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首页> 外文期刊>ournal of the Meteorological Society of Japan >Structure and Evolution of Precipitation Cores in an Isolated Convective Storm Observed by Phased Array Weather Radar
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Structure and Evolution of Precipitation Cores in an Isolated Convective Storm Observed by Phased Array Weather Radar

机译:分阶段阵列天气雷达观察到分离的对流风暴中沉淀芯的结构和演变

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摘要

A phased array weather radar (PAWR) can complete one volume scan in 30 s, thus enabling us to obtain high spatiotemporal resolution echo intensities and wind fields of storms. Using its rapid scanning capability, we investigated the evolution of a convective storm in detail. To describe the evolution of convective storms, we used the following definitions. The precipitation cell is defined as a three-dimensionally contiguous region of 40 dBZ or greater. The precipitation core is defined by a threshold of positive deviation greater than 7 dBZ, which is a difference from the average reflectivity during the mature stage of the cell. An updraft core is defined as an updraft region of 1 m s ?1 or stronger at a height of 2 km.
机译:分阶段阵列天气雷达(PAWR)可以在30秒内完成一个体积扫描,从而使我们能够获得高时的时空分辨率回声强度和风暴风暴。 利用其快速扫描能力,我们详细探讨了对流风暴的演变。 要描述对流风暴的演变,我们使用以下定义。 沉淀细胞定义为40dBz或更大的三维连续区域。 沉淀核心由大于7dBz的正偏差的阈值限定,这是与细胞成熟阶段期间的平均反射率的差异。 上升磁芯被定义为1M S?1或更强的高度为2公里的上升区域。

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