Paper
10 October 2011 Development of adaptive optics devices for solar telescope
L. V. Antoshkin, O. N. Emaleev, N. N. Botugina, P. A. Konyaev, E. A. Kopylov, V. P. Lukin
Author Affiliations +
Abstract
We are considering of new devices for solar astronomical telescope as a tools for adaptive optics correction. One of them is a high precision Shack-Hartmann wave-front sensor has been developed on the basis of a low-aperture offaxis diffraction lens array. The second device is image quality analyzer. Efficiency of the adaptive optical in system of the imaging is valued by quality of the updated image.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
L. V. Antoshkin, O. N. Emaleev, N. N. Botugina, P. A. Konyaev, E. A. Kopylov, and V. P. Lukin "Development of adaptive optics devices for solar telescope", Proc. SPIE 8178, Optics in Atmospheric Propagation and Adaptive Systems XIV, 81780G (10 October 2011); https://doi.org/10.1117/12.897508
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Cited by 1 scholarly publication.
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KEYWORDS
Sensors

Reconstruction algorithms

Adaptive optics

Wavefront sensors

Algorithm development

Image quality

Solar telescopes

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