講演情報
[PEM03-04]Coupling process among the mesosphere, thermosphere and ionosphere elucidated by the ISS-IMAP mission
*齊藤 昭則1、山崎 敦2、坂野井 健3、吉川 一朗4、大塚 雄一5、穂積 裕太1 (1.京都大学大学院理学研究科地球物理学教室、2.宇宙航空研究開発機構 宇宙科学研究所、3.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、4.東京大学、5.名古屋大学)
キーワード：
Ionosphere、Thermosphere、airglow
ISS-IMAP (Ionosphere, Mesosphere, upper Atmosphere, and Plasmasphere mapping) mission was installed on the Exposed Facility of Japanese Experiment Module of the International Space Station, EF of ISS-JEM, and consisted of two sets of imagers to observe the structures in the Mesosphere, Thermosphere and Ionosphere (MTI) region. Visible-light and infrared spectrum imager (VISI) of ISS-IMAP observed the airglow of 730nm (OH, Alt. 85km), 762nm (O2, Alt. 95km), and 630nm (O, Alt. 250km) in the MTI region, and Extra ultraviolet imager (EUVI) observed the resonant scattering of 30.4nm (He+) and 83.4nm (O+) from ion in the Ionosphere and Plasmasphere. ISS-IMAP was operated from 2012 to 2015. VISI elucidated global distributions of the airglow structures whose scale size is 50-500km in he nightside. The wavy structures that are interpreted to be generated by atmospheric wave were frequently observed. Some of them showed clear relationship with tropospheric phenomena as its source. EUVI elucidated global distributions of He ion. Its seasonal distribution indicates the thermospheric wind dominates the ion distribution of the topside ionosphere and the plasmasphere. Coupling processes among the MTI region and the lower atmosphere will be discussed in the presentation.