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Proceedings Paper

Solar adaptive optics system at the Hida Observatory
Author(s): Noriaki Miura; Yuuki Noto; Shuusuke Kato; Susumu Kuwamura; Naoshi Baba; Yoichiro Hanaoka; Shin'ichi Nagata; Satoru Ueno; Reizaburo Kitai; Hideki Takami
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Paper 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.

Paper Details

Date Published: 15 July 2008
PDF: 8 pages
Proc. SPIE 7015, Adaptive Optics Systems, 70156U (15 July 2008); doi: 10.1117/12.788308
Show Author Affiliations
Noriaki Miura, Kitami Institute of Technology (Japan)
Yuuki Noto, Kitami Institute of Technology (Japan)
Shuusuke Kato, Kitami Institute of Technology (Japan)
Susumu Kuwamura, Kitami Institute of Technology (Japan)
Naoshi Baba, Hokkaido Univ. (Japan)
Yoichiro Hanaoka, National Astronomical Observatory of Japan (Japan)
Shin'ichi Nagata, Hida Observatory, Kyoto Univ. (Japan)
Satoru Ueno, Hida Observatory, Kyoto Univ. (Japan)
Reizaburo Kitai, Hida Observatory, Kyoto Univ. (Japan)
Hideki Takami, Subaru Telescope, National Astronomical Observatory of Japan (United States)


Published in SPIE Proceedings Vol. 7015:
Adaptive Optics Systems
Norbert Hubin; Claire E. Max; Peter L. Wizinowich, Editor(s)

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