Daylight operation of a sodium laser guide star for adaptive optics wavefront sensing
Citation
Daylight operation of a sodium laser guide star for adaptive optics wavefront sensing 2016, 2 (4):040501 Journal of Astronomical Telescopes, Instruments, and SystemsRights
© 2016 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We report contrast measurements of a sodium resonance guide star against the daylight sky when observed through a tuned magneto-optical filter (MOF). The guide star was created by projection of a laser beam at 589.16 nm into the mesospheric sodium layer and the observations were made with a collocated 1.5-m telescope. While MOFs are used with sodium light detecting and ranging systems during the day to improve the signalto- noise ratio of the measurements, they have not so far been employed with laser guide stars to drive adaptive optics (AO) systems to correct atmospherically induced image blur. We interpret our results in terms of the performance of AO systems for astronomy, with particular emphasis on thermal infrared observations at the next generation of extremely large telescopes now being built. (C) 2016 Society of Photo-Optical Instrumentation Engineers (SPIE)ISSN
2329-4124Version
Final published versionSponsors
US Air Force Office of Scientific Research [FA9550-14-1-0178]Additional Links
http://astronomicaltelescopes.spiedigitallibrary.org/article.aspx?doi=10.1117/1.JATIS.2.4.040501ae974a485f413a2113503eed53cd6c53
10.1117/1.JATIS.2.4.040501
