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Split atmospheric tomography using laser and natural guide stars

Gilles, Luc and Ellerbroek, Brent L. (2008) Split atmospheric tomography using laser and natural guide stars. Journal of the Optical Society of America A, 25 (10). pp. 2427-2435. ISSN 1084-7529. https://resolver.caltech.edu/CaltechAUTHORS:GILjosaa08

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Abstract

Laser guide star (LGS) atmospheric tomography is described in the literature as integrated minimum-variance tomographic wavefront reconstruction from a concatenated wavefront-sensor measurement vector consisting of many high-order, tip/tilt (TT)-removed LGS measurements, supplemented by a few low-order natural guide star (NGS) components essential to estimating the TT and tilt anisoplanatism (TA) modes undetectable by the TT-removed LGS wavefront sensors (WFSs). The practical integration of these NGS WFS measurements into the tomography problem is the main subject of this paper. A split control architecture implementing two separate control loops driven independently by closed-loop LGS and NGS measurements is proposed in this context. Its performance is evaluated in extensive wave optics Monte Carlo simulations for the Thirty Meter Telescope (TMT) LGS multiconjugate adaptive optics (MCAO) system, against the delivered performance of the integrated control architecture. Three iterative algorithms are analyzed for atmospheric tomography in both cases: a previously proposed Fourier domain preconditioned conjugate gradient (FDPCG) algorithm, a simple conjugate gradient (CG) algorithm without preconditioning, and a novel layer-oriented block Gauss-Seidel conjugate gradient algorithm (BGS-CG). Provided that enough iterations are performed, all three algorithms yield essentially identical closed-loop residual RMS wavefront errors for both control architectures, with the caveat that a somewhat smaller number of iterations are required by the CG and BGS-CG algorithms for the split approach. These results demonstrate that the split control approach benefits from (i) a simpler formulation of minimum-variance atmospheric tomography allowing for algorithms with reduced computational complexity and cost (processing requirements), (ii) a simpler, more flexible control of the NGS-controlled modes, and (iii) a reduced coupling between the LGS- and NGS-controlled modes. Computation and memory requirements for all three algorithms are also given for the split control approach for the TMT LGS AO system and appear feasible in relation to the performance specifications of current hardware technology.


Item Type:Article
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http://www.opticsinfobase.org/josaa/abstract.cfm?URI=josaa-25-10-2427PublisherUNSPECIFIED
Additional Information:© 2008 Optical Society of America. Received May 22, 2008; revised July 15, 2008; accepted August 6, 2008; posted August 12, 2008 (Doc. ID 96540); published September 9, 2008. The authors gratefully acknowledge the support of the TMT partner institutions. They are the Association of Canadian Universities for Research in Astronomy (ACURA), the California Institute of Technology, and the University of California. This work was supported as well by the Gordon and Betty Moore Foundation, the Canada Foundation for Innovation, the Ontario Ministry of Research and Innovation, the National Research Council of Canada (NRC), the Natural Sciences and Engineering Research Council of Canada, the British Columbia Knowledge Development Fund, the Association of Universities for Research in Astronomy (AURA), and the U.S. National Science Foundation (NSF).
Funders:
Funding AgencyGrant Number
Association of Canadian Universities for Research in Astronomy (ACURA)UNSPECIFIED
California Institute of TechnologyUNSPECIFIED
University of CaliforniaUNSPECIFIED
Gordon and Betty Moore FoundationUNSPECIFIED
Canada Foundation for InnovationUNSPECIFIED
Ontario Ministry of Research and InnovationUNSPECIFIED
National Research Council of CanadaUNSPECIFIED
British Columbia Knowledge Development FundUNSPECIFIED
Association of Universities for Research in Astronomy (AURA)UNSPECIFIED
National Science FoundationUNSPECIFIED
Issue or Number:10
Record Number:CaltechAUTHORS:GILjosaa08
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:GILjosaa08
Official Citation:L. Gilles and B. L. Ellerbroek, "Split atmospheric tomography using laser and natural guide stars," J. Opt. Soc. Am. A 25, 2427-2435 (2008) http://www.opticsinfobase.org/josaa/abstract.cfm?URI=josaa-25-10-2427
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:12522
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:12 Dec 2008 06:48
Last Modified:03 Oct 2019 00:29

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