日本地球惑星科学連合2025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-AS08] 湿潤大気の多様な現象

2025年5月28日(水) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・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)、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)

17:15 〜 19:15

[AAS08-P09] Convective aggregation in deep convective gray zone mock-walker simulations

*Chun-Yian Su1、John Peters2 (1.National Taiwan University、2.Penn State)

キーワード:tropical convection, deep convective gray zone, mock-walker simulations, radiative-convective equilibrium

To better understand the multi-scale interactions between cloud systems and the large-scale overturning circulations over tropical ocean, this study aims to investigate how deep convective processes modulate the response of convective aggregation to the increase of SST gradient. We’ve carried out CM1 convection-permitting RCE simulations with non-interactive prescribed SST gradients using different horizontal grid spacings at the deep convective gray zone (3 and 9 km) and different representations of deep convection (NoCP, RAS, URAS, and URASca). Preliminary results highlight the impact of convection representation on the response of convective aggregation to SST gradient. For example, the upward branches of the circulation are located away from maximum SSTs when the prescribed SST gradient (dSST) is smaller than 0.75 K in simulations at the 3 km horizontal grid spacing. In contrast, the upward branches co-locate with maximum SSTs when the dSST is larger than 1.0 K. Interestingly, the convective aggregation driven by the SST gradient takes place at a larger dSST when the 9 km horizontal grid spacing is used. Meanwhile, the upward branches are narrower and stronger in the simulations with a cumulus parameterization. The underlying mechanisms and their implications will be further discussed.