[1] [1] F Roddier. The effects of atmospheric turbulence in optical astronomy[J]. Progress in Optics, 1981, 19: 281-376.

[2] [2] Hu Yuehong, Qiang Xiwen, Feng Shuanglian, et al.. Modeling of atmospheric turbulence in boundary layer over desert[J]. Acta Optica Sinica, 2013, 33(s1): s101005.

[3] [3] M S Belen′kii, D W Roberts, J M Stewart, et al.. Experimental validation of the differential image motion lidar concept[J]. Opt Lett, 2000, 25(8): 518-520.

[4] [4] G G Gimmestad, M W Dawsey, D W Roberts, et al.. Field validation of optical turbulence lidar technique[C]. SPIE, 2005, 5793: 10-16.

[5] [5] G G Gimmestad, D W Roberts, J M Stewart, et al.. Testing of LIDAR system for turbulence profiles[C]. SPIE, 2008, 6951: 695109.

[6] [6] Gatland, J M Stewart, G G Gimmestad. Inversion techniques for the differential image motion lidar[C]. SPIE, 2009, 7324: 73240C1.

[7] [7] G G Gimmestad, David Roberts, John Stewart, et al.. Development of a lidar technique for profiling optical turbulence[J]. Opt Eng, 2012, 51(10): 101713.

[8] [8] Dai Yang, Lin Zhaoxiang, Zhang Wenyan, et al.. Method of atmospheric turbulence measurement by lidar[J]. High Power Laser and Particle Beams, 2006, 18(11): 1769-1773.

[9] [9] F D Eaton, W A Peterson, J R Hines, et al.. Comparison of two techniques for determining atmospheric seeing[C]. Orlando Technical Symposium, 1988, 296: 319-334.

[10] [10] M Sarazin, F Roddier. The ESO differential image motion monitor[J]. Astronomy and Astrophysics, 1990, 227: 294-300.

[11] [11] G Palladino, A Basili, G Di Cocco, et al.. Design of a high update-rate star sensor for arcsec-level attitude determination from balloon-borne X/γ astronomy platforms[J]. Experimental Astronomy, 2006, 21(3): 169-187.

[12] [12] B R Frieden.Probability, Statistical Optics, and Data Testing[M]. New York: Springer, 2001. 256.