日本地球惑星科学連合2025年大会

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] Coupling Processes in the Atmosphere-Ionosphere System

2025年5月26日(月) 10:45 〜 12:15 303 (幕張メッセ国際会議場)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、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)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、座長:齊藤 昭則(京都大学大学院理学研究科地球物理学教室)、穂積 裕太(The Catholic University of America)


11:30 〜 11:45

[PEM12-28] ROKITS: Imaging the Aurora and Airglow from Space

★Invited Papers

*Woo Kyoung Lee1,2Hyosub Kil1,3Young-Sil Kwak1,2 (1.Korea Astronomy and Space Science Institute、2.University of Science and Technology、3.Johns Hopkins University Applied Physics Laboratory)

キーワード:ROKITS, aurora, plasma bubble, atmospheric gravity waves

The Republic of Korea Imaging Test System (ROKITS), a wide-field auroral and airglow imager onboard the Korean satellite CAS500-3, is scheduled for launch in November 2025. This imager will operate in a noon-midnight sun-synchronous orbit at an altitude of 600 km. ROKITS features three lens assemblies and an onboard computer, enabling it to capture auroral and airglow images in two spectral bands (OI 557.7 nm and OI 630.0 nm) through a narrow bandpass filter (3 nm FWHM), as well as visible images without a filter. Its 90° field of view allows ROKITS to image a swath approximately 700 km wide. The main scientific objective of ROKITS is to identify the boundaries of the auroral oval and investigate the diverse shapes of auroras. In addition to auroral studies, ROKITS' OI 557.7 nm emission data will aid in research on atmospheric gravity waves, their role in generating plasma bubbles, and the influence of traveling ionospheric disturbances in low- and mid-latitude regions. This approach offers valuable insights into the complex interactions between atmospheric phenomena and space weather.