Paper
11 August 2009 The aggregate behavior of branch points: branch point density as a characteristic of an atmospheric turbulence simulator
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Abstract
The Atmospheric Turbulence Simulator used in testing in the Atmospheric Simulation and Adaptive-optic Laboratory Test-bed at Air Force Research Laboratory, Directed Energy Directorate's Starfire Optical Range is configured based on three characteristics; Fried's parameter, r0, the Rytov number, σ2χ , and the Greenwood Frequency, fG. All three may be estimated from open loop data as a means of verifying the simulated turbulence conditions for a given test configuration. However, unlike r0 and fG, the Rytov number isn't directly calculated. Instead the scintillation index is estimated from intensity measurements. At low Rytov values, (< 0.3 - 0.4), this measurement can approximate the Rytov number, however beyond a Rytov of 0.4 this parameter becomes saturated. Branch Points begin to appear after the Rytov value exceeds 0.1. In this work the behavior of the branch point density is examined to determine its viability as another parameter for calibration our turbulence simulator.
© (2009) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Denis W. Oesch, Darryl J. Sanchez, Carolyn M. Tewksbury-Christle, and Patrick R. Kelly "The aggregate behavior of branch points: branch point density as a characteristic of an atmospheric turbulence simulator", Proc. SPIE 7466, Advanced Wavefront Control: Methods, Devices, and Applications VII, 746606 (11 August 2009); https://doi.org/10.1117/12.829277
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Cited by 9 scholarly publications.
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KEYWORDS
Turbulence

Atmospheric propagation

Atmospheric turbulence

Atmospheric optics

Adaptive optics

Scintillation

Calibration

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