Paper
27 July 2016 Status of Hida solar adaptive optics system and experiment of tomographic wavefront sensing
Author Affiliations +
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.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Noriaki Miura, Akira Oh-ishi, Susumu Kuwamura, Naoshi Baba, Yoichiro Hanaoka, Satoru Ueno, Yoshikazu Nakatani, and Kiyoshi Ichimoto "Status of Hida solar adaptive optics system and experiment of tomographic wavefront sensing", Proc. SPIE 9909, Adaptive Optics Systems V, 99092N (27 July 2016); https://doi.org/10.1117/12.2232141
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Cited by 3 scholarly publications.
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KEYWORDS
Adaptive optics

Wavefront sensors

Wavefronts

Tomography

Observatories

Data acquisition

Sensors

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