Scintillation index analysis of radial Gaussian vortex beam array propagation in atmosphere
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摘要:
涡旋光束阵列在自由空间光通信上有很大的应用价值。采用多相位屏模拟大气湍流,研究了径向高斯涡旋光束阵列在大气湍流环境中传输的光场演化过程和轴上闪烁特性,分析了不同初始光束参数对径向高斯涡旋光束阵列的轴上闪烁指数的影响,并将其与单束高斯涡旋光束的轴上闪烁指数进行了对比。研究结果表明:在弱湍流区域,rytov指数小于0.5时,单束高斯涡旋光束的轴上闪烁指数一直保持在小于1的数值区域,远小于径向高斯涡旋光束的轴上闪烁指数;而在中等强度湍流区域,径向高斯涡旋光束阵列的轴上闪烁指数小于单束高斯涡旋光束的轴上闪烁指数;径向高斯涡旋光束阵列的轴上闪烁指数会随着轨道角动量值的减小和径向阵列半径的增大而减小。研究结果对于大气湍流环境下的涡旋光通信具有一定的理论意义和应用价值。
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关键词:
- 径向高斯涡旋光束阵列 /
- 轴上闪烁指数 /
- 相位屏仿真
Abstract:Beam arrays have great application value in free-space optical communication. The light intensity evolution and the on-axis scintillation index of radial Gaussian vortex beam array propagating through atmospheric turbulence are analyzed based on multi-phase screen simulation. The effect of initial beam parameters on the scintillation properties of radial Gaussian vortex beam array is studied, and the variation of the on-axis scintillation index values of radial Gaussian vortex beam array and a Gaussian vortex beam is compared. The results indicate that in the weak fluctuation regime, the on-axis scintillation index of Gaussian vortex beams remains within a numerical range of less than 1, while the on-axis scintillation index of radial Gaussian vortex beam arrays is around 1. In the medium fluctuation regime, the on-axis scintillation index of the radial Gaussian vortex beam array is smaller than that of a single Gaussian vortex beam. And the on-axis scintillation index of radial Gaussian vortex beam array decreases with the decrease of orbital angular momentum and the increase of radial array radius. The research results have certain theoretical significance and application value for vortex optical communication in turbulent atmospheric environments.
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图 3 RGVBA在真空中不同传输距离处的光强和相位分布图 (a)
$Z $ =0 m,光强 (b)$Z $ =50 m,光强 (c)$Z $ =1000 m, 光强 (d)$Z $ =2000 m,光强 (e)$Z $ =0 m,相位 (f)$Z $ =50 m,相位 (g)$Z $ =1000 m,相位 (h)$Z $ =2000 m,相位Figure 3. Light intensity distribution of RGVBA at different propagation distances in free space (a)
$Z $ =0 m, light intensity (b)$Z $ =50 m, light intensity (c)$Z $ =1000 m, light intensity (d)$Z $ =2000 m, light intensity (e)$Z $ =0 m, phase (f)$Z $ =50 m, phase (g)$Z $ =1000 m, phase (h)$Z $ =2000 m, phase图 4 不同折射率结构常数
$C_n^2$ 下RGVBA的光强分布($l = 2$ ,$Num = 9$ ,Z=2000 m) (a)$C_n^2 = 0$ (b)$ C_n^2 = $ $ 5 \times {10^{ - 15}}{m^{{{ - 2} / 3}}} $ (c)$ C_n^2 = 5 \times {10^{ - 14}}{m^{{{ - 2} \mathord{\left/ {\vphantom {{ - 2} 3}} \right. } 3}}} $ (d)$ C_n^2 = 1 \times $ $ {10^{ - 13}}{m^{{{ - 2} / 3}}} $ Figure 4. The intensity distribution of RGVBA under different refractive index structure constants
$C_n^2$ ($l = 2$ ,$Num = 9$ , Z=2000 m) (a)$C_n^2 = 0$ (b)$ C_n^2 = $ $ 5 \times {10^{ - 15}}{m^{{{ - 2} / 3}}} $ (c)$ C_n^2 = 5 \times {10^{ - 14}}{m^{{{ - 2} \mathord{\left/ {\vphantom {{ - 2} 3}} \right. } 3}}} $ (d)$ C_n^2 = 1 \times $ $ {10^{ - 13}}{m^{{{ - 2} /3}}} $ 表 1 相位屏仿真参数
Table 1. Phase screen simulation parameters
采样网格$N$ 采样间隔$\Delta x$ 相位屏间隔$\Delta Z$ 湍流内尺度${l_0}$ 湍流外尺度${L_0}$ 1024 1.7 mm 200 m 0.01 m 10 m 波长$\lambda $ OAM值$l$ 子光束半径${w_0}$ 阵列半径${r_0}$ 子光束数目$Num$ 1550 nm1~3 3 mm 1.8 cm 6 表 2 不同折射率结构常数和传输距离对应的rytov指数
Table 2. The rytov index corresponding to different refractive index structure constants and transmission distances
折射率结构常数$C_n^2$ 传输距离范围$Z$ rytov指数$\sigma _R^2$ $1 \times {10^{ - 15}}{m^{{{ - 2} \mathord{\left/ {\vphantom {{ - 2} 3}} \right. } 3}}}$ 200 m− 2400 m0.0010 −0.0991 $5 \times {10^{ - 15}}{m^{{{ - 2} \mathord{\left/ {\vphantom {{ - 2} 3}} \right. } 3}}}$ 200 m− 2400 m0.0052 −0.4953 $1 \times {10^{ - 14}}{m^{{{ - 2} \mathord{\left/ {\vphantom {{ - 2} 3}} \right. } 3}}}$ 200 m− 2400 m0.0104 −0.9905 -
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