JpGU-AGU Joint Meeting 2020

講演情報

[E] 口頭発表

セッション記号 M (領域外・複数領域) » M-SD 宇宙開発・地球観測

[M-SD46] Effects of lightning, severe weather and tropical storms

コンビーナ:佐藤 光輝(北海道大学 大学院理学研究院)、Yoav Yair(Interdisciplinary Center Herzliya)、Xiushu Qie(Institute of Atmospheric Physics, Chinese Academy of Sciences)、高橋 幸弘(北海道大学・大学院理学院・宇宙理学専攻)

[MSD46-03] Cell-Scale Analysis of Convective Cloud Merging in a Squall Line and the Associated Lightning Behaviour

★招待講演

*Lu Jingyu1,2Qie Xiushu1,2Jiang Rubin1Liu Dongxia1Wang Dongfang1Yuan Shanfeng1Chen Zhixiong1,2Li Jinliang3Xiao Xian4,5Yi Xiaoyuan6 (1.Key Laboratory of Middle Atmosphere and Global Environment Observation (LAGEO), Institute of Atmospheric Physics, Chinese Academy of Science, Beijing, China.、2.College of Earth and Planetary Science, University of Chinese Academy of Science, Beijing, China.、3.Key Laboratory of Semi-Arid Climate Change, Ministry of Education, College of Atmospheric Sciences, Lanzhou University, Lanzhou, China.、4.Institute of Urban Meteorology, China Meteorological Administration, Beijing, China.、5.Beijing Urban Meteorological Engineering Research Center, Beijing, China.、6.Tianjin Meteorological Observatory, Tianjin, China.)

キーワード:squall line、convective cloud merger、cloud bridge、lightning activity、radar reflectivity

The merging process of convective cells in a severe squall line and its impact on lightning behaviour is analysed in detail, by using the observations from the Beijing Lightning Network (BLNET), Doppler weather radar, and other meteorological data. The vertical profiles of the radar reflectivity indicate that the convective cells connected each other through cloud bridges at heights of 3~7 km during the merging process. The lightning data with high spatiotemporal resolution show that the total flash rate dropped immediately at the beginning of the cloud merger, then increased sharply and eventually peaked when the merger finished. A Similar feature was also involved in the cloud-to-ground (CG) lightning activity. At the later stage of the merger, the lightning activity of the cells in the front seemed to be more consistent. It is found that the cell-merging process had significantly different effects on different cells. The cells at the rear of the storm tended to be weakened by the merging and they dissipated thereafter, while the front cells were enhanced substantially with rapid growth in scale and intensity, termed as a rear-cell feeding merger. The dynamic field inferred from the VDRAS (Variational Doppler Radar Analysis System) shows that the updraft was dominant at the front cells of the storm, while downdraft was dominant in the middle and in the lower layers at the rear cells during the merger, as combined with strong low-level wind shear. The inflow contains both the humid air in the lower layer ahead of the cell and the outflow of the rear cells, providing abundant water vapour which favoured the development of the front cells.