Radial Gaussian-Schell-model array beams in oceanic turbulence

被引：10
|
作者：
Mao, Yonghua [1 ,2 ]
Mei, Zhangrong [1 ]
Gu, Juguan [1 ]
Zhao, Yuchen [3 ]
机构：
[1] Huzhou Univ, Dept Phys, Huzhou 313000, Peoples R China
[2] Zhejiang Univ Technol, Dept Phys, Hangzhou 310014, Zhejiang, Peoples R China
[3] Deloitte Consulting Co Ltd, Shanghai 200002, Peoples R China
来源：
APPLIED PHYSICS B-LASERS AND OPTICS | 2017年 / 123卷 / 04期
基金：
中国国家自然科学基金;
关键词：
PROPAGATION; ATMOSPHERE; INTENSITY; LIGHT;
D O I：
10.1007/s00340-017-6680-4
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
Based on the extended Huygens-Fresnel principle, the analytical expression for the cross-spectral density (CSD)function of the radial Gaussian-Schell-model array (RGSMA) beams propagating in oceanic turbulence is derived. Then, combined with the spatial power spectrum of oceanic turbulence, analytical formulas for the average intensity and the root-mean-square (rms) beam width of the RGSMA beams propagating in oceanic turbulence are obtained. The changes of the average intensity and the rms beam width with propagation distance z and three oceanic turbulence parameters, including temperature-salinity balance parameter w, mean square temperature dissipation rate xT, and energy dissipation rate per unit mass epsilon, are investigated in detail. The results have certain reference value for the propagation properties of the RGSMA beams in oceanic turbulence.
引用
收藏
页数：7
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