Year-end Sale % OFF 
Abstract
The effects of atmospheric turbulence on the propagation of Hollow Gaussian beams (HGBs) within the regime of weak fluctuations have been investigated using the paraxial approximation and the Rytov theory. The statistical moments, the scintillation index, the probability of fade, and the duration of fade are studied analytically and numerically. The numerical results show that these parameters depend on the beam order n, the spot size w0, the refractive index structure parameter n, and the wavelength λ.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
