Two-Mirror Adaptive System for Correction of Atmospheric Disturbances of the Large Solar Vacuum Telescope


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Abstract

Features of a two-mirror adaptive system for correction of atmospheric disturbances of the Large Solar Vacuum Telescope are described. The system has been developed with allowance for the correction of instrumental vibrations of the telescope in a wide amplitude-frequency range, with an open siderostat supply mirror. The light wavefront tilt and its deformations are corrected separately. The adaptive optics system is designed to work with extended light sources (the Sun), with low-contrast image details.

About the authors

N. N. Botygina

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch

Email: lukin@iao.ru
Russian Federation, Tomsk, 634055

D. Yu. Kolobov

Institute of Solar-Terrestrial Physics, Siberian Branch

Email: lukin@iao.ru
Russian Federation, Irkutsk, 664033

P. G. Kovadlo

Institute of Solar-Terrestrial Physics, Siberian Branch

Email: lukin@iao.ru
Russian Federation, Irkutsk, 664033

V. P. Lukin

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch

Author for correspondence.
Email: lukin@iao.ru
Russian Federation, Tomsk, 634055

S. A. Chuprakov

Institute of Solar-Terrestrial Physics, Siberian Branch

Email: lukin@iao.ru
Russian Federation, Irkutsk, 664033

A. Yu. Shikhovtsev

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch

Email: lukin@iao.ru
Russian Federation, Tomsk, 634055

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