Propagation properties of radially polarized multi-Gaussian Schell-model beams in oceanic turbulence

被引：12

作者：

Song, Zhenzhen ^{[1
]}

Han, Zhiyuan ^{[1
]}

Ye, Jingfei ^{[1
]}

Liu, Zhengjun ^{[2
]}

Liu, Shutian ^{[3
]}

Liu, Bo ^{[1
]}

机构：

[1] Nanjing Univ Informat Sci & Technol, Sch Phys & Optoelect Engn, Nanjing 210044, Jiangsu, Peoples R China

[2] Harbin Inst Technol, Dept Automat Test & Control, Harbin 150001, Heilongjiang, Peoples R China

[3] Harbin Inst Technol, Dept Phys, Harbin 150001, Heilongjiang, Peoples R China

来源：

JOURNAL OF THE OPTICAL SOCIETY OF AMERICA A-OPTICS IMAGE SCIENCE AND VISION | 2019年 / 36卷 / 10期

基金：

中国国家自然科学基金;

关键词：

OPTICAL WIRELESS COMMUNICATION; STATISTICAL PROPERTIES; 2ND-ORDER STATISTICS; AVERAGE INTENSITY; VORTEX BEAM; FREE-SPACE; COHERENCE; QUALITY;

D O I：

10.1364/JOSAA.36.001719

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

By utilizing the extended Huygens-Fresnel principle, we derive the analytical formulas for the cross-spectral density matrix elements of a radially polarized multi-Gaussian Schell-model (RPMGSM) beam propagating in oceanic turbulence. Effects of beam parameters and oceanic turbulence parameters on the propagation properties of RPMGSM beams are investigated in detail by numerical simulation. Our results show that the RPMGSM beam with larger beam order M has an advantage over the radially polarized Gaussian Schell-model beam for reducing turbulence-induced degradation. Compared with temperature-induced turbulence fluctuation, the salinity-induced turbulence fluctuation makes a greater contribution to the influence on propagation properties of RPMGSMbeams. (C) 2019 Optical Society of America

引用

页码：1719 / 1726

页数：8

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