Average Polarization of Electromagnetic Gaussian Schell Model Beams through Anisotropic Non Kolmogorov Turbulence
Polarization properties of electromagnetic Gaussian Schell model beams propagating through the anisotropic non Kolmogorov turbulence of marine atmosphere channel are studied based on the cross spectral density matrix. Detailed analysis shows that the average polarization decreases with increasing the spectral index, inner scale of turbulence and generalized refractive index structure parameter. We find the effects of anisotropic turbulence on the average polarization is less than that of the isotropic turbulence and the depolarization effect of turbulence in marine atmosphere is larger than terreneatmosphere. The electromagnetic Gaussian Schell model beam with the parameters of smaller dyy, dxx and Ax, but larger Ay will reduce the interference of turbulence.