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LOLAS: an optical turbulence profiler in the atmospheric boundary layer with extreme altitude resolution
Authors:R. Avila,J. L. Avilé  s,R. W. Wilson,M. Chun,T. Butterley, E. Carrasco
Affiliation:Centro de Radioastronomía y Astrofísica, UNAM, Apartado Postal 3-72, Morelia, Michoacán C.P. 58089, México;Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis Enrique Erro 1, Tonantzintla, Puebla C.P. 72840, México;Department of Physics, University of Durham, Rochester Building, South Road, Durham DH1 3LE;Institute for Astronomy, University of Hawaii, 640 North A'ohoku Place, 209 Hilo, HI 96720-2700, USA
Abstract:
We report the development and first results of an instrument called Low Layer SCIDAR (Scintillation Detection and Ranging) (LOLAS) which is aimed at the measurement of optical-turbulence profiles in the atmospheric boundary layer with high altitude resolution. The method is based on the Generalized SCIDAR (GS) concept, but unlike the GS instruments which need a 1-m or larger telescope, LOLAS is implemented on a dedicated 40-cm telescope, making it an independent instrument. The system is designed for widely separated double-star targets, which enables the high altitude resolution. Using a 200-arcsec-separation double star, we have obtained turbulence profiles with unprecedented 12-m resolution. The system incorporates necessary novel algorithms for autoguiding, autofocus and image stabilization. The results presented here were obtained at Mauna Kea Observatory. They show LOLAS capabilities but cannot be considered as representative of the site. A forthcoming paper will be devoted to the site characterization. The instrument was built as part of the Ground Layer Turbulence Monitoring Campaign on Mauna Kea for Gemini Observatory.
Keywords:turbulence    atmospheric effects    instrumentation: adaptive optics    instrumentation: high angular resolution    site testing
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