日本地球惑星科学連合2016年大会

講演情報

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セッション記号 A (大気水圏科学) » A-AS 大気科学・気象学・大気環境

[A-AS13] ミクロスケール気象現象解明にむけた稠密観測・予報の新展開

2016年5月23日(月) 10:45 〜 12:15 301A (3F)

コンビーナ:*古本 淳一(京都大学生存圏研究所)、常松 展充(東京都環境科学研究所)、荒木 健太郎(気象研究所)、座長:東 邦明(京都大学生存圏研究所・メトロウェザー株式会社)

12:00 〜 12:15

[AAS13-12] スキャン型Kaバンドドップラーレーダとステレオ写真測量による山岳上の積乱雲発生過程の観測

★招待講演

*三隅 良平1櫻井 南海子1前坂 剛1鈴木 真一1清水 慎吾1岩波 越1 (1.防災科学技術研究所)

It is known that convective storms are frequently initiated over mountains in warm and humid environment. According to previous studies, shallow cumuli initiated over heated mountains develop into a deep convective storm. However, the transition process from shallow to deep convection is not well understood due to a lack of observation data. In order to elucidate this problem, we observed convective clouds initiated over mountains in Kanto, Japan on 18 August 2011 using a 35 GHz scanning Doppler radar and a pair of digital cameras. The first cloud observed over the mountains reached the 6 km level, while the maximum echo-top height was about 1 km lower than the cloud top. The maximum radar reflectivity in the cloud was about 10 dBZ found around the 2 to 3 km levels. The reason why the echo-top altitude was lower than the cloud-top height was considered to be due to the mixing with surrounding dry air. After such shallow cumuli appeared three times repeatedly, a deep convective cloud developed. These results are consistent with a "pre-conditioning" hypothesis, that shallow cumuli moisten midlevel air and produce favorable condition for development of deep convective storms.