Mei Li

TL;DR: In this article, a high-order solar adaptive optics (AO) system including a fine tracking loop and a highorder wavefront correction loop has been installed at the 1 m New Vacuum Solar Telescope of the Fuxian Solar Observatory, in routine operation since 2016.

TL;DR: A 127-element adaptive optical system has been developed and integrated into a 18m astronomical telescope in September 2009 as mentioned in this paper, and the first light on a high-resolution imaging for stars has been achieved.

TL;DR: In this paper, a 21-element adaptive optical system for stellar objects on the Yunnan Observatory 1.2m telescope is described. And the experimental results show that the adaptive system can work satisfactorily when the photon counts are as low as 93 per subaperture per integrating time, and the effects of adaptive optics in reducing the divergence and wandering of the image spot, improving resolution, and in increasing image contrast are significant.

TL;DR: The Chinese Large Solar Telescope (CLST) as mentioned in this paper is a classic Gregorian configuration telescope with an open structure, alt-azimuth mount, retractable dome, and a large mechanical de-rotator.

TL;DR: A tilt-correction adaptive optical system installed on the 430 mm solar telescope of Nanjing University has been put in operation as discussed by the authors. But the system is not suitable for large-scale observations.