Paper
6 February 2007 Free space optical system performance for laser beam propagation through non-Kolmogorov turbulence
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Abstract
Free space laser system performance is limited by atmospheric turbulence that has been described for many years by Kolmogorov's power spectral density model because of its simplicity. Unfortunately several experiments have been reported recently that show Kolmogorov theory is sometimes incomplete to describe atmospheric statistics properly, in particular in portions of the troposphere and stratosphere. In this paper we present a Non-Kolmogorov power spectrum which uses a generalized exponent instead of constant standard exponent value 11/3 and a generalized amplitude factor instead of constant value 0.033. Using this new spectrum in weak turbulence, we carry out, for horizontal path, analysis of Long Term Beam Spread, Scintillation index, Probability of fade, mean SNR and mean BER as variation of the spectrum exponent.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Italo Toselli, Larry C. Andrews, Ronald L. Phillips, and Valter Ferrero "Free space optical system performance for laser beam propagation through non-Kolmogorov turbulence", Proc. SPIE 6457, Free-Space Laser Communication Technologies XIX and Atmospheric Propagation of Electromagnetic Waves, 64570T (6 February 2007); https://doi.org/10.1117/12.698707
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KEYWORDS
Scintillation

Signal to noise ratio

Spherical lenses

Turbulence

Free space

Atmospheric modeling

Atmospheric turbulence

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