Paper
11 September 1998 Increasing the useful field of view of an adaptive optics system
Mark Richard Chun, Walter J. Wild, Fang Shi, Michael F. Smutko, Edward J. Kibblewhite, Robert Q. Fugate, Julian C. Christou
Author Affiliations +
Abstract
The size of the corrected field of view of an adaptive optics system is though to be a severe limitation on the usefulness of an adaptive optics system. We show that under good seeing conditions the useful field of view is an order of magnitude larger than the field predicted by the classical isoplanatic angle. The corrected field of view is experimentally shown to increase when using spatially degraded wavefront corrections. Two methods of spatially degrading the wavefront were tested: low-order modal wavefront reconstructions and the use of a low-altitude Rayleigh wavefront reference beacon. In both cases the on- axis performance is sacrificed for an increased field of view.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark Richard Chun, Walter J. Wild, Fang Shi, Michael F. Smutko, Edward J. Kibblewhite, Robert Q. Fugate, and Julian C. Christou "Increasing the useful field of view of an adaptive optics system", Proc. SPIE 3353, Adaptive Optical System Technologies, (11 September 1998); https://doi.org/10.1117/12.321631
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Wavefronts

Adaptive optics

Stars

Rayleigh guide stars

Telescopes

Turbulence

Wavefront reconstruction

RELATED CONTENT

CANARY phase B on sky open loop tomographic LGS...
Proceedings of SPIE (July 21 2014)
Beams and image formation with adaptive correction
Proceedings of SPIE (May 31 1994)
Rayleigh laser guide stars in multiconjugate correction
Proceedings of SPIE (October 25 2004)
Horizontal turbulence measurements using SLODAR
Proceedings of SPIE (August 18 2005)
ASSIST: the test setup for the VLT AO facility
Proceedings of SPIE (July 16 2008)
Plate scale variation detecting method for LINC-NIRVANA
Proceedings of SPIE (December 13 2021)

Back to Top