Japan Geoscience Union Meeting 2014

Presentation information

Oral

Symbol P (Space and Planetary Sciences) » P-CG Complex & General

[P-CG38_1AM2] Planetary atmosphere, ionosphere and magnetosphere

Thu. May 1, 2014 11:00 AM - 12:45 PM 423 (4F)

Convener:*Takeshi Imamura(Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science), Kanako Seki(Solar-Terrestrial Environment Laboratory, Nagoya University), Yukihiro Takahashi(Department of Cosmosciences, Graduate School of Science, Hokkaido University), Yoshiyuki O. Takahashi(Center for Planetary Science), Keiichiro Fukazawa(Research Institute for Information Technology,Kyushu University), Hiromu Nakagawa(Planetary Atmosphere Physics Laboratory, Department of Geophysics, Graduate School of Science, Tohoku University), Chair:Takeshi Imamura(Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science)

12:15 PM - 12:30 PM

[PCG38-13] Observing Jupiter with an infrared camera NIIHAMA

*Takehiko SATOH1, Mizuki YONEDA2, Masato KAGITANI2, Jeff KUHN3 (1.Japan Aerospace Exploration Agency, 2.Tohoku University, 3.University of Hawaii)

Keywords:Infrared camera, Jupiter, aurora, Io, Venus, Haleakala

An infrared camera, NIIHAMA (1024x1024 pixels, PtSi array sensor), is attached to the SOLAR-C telescope (45-cm diameter off-axis Gregorian reflector) atop Haleakara in December 2013 and is now observing Jupiter.NIIHAMA's 6-position wheel houses Dark, J, H, K, 3.4-micron (for Jupiter's H3+ aurora) and 2.26-micron (for Venus night-side IR emission) filters. The primary target of this project is to monitor the brightness of Jupiter's aurora simultaneously with SPRINT-A/HISAKI and other telescopes. However, due to smaller aperture of telescope, rather low quantum efficiency of PtSi sensor, etc., Jupiter's aurora has not yet been imaged so far. On the other hand, the satellite Io while in Jupiter's shadow was observed in K band, and the night-side IR emission of Venus was successfully imaged in 2.26-micron filter. We report the result of first-light observations and also discuss improvement and observing plans in near future.