日本地球惑星科学連合2021年大会

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[J] 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-AS06] 成層圏・対流圏過程とその気候への影響

2021年6月3日(木) 13:45 〜 15:15 Ch.06 (Zoom会場06)

コンビーナ:木下 武也(海洋研究開発機構)、坂崎 貴俊(京都大学 大学院理学研究科)、高麗 正史(東京大学大学院理学系研究科地球惑星科学専攻大気海洋科学講座)、江口 菜穂(Kyushu University)、座長:高麗 正史(東京大学大学院理学系研究科地球惑星科学専攻大気海洋科学講座)

14:35 〜 14:55

[AAS06-16] 2021年1月に発生した北半球大規模突然昇温における惑星規模波束伝播の特徴

★招待講演

*原田 やよい1、木下 武也2、佐藤 薫3、廣岡 俊彦4 (1.気象庁気象研究所、2.海洋研究開発機構、3.東京大学、4.九州大学)

キーワード:成層圏突然昇温、惑星規模波束伝播、3次元波活動度フラックス

Observational features of atmospheric fields during a major sudden stratospheric warming (MSSW) event that occurred in January 2021 (MSSW21) are analyzed using the Japanese 55-year Reanalysis, and a three-dimensional wave activity flux (3D-flux-W, Kinoshita and Sato 2013; Sato et al. 2013; Harada et al. 2019). MSSW21 is characterized by strong easterlies over 70 m s-1 around the stratopause observed in early January 2021 and a mixed signature of wavenumber 1 (WN1), WN2 and WN3 planetary waves, although WN1 has been predominant during MSSW21 except its early stage (from late December 2020 to early January 2021). In the early stage, the polar vortex was displaced from the North Pole and simultaneously broken up into two centers. After a couple of days, they were merged into one but again broken around mid-January. After that the two centers were again merged and the polar vortex begun to travel eastward around the North Pole. Thus, the synoptic feature of the polar vortex was very variable. Resultantly, MSSW21 lasted until mid-February and several warming peaks were observed during the course of its time evolution.

Further analyses revealed that wave packets repeatedly propagated upward in the Eastern Hemisphere during MSSW21. During the early stage, localized wave packets propagated upward into the upper stratosphere over western Siberia. During the mature stage (mid-January 2021), upward wave-packet propagation was observed over eastern Siberia and even in the easterly region of the upper stratosphere.