Physics – Optics
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004spie.5490..527g&link_type=abstract
Advancements in Adaptive Optics. Edited by Domenico B. Calia, Brent L. Ellerbroek, and Roberto Ragazzoni. Proceedings of the SPI
Physics
Optics
1
Scientific paper
On the way to the Extremely Large Telescopes (ELT) the Large Binocular Telescope (LBT) is an intermediate step. The two 8.4m mirrors create a masked aperture of 23m. LINC-NIRVANA is an instrument taking advantage of this opportunity. It will get, by means of Multi-Conjugated Adaptive Optics (MCAO), a moderate Strehl Ratio over a 2 arcmin field of view, which is used for Fizeau (imaging) interferometry in J,H and K. Several MCAO concepts, which are proposed for ELTs, will be proven with this instrument. Studies of sub-systems are done in the laboratory and the option to test them on sky are kept open. We will show the implementation of the MCAO concepts and control aspects of the instrument and present the road map to the final installation at LBT. Major milestones of LINC-NIRVANA, like preliminary design review or final design review are already done or in preparation. LINC-NIRVANA is one of the few MCAO instruments in the world which will see first light and go into operation within the next years.
Andersen David R.
Arcidiacono Carmelo
Baumeister Harald
Beckmann Udo
Behrend Jan
No associations
LandOfFree
LINC-NIRVANA: how to get a 23-m wavefront nearly flat 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 LINC-NIRVANA: how to get a 23-m wavefront nearly flat, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and LINC-NIRVANA: how to get a 23-m wavefront nearly flat will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1809409