日本地球惑星科学連合2016年大会

講演情報

インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM09] Study of coupling processes in solar-terrestrial system

2016年5月23日(月) 15:30 〜 17:00 106 (1F)

コンビーナ:*山本 衛(京都大学生存圏研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、小川 泰信(国立極地研究所)、橋口 浩之(京都大学生存圏研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:小川 泰信(国立極地研究所)

15:30 〜 15:50

[PEM09-12] 国際共同観測およびモデルに基づく南北両半球結合過程の研究 (ICSOM)

★招待講演

*佐藤 薫1 (1.東京大学 大学院理学系研究科 地球惑星科学専攻)

キーワード:南北半球結合、中層大気、成層圏突然昇温、MSTレーダー、大気大循環、重力波

Recent observational and modelling studies suggest that the Northern and Southern Hemispheres of the earth atmosphere are potentially coupled by the Lagrangian mean flow in the mesosphere modulated by waves interacting with the mean flow. However, observations of modulated wave and flow fields which are needed for quantitative understanding of the interhemispheric coupling are not sufficient. Simultaneous observations of gravity waves at various locations are most important because they are a main driver of the Lagrangian mean flow in the mesosphere.
With the start of full system observation by the PANSY radar in the Antarctic in March 2015, a global mesosphere-stratosphere-troposphere (MST) radar network extending from the Arctic to the Antarctic has been realized. The MST radars are able to observe wind vectors with fine temporal and vertical resolutions including vertical wind components in the troposphere, stratosphere and mesosphere, although an observational gap of the middle and upper stratosphere remains. Thus, the characteristics of small-scale or short-period wave motions including gravity waves and the momentum fluxes associated with these waves can be estimated with a good accuracy.
In addition, recent high-resolution general circulation models enable an explicit simulation of gravity waves under ideal and/or climatological boundary conditions and allow us to examine the momentum budget in the MST region including gravity waves, although their resolution is currently not sufficient to resolve the entire gravity wave spectrum. Real atmosphere simulations utilizing such high-resolution models are still a challenge for the MST region. However, if such real atmosphere simulations are successful, they will help quantitative interpretation of the dynamical fields observed by the MST radar network, and the observations will provide invaluable validation data for the model improvement.
Therefore we will examine the interhemispheric coupling of the earth atmosphere through a combination of simultaneous observations by networking the MST radars over the world and high-resolution model simulations of the observed atmosphere. The first international campaign was performed in 22 January-17 February 2016. Two minor stratospheric warmings occurred in the Arctic. The second one was a minor warming by its definition but the temperature at the north pole increased by about 70 K in two days at 10 hPa. Seven MST radars over the world and a lot of complementary observations were performed by more than 30 participants in eight countries. Preliminary results from this campaign will be reported.