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气象:2022,48(9):1077-1089
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CMA-REPS区域集合预报随机动能后向散射方案敏感性试验
范宇恩,李红祺,陈静,徐致真,陈法敬,邓国
(四川省气象探测数据中心,成都 610072; 高原与盆地暴雨旱涝灾害四川省重点实验室,成都 610072;中国气象局地球系统数值预报中心,北京 100081; 灾害天气国家重点实验室,北京 100081;复旦大学大气与海洋科学系,上海 200438)
Sensitivity Experiments of a Stochastic Kinetic Energy Backscatter Scheme Within the CMA-REPS Regional Ensemble Prediction System
FAN Yuen,LI Hongqi,CHEN Jing,XU Zhizhen,CHEN Fajing,DENG Guo
(Sichuan Meteorological Observation Data Centre, Chengdu 610072; Sichuan Key Laboratory of Rainstorm, Drought and Flood Disasters in Plateau and Basin, Chengdu 610072;Centre for Earth System Modeling and Prediction of CMA (CEMC), Beijing 100081; State Key Laboratory of Severe Weather (LaSW), Beijing 100081;Department of Atmospheric and Oceanic Sciences, Fudan University, Shanghai 200438)
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投稿时间:2021-07-14    修订日期:2022-05-05
中文摘要: 模式中常应用水平扩散项以抑制非线性计算不稳定或阻尼虚假短波,但这会导致数值模式在截断尺度附近出现小尺度动能过度耗散。为了将被过度耗散的小尺度动能补偿回模式,将随机动能后向散射扰动方法(stochastic kinetic energy backscatter,SKEB)引入CMA-REPS区域集合预报系统。首先基于由一阶自回归随机过程在水平方向上进行球谐函数展开得到的随机型,然后计算由数值扩散方案引起的局地动能耗散率,进而构造随机流函数强迫,并将其转化为水平风速扰动,对耗散的动能进行随机补偿。开展了2018年9月、10月(选取1日、7日、13日、19日、25日)的10 d集合预报随机型时间及空间尺度敏感性试验,并对试验结果进行评估。获得如下结论:在CMA-REPS区域集合预报中应用SKEB方案,可在一定程度上补偿过度耗散的小尺度动能,进而改善了模式对实际大气动能谱的模拟能力。就集合预报技巧改进而言,SKEB方案可以显著改善区域模式水平风场U、V的离散度,同时水平风场、温度等要素连续分级概率评分(CRPS)和离群值评分均获得改善。对SKEB方案开展的6个时间尺度(失相关时间尺度τ选取1、3、6、9、12、15 h)和6个空间相关尺度(最大截断波数Lmax选取80、100、120、160、200、240)敏感性试验结果表明,12 h失相关时间尺度和最大截断波数为240空间相关尺度的集合概率预报技巧更优。结论证明 SKEB方案可以补偿在截断尺度耗散的小尺度动能,有效提高集合预报技巧。
Abstract:The horizontal diffusion term is often used in the model to suppress nonlinear calculation instability or dampen of false short waves, but this will cause excessive dissipation of small-scale kinetic energy in the numerical model near the truncation scale. To compensate the excessively dissipated small-scale kinetic energy back to the model, a stochastic kinetic energy backscatter (SKEB) method is introduced into the CMA-REPS regional ensemble prediction system. First, based on the random field obtained in the first-order autoregressive random process in the horizontal direction expanding the spherical harmonic function we calculate the local kinetic energy dissipation rate caused by numerical diffusion scheme. Then, we construct the random flow function forcing, transform it into horizontal wind speed disturbance, and make random compensation for the dissipated kinetic energy. We carried out a 10 d ensemble prediction test and a randomized time and space scale sensitivity test in September and October 2018 (choose 1st, 7th, 13th, 19th, and 25th), and evaluated the test results here. The main conclusions of the research work are as follows. By comparing the ensemble prediction results of the test using the SKEB scheme and the test without the SKEB scheme, we see that the use of the SKEB scheme can increase the kinetic energy spectrum of the CMA-REPS regional model in the small scale region, improving the CMA-REPS ensemble prediction system to the actual atmosphere to some extent. The introduction of SKEB scheme in regional ensemble prediction can significantly improve the spread of U and V in horizontal wind field of regional model. The SKEB program has improved the forecasting skills to a certain extent, such as reducing the CRPS scores of the horizontal wind fields U and V, and also reducing the outlier scores of the horizontal wind field, temperature and 10 m wind speed. The sensitivity tests based on the SKEB method for six time scales of random pattern (1, 3, 6, 9,12, 15 h of the time series τ) and five spatial correlation scales (the maximum cutoff wave number Lmax is selected as 80, 100, 120, 160, 200, 240) show that the ensemble prediction is sensitive to the six time scales of the stochastic model of the SKEB method. And the experiment whose time scale is set to 12 h and the maximum truncation wave number is set to 240 show the best performance. Therefore, we can draw the conclusion that the SKEB scheme can compensate for the small-scale kinetic energy dissipated at the truncated scale, and effectively improve forecasting skills.
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基金项目:国家重点研发计划(2018YFC1507405)资助
引用文本:
范宇恩,李红祺,陈静,徐致真,陈法敬,邓国,2022.CMA-REPS区域集合预报随机动能后向散射方案敏感性试验[J].气象,48(9):1077-1089.
FAN Yuen,LI Hongqi,CHEN Jing,XU Zhizhen,CHEN Fajing,DENG Guo,2022.Sensitivity Experiments of a Stochastic Kinetic Energy Backscatter Scheme Within the CMA-REPS Regional Ensemble Prediction System[J].Meteor Mon,48(9):1077-1089.