日本地球惑星科学連合2024年大会

講演情報

[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-AS03] 大規模な水蒸気場と組織化した雲システム

2024年5月29日(水) 10:45 〜 12:00 103 (幕張メッセ国際会議場)

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)、高須賀 大輔(東北大学大学院理学研究科)、濱田 篤(富山大学)、横井 覚(海洋研究開発機構)、座長: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)、高須賀 大輔(東京大学大気海洋研究所)

11:00 〜 11:15

[AAS03-08] Up-scale Processes of Aggregated Convection

★Invited Papers

*Chien-Ming Wu1、Fu-Sheng Kao1 (1.Department of Atmospheric Sciences, National Taiwan University)

キーワード:cloud-resolving model, buoyancy structure, Gaussian convolution , Radiative-Convective Equilbrium

In this study, we use cloud-resolving simulations of aggregated convection with a slab ocean and a mock-Walker circulation setup to diagnose the upscale processes of aggregated convection. This diagnosis is performed using the vector vorticity equation in a cloud-resolving model (VVM). We apply a Gaussian convolution filter to the simulated data to determine the structures at the filtered scale (Psi~) and the eddy scale (Psi'). By diagnosing the partition between the eddy transport of moist static energy (MSE) flux and the filtered scale MSE transport, we identify the horizontal scale and the onset of aggregated convection. This is achieved when the filter scale accounts for the majority of the transport. Our results indicate that, with a sharp onset, the horizontal scale of aggregated convection can expand from 12 km to 192 km within three days. Conversely, with a weak onset, the upscale processes can take more than a week. We examine the buoyancy structure during aggregation to understand this discrepancy. The diagnostic approaches developed in this study quantify the moisture convection feedbacks and can be applied to other types of aggregation simulations (RCEMIP) or global storm-resolving simulations (DYAMOND).