日本地球惑星科学連合2016年大会

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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-EM03] Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere

2016年5月22日(日) 10:45 〜 12:15 A01 (アパホテル&リゾート 東京ベイ幕張)

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)、齊藤 昭則(京都大学大学院理学研究科地球物理学教室)、Chang Loren(Institute of Space Science, National Central University)、新堀 淳樹(京都大学生存圏研究所)、座長: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)

10:45 〜 11:05

[PEM03-06] A numerical study of the effects of migrating tides on thermosphere midnight density maximum

★招待講演

*Jiuhou Lei1Haibing Ruan1Jian Du2Wenbin Wang3 (1.USTC University of Science and Technology of China、2.Department of Physics and Astronomy, University of Louisville, USA、3.High Altitude Observatory, National Center for Atmospheric Research, USA)

キーワード:thermosphere, midnight density maximum, migrating tides

We employed the NCAR Thermosphere Ionosphere Electrodynamics General Circulation Model (TIEGCM) and the extended Canadian Middle Atmosphere Model (eCMAM) to investigate the role of the migrating terdiurnal tide on the formation and variation of the thermosphere midnight temperature maximum (MTM) and midnight mass density maximum (MDM). The migrating terdiurnal tide from the eCMAM was applied at the TIEGCM’s lower boundary, along with the migrating diurnal and semidiurnal tides from the Global Scale Wave Model (GSWM). Several numerical experiments with different combinations of tidal forcing at the TIEGCM’s lower boundary were carried out to determine the contribution of each tide to MTM/MDM. We found that the interplay between diurnal, semidiurnal and terdiurnal tides determines the formation of MTM/MDM and their structure in the upper thermosphere. The decrease of thermospheric mass density after MDM reaches its maximum at ~02:00 local time is mainly controlled by the terdiurnal tide. Furthermore, we examined the generation mechanisms of the migrating terdiurnal tide in the upper thermosphere and found that they come from three sources: upward propagation from the lower thermosphere, in-situ generation via nonlinear interaction and thermal excitation.