Physics – Optics
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1114..174f&link_type=abstract
IN: Active telescope systems; Proceedings of the Meeting, Orlando, FL, Mar. 28-31, 1989 (A90-30852 12-74). Bellingham, WA, Socie
Physics
Optics
3
Adaptive Optics, Atmospheric Correction, Laser Applications, Reference Stars, Telescopes, Wave Front Deformation, Atmospheric Turbulence, Laser Beams, Seeing (Astronomy), Yag Lasers
Scientific paper
An artificial reference source must be provided in order to operate adaptive-optics devices in the visible range; this artificial source could be the backscattered light from a laser beam emitted out through the telescope aperture. The ATLAS experiment has undertaken a proof of this concept, using the 300-mJ doubled Nd:YAG laser of the CERGA Lunar Laser Ranging Station in conjunction with specially-developed Shack-Hartmann sensors to compare the wavefronts restored from near-simultaneous observations of an actual bright star and of a laser spot.
Foy Renaud
Hubin Norbert N.
Sechaud Marc
Tallon Michel
No associations
LandOfFree
ATLAS experiment to test the laser probe technique for wavefront measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with ATLAS experiment to test the laser probe technique for wavefront measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ATLAS experiment to test the laser probe technique for wavefront measurements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1827813