Comparison of Index of Refraction Structure Function ( C <sub>n</sub> <sup>2</sup>) Profiles Derived from Polar-orbiting Satellite Data and Numerical Weather Prediction Models

David C. Meier; Steven T. Fiorino

doi:10.1364/PCDVTAP.2015.PM1C.3

Imaging and Applied Optics 2015
OSA Technical Digest (online) (Optica Publishing Group, 2015),
paper PM1C.3
•https://doi.org/10.1364/PCDVTAP.2015.PM1C.3

Comparison of Index of Refraction Structure Function ( $C_{n}^{2}$ ) Profiles Derived from Polar-orbiting Satellite Data and Numerical Weather Prediction Models

David C. Meier and Steven T. Fiorino

Propagation through and Characterization of Distributed Volume Turbulence and Atmospheric Phenomena 2015

Arlington, Virginia United States
7–11 June 2015
ISBN: 978-1-943580-00-2

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pcDVT: Structure of Turbulence (PM1C)

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D. C. Meier and S. T. Fiorino, "Comparison of Index of Refraction Structure Function ( C _n ²) Profiles Derived from Polar-orbiting Satellite Data and Numerical Weather Prediction Models," in Imaging and Applied Optics 2015, OSA Technical Digest (online) (Optica Publishing Group, 2015), paper PM1C.3.

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Abstract

Paper describes novel technique to derive wind and turbulence fields from satellite data. Results are compared to numerical weather data, and modifications to the method to characterize turbulence in a neutrally-buoyant boundary layer are discussed.

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