“…The atmospheric refractive index structure constant ( ) is commonly used to characterize atmospheric optical turbulence, and its distribution with height is called the atmospheric optical turbulence profile (Hutt, 1999;Wu et al, 2007). As light waves propagate in the atmosphere, they are affected by atmospheric optical turbulence, resulting in light-intensity flicker, image-point jitter, and image blurring, which affect the performance of photoelectric systems (e.g., the decline in the observation level of astronomical telescopes, the interference of laser transmission, the degradation of optical remote sensing imaging quality) (Bendersky et al, 2004;Bi et al, 2020;He et al, 2008;Rani et al, 2019). Therefore, obtaining the atmospheric optical turbulence profile is essential for improving the performance of optical systems.…”