Fig. 1. Influences of inner scale and length on Cn2 using two atmospheric turbulence spectrum models. (a) Modified Hill spectrum; (b) Rytov improved model

Fig. 2. Comparison of Cn2 calculated by modified Hill spectrum under different inner scales and Kolmogorov spectrum. (a) Experimental result of all day when L=1020 m; (b) enlarged experimental result in 18:00/19:15 when L=1020 m; (c) experimental result of all day when L=2040 m; (d) enlarged experimental result in 18:00/19:15 when L=2040 m

Fig. 3. Comparison of Cn2 calculated by Rytov improved model under different inner scales and Kolmogorov spectrum. (a) Experimental result of all day when L=1020 m; (b) enlarged experimental result in 18:00/19:15 when L=1020 m; (c) experimental result of all day when L=2040 m; (d) enlarged experimental result in 18:00/19:15 when L=2040 m

Table 1. Statistical analysis for lg Cn2 of finite inner scale and not considering inner scale using modified Hill spectrum

Table 2. Statistical analysis for lg Cn2 of finite inner scale and not considering inner scale using Rytov improved model