Published September 16, 2004 | Version Published
Book Section - Chapter Open

Modeling tools to estimate the performance of the Thirty Meter Telescope: an integrated approach

  • 1. ROR icon Association of Universities For Research In Astronomy
  • 2. ROR icon National Research Council Canada
  • 3. ROR icon California Institute of Technology

Abstract

A sound system engineering approach and the appropriate tools to support it are essential in achieving the scientific and financial objectives of the Thirty Meter Telescope project. Major elements of the required tool set are those providing estimates for the performance of the telescope. During the last couple of years, the partners in the consortium developed a wide range of modeling and simulation tools with various levels of fidelity and flexibility. There are models available for time domain and frequency domain simulations and analysis, as well as for lower fidelity, parametric investigations of design trade-offs and for high fidelity, integrated modeling of structure, optics and control. Presented are characteristic simulation results using the existing preliminary point designs of the TMT, with emphasis on the telescope performance degradation due to wind buffeting. Under the conditions modeled, the wind induced image jitter and image quality degradation was found comparable to good atmospheric seeing.

Additional Information

© 2018 Society of Photo-Optical Instrumentation Engineers. The authors would like to thank Robert Upton of AURA New Initiatives Office for his valuable suggestions and comments. We are also grateful to Brent Ellerbroek and Myung Cho of AURA New Initiatives Office for their reviews and comments. The authors present this paper as part of the work of the Thirty Meter Telescope (TMT) Project. TMT is a partnership of the Association of Universities for Research in Astronomy (AURA), the Association of Canadian Universities for Research in Astronomy (ACURA), the California Institute Of Technology and the University of California. The partners gratefully acknowledge the support of the Gordon and Betty Moore Foundation, the US National Science Foundation, the National Research Council of Canada, the Natural Sciences and Engineering Research Council of Canada, and the Gemini Partnership. The New Initiatives Office is a partnership between two divisions of the Association of Universities for Research in Astronomy (AURA), Inc.: the National Optical Astronomy Observatory (NOAO) and the Gemini Observatory. NOAO is operated by AURA under cooperative agreement with the National Science Foundation (NSF). The Gemini Observatory is operated by AURA under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Particle Physics and Astronomy Research Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), CNPq (Brazil) and CONICET (Argentina).

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Additional details

Identifiers

Eprint ID
91878
Resolver ID
CaltechAUTHORS:20181218-073900375

Funding

Association of Universities for Research in Astronomy (AURA)
Association of Canadian Universities for Research in Astronomy (ACURA)
Caltech
University of California
Gordon and Betty Moore Foundation
NSF
National Research Council of Canada
Natural Sciences and Engineering Research Council of Canada (NSERC)
Gemini Partnership
Particle Physics and Astronomy Research Council (PPARC)
Comisión Nacional de Investigación Científica y Tecnológica (CONICYT)
Australian Research Council
Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET)

Dates

Created
2018-12-18
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Thirty Meter Telescope
Series Name
Proceedings of SPIE
Series Volume or Issue Number
5497