Development of adaptive optics devices for solar telescope

摘要

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 off-axis 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.