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Proceedings Paper

Launch telescope for astronomical adaptive optics
Author(s): Alberto Caruso; Andrea Novi; Giuseppe Basile
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Paper Abstract

The Launch Telescope Assembly (LTA) consists of a 50 cm class beam expander (angular magnification 12.5x) and it is an essential subsystem of Laser Guide Star Facility (LGSF), which provides an artificial reference star for adaptive compensation of atmospheric turbulence for one of the VLT (Very Large Telescope) 8-meters telescopes of ESO (European Southern Observatory). LTA is an afocal system, with parabolic primary and secondary mirrors, a flat 45° tertiary mirror and an exit window. It is fed with collimated Sodium laser beam, expanding and directing it along the line of sight of the 8-m telescope. Resonance backscatter from atmospheric Sodium layer at about 90 km altitude produces a point like artificial source at this altitude. The high optical quality requested for very fast optics, the severe constraints of the layout accommodation and the mass reduction made LTA a technological challenge that Galileo Avionica has been able to design, realise, align and test as requested. LTA will be positioned atop the secondary mirror unit of one of the four VLTs.

Paper Details

Date Published: 15 October 2005
PDF: 9 pages
Proc. SPIE 5962, Optical Design and Engineering II, 596224 (15 October 2005); doi: 10.1117/12.625091
Show Author Affiliations
Alberto Caruso, Galileo Avionica S.p.A. (Italy)
Andrea Novi, Galileo Avionica S.p.A. (Italy)
Giuseppe Basile, Galileo Avionica S.p.A. (Italy)

Published in SPIE Proceedings Vol. 5962:
Optical Design and Engineering II
Laurent Mazuray; Rolf Wartmann, Editor(s)

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