日本地球惑星科学連合2014年大会

講演情報

インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM07_30PM1] Lightning and TLEs and their effects on the lower and middle atmosphere

2014年4月30日(水) 14:15 〜 16:00 213 (2F)

コンビーナ:*佐藤 光輝(北海道大学 大学院理学研究院)、足立 透(早稲田大学高等研究所)、牛尾 知雄(大阪大学大学院工学研究科情報通信工学部門)、高橋 幸弘(北海道大学・大学院理学院・宇宙理学専攻)、座長:牛尾 知雄(大阪大学大学院工学研究科情報通信工学部門)、足立 透(早稲田大学高等研究所)

15:30 〜 15:45

[PEM07-06] 航空機観測に基づくスプライトストリーマの三次元空間分布及び立体構造

*小林 縫1 (1.北海道大学理学院宇宙理学専攻)

the discovery of sprites. Though the detailed three-dimensional spatial structures and the temporal evolution of sprite streamers are the key parameters to clarify the occurrence conditions, these spatiotemporal characteristics are not clearly identified. In order to specify the detailed spatial and temporal evolution of sprite streamers, we have conducted the optical observation campaign using high-speed cameras from two jet aircrafts in summer US. In this campaign, we succeeded to capture sprite images for 28 events by the high-speed cameras with a sampling rate over 8,000 fps at each aircraft simultaneously. Using these image data, we have performed triangulation analysis to estimate the horizontal spatial distribution and vertical extent of sprite streamers. We have analyzed two types of columniform sprites; one is the columniform sprite with a preceding dense inhomogeneous halo, and the other is the columniform sprite with a preceding dim halo or without a halo. In the later case (dim halo plus columns), the following results are identified. (1) The longer the distance between sprite columns and the parent CG becomes, the higher the bottom altitude of columns becomes. (2) The longer the distance between sprite columns and the parent CG becomes, the slower the speed of downward streamer tips becomes. These results are first clear observational evident showing the horizontal spatial gradient of the quasi-electrostatic field produced by the parent CG discharge. At the presentation, we will show the electrical characteristics of the parent CG discharges derived from CMC waveforms and will discuss the possible mechanisms determining such spatial dependences.