[1] [1] Hubin N, Arsenault R, Conzelmann R, et al. Ground layer adaptive optics[J]. Comptes Rendus Physique, 2005, 6(10): 1099-1109.

[2] [2] Marchetti E, Brast R, Delabre B, et al. MAD on sky results in star-oriented mode[C]. SPIE Astronomical Telescopes + Instrumentation. Proc SPIE 7015, Adaptive Optics Systems, Marseille, France. 2008, 7015: 61-72.

[3] [3] Rimmele T R, Woeger F, Marino J, et al. Solar multiconjugate adaptive optics at the dunn solar telescope[C]. SPIE Astronomical Telescopes + Instrumentation. Proc SPIE 7736, Adaptive Optics Systems II, San Diego, California, USA. 2010, 7736: 1086-1092.

[4] [4] Ren D Q, Jolissaint L, Zhang X, et al. Solar ground-layer adaptive optics[J]. Publications of the Astronomical Society of the Pacific, 2015, 127(951): 469-478.

[5] [5] Baranec C, Lloyd-Hart M, Milton N M. Ground-layer wave front reconstruction from multiple natural guide stars[J]. The Astrophysical Journal Letters, 2007, 661(2): 1332-1338.

[6] [6] Hart M, Milton N M, Baranec C, et al. A ground-layer adaptive optics system with multiple laser guide stars[J]. Nature, 2010, 466(7307): 727-729.

[7] [7] Rao C H, Gu N T, Rao X J, et al. First light of the 1.8-m solar telescope—CLST[J]. Science China Physics, Mechanics & Astronomy, 2020, 63(10): 109631.

[8] [8] Zhang L Q. Solar Multi-Conjugate Adaptive Optics for High Resolution Imaging[D]. Chengdu: Institute of Optics and Electronics, University of Chinese Academy of Sciences, 2014.

[9] [9] Tokovinin A. Seeing improvement with ground-layer adaptive optics[J]. Publications of the Astronomical Society of the Pacific, 2004, 116(824): 941-951.

[10] [10] Liu Z, Xu J. 1-meter near-infrared solar telescope[J]. Astronomical Society of India Conference Series, 2011, 2: 9-17.

[11] [11] Ellerbroek B L, Rigaut F J. Scaling multiconjugate adaptive optics performance estimates to extremely large telescopes[C]. Astronomical Telescopes and Instrumentation. Proc SPIE 4007, Adaptive Optical Systems Technology, Munich, Germany. 2000, 4007: 1088-1099.

[12] [12] Wang Z Y, Zhang L Q, Rao C H. Characterizing daytime wind profiles with the wide-field Shack-Hartmann wavefront sensor[J]. Monthly Notices of the Royal Astronomical Society, 2019, 483(4): 4910-4921.