星地探測閃電在一次中尺度對流系統中的活動特征分析
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山東省氣象局科研項目(2020sdqxz07)資助


Analysis of Activity Characteristics of Satellite-to-Ground Lightning Detection in A Mesoscale Convective System
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    摘要:

    為更好地發揮星地閃電探測資料在中尺度對流系統中的監測預警應用潛力,本文以2018年6月27日山東地區的一次中尺度對流系統為例,利用云頂溫度、云頂降溫率、雷達等資料與FY-4A閃電成像儀LMI(Lightning Mapping Imager)、ADTD(Advanced TOA and Direction system)閃電定位系統星地閃電探測資料,分析了星地閃電數據在中尺度對流系統中閃電分布特征及其與對流演變的關系,結果表明:星地探測閃電一致性較好,LMI相對位于對流云前方,星地閃電與降水區域吻合度較高。在系統發展初期,LMI超前于ADTD探測到閃電,且位于回波中心和前側,回波垂直方向呈現出向前傾斜特征,這對于判識對流移動和演變趨勢有較好的指示作用,在預報業務中可采用LMI的位置來輔助制作強對流落區預報。在成熟階段,星地閃電頻次出現躍增,正地閃比例較高,該時段山東多地發生冰雹災害,LMI多出現在對流系統移動方向前方的弱回波或無回波區內,ADTD則更接近回波中心位置。合并階段,部分LMI位于前方強回波區后部,與強回波區相對應。

    Abstract:

    In order to better exert the monitoring and early warning application potential of satellitetoground lightning detection data in the Mesoscale Convective System (MCS), this study takes an MCS in Shandong on June 27, 2018, as a case, using the cloud top temperature, cooling rate, the reflectivity from radar and the satellite-to-ground lightning data from FY-4A Lightning Mapping Imager (LMI) and Advanced TOA and Direction system (ADTD) to analyze the lightning distribution characteristics and its relationship with the evolution of convection. The results show a good consistence of the satellite-to-ground lightning data. The lighting of LMI was further located in front of the convective cloud and had a high agreement with the precipitation region. In the early development stage of MSC, LMI detected lightning earlier than ADTD, and the lightning was located in the centre and the front side of the radar echo. The vertical section of the echo showed a forward tilting, which was a good indicator of the movement and evolution trend of convection. Thus, the location of the lightning from LMI could be used to assist in the forecast of strong convection areas. In the mature stage, the frequency of satellite-to-ground lightning increased, and the proportion of positive ground lightning was relatively large. Hail disasters occurred in many places in Shandong Province during this period. The LMI mostly appeared in the weak or no-echo area in front of the moving direction of the convective system, while the ADTD lightning was closer to the centre position of the echo. During the merging stage, some of the LMI lightning was located at the backside of the front, strong echo area corresponding to the strong echo area.

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劉向科,康寧,張琴,劉暢.星地探測閃電在一次中尺度對流系統中的活動特征分析[J].氣象科技,2023,51(1):14~21

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  • 收稿日期:2022-03-17
  • 定稿日期:2022-10-10
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  • 在線發布日期: 2023-03-03
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