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13 September 2012 Solar adaptive optics at the Hida Observatory: latest achievements of current system and design of new system
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Abstract
Solar adaptive optics (AO) systems are developed at the 60cm domeless solar telescope in the Hida Observatory, Japan. An AO system currently used has a deformable mirror with high-speed 97 electromagnetic actuators and a Shack- Hartmann wavefront sensor with a 10x10-microlens array and 4000fps-CMOS camera. Its control frequency is about 1100-1400 Hz, and hence the -3dB cutoff frequency of the system is theoretically above 100 Hz. In parallel to developing the system, a new full-scaled AO system is designed to be applicable to various observations, such as highdispersion spectroscopy and simultaneous wide-range spectroscopy. The new system will work as classical AO at first. The details of the current system, observational results using it, and the design of the new AO system are described.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Noriaki Miura, Jun'ichi Miyazaki, Susumu Kuwamura, Naoshi Baba, Yoichiro Hanaoka, Masashi Yamaguchi, Satoru Ueno, Yoshikazu Nakatani, Shin'ichi Nagata, Reizaburou Kitai, Kiyoshi Ichimoto, and Hideki Takami "Solar adaptive optics at the Hida Observatory: latest achievements of current system and design of new system", Proc. SPIE 8447, Adaptive Optics Systems III, 84474D (13 September 2012); https://doi.org/10.1117/12.925848
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