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Proceedings Paper

Status of Hida solar adaptive optics system and experiment of tomographic wavefront sensing
Author(s): Noriaki Miura; Akira Oh-ishi; Susumu Kuwamura; Naoshi Baba; Yoichiro Hanaoka; Satoru Ueno; Yoshikazu Nakatani; Kiyoshi Ichimoto
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Paper Abstract

An adaptive optics (AO) system is developed for the 60cm domeless solar telescope of the Hida Observatory, Japan. Its performances are analyzed by the computer simulations, and improved by replacing the Zernike polynomials by Karhunen-Loève functions. Also, a tomographic wavefront sensor is developed for a ground-layer AO system. From test data acquired at the Hida observatory, wavefront-phase maps both in the ground-layer and in an upper layer are successfully derived.

Paper Details

Date Published: 27 July 2016
PDF: 6 pages
Proc. SPIE 9909, Adaptive Optics Systems V, 99092N (27 July 2016); doi: 10.1117/12.2232141
Show Author Affiliations
Noriaki Miura, Kitami Institute of Technology (Japan)
Akira Oh-ishi, Kitami Institute of Technology (Japan)
Susumu Kuwamura, Kitami Institute of Technology (Japan)
Naoshi Baba, Hokkaido Univ. (Japan)
Muroran Institute of Technology (Japan)
Yoichiro Hanaoka, National Astronomical Observatory of Japan (Japan)
Satoru Ueno, Kyoto Univ. (Japan)
Yoshikazu Nakatani, Kyoto Univ. (Japan)
Kiyoshi Ichimoto, Kyoto Univ. (Japan)

Published in SPIE Proceedings Vol. 9909:
Adaptive Optics Systems V
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

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