Propagation of Bessel Gaussian beams through non-Kolmogorov turbulence based on Rytov theory

被引:21
|
作者
Wang Wanjun [1 ]
Wu Zhensen [1 ,2 ]
Shang Qingchao [1 ]
Bai Lu [1 ]
机构
[1] Xidian Univ, Sch Phys & Optoelect Engn, Xian 710071, Shaanxi, Peoples R China
[2] Xidian Univ, Collaborat Innovat Ctr Informat Sensing & Underst, Xian 710071, Shaanxi, Peoples R China
来源
OPTICS EXPRESS | 2018年 / 26卷 / 17期
基金
中国国家自然科学基金;
关键词
ORBITAL-ANGULAR-MOMENTUM; SPACE OPTICAL COMMUNICATION; ATMOSPHERIC-TURBULENCE; MARINE-ATMOSPHERE; INDEX; PERFORMANCE; CHANNELS; SPECTRUM; SYSTEMS; MODEL;
D O I
10.1364/OE.26.021712
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The average intensity of the Bessel Gaussian beams propagating through the non-Kolmogorov turbulence based on Rytov theory is derived without the quantic approximation in this paper. Therefore, this result is comparatively more accurate than that calculated by the extended Huygens-Fresnel principle, especially when the inner scale of the turbulence is small or the beams width is large. There is an interesting finding which does not exist in Gaussian beams propagation. It is the intensity variation with the inner scale that displays different behaviors when the beams width is different. Moreover, there will be some beams with specific source width, whose average intensities on the axis do not affected by the turbulence after the inner scale increasing to a certain value as their turbulence perturbation is zero. And the beams here become to the flat top beams. In summary, this paper provides an accurate method for the investigation of the Bessel Gaussian beams propagation through the non-Kolmogorov turbulence and improves the theoretical basis for the applications. (C) 2018 Optical Society of America under the terms of the OSA Open Access Publishing Agreement
引用
收藏
页码:21712 / 21724
页数:13
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