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Scaling multiconjugate adaptive optics performance estimates to extremely large telescopes

Ellerbroek, B. L. and Rigaut, F. J. (2000) Scaling multiconjugate adaptive optics performance estimates to extremely large telescopes. In: Adaptive Optical Systems Technology. Proceedings of SPIE. No.4007. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, pp. 498-509. ISBN 9780819436320. http://resolver.caltech.edu/CaltechAUTHORS:20190118-133718176

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Abstract

Multi-conjugate adaptive optics (MCAO) is a key technology for extremely large, ground-based telescopes (ELT's) because it enables near-uniform atmospheric turbulence compensation over fields-of-view considerably larger than can be corrected with more conventional AO systems. Quantitative performance evaluation using detailed analytical or simulation models is difficult, however, due to the very large number of deformable mirror (DM) actuators, wave front sensors (WFS) subapertures, and guide stars which might comprise an MCAO system for an ELT. This paper employs more restricted minimal variance estimation methods to evaluate the fundamental performance limits imposed by anisoplanatism alone upon MCAO performance for a range of sample cases. Each case is defined by a atmospheric turbulence profile, telescope aperture diameter, field-of-view, guide star constellation, and set of DM conjugate ranges. For a Kolmogorov turbulence spectrum with an infinite outer scale, MCAO performance for a whole range of aperture diameters and proportional fields-of-view can be computed at once using a scaling law analogous to the (D/d_O)^(5/3) formula for the cone effect. For 30 meter telescopes, useful levels of performance are possible across a 1.0 - 2.0 arc minute square field-of-view using 5 laser guide stars (LGS's) and 3 DM's, and somewhat larger fields can be corrected using 9 guide stars and 4 mirrors. 3 or more tip/tilt natural guide stars (NGS's) are necessary to detect modes of tilt anisoplanatism which cannot be detected using LGS's, however. LGS MCAO performance is a quite weak function of aperture diameter for a fixed field-of-view, and it is tempting to scale these results to larger apertures. NGS MCAO performance is moderately superior to LGS MCAO if the NGS constellation is within the compensated field-of-view, but degrades rapidly as the guide stars move away from the field. The penalty relaxes slowly with increasing aperture diameter, but how to extrapolate this trend to telescopes with diameters much larger than 30 meters is unclear.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.390314DOIArticle
Alternate Title:Scaling Multi-Conjugate Adaptive Optics Performance Estimates to Extremely Large Telescopes
Additional Information:© 2000 Society of Photo-optical Instrumentation Engineers (SPIE). The Gemini 8-m Telescopes Project and Observatory is managed by the Association of Universities for Research in Astronomy, for the National Science Foundation and the Gemini Board, under an international partnership agreement.
Group:Thirty Meter Telescope
Funders:
Funding AgencyGrant Number
Association of Universities for Research in Astronomy (AURA)UNSPECIFIED
NSFUNSPECIFIED
Gemini PartnershipUNSPECIFIED
Subject Keywords:Multi-conjugate adaptive optics, extremely large telescopes
Record Number:CaltechAUTHORS:20190118-133718176
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190118-133718176
Official Citation:Brent L. Ellerbroek, Francois J. Rigaut, "Scaling multiconjugate adaptive optics performance estimates to extremely large telescopes," Proc. SPIE 4007, Adaptive Optical Systems Technology, (7 July 2000); doi: 10.1117/12.390314
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92377
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Jan 2019 23:40
Last Modified:22 Jan 2019 19:45

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