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Solar Adaptive Optics System Based on Software Control
Authors:Noriaki Miura  Takashi Kobayashi  Shinnosuke Sakuma  Susumu Kuwamura  Naoshi Baba  Yoichirou Hanaoka  Satoru Ueno  Reizaburou Kitai
Affiliation:(1) Department of Computer Sciences, Kitami Institute of Technology, 165 Koen-cho, Kitami Hokkaido 090-8507, Japan;(2) Department of Applied Physics, Graduate School of Engineering, Hokkaido University, Sapporo 060-8628, Japan;(3) National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;(4) Hida Observatory, Graduate School of Science, Kyoto University, Kamitakara, Takayama Gifu 506-1314, Japan
Abstract:An adaptive optics (AO) system for solar observations at the Hida Observatory is described, which is composed of commercially available low-cost devices and fully controlled with software in standard personal computers. This AO system operates at a frame rate of more than 250 Hz by virtue of the image processing procedures used. From laboratory experiments, it was confirmed that this AO system was useful for the temporal wavefront-variation of less than 64 Hz. During solar observations at the Hida Observatory the AO system worked well, except for a few cases.
Keywords:adaptive optics  solar observation
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