日本地球惑星科学連合2018年大会

講演情報

[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] 大規模な水蒸気場と組織化した雲システム

2018年5月22日(火) 13:45 〜 15:15 301B (幕張メッセ国際会議場 3F)

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)、濱田 篤(富山大学都市デザイン学部)、横井 覚(海洋研究開発機構、共同)、佐藤 正樹(東京大学大気海洋研究所)、座長:三浦 裕亮

14:30 〜 14:45

[AAS02-04] MJO in a Cloud-Permitting Near-Global Equatorial Aqua-Planet Model

★Invited Papers

*Marat Khairoutdinov1 (1.Stony Brook University)

キーワード:MJO, Organized convection, cloud-resolving models

The System for Atmospheric modeling (SAM) has been run at a horizontal grid spacing of 4 km and 20 km on an equatorial aqua planet with actual equatorial circumference, extending from 46o S to 46o N latitude with a fixed, uniform sea surface temperature (SST) with perpetual equinox solar radiation. The simulations have been run for as long as one year. Despite the uniform SST, a whole range of equatorially trapped disturbances, such as Kelvin waves and a strong Madden-Julian Oscillation (MJO) have developed. Homogenizing the surface fluxes, does not prevent the formation of zonal number one mode, but completely arrests its eastward propagation. In this and in other respects, the mode behaves like self-aggregation on a sphere. The results of other mechanism denial experiments, such as homoginization of radiation and eliminating WISHE, will also be discussed.