Inner- and outer-scale effects on the scintillation index of an optical wave propagating through moderate-to-strong non-Kolmogorov turbulence

被引:29
|
作者
Yi, Xiang [1 ]
Liu, Zengji [1 ]
Yue, Peng [1 ]
机构
[1] Xidian Univ, State Key Lab Integrated Serv Networks, Xian 710071, Peoples R China
来源
OPTICS EXPRESS | 2012年 / 20卷 / 04期
关键词
LOG-AMPLITUDE VARIANCE; SPECTRAL MODEL; PERFORMANCE; TROPOSPHERE; SYSTEMS;
D O I
10.1364/OE.20.004232
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
By use of the generalized von Karman spectrum model that features both inner scale and outer scale parameters for non-Kolmogorov turbulence and the extended Rytov method that incorporates a modified amplitude spatial-frequency filter function under strong-fluctuation conditions, theoretical expressions are developed for the scintillation index of a horizontally propagating plane wave and spherical wave that are valid under moderate-to-strong irradiance fluctuations. Numerical results show that the obtained expressions also compare well with previous results in weak-fluctuation regimes. Based on these general models, the impacts of finite inner and outer scales on the scintillation index of an optical wave are examined under various non-Kolmogorov fluctuation conditions. (C) 2012 Optical Society of America
引用
收藏
页码:4232 / 4247
页数:16
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