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WRF 模式下孟加拉湾气旋模拟中的物理方案优化:使用单向方差分析和图基检验。

Optimization of physical schemes in WRF model on cyclone simulations over Bay of Bengal using one-way ANOVA and Tukey's test.

机构信息

Centre for Ocean Atmospheric Science and Technology, Amity University Rajasthan, Kant Kalwar, Jaipur, Rajasthan, India.

Amity School of Applied Sciences, Amity University Rajasthan, Kant Kalwar, Jaipur, Rajasthan, India.

出版信息

Sci Rep. 2021 Dec 24;11(1):24412. doi: 10.1038/s41598-021-02723-z.

DOI:10.1038/s41598-021-02723-z
PMID:34952900
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8709857/
Abstract

Evaluation of appropriate physics parameterization schemes for the Weather Research and Forecasting (WRF) model is vital for accurately forecasting tropical cyclones. Three cyclones Nargis, Titli and Fani have been chosen to investigate the combination of five cloud microphysics (MP), three cumulus convection (CC), and two planetary boundary layer (PBL) schemes of the WRF model (ver. 4.0) with ARW core with respect to track and intensity to determine an optimal combination of these physical schemes. The initial and boundary conditions for sensitivity experiments are drawn from the National Centers for Environmental Prediction (NCEP) global forecasting system (GFS) data. Simulated track and intensity of three cyclonic cases are compared with the India Meteorological Department (IMD) observations. One-way analysis of variance (ANOVA) is applied to check the significance of the data obtained from the model. Further, Tukey's test is applied for post-hoc analysis in order to identify the cluster of treatments close to IMD observations for all three cyclones. Results are obtained through the statistical analysis; average root means square error (RMSE) of intensity throughout the cyclone period and time error at landfall with the step-by-step elimination method. Through the elimination method, the optimal scheme combination is obtained. The YSU planetary boundary layer with Kain-Fritsch cumulus convection and Ferrier microphysics scheme combination is identified as an optimal combination in this study for the forecasting of tropical cyclones over the Bay of Bengal.

摘要

评估天气研究与预测 (WRF) 模型的适当物理参数化方案对于准确预测热带气旋至关重要。选择了三个气旋纳尔吉斯、提特里和法尼,以研究 WRF 模型(版本 4.0)与 ARW 核心的五种云微物理 (MP)、三种积云对流 (CC) 和两种行星边界层 (PBL) 方案的组合,以确定这些物理方案的最佳组合。敏感性实验的初始和边界条件取自美国国家环境预报中心 (NCEP) 全球预报系统 (GFS) 数据。模拟的三个气旋案例的轨迹和强度与印度气象局 (IMD) 的观测结果进行了比较。单向方差分析 (ANOVA) 用于检查模型获得的数据的显著性。此外,还应用了 Tukey 的事后检验法,以便为所有三个气旋识别接近 IMD 观测值的处理群集。通过统计分析获得结果;在整个气旋期间的平均均方根误差 (RMSE) 和登陆时的时间误差,采用逐步消除法。通过消除法,获得了最佳方案组合。在本研究中,对于孟加拉湾热带气旋的预报,YSU 行星边界层与凯恩-弗里奇积云对流和费里尔微物理方案的组合被确定为最佳组合。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c0bb/8709857/97f5ce77e45b/41598_2021_2723_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c0bb/8709857/37c35ebb5fe6/41598_2021_2723_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c0bb/8709857/97f5ce77e45b/41598_2021_2723_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c0bb/8709857/37c35ebb5fe6/41598_2021_2723_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c0bb/8709857/97f5ce77e45b/41598_2021_2723_Fig2_HTML.jpg

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