首页|Solar adaptive optics systems for the New Vacuum Solar Tele-scope at the Fuxian Lake Solar Observatory
Solar adaptive optics systems for the New Vacuum Solar Tele-scope at the Fuxian Lake Solar Observatory
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Adaptive optics(AO)is essential for high-quality ground-based observations with large telescopes because it counters the impact of wavefront aberrations caused by atmospheric turbulence.The new vacuum solar telescope(NVST)is one of the most important high-resolution solar observation instruments in the world.Three sets of solar adaptive optics systems have been developed and installed on this telescope:conventional adaptive optics,ground layer adaptive optics,and multi-conjugate adaptive optics.These have been in operation from 2018 to 2023.This paper details the development and application of solar adaptive optics on the NVST and discusses the newest instrumentation.
Solar observationAdaptive opticsMulti-conjugate adaptive optics
National Laboratory on Adaptive Optics,Chengdu 610209,China
The Laboratory on Adaptive Optics,Institute of Optics and Electronics,Chinese Academy of Sciences,Chengdu 610209,China
University of Chinese Academy of Sciences,Beijing 100049,China
National Natural Science Foundation of ChinaNational Natural Science Foundation of ChinaYouth Innovation Promotion Association of the Chinese Academy of Sciences
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