Loading…

Scintillation Index of a Plane Wave Propagating Through Kolmogorov and Non-Kolmogorov Turbulence along Laser-Satellite Communication Downlink at Large Zenith Angles

Now it is indisputable fact that the Earth’s aerosphere contains Kolmogorov and non-Kolmogorov turbulence, which has been confirmed by increasing experimental evidences and theoretical investigations. Based on this, the scientific community conducts investigations on the combined influence of Kolmog...

Full description

Saved in:
Bibliographic Details
Published in:Journal of Russian laser research 2020-11, Vol.41 (6), p.616-627
Main Authors: Du, Wenhe, Cheng, Xiujuan, Wang, Yanchun, Jin, Zhan, Liu, Daosen, Feng, Shuang, Yang, Zhanyu
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Now it is indisputable fact that the Earth’s aerosphere contains Kolmogorov and non-Kolmogorov turbulence, which has been confirmed by increasing experimental evidences and theoretical investigations. Based on this, the scientific community conducts investigations on the combined influence of Kolmogorov turbulence and non-Kolmogorov one on optical wave propagating in the aerosphere. In this paper, based on the further additional measurements, a three-layer altitude-dependent turbulent spectrum model of refractive-index fluctuations for vertical/slant path is proposed to describe the variations of turbulent statistical characteristics with altitude in the aerosphere. This model that is more accurate than the two-layer model is used to estimate the performance of laser-satellite communication system for satellite-to-ground link. Using the extended Rytov theory, the scintillation index of a plant wave propagating through Kolmogorov and non-Kolmogorov turbulence along laser-satellite communication downlink at large zenith angles is presented. It is noteworthy that this expression is also valid in all regimes of turbulent fluctuations.
ISSN:1071-2836
1573-8760
DOI:10.1007/s10946-020-09916-3