[1] Jiakang Zhu, Qichang An, Fei Yang. Review on the measurement methods of mirror seeing of large-aperture telescope. Infrared and Laser Engineering, 52, 20220488(2023).

[2] Xiaochuan Hu, Yehuan He, Shuang Wu, et al. Effect of axial wind speed in inner propagation channel on phase characteristics of high-power lasers. Infrared and Laser Engineering, 45, 0806003(2016).

[3] C M Lowne. An investigation of the effects of mirror temperature upon telescope seeing. MNRAS, 188, 249-259(1979).

[4] M Iye, T Noguchi, Y Torii, et al. Evaluation of seeing on a 62 cm mirror. PASP, 103, 712-722(1991).

[5] Lenzo Z. The effect of the local atmospheric environment on astronomical observations[D]. Lausanne: École Polytechnique Fédérale de Lausanne, 1995.

[6] Qichang An, Xiaoxia Wu, Jingxu Zhang, et al. Detection method of mirror seeing based on curvature/slope hybrid sensing. Infrared and Laser Engineering, 50, 20200419(2021).

[7] Shanjie Huang, Zhi Li, Jun Xu, et al. Design of the LCS for the 1 m infrared solar telescope of the Yunnan Observatory. ART (Astronomical Research & Technology), 7, 344-354(2010).

[8] E P Zhang, X Q Cui, G P Li, et al. Preliminary numerical simulation of mirror seeing for the Chinese Future Giant Telescope. Research in Astronomy and Astrophysics, 16, 98(2016).

[9] Liu Yangyi. Research on active temperature control technology f large aperture groundbased solar telescopes [D]. Chengdu: Graduate School of Chinese Academy of Sciences(Institute of Optics Electronics), 2016.du: Graduate School of Chinese Academy of Sciences (Institute of Optics Electronics, Chinese Academy of Sciences), 2016. (in Chinese)

[10] Xiangyi Liu, Zhichen Wang, Zhi Wang. Dome design of large ground-based telescope. Optics and Precision Engineering, 30, 3031-3038(2022).

[11] Z Liu, Y Y Deng, D H Yang, et al. Chinese giant solar telescope. Sci Sin-Phys Mech Astron, 49, 059604(2019).

[12] Yiming Guo, Xiaoqing Wu, Chun Qing, et al. Calculation of near-surface atmospheric optical turbulence parameter based on MAD optical flow. Acta Optica Sinica, 42, 2401006(2022).

[13] D L Fried. Limiting resolution looking down through the atmosphere. J Opt Soc Am, 56, 1380-1384(1966).

[14] J A Hertig. Modélisation des impacts de perturbations thermiques dans les basses couches de l’atmosphere. IENER, N511, 134(1986).

[15] Giovannoni J M. Contribution à L''analyse de L''effet de Convection Engendré Par Un Ilot de Chaleur en Milieu Calme et Stratifié[M]. Lausanne: EPFL, 1986: 632.

[16] Sarazin. Caracterisation des Proprietes Optiques de La Turbulence Atmospherique: Application AU Choix du Site du VLT de L’observatoire Europeen Austral (ESO) [M]. Marseille: Universite, 1992.

[17] Sasiela R J . Electromagic Wave Propagation in Turbulence: Evaluation Application of Mellin Transfms[M]. 2nd ed. Berlin: Springer, 2007.

[18] Zago L, Genequ P M, Kjelberg L. Application of flexure structures to active adaptive optomechanical mechanisms[C]SPIE, 1997, 2871: 269023.