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《Chinese Journal of Atmospheric Sciences》 2004-03
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Three-Dimensional Numerical Simulation of a Strong Convective Storm in Beijing

Liu Shuyan 1,2) , Xiao Hui 2) , Du Bingyu 1) , He Yuxiang 2) , and Zhang Ronglin 3) 1) (Nanjing Institute of Meteorology, Nanjing 210044) 2) (Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029) 3) (Chinese Academy of Meteorological Sciences, Beijing 100081)  
The fully elastic three dimensional convective storm model (IAP CSM3D) developed by the Institute of Atmospheric Physics (IAP), the Chinese Academy of Sciences was used to simulate a strong convective storm that occurred in the northeast of Beijing on June 29, 1996. The initial field of the model is the in situ observational data. Combining the observational data by the Doppler weather radar, the distribution and evolution of macro physical as well as micro-physical variations such as wind field structure, radar echo structure, overhang echo, bound weak echo region, strong echo wall, water content, etc. in the storm were analyzed. Some typical features of supercell structure were revealed on the basis of the analysis. The formation mechanism of hailstones in the storm was analyzed too. The results show that the auto conversion of frozen drops and graupels (CNfh, CNgh) are the main sources of the hailstones in the strong convective storm studied in the paper, but the contribution of frozen drops is greater than that of graupels. Hailstones mainly depend on the processes of collecting supercooled water (CLch,CLrh) to grow.
【Fund】: 国家“十五”科技攻关计划2 0 0 1BA61 0A 0 6 0 5专题;; 国家重点基础研究规划项目G1 9980 40 90 7 0 2 0 3;; 国家科技攻关计划“奥运科技”专项 2 0 0 1BA90 4B0 9课题;; 国家自然科学基金资助项目40 1 75 0 0 1;; 中国科学院大气物理研究所创新基金领域前沿项目 8 46
【CateGory Index】: P458.121.2
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