日本地球惑星科学連合2023年大会

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[E] 口頭発表

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-AS05] 大規模な水蒸気場と組織化した雲システム

2023年5月26日(金) 15:30 〜 16:45 201A (幕張メッセ国際会議場)

コンビーナ:高須賀 大輔(東京大学大気海洋研究所)、横井 覚(海洋研究開発機構)、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)、座長:濱田 篤(富山大学)、高須賀 大輔(東京大学大気海洋研究所)

16:30 〜 16:45

[AAS05-11] The relationship between convective self-aggregation and cloud vertical mass flux distribution in cloud-resolving simulations

*神野 拓哉1三浦 裕亮1 (1.東京大学大学院理学系研究科)

キーワード:放射対流平衡、対流自己組織化

Studying the statistical characteristics of cumulus convection in an equilibrium atmosphere provides a theoretical basis for cumulus parameterization, especially when incorporating stochastic properties. In this study, 3-D radiative-convective equilibrium simulations are performed using a cloud-resolving model, and the frequency distributions of convective vertical mass flux over a wide range of model domain sizes and uniform sea surface temperatures are compared. In experiments where convection cells are spatially random, the distribution function of the mass flux of individual convection cells can be approximated as an exponential distribution. This feature supports the theory of previous studies derived from the analogy with the kinetics for ideal gases. On the other hand, in the experiments with large domain size and high sea surface temperature, where convection and moisture spontaneously form clusters (convective self-aggregation [CSA]), the mass flux distributions deviate strongly from exponential. This feature indicates that the large-scale atmospheric circulation of CSA and the local interaction between clouds affect the statistical properties of the convective cells. We also investigate the effect of prescribed sea surface temperature on various physical processes which contribute to CSA such as radiative heating and lateral entrainment.