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台风利奇马(1909)与台风摩羯(1814)云特征对比
引用本文:郑倩,毛程燕,丁丽华,廖君钰,潘欣,刘佩,雷奕文,黄亿.台风利奇马(1909)与台风摩羯(1814)云特征对比[J].应用气象学报,2022,33(1):43-55.
作者姓名:郑倩  毛程燕  丁丽华  廖君钰  潘欣  刘佩  雷奕文  黄亿
作者单位:1.浙江省衢州市气象局,衢州 324000
基金项目:国家自然科学基金项目(41590873,41705089);浙江省气象局一般项目(2020YB19);浙江省气象局青年项目(2020QN34)。
摘    要:利用FY-2H, Aqua, CALIPSO(Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation)和GPM(Global Preciptation Measurement)卫星产品, 对比同在浙江温岭沿海登陆且路径相似的台风利奇马(1909)和台风摩羯(1814), 分析其发展过程中云系水平、垂直结构特征以及登陆前台风三维结构特征。结果表明: 台风眼区是否可见、台风云系的螺旋明显程度、最强降水中心的形状变化、螺旋雨带区南北侧云顶高度的差异均是台风发展强弱的重要标志。台风发展成熟阶段云顶高度最大位于台风眼附近。台风登陆前, 台风越强, 单层云占比越高, 多层云占比越少; 台风越强, 光学厚度越大; 台风云系类别主要是深对流云和卷云, 成分以非定向冰为主; 螺旋雨带区云系的云底高度及厚度与台风发展强弱相关; 同一通道下高低亮温区的面积、台风的降水类型、三维降水结构中的对流柱长度和数量、垂直方向上的降水率均可作为台风发展强弱的依据。

关 键 词:台风利奇马(1909)    台风摩羯(1814)    相似路径台风
收稿时间:2021-09-19

Comparison of Cloud Characteristics Between Typhoon Lekima(1909)and Typhoon Yagi(1814)
Zheng Qian,Mao Chengyan,Ding Lihua,Liao Junyu,Pan Xin,Liu Pei,Lei Yiwen,Huang Yi.Comparison of Cloud Characteristics Between Typhoon Lekima(1909)and Typhoon Yagi(1814)[J].Quarterly Journal of Applied Meteorology,2022,33(1):43-55.
Authors:Zheng Qian  Mao Chengyan  Ding Lihua  Liao Junyu  Pan Xin  Liu Pei  Lei Yiwen  Huang Yi
Affiliation:1.Quzhou Meteorological Bureau of Zhejiang, Quzhou 3240002.Yangling Meteorological Bureau of Shaanxi, Yangling 7121003.Changshan Meteorological Bureau of Zhejiang, Quzhou 324400
Abstract:Previous studies show that two typhoons with similar landing area and similar moving tracks may have significant differences in precipitation intensity, which are caused by different structure and characteristics of the cloud systems. Based on FY-2H, Aqua, CALIPSO(Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation) and GPM(Global Precipitation Measurement) satellite data, the horizontal and vertical structural characteristics of the cloud system, 3-dimensional structure and characteristics of Typhoon Lekima(1909) and Typhoon Yagi(1814), which landed along the Wenling coast of Zhejiang Province, are discussed. The visibility of typhoon eye area and the helicity of typhoon cloud system in TBB images are important indicators of typhoon development. The precipitation near the typhoon center is the largest, and the spatial distribution of typhoon precipitation is asymmetrical. For the typhoons with similar paths, strong typhoon induces circular strong precipitation center, while weak typhoon is along with belt-type strong precipitation center. In the mature stage of typhoon development, the maximum cloud top height is near the typhoon eye. When the cloud top height on the north side of the spiral rain belt area is lower than that on the south side, the typhoon develops strongly. When the cloud top height on the south side of the spiral rain belt area is lower than that the the north side, the typhoon is relatively weak. Before typhoon landing, the proportion of single layer cloud is higher when the typhoon is stronger, and the atmosphere is optically thicker. Typhoon clouds are mainly deep convective clouds and cirrus clouds consisting of non-directional ice. The height of cloud base and thickness in spiral rainband are related to the development of typhoon. Before typhoon landing, the area of high and low brightness temperature under the same channel, the precipitation type of typhoon, the length and number of convective columns in the 3-dimensional precipitation structure, and the precipitation rate in vertical direction can all indicate the development of typhoon. Regardless the typhoon strength, the total amount of ice water particles is roughly the same, and the difference in intensity is reflected in the areas of the high and low brightness temperature under the same channel. The spiral rain belt of a strong typhoon is dominated by stratiform precipitation, while a weak typhoon is dominated by convective precipitation. The number and length of convective columns of a strong typhoon are far greater than those of a weak typhoon.
Keywords:Typhoon Lekima(1909)  Typhoon Yagi(1814)  similar track typhoon
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