[1] Hutt D L. Modeling and measurements of atmospheric optical turbulence over land[J]. Optical Engineering, 38, 1288-1295(1999).

[2] Liu L Y, Yao Y Q, Vernin J et al. Atmospheric turbulence measurements at Ali observatory, Tibet[J]. Proceedings of SPIE, 8444, 844464(2012).

[3] Ye Q Z, Su M, Li H et al. Tibet's Ali:asia's Atacama?[J]. Monthly Notices of the Royal Astronomical Society: Letters, 457, L1-L4(2016).

[4] Qian X, Yao Y Q, Wang H S et al. Thecharacteristics at the Ali observatory based on radiosonde observations[J]. Publications of the Astronomical Society of the Pacific, 130, 125002(2018).

[5] Li M S, Ma Y M, Ma W Q et al. Analysis of turbulence characteristics over the northern Tibetan Plateau area[J]. Advances in Atmospheric Sciences, 23, 579-585(2006).

[6] Bian L G, Xu X D, Lu L H et al. Analyses of turbulence parameters in the near-surface layer at Qamdo of the Southeastern Tibetan Plateau[J]. Advances in Atmospheric Sciences, 20, 369-378(2003).

[7] Wang S G, Lan S Z, Jiang S Y et al. Preliminary investigation on potential astronomical sites in Tibet[J]. Publications of Shanxi Observatory, 12, 1-17(1989).

[8] Wang H S. Modeling research of practice on atmospheric optical turbulence Beijing: National Astronomical Observatories,[D]. Chinese Academy of Sciences, 69-74(2012).

[9] Zhang Y J, Wang P X, Yao Y Q et al. Climate regionalization in China for astronomical observations[J]. Science in China Series G-Physics, Mechanics & Astronomy (in Chinese), 40, 1302-1314(2010).

[10] Marks R D, Vernin J, Azouit M et al. Antarctic site testing-microthermal measurements of surface-layer seeing at the South Pole[J]. Astronomy and Astrophysics Supplement Series, 118, 385-390(1996).

[11] Kornilov V, Tokovinin A, Shatsky N et al. Combined MASS-DIMM instruments for atmospheric turbulence studies[J]. Monthly Notices of the Royal Astronomical Society, 382, 1268-1278(2007).

[12] Avila R, Vernin J, Masciadri E. Whole atmospheric-turbulence profiling with generalized scidar[J]. Applied Optics, 36, 7898-7905(1997).

[13] Vernin J, Roddier F. Experimental determination of two-dimensional spatiotemporal power spectra of stellar light scintillation evidence for a multilayer structure of the air turbulence in the upper troposphere[J]. Journal of the Optical Society of America, 63, 270-273(1973).

[14] Cai J, Li X B, Zhan G W et al. A new model for the profiles of optical turbulence outer scale and Cn2 on the coast[J]. Acta Physica Sinica, 67, 014206(2018).

[15] Tatarskii V I. The effects of the turbulent atmosphere on wave propagation[M]. Jerusalem: Israel Program for Scientific Translations, 66-80(1971).

[16] Lawrence R S, Ochs G R, Clifford S F. Measurements of atmospheric turbulence relevant to optical propagation[J]. Journal of the Optical Society of America, 60, 826-830(1970).

[17] Good R E, Beland R R, Murphy E A et al. Atmospheric models of optical turbulence[J]. Proceedings of SPIE, 0928, 165-186(1988).

[18] Beland R R, Brown J H, Good R E et al. AFGL-TR-88-0153(1985).

[19] Hufnagel R E, Stanley N R. Modulation transfer function associated with image transmission through turbulent media[J]. Journal of the Optical Society of America, 54, 52-61(1964).

[21] Qing C, Wu X Q, Li X B et al. Estimation ofatmospheric optical turbulence profile by WRF model at Gaomeigu[J]. Chinese Journal of Lasers, 42, 0913001(2015).

[22] Qing C, Wu X Q, Li X B et al. Research on simulating atmospheric optical turbulence in typical area[J]. Acta Optica Sinica, 36, 0501001(2016).

[23] Wu X Q, Qian X M, Huang H H et al. Measurements of seeing, isoplanatic angle, and coherence time by using balloon-borne microthermal probes at Gaomeigu[J]. Acta Astronomica Sinica, 55, 144-153(2014).