日本地球惑星科学連合2023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-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) 13:45 〜 15:15 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:高須賀 大輔(東京大学大気海洋研究所)、濱田 篤(富山大学)

13:45 〜 14:00

[AAS05-01] Coupling Momentum and Variance in a MMF with a 2D CRM

★Invited Papers

*Walter Michael Hannah1、Kyle Pressel2、Mikhail Ovchinnikov2、Qiu Yang2、Ruby Leung2、Gregory Elsaesser3、Matthew Norman4、Ben Hillman5 (1.Lawrence Livermore National Laboratory、2.Pacific Northwest National Laboratory、3.NASA、4.Oak Ridge Leadership Computing Facility、5.SNL)

キーワード:atmospheric modelling, multiscale modelling framework, convective momentum transport, GPU acceleration, tropical variability

An atmospheric multiscale modeling framework (MMF) allows an explicit representation of convection by coupling a cloud resolving model (CRM) with a general circulation model (GCM). This avoids the need for conventional parameterizations of clouds and turbulence. Traditional MMF implementations often use a 2D CRM with periodic boundary conditions to constrain the computational cost, but some consequences of this approach are that convective momentum transport cannot be explicitly represented and small-scale fluctuations within the CRM cannot be transported by the large-scale flow. These limitations can be problematic because they force the model to ignore key atmospheric processes. Two enhancements have been implemented in the E3SM-MMF to address these deficiencies. The first is the momentum transport scheme of Tulich (2015) in which the large-scale momentum field is represented in the CRM by two scalars, which allows the 3D momentum transport to be approximated by a 2D CRM. The second feature is a scheme that allows small scale fluctuations within the CRM to be transported between CRM instances on the global grid.