Share Email Print
cover

Proceedings Paper

Status of the MMT Observatory multiple laser beacon projector
Author(s): Thomas E. Stalcup; Roger Angel; Michael Lloyd-Hart; Matthew J. Rademacher
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

The laser guidestar system at the MMT Observatory has produced its first closed loop results and should be producing ground-layer corrected closed loop images within a few months. The LGS system at the MMT is one of few in the world that uses atmospheric Rayleigh scattering from reliable, low-cost lasers, and is unique in its use of a dynamic refocus technique to increase the telescope depth of field for increased return flux. The resulting 10 km depth of field introduces additional constraints on the minimum spot size for the beam projector design. The short exposure spot size as measured at the telescope cassegrain focus is 0.65 arcseconds in 0.59 arcsecond seeing in the visible. Additionally, a method to correct for image motion due to telescope vibrations using accelerometer data has been successfully implemented.

Paper Details

Date Published: 24 September 2007
PDF: 11 pages
Proc. SPIE 6691, Astronomical Adaptive Optics Systems and Applications III, 66910M (24 September 2007); doi: 10.1117/12.735067
Show Author Affiliations
Thomas E. Stalcup, MMT Observatory (United States)
Roger Angel, Steward Observatory, Univ. of Arizona (United States)
Michael Lloyd-Hart, Steward Observatory, Univ. of Arizona (United States)
Matthew J. Rademacher, Steward Observatory, Univ. of Arizona (United States)


Published in SPIE Proceedings Vol. 6691:
Astronomical Adaptive Optics Systems and Applications III
Robert K. Tyson; Michael Lloyd-Hart, Editor(s)

© SPIE. Terms of Use
Back to Top