Paper
6 August 2010 Surface layer characterization at Paranal Observatory
G. Lombardi, J. Melnick, R. H. Hinojosa Goñi, J. Navarrete, M. Sarazin, A. Berdja, A. Tokovinin, R. Wilson, J. Osborn, T. Butterley, H. Shepherd
Author Affiliations +
Abstract
In this paper the Paranal Surface Layer characterization is presented. Causes, physics and behavior of the SL above Paranal surface are discussed. The analysis is developed using data from different turbulence profilers operated during several campaigns between 2007 and 2009. Instruments used are SL-SLODAR, DIMM, Elevated DIMM, MASS, Lunar Scintillometer and Ultrasonic Anemometers with temperature sensors positioned at different strategic heights.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
G. Lombardi, J. Melnick, R. H. Hinojosa Goñi, J. Navarrete, M. Sarazin, A. Berdja, A. Tokovinin, R. Wilson, J. Osborn, T. Butterley, and H. Shepherd "Surface layer characterization at Paranal Observatory", Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 77334D (6 August 2010); https://doi.org/10.1117/12.856772
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Cited by 7 scholarly publications.
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KEYWORDS
Turbulence

Stars

Stereolithography

Ultrasonics

Observatories

Telescopes

Temperature metrology

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