28 September 2004 Solar site testing for the Advanced Technology Solar Telescope
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The location of the Advanced Technology Solar Telescope (ATST) is a critical factor in the overall performance of the telescope. We have developed a set of instrumentation to measure daytime seeing, sky brightness, cloud cover, water vapor, dust levels, and weather. The instruments have been located at six sites for periods of one to two years. Here we describe the sites and instrumentation, discuss the data reduction, and present some preliminary results. We demonstrate that it is possible to estimate seeing as a function of height near the ground with an array of scintillometers, and that there is a distinct qualitative difference in daytime seeing between sites with or without a nearby lake.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Frank Hill, Frank Hill, Jacques Beckers, Jacques Beckers, Peter Brandt, Peter Brandt, John Briggs, John Briggs, Timothy Brown, Timothy Brown, W. Brown, W. Brown, Manuel Collados, Manuel Collados, Carsten Denker, Carsten Denker, Steven Fletcher, Steven Fletcher, Steven Hegwer, Steven Hegwer, T. Horst, T. Horst, Mark Komsa, Mark Komsa, Jeff Kuhn, Jeff Kuhn, Alice Lecinski, Alice Lecinski, Haosheng Lin, Haosheng Lin, Steve Oncley, Steve Oncley, Matthew Penn, Matthew Penn, Thomas R. Rimmele, Thomas R. Rimmele, Hector Socas-Navarro, Hector Socas-Navarro, Kim Streander, Kim Streander, } "Solar site testing for the Advanced Technology Solar Telescope", Proc. SPIE 5489, Ground-based Telescopes, (28 September 2004); doi: 10.1117/12.551812; https://doi.org/10.1117/12.551812

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