27 July 2016 Solar adaptive optics for 1m new vacuum solar telescope
Author Affiliations +
Adaptive Optics (AO) has become the requisite equipment of the ground-based large solar telescope to correct the wavefront aberration induced by the atmospheric turbulence. Two generation solar AO systems, one is the 37-element loworder AO system with 2100Hz frame rate and the other is 151-element high-order AO system with 3500Hz frame rate, were successfully developed in 2013 and 2015 respectively. In this presentation, the development of the two AO systems for 1-m New Vacuum Solar Telescope (NVST) at Fuxian Solar Observatory (FSO) will be introduced and the solar high resolution observational results are presented.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Changhui Rao, Changhui Rao, Lei Zhu, Lei Zhu, Xuejun Rao, Xuejun Rao, Lanqiang Zhang, Lanqiang Zhang, Hua Bao, Hua Bao, Lin Kong, Lin Kong, Youming Guo, Youming Guo, Libo Zhong, Libo Zhong, Xue'an Ma, Xue'an Ma, Mei Li, Mei Li, Cheng Wang, Cheng Wang, Xiaojun Zhang, Xiaojun Zhang, Xinlong Fan, Xinlong Fan, Donghong Chen, Donghong Chen, Zhongyi Feng, Zhongyi Feng, Xiaoyun Wang, Xiaoyun Wang, Naiting Gu, Naiting Gu, Zhiyong Wang, Zhiyong Wang, "Solar adaptive optics for 1m new vacuum solar telescope", Proc. SPIE 9909, Adaptive Optics Systems V, 99092I (27 July 2016); doi: 10.1117/12.2231057; https://doi.org/10.1117/12.2231057


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