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Proceedings Paper

Development of adaptive optics devices for solar telescope
Author(s): L. V. Antoshkin; O. N. Emaleev; N. N. Botugina; P. A. Konyaev; E. A. Kopylov; V. P. Lukin
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Paper 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.

Paper Details

Date Published: 11 October 2011
PDF: 7 pages
Proc. SPIE 8178, Optics in Atmospheric Propagation and Adaptive Systems XIV, 81780G (11 October 2011); doi: 10.1117/12.897508
Show Author Affiliations
L. V. Antoshkin, V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
O. N. Emaleev, V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
N. N. Botugina, V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
P. A. Konyaev, V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
E. A. Kopylov, V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
V. P. Lukin, Tomsk State Univ. (Russian Federation)


Published in SPIE Proceedings Vol. 8178:
Optics in Atmospheric Propagation and Adaptive Systems XIV
Karin Stein; John D. Gonglewski, Editor(s)

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