Japan Geoscience Union Meeting 2025

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM12] Coupling Processes in the Atmosphere-Ionosphere System

Mon. May 26, 2025 10:45 AM - 12:15 PM 303 (International Conference Hall, Makuhari Messe)

convener:Keisuke Hosokawa(Department of Communication Engineering and Informatics, University of Electro-Communications), Huixin Liu(Earth and Planetary Science Division, Kyushu University SERC, Kyushu University), Yuichi Otsuka(Institute for Space-Earth Environmental Research, Nagoya University), Loren Chang(Department of Space Science and Engineering, National Central University), Chairperson:Akinori Saito(Department of Geophysics, Graduate School of Science, Kyoto University), Yuta Hozumi(The Catholic University of America)


11:30 AM - 11:45 AM

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

★Invited Papers

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

Keywords: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.