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)

[PEM12-16] Comparison between migrating atmospheric tides in TIMED/SABER observations and free running WACCM-X simulations

*Yi Chung Chiu1Loren Chang1Cornelius Csar Jude Salinas1Qian Liying 2 (1.Graduate Institute of Space Science and Engineering, National Central University, Taiwan、2.High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA)

キーワード:WACCM-X, TIMED/SABER, Atmospheric Tides

The Whole Atmosphere Community Climate model – eXtended (WACCM-X) is a comprehensive numerical model with a range from the Earth’s surface to the upper thermosphere (~ 500 km) and also includes the ionosphere. Excited in the troposphere and stratosphere, atmospheric tides are the dominant dynamical feature in the mesosphere and lower thermosphere and play an important role in vertical coupling. In this study, we used the least squares method to extract diurnal and semidiurnal migrating tides from free running WACCM-X temperatures in the mesosphere and lower thermosphere region (MLT). The results are compared to observations from TIMED/SABER. Differences in tidal structure and variation during solar maximum and minimum in March and June are examined, to better understand the variation of migrating tides resolved in free running WACCM-X, and its implications for future studies utilizing this model.