日本地球惑星科学連合2023年大会

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[E] 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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2023年5月21日(日) 13:45 〜 15:00 101 (幕張メッセ国際会議場)

コンビーナ:Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、Yue Deng(University of Texas at Arlington)、Chairperson:Thomas J Immel(University of California Berkeley)、Chang Loren(Institute of Space Science, National Central University)


14:00 〜 14:15

[PEM12-12] Impact of El Nino-induced tropospheric ozone modulation on tides

*Huixin Liu1Masaru Kogure1Hidekatsu Jin2 (1.Earth and Planetary Science Division, Kyushu University、2.National Institute for Communication and Technology (NICT))

キーワード:atmosphere tides in MLT, troposphere ozone, tidal generation

To assess the impacts of the tropospheric ozone modulation due to El Niño on tides, we performed two simulations by using the GAIA model: zonally symmetric ozone density and longitudinal ozone variation of an El Niño pattern. Our results show that the ozone modulation strengthens (attenuates) the first symmetric mode of the DW2 (D0 and DW1) tide by ~+5% (~-1% and ~-4%) from ~20 km to ~100 km altitudes on average. These responses are probably attributed to the tropospheric ozone modulation. These responses are reasonable because both the ozone modulation and these first modes have a peak in the equator. Also, the vertical wavelengths of the first modes are about twice as long as the vertical thickness of the ozone modulation. Our results suggest that the ozone modulation due to El Niño influences the diurnal tides by a few percent because of the ozone modulation spatial structure.