2014
DOI: 10.1117/12.2055786
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Development of a new solar adaptive optics system at the Hida Observatory

Abstract: We are developing a new adaptive optics (AO) system for the 60cm domeless solar telescope of the Hida Observatory, Japan. The system has a deformable mirror with 97 piezo-actuators, a Shack-Hartmann wavefront sensor with a 10x10-microlens array and standard personal computers. We conducted solar observations in September, 2013, and confirmed that our AO system cancelled image-shifts so that the deviations were within the resolution of the telescope. We report the detailed performances of our new AO system.

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Cited by 6 publications
(3 citation statements)
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“…The limited numbers of subapertures and actuators had almost same contributions to the wavefront errors. We are developing a new full-scaled AO system with higher performances [6]. Using the new AO system, we will make further experiments to state our solar DWFS technique more specifically, not only for the Strehl ratio but also for other factors, such as the SN ratio and dynamic range of the science camera.…”
Section: Summary and Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The limited numbers of subapertures and actuators had almost same contributions to the wavefront errors. We are developing a new full-scaled AO system with higher performances [6]. Using the new AO system, we will make further experiments to state our solar DWFS technique more specifically, not only for the Strehl ratio but also for other factors, such as the SN ratio and dynamic range of the science camera.…”
Section: Summary and Discussionmentioning
confidence: 99%
“…Adaptive optics (AO) systems are being used for solar observation in various observatories [1][2][3]. We are also developing an AO system for the 60-cm domeless solar telescope at the Hida Observatory in Japan [4][5][6], which will be used for various purposes from near ultra violet to near infrared. It is, however, hard to attain full compensation especially in shorter wavelength because of severer influence of turbulence.…”
Section: Introductionmentioning
confidence: 99%
“…Instead of a point-like guide star, nonpoint structures of the target are used for the SH-wavefront sensing. This technique has already been used as a correlation-based technique in solar AO 12 14 and has gradually been recognized as a scene-based technique in biological microscopy. 15 , 16 In such sensors, correlations between SA images are evaluated to detect their relative shifts.…”
Section: Introductionmentioning
confidence: 99%