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Numerical study on the periodic bahavior of mesoscale convective systems

机译:中尺度对流系统周期性行为的数值研究

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The observed or simulated MCSs often shows pulsation with a period of a few hours. Two-dimensional experiment in this study suggest that such periodicity can be interpreted in terms of interaction between gravity waves and convective system. In a medium range of low-level environmental wind shear, simulated convective clouds are periodically organized into a larger convective clouds with the time period of a few hours and pulsative strong rainfall occured. The analysis of model output demonstrates rearward propagating meso-β cloud and assosicated updrafts/downdrafts have characteristics of 'vertically propagating' gravity waves. A conceptual model of a evolution of MCS in one cycle is proposed in Fig.6. In response to the tilted heating in the meso-β cloud, internal gravity waves with reaward tilting phase-lines are generated and these disturbances propagates rearward as wave train. Propagation of downdraft phase over the low-level convective clouds supresses the development of each clouds and weakning of the system. As the downward phase propagates further rearward and an updraft phase of the waves arrives over the cloud area, it contribute to the development of next meso-β cloud and reintensification of the system. The periodic formations of highly tilted clouds in the medium shear range, are not usually reported in other numerical studies of midlatitude squall lines (e.g. Fovell and Ogura, 1989) . The difference of the storm behavior can be attributed to the thermody-namic profiles used in our study. We used input ther-modynamic conditions which are conductive to producing weak cold pool (~ -6K), while many other simulated midlatitude storms possesed rather strong cold pool (~ -10K). When the cold pool is strong and the gust front propagates fast, the clouds formed at the gust front are readily broken away from the top of the gust front and rapidly decay as it propagates reai-ward. On the othehand, when the cold pool is weak and gust front is slow moving, the cloud can be connected to the gust front long time and the formation of highly sloped cloud is possible.
机译:观察到的或模拟的MCS经常显示出几个小时的脉动。这项研究中的二维实验表明,这种周期性可以用重力波与对流系统之间的相互作用来解释。在中等水平的低水平环境风切变作用下,模拟对流云会定期组织成较大的对流云,时间为数小时,并且会产生强烈的强降雨。对模型输出的分析表明,向后传播的中观β云和相关的上升/下降气流具有“垂直传播”重力波的特征。图6提出了MCS在一个周期内演化的概念模型。响应于中层β云中的倾斜加热,产生了具有倾斜倾斜相线的内部重力波,这些扰动随着波列向后传播。低层对流云上向下气流阶段的传播阻碍了每个云层的发展和系统的弱化。随着下行阶段进一步向后传播,并且波的上升阶段到达整个云区域,这有助于下一个中观β云的发展和系统的增强。在中纬度qua线的其他数值研究中(例如Fovell和Ogura,1989)通常没有报道中等剪切范围内高倾斜云的周期性形成。风暴行为的差异可以归因于我们的研究中使用的热力风廓线。我们使用的输入热力学条件有助于产生弱冷池(〜-6K),而许多其他模拟的中纬度风暴则具有较强的冷池(〜-10K)。当冷池结实且阵风锋面快速传播时,在阵风锋面形成的云很容易从阵风锋面的顶部破裂,并在向后传播时迅速衰减。另一方面,当冷池较弱且阵风前沿移动缓慢时,云可以长时间连接到阵风前沿,并且可能形成高度倾斜的云。

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  • 来源
    《Workshop on Flood Forecasting》|2000年|p.33-36|共4页
  • 会议地点 Beijing(CN)
  • 作者

    Masayuki Kawashima;

  • 作者单位

    Institute of Low Temperature Science Hokkaido University N19 W8 Kita-ku Sapporo 060-0819 Japan;

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