Statistical properties of electromagnetic anomalous vortex beam with orbital angular momentum in atmospheric turbulence

被引:10
作者
Xu, Yonggen [1 ]
Dan, Youquan [2 ]
机构
[1] Xihua Univ, Sch Sci, Dept Phys, Chengdu 610039, Sichuan, Peoples R China
[2] Civil Aviat Flight Univ China, Dept Phys, Guanghan 618307, Sichuan, Peoples R China
来源
OPTIK | 2019年 / 179卷
基金
中国国家自然科学基金;
关键词
Electromagnetic anomalous vortex beam with orbital angular momentum; Atmospheric turbulence; Average intensity; Degree of polarization; M-2-factor; LAGUERRE-GAUSSIAN BEAMS; FLAT-TOPPED BEAMS; PARTIALLY COHERENT BEAMS; SCHELL-MODEL BEAM; DARK HOLLOW BEAMS; PROPAGATION PROPERTIES; KOLMOGOROV; POLARIZATION; GENERATION; M-2-FACTOR;
D O I
10.1016/j.ijleo.2018.10.194
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Statistical properties of an electromagnetic anomalous vortex (EAV) beam with orbital angular momentum (OAM) through a turbulent atmosphere are studied. Analytical formulae for the average intensity (AI) and degree of polarization (DOP) of EAV beam in a strong turbulence are derived. Accurate analytical formulae (without any approximations) for M-2-factor of EAV beam under all turbulence conditions are also derived based on the second-order moments of the Wigner distribution function. Numerical results show that the transverse distributions for Al of EAV beam depend mainly on topological charge, beam order and structure constant of turbulence. An anomalous result is found that the on-axis intensity is larger for an EAV beam in a stronger turbulence (i.e., larger structure constant and smaller inner scale). Inner scale effects of DOP of the EAV beam in strong turbulence are also investigated. Off-axis DOPs of an EAV beam will appear oscillation near the propagation axis. It can be also found that M-2-factor of an EAV beam propagating through the strong and weak turbulence are smaller for smaller transverse coherent length and structure constant of turbulence, larger beam order, topological charge and inner scale of turbulence.
引用
收藏
页码:654 / 664
页数:11
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