日本地球惑星科学連合2019年大会

講演情報

[E] ポスター発表

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-AS03] 大規模な水蒸気場と組織化した雲システム

2019年5月28日(火) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:三浦 裕亮(国立大学法人 東京大学大学院 理学系研究科 地球惑星科学専攻)、濱田 篤(富山大学)、横井 覚(海洋研究開発機構)、佐藤 正樹(東京大学大気海洋研究所)

[AAS03-P09] ひまわり8号観測と高解像度シミュレーションにおける熱帯の雲辺縁のフラクタル的性質について

*神野 拓哉1 (1.東京大学大学院理学系研究科)

キーワード:フラクタル、ひまわり8号、雲解像モデル

Cloud clusters show a wide variety of shape and size, and their spatial pattern is often taken up as a typical example of fractal. However, the methods of studying fractal are in an early stage of development. In this study, we conducted fractal analysis on the perimeter of tropical clouds using satellite observation and cloud-resolving simulation of sub-kilometer resolution. We evaluated fractal dimension as a function of spatial scale (transient fractal dimension) and quantified the characteristic spatial scale of the pattern from the scale where self-similarity breaks down. From the observational data from HIMAWARI-8, It is shown that the self-similarity of the cloud perimeter persists only in the spatial scale range from 2 km up to 30 km. The limit of the self-similarity is suggested to be the characteristic scale of the pattern formation of tropical clouds. The cloud-resolving simulation data with NICAM also shows finite-size self-similarity. However, the profile of the transient fractal dimension changed with integration time far more rapidly than HIMAWARI-8 observation, and it lost its self-similarity at the end of the 48-hour simulation. This process is suggested to reflect the increase of stratiform cloud in the upper-troposphere as an adjustment to the transition of spatial resolution.