日本地球惑星科学連合2021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-AS01] 大規模な水蒸気場と組織化した雲システム

2021年6月4日(金) 17:15 〜 18:30 Ch.07

コンビーナ: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)、佐藤 正樹(東京大学大気海洋研究所)

17:15 〜 18:30

[AAS01-P02] The Different Pathways to self-aggregation between SCALE and VVM

★Invited Papers

*Ching-Shu Hung1、Hiroaki Miura1、Jin-De Huang2、Chien-Ming Wu2 (1.The University of Tokyo、2.National Taiwan University)

キーワード:self-aggregation

In this study, self-aggregation simulations following Wing et al. (2018) are conducted focusing on the development toward self-aggregation by two cloud-resolving models (SCALE and VVM). Even though the two models reach self-aggregation state after 40 days of simulations, the pathways toward aggregation are very different given the same sea surface temperature. The dry area expansion through radiative cooling is evident in SCALE which effectively shrinks the moist region while VVM takes a different route through the convection development in the moist region. The subsidence induced by the convection organization further enhances the expansion of the dry region leading to the self-aggregation. The isentropic analyses show that the aggregation in SCALE is through the development of strong shallow circulation while it is through the subsidence warming from aloft in VVM. The time evolution of convective core clouds distribution can be a precursor of the different pathway.