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A Generalized SCIDAR Facility for the LBT
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In short, one can say that SCIDAR is a method to measure (among others) the vertical profile of atmospheric optical turbulence. The method is based on an analysis of spatio-temporal correlations of stellar scintillation images. In astronomy, SCIDAR is more and more used to characterize astronomical sites on a regular base. In particular adaptive optics instruments may benefit from real-time SCIDAR data, e.g. knowing the iso-planatic angle and windspeed may help to optimize AO observations. A nice and compact introduction to SCIDAR can be found here. An excellent and detailed description of SCIDAR in the context of multi-conjugated adaptive optics can be found here. MPIA and Steward Observatory have built a SCIDAR facility for the Large Binocular Telescope (LBT) on Mount Graham, Arizona. While Steward Observatory was engaged in the optical and opto-mechanical design of the instrument, MPIA was responsible to deliver the real-time data reduction system. An overview of the hard- and software architecture is shown here. Status of the project as of September 2001 is here; March 2001 can be found here. Since about 2002 (see this conference paper) the system is fully operational. Links: Remy Avila's homepage http://www.astrosmo.unam.mx/~r.avila Publications: LBT facility SCIDAR: recent results Simultaneous SCIDAR and Adaptive Optics Measurements: Results and Applications Simultaneous Measurements of the Fried Parameter r0 and the Isoplanatic Angle theta0 Using SCIDAR and Adaptive Optics - First Results |
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last update: 2 March 2007
editor of this page: Stefan Hippler |
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