Paper
24 October 2012 Optical propagation in a turbulent atmosphere using the split step method
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Abstract
It is well known that optical signals propagating through the atmosphere are subject to random fluctuations in phase and amplitude. These fluctuations are caused by random temperature distributions in the atmosphere, which manifests themselves as a random index of refraction changes along the propagation path. We introduce a simulation method for modeling atmospheric turbulence effects, which is based on a split-step approach to numerically solve the parabolic wave equation. Atmospheric turbulence effects are modeled by a number of phase screens. These phase screens are generated on a numerical grid of finite size, which corresponds to a narrow spatial area of atmospheric turbulence.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Heba Yuksel and Fulya C. Kunter "Optical propagation in a turbulent atmosphere using the split step method", Proc. SPIE 8517, Laser Communication and Propagation through the Atmosphere and Oceans, 85170O (24 October 2012); https://doi.org/10.1117/12.929598
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Atmospheric propagation

Atmospheric optics

Wave propagation

Turbulence

Atmospheric turbulence

Radio propagation

Atmospheric modeling

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