Near-ground turbulence profiles from lunar scintillometer

A simple and inexpensive six-channel array of photodiodes, LuSci, can measure weak moonlight scintillation produced by optical turbulence within few hundred metres above the ground. We describe the instrument, its operation and data reduction. Measured covariances of lunar scintillation are fitted t...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society Vol. 404; no. 3; pp. 1186 - 1196
Main Authors: Tokovinin, A., Bustos, E., Berdja, A.
Format: Journal Article
Language:English
Published: Oxford, UK Blackwell Publishing Ltd 21-05-2010
Wiley-Blackwell
Oxford University Press
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Online Access:Get full text
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Summary:A simple and inexpensive six-channel array of photodiodes, LuSci, can measure weak moonlight scintillation produced by optical turbulence within few hundred metres above the ground. We describe the instrument, its operation and data reduction. Measured covariances of lunar scintillation are fitted to a smooth turbulence profile model with few parameters. Complete recipe for calculating the instrument response (including the effects of Moon's phases) is given. The robustness of the results relative to various experimental factors and model assumptions is investigated. We give examples of the data and compare LuSci with other turbulence profilers. LuSci finds numerous applications in nighttime site testing and monitoring.
Bibliography:istex:8C4280764A92FE3941C73529132B3FFF62FC2C31
ark:/67375/HXZ-XB59RH3Q-C
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
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ISSN:0035-8711
1365-2966
DOI:10.1111/j.1365-2966.2010.16367.x