First light of solar multi-conjugate adaptive optics at the 1-m new vacuum solar telescope
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摘要:
Observations play a leading role in any branches of astronomy,including solar physics.In order to solve fundamental problems,such as solar dynamo [1],coronal heating [2] and the triggering of major solar eruptions [3],solar observations with spatial resolution better than 0.1 arcsec are required.Such a goal cannot be achieved without the help of adaptive optics (AO),which eliminates the wavefront distortion caused by atmosphere turbulence [4,5].However,solar observations are performed over an extended field of view (FoV).