Two campaigns to compare three turbulence profiling techniques at las campanas observatory

Joanna Thomas Osip, Edison Bustos, Michael Goodwin, Charles Jenkins, Andrew Lambert, Gabriel Prieto, Andrei Tokovinin

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    12 Citations (Scopus)

    Abstract

    In preparation to characterize the Giant Magellan Telescope site and guide the development of its adaptive optics system, two campaigns to systematically compare the turbulence profiles obtained independently with three different instruments were conducted at Las Campanas Observatory in September, 2007 and January 2008. Slope detection and ranging (SLODAR) was used on the 2.5-m duPont telescope. SLODAR measures the C2n profile as a function of altitude through observations of double stars. The separation of the observed double star sets the maximum altitude and height resolution. Ground layer (altitudes < 1 km) and free atmosphere turbulence profiles are compared with those obtained with a lunar scintillometer (LuSci) and a multi-aperture scintillation sensor (MASS), respectively. In addition, the total atmospheric seeing was measured by both SLODAR and a differential image motion monitor (DIMM).

    Original languageEnglish
    Title of host publicationGround-based and Airborne Instrumentation for Astronomy II
    DOIs
    Publication statusPublished - 2008
    EventGround-based and Airborne Instrumentation for Astronomy II - Marseille, France
    Duration: 23 Jun 200828 Jun 2008

    Publication series

    NameProceedings of SPIE - The International Society for Optical Engineering
    Volume7014
    ISSN (Print)0277-786X

    Conference

    ConferenceGround-based and Airborne Instrumentation for Astronomy II
    Country/TerritoryFrance
    CityMarseille
    Period23/06/0828/06/08

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