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Proceedings Paper

Optical turbulence above mountains seen in 3D
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Paper Abstract

Atmospheric optical turbulence is the main driver of wavefront distortions which affect optical telescope performance. Therefore, many techniques have been developed to measure the optical turbulence strength along the line of sight. Based on data collected with the MASS (Multi Aperture Scintillation Sensor), we show that a large sample of such measurements can be used to assess the average three dimensional turbulence distribution above ground. The use of, and a more sophisticated instrumental setup for, such turbulence tomography will be discussed.

Paper Details

Date Published: 5 August 2010
PDF: 11 pages
Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 77331Q (5 August 2010); doi: 10.1117/12.856304
Show Author Affiliations
S. G. Els, Gaia Data Analysis and Processing Consortium (Spain)
Cerro Tololo Inter-American Observatory (Chile)
K. Vogiatzis, TMT Observatory Corp. (United States)
A. Otárola, TMT Observatory Corp. (United States)
R. Riddle, TMT Observatory Corp. (United States)
Caltech Optical Observatories (United States)
M. Schöck, TMT Observatory Corp. (United States)
W. Skidmore, TMT Observatory Corp. (United States)
T. Travouillon, TMT Observatory Corp. (United States)


Published in SPIE Proceedings Vol. 7733:
Ground-based and Airborne Telescopes III
Larry M. Stepp; Roberto Gilmozzi; Helen J. Hall, Editor(s)

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