Geoscientific Model Development
Geoscientific Model Development
Geoscientific Model Development
Articles | Volume 15, issue 21
Articles | Volume 15, issue 21
Geosci. Model Dev., 15, 8111–8134, 2022
https://doi.org/10.5194/gmd-15-8111-2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.
Geosci. Model Dev., 15, 8111–8134, 2022
https://doi.org/10.5194/gmd-15-8111-2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 15, issue 21
Model evaluation paper
11 Nov 2022
Model evaluation paper | 11 Nov 2022

Impact of physical parameterizations on wind simulation with WRF V3.9.1.1 under stable conditions at planetary boundary layer gray-zone resolution: a case study over the coastal regions of North China

Entao Yu et al.

Data sets

Impact of physical parameterizations on wind simulation with WRF V3.9.1.1 under stable conditions at PBL gray-zone resolution: a case study over the coastal regions of North China Entao Yu, Rui Bai, Xia Chen, and Lifang Shao https://doi.org/10.5281/zenodo.6505423

ERA5 hourly data on pressure levels from 1959 to present H. Hersbach, B. Bell, P. Berrisford, G. Biavati, A. Horányi, J. Muñoz Sabater, J. Nicolas, C. Peubey, R. Radu, I. Rozum, D. Schepers, A. Simmons, C. Soci, D. Dee, and J.-N. Thépaut https://doi.org/10.24381/cds.bd0915c6

A description of the Advanced Research WRF version 3 (https://www2.mmm.ucar.edu/wrf/users/download/get_source.html) William C. Skamarock, Joseph B. Klemp, Jimy Dudhia, David O. Gill, Dale Barker, Michael G. Duda, Xiang-yu Huang, Wei Wang, and Jordan G. Powers https://doi.org/10.5065/D68S4MVH

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Short summary
A large number of simulations are conducted to investigate how different physical parameterization schemes impact surface wind simulations under stable weather conditions over the coastal regions of North China using the Weather Research and Forecasting model with a horizontal grid spacing of 0.5 km. Results indicate that the simulated wind speed is most sensitive to the planetary boundary layer schemes, followed by short-wave/long-wave radiation schemes and microphysics schemes.
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