Paper
25 October 2004 Development of a portable SLODAR turbulence profiler
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Abstract
We report on the development of a prototype portable monitor for profiling of the altitude and velocity of atmospheric optical turbulence. The instrument is based on the SLODAR Shack-Hartmann wave-front sensing technique, applied to a portable telescope and employing an electron-multiplication (EM) CCD camera as the wave-front sensor detector. Constructed for ESO by the astronomical instrumentation group at the University of Durham, the main applications of the monitor will be in support of the ESO multi-conjugate adaptive optics demonstrator (MAD) project, and for site characterization surveys for future extremely large telescopes. The monitor can profile the whole atmosphere or can be optimized for profiling of low altitude (0-1km) turbulence, with a maximum altitude resolution of approximately 150m. First tests of the system have been carried out at the La Palma observatory.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Richard W. Wilson, John Bate, Juan Carlos Guerra, Norbert N. Hubin, Marc Sarazin, and Christopher D. Saunter "Development of a portable SLODAR turbulence profiler", Proc. SPIE 5490, Advancements in Adaptive Optics, (25 October 2004); https://doi.org/10.1117/12.551258
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Cited by 15 scholarly publications.
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KEYWORDS
Turbulence

Telescopes

Stars

Profiling

Adaptive optics

Sensors

Binary data

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