Paper
16 July 2008 High-resolution SLODAR measurements on Mauna Kea
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Abstract
We have made high order (32x32 subaperture) Shack-Hartmann wavefront sensor observations of binary stars with separations of approximately 20 arcseconds using the University of Hawaii 2.2 m telescope. We present preliminary results of a Slope Detection and Ranging (SLODAR) analysis of the data yielding measurements of turbulence strength, wind velocity and velocity dispersion as a function of altitude, with approximately 500 m vertical resolution. The aim of the investigation is to explore the validity of the Taylor frozen flow approximation and the implications for layer-oriented predictive AO reconstruction algorithms.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Timothy Butterley, Richard W. Wilson, Mark R. Chun, Remy Avila, and Jose-Luis Aviles "High-resolution SLODAR measurements on Mauna Kea", Proc. SPIE 7015, Adaptive Optics Systems, 70154L (16 July 2008); https://doi.org/10.1117/12.790351
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Cited by 1 scholarly publication.
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KEYWORDS
Telescopes

Stars

Turbulence

Adaptive optics

Wavefront sensors

Sensors

Reconstruction algorithms

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