Assessment of the impact of WRF microphysical schemes on precipitation forecasting during spring in the Democratic People's Republic of Korea

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Hyok-Chol Kim, Ju-Song Kim, Kum-Ryong Jo, Song-Nam Ri
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引用次数: 0

Abstract

In this study, the WRF model was used to evaluate the impact of microphysics schemes on the prediction of rainfall during spring in the Democratic People's Republic of Korea (DPRK). The rainfall event was divided into two categories according to the daily accumulative rainfall amount and rainfall distribution: rainfall events with small precipitation(<10 mm/d) and partial coverage of the precipitation area (hereafter SPRE) and rainfall event with relatively large precipitation(≥10 mm/d) and entirely covered area (hereafter LERE), and numerical simulations were carried out for six typical rainfall events (three days for each category) in 2021–2022. The simulation results confirmed that the effects of microphysics schemes differ from each other according to the precipitation event. In the analysis of the simulation results, the accuracy was evaluated using the critical success index (CSI) and false alarm ratio (FAR) indices for SPRE, and MODE analysis was used to assess the agreement with centers of rainfall patterns for LERE. For SPRE, the one-moment bulk microphysics scheme is rather efficient than the more sophisticated two-moment bulk microphysics scheme, and the Ferrier scheme performs best. For LERE, the two-moment bulk microphysics scheme performs better than the one-moment microphysics scheme. In particular, the Thompson and Thompson aerosol-aware schemes have a higher performance than the other schemes. The results of this study suggest that seasonal effective physical process schemes should be selected for operational forecasting, and will help to improve the accuracy of the forecast for spring in the DPRK.
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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