JpGU-AGU Joint Meeting 2020

講演情報

[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] 大気圏ー電離圏結合

コンビーナ:Huixin Liu(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)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)

[PEM12-18] Dynamical response in the upper atmosphere: GAIA simulation with doubled CO2

*Liu Huixin1Tao Chihiro2Jin H.2 (1.九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、2.NICT)

キーワード:温暖ガス、寒冷化、大気循環、大気力学

It is known that increasing CO2 in the atmosphere will produce global cooling in the thermosphere, in contrast to global warming in the troposphere. However, how will thermosphere dynamics and wave activity change remain unclear. In this study, we explore these aspects via a doubled-CO_2 numerical experiment using the whole atmosphere model GAIA. Model simulations were done for solar minimum under geomagnetic quiet conditions, with the CO2 mixing ratio set at 345 ppm and 690 ppm, respectively. The results reveal three major features in the doubled-CO_2 impacts. 1. The thermosphere cools about 10K more around solstices than equinoxes, more at the summer pole than the winter pole. 2. The meridional circulation strongly accelerates by 5--15 m/s. 3. The tidal activity experiences dramatic changes, with a 40--60% reduction in the semi-diurnal tides (SW2) throughout the thermosphere, but an 30-50% enhancement in diurnal tides (DW1) below 200 km altitude. The non-migrating tide DE3 changes only about 3K. These changes in meridional circulation and tides are robust features in all seasons, and can profoundly affect the spatial and local time distribution of the ionospheric responses via composition and electrodynamics.