JpGU-AGU Joint Meeting 2017

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[EE] 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-AS02] [EE] Cloud-Resolving Model Simulations for Cloud-Related Processes in Climate and Weather Studies

2017年5月22日(月) 13:45 〜 15:15 301B (国際会議場 3F)

コンビーナ:Toshi Matsui(NASA GSFC & ESSIC UMD)、佐藤 正樹(東京大学大気海洋研究所)、Wei-Kuo Tao(Senior Scientist)、座長:Matsui Toshihisa(NASA GSFC / ESSIC UMD)、座長:佐藤 正樹(東京大学大気海洋研究所)、座長:Tao Wei-Kuo (NASA GSFC)

Cloud-system-related problems are at the heart of global and regional climate simulations and the understanding of climate change. Convective clouds not only release latent heat from condensation and vertically redistribute heat and moisture, but also play important role in the global and regional hydrological cycle through the precipitation and the modification of shortwave and longwave radiative fluxes at the ocean and land surface. However, the representation of cloud systems in general circulation models (GCMs) and regional climate models (RCMs) remains one of major challenges for the climate simulations. The improvement to the existing convection and cloud parameterization schemes in GCMs has been slow. The development of cloud-resolving models (CRMs) provides a unique opportunity to evaluate and improve the existing convection, cloud and radiation schemes. While GCMs require convection and cloud parameterizations, CRMs explicitly resolve convection and mesoscale organization, where cloud microphysical processes and cloud-radiation interactions directly respond to the cloud-scale dynamics. Increasing studies have been focused on the application of CRM simulations to improve parameterizations of subgrid-scale physical processes in GCMs; to understand the interaction of cloud systems with large-scale circulations; and to replace the cloud-related parameterizations in GCMs. The goal of this session is to showcase the current efforts on this challenging task and encourage the collaboration between the CRM, GCM and RCM modelers. Wider areas of studies on applications of CRM in climate, weather, and environmental simulations are also acceptable.

15:00 〜 15:15

*佐藤 陽祐1三浦 裕亮2八代 尚1五藤 大輔3竹村 俊彦4道端 拓朗4鈴木 健太郎5中島 映至6 (1.理化学研究所計算科学研究機構、2.東京大学大学院地球惑星科学専攻、3.国立環境研究所、4.九州大学応用力学研究所、5.東京大学大気海洋研究所、6.宇宙航空研究開発機構地球観測研究センター)

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