Paper
15 July 2008 Solar adaptive optics system at the Hida Observatory
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Abstract
A solar adaptive optics system is developed for the 60 cm domeless solar telescope of the Hida Observatory in Japan. It is designed for compensating low order turbulence in G-band using a 52-electromagnetic-actuator deformable mirror, a 6x6 Shack-Hartmann wavefront sensor and standard personal computers. The details of the system, particularly features of the deformable mirror are described. Laboratory experiments show that the use of adaptive optics raises the Strehl ratio by a factor of five for turbulence of under 99Hz. In solar observations, the improvement of resolution in long-exposure images with the adaptive optics system is demonstrated.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Noriaki Miura, Yuuki Noto, Shuusuke Kato, Susumu Kuwamura, Naoshi Baba, Yoichiro Hanaoka, Shin'ichi Nagata, Satoru Ueno, Reizaburo Kitai, and Hideki Takami "Solar adaptive optics system at the Hida Observatory", Proc. SPIE 7015, Adaptive Optics Systems, 70156U (15 July 2008); https://doi.org/10.1117/12.788308
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Cited by 6 scholarly publications.
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KEYWORDS
Adaptive optics

Deformable mirrors

Mirrors

Wavefront sensors

Observatories

Turbulence

Cameras

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