower surface temperature. The nighttime warm bias found in the southern Great Plains is attributed to overestimation of vertical mixing in the K-profile-based eddy-diffusivity mass-flux (K-EDMF) PBL scheme and insufficient land–atmospheric coupling from the GFS surface layer scheme over short vegetation. A few key parameters driving these systematic biases are identified.

Funder

NOAA Center for Earth System Sciences and Remote Sensing Technologies

National Science Foundation

Publisher

American Meteorological Society

Subject

Atmospheric Science

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