Paper
25 September 2007 The Levy fractional Brownian motion family as a new paradigm in the modeling of turbulent wave-front phase
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Abstract
In Perez et al. [J. Opt. Soc. Am. A 21 (10), 2004] we have given a general formalism to model the turbulent wave-front phase by using fractional Brownian motion processes. Moreover, it extends classical results to non- Kolmogorov turbulence: the Strehl ratio and the angle-of-arrival variance are shown to be dependent on the dynamic state of the turbulence. Nevertheless, this model has its drawbacks as it is unable of handling the stationarity of the phase increments over the full inertial range. The Levy fractional Brownian motion (LfBm) family is then introduced here in order to overcome this problem.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Darío G. Pérez, Luciano Zunino, and Mario Garavaglia "The Levy fractional Brownian motion family as a new paradigm in the modeling of turbulent wave-front phase", Proc. SPIE 6708, Atmospheric Optics: Models, Measurements, and Target-in-the-Loop Propagation, 670806 (25 September 2007); https://doi.org/10.1117/12.734391
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Cited by 1 scholarly publication.
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KEYWORDS
Motion models

Turbulence

Lanthanum

Atmospheric propagation

Telescopes

Wavefronts

Fractal analysis

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