JpGU-AGU Joint Meeting 2017

講演情報

[EE] 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-EM11] [EE] Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere

2017年5月23日(火) 15:30 〜 17:00 A01 (東京ベイ幕張ホール)

コンビーナ:Chang Loren(Institute of Space Science, National Central University)、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)、Tzu-Wei Fang、座長:Fang Tzu-Wei(University of Colorado, USA)

16:30 〜 16:45

[PEM11-04] Coupling processes in the upper atmosphere revealed by imaging observation of the ISS-IMAP mission

*齊藤 昭則1穂積 裕太1坂野井 健2Perwitasari Septi2吉川 一朗3山崎 敦4大塚 雄一5 (1.京都大学大学院理学研究科地球物理学教室、2.東北大学大学院理学研究科惑星プラズマ・大気研究センター 、3.東京大学 、4.宇宙航空研究開発機構 宇宙科学研究所 、5.名古屋大学宇宙地球環境研究所 )

キーワード:Thermosphere, Ionosphere, Mesosphere, Atmospheric gravity wave, Airglow, International Space Station

Imaging observation of the ISS-IMAP (Ionosphere, Mesosphere, upper Atmosphere, and Plasmasphere mapping) mission detected the airglow in the mesosphere and the lower thermosphere (MLT), and the ion resonant scattering in the ionosphere from 2012 and 2015. It was installed on the Exposure Facility of Japanese Experiment Module of the International Space Station, EF of ISS-JEM, and consisted of two sets of imagers. Visible-light and infrared spectrum imager (VISI) observed the airglow of 730nm (OH, Alt. 85km), 762nm (O2, Alt. 95km), and 630nm (O, Alt. 250km) in the MLT region, and Extra ultraviolet imager (EUVI) observed the resonant scattering of 30.4nm (He+) and 83.4nm (O+) from ion in the Ionosphere. Horizontal two-dimensional imaging of VISI frequently detected concentric wave structures in the mesosphere. The wave features of the concentric wave structures imply the propagation direction and the center of the structure. Using them, some of them can be directly connected with the lower atmospheric phenomena, such as tornado and tropical cyclone. This observation revealed the coupling between the lower and the upper atmospheres with atmospheric gravity waves. On the topside of the ionosphere, EUVI detected the interhemispheric asymmetry of the He+ ion distribution. It shows clearly longitudinal variations, and implies that the interhemispheric neutral wind and the configuration of the geomagnetic field affect the transport of He+ as the result of the coupling process between the neutral atmosphere and the ionized atmosphere on the bottomside of the ionosphere. Results of the imaging observation of the MLT region and the ionosphere from ISS, and the coupling processes will be discussed in the presentation.