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TMT adaptive optics systems control architecture

Boyer, C. and Ellerbroek, B. and Herriot, G. and Veran, J. P. and Browne, S. and Tyler, G. (2006) TMT adaptive optics systems control architecture. In: Advances in Adaptive Optics II. Proceedings of SPIE. No.6272. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 627211. ISBN 9780819463371. http://resolver.caltech.edu/CaltechAUTHORS:20190520-153722192

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Abstract

Achieving the science goals of TMT will require AO subsystems of unprecedented power and sophistication, including a Real Time Controller (RTC) subsystem that will implement wavefront reconstruction and control algorithms for up to four different laser guide star (LGS) AO systems. The requirements for the RTC represent a significant advance over the current generation of astronomical AO control systems, both in terms of the wavefront reconstruction algorithms to be employed and the new hardware approaches that will be required. Additionally, the number of active components included in the AO systems and the complexity of their interactions will require a highly automated AO Sequencer that will work in concert with the TMT Telescope and Instrument Sequencers. In this paper, we will describe the control and software requirements for the whole AO system, and in particular for the RTC and the AO Sequencer. We will describe the challenges involved in developing these systems and will present a conceptual design.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.669595DOIArticle
Additional Information:© 2006 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors gratefully acknowledge the support of the TMT partner institutions. They are the Association of Canadian Universities for Research in Astronomy (ACURA), the Association of Universities for Research in Astronomy (AURA), the California Institute of Technology and the University of California. This work was supported, as well, by the Canada Foundation for Innovation, the Gordon and Betty Moore Foundation, the National Optical Astronomy Observatory, which is operated by AURA under cooperative agreement with the National Science Foundation, the Ontario Ministry of Research and Innovation, and the National Research Council of Canada.
Group:Thirty Meter Telescope
Funders:
Funding AgencyGrant Number
Association of Canadian Universities for Research in Astronomy (ACURA)UNSPECIFIED
Association of Universities for Research in Astronomy (AURA)UNSPECIFIED
CaltechUNSPECIFIED
University of CaliforniaUNSPECIFIED
Canada Foundation for InnovationUNSPECIFIED
Gordon and Betty Moore FoundationUNSPECIFIED
National Optical Astronomy Observatory (NOAO)UNSPECIFIED
NSFUNSPECIFIED
Ontario Ministry of Research and InnovationUNSPECIFIED
National Research Council of CanadaUNSPECIFIED
Subject Keywords:Thirty Meter Telescope Project, Adaptive Optics, Real Time Controller, Adaptive Optics Sequencer
Record Number:CaltechAUTHORS:20190520-153722192
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190520-153722192
Official Citation:C. Boyer, B. Ellerbroek, G. Herriot, J. P. Veran, S. Browne, and G. Tyler "TMT adaptive optics systems control architecture", Proc. SPIE 6272, Advances in Adaptive Optics II, 627211 (27 June 2006); doi: 10.1117/12.669595; https://doi.org/10.1117/12.669595
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95620
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:20 May 2019 22:49
Last Modified:20 May 2019 22:49

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