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Published February 1, 2010 | Published
Journal Article Open

Wind buffeting of large telescopes

Abstract

Unsteady wind loads due to turbulence within the telescope enclosure are one of the largest dynamic disturbances for ground-based optical telescopes. The desire to minimize the response to the wind influences the design of the telescope enclosure, structure, and control systems. There is now significant experience in detailed integrated modeling to predict image jitter due to wind. Based on this experience, a relatively simple model is proposed that is verified (from a more detailed model) to capture the relevant physics. In addition to illustrating the important elements of the telescope design that influence wind response, this model is used to understand the sensitivity of telescope image jitter to a wide range of design parameters.

Additional Information

© 2010 Optical Society of America. Received 4 November 2009; accepted 3 December 2009; posted 22 December 2009 (Doc. ID 119505); published 26 January 2010. This work was supported by the TMT Project. The TMT Project gratefully acknowledges the support of 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/Conseil National Recherches Canada (NRC/CNRC), 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 United States National Science Foundation (NSF).

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August 19, 2023
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October 19, 2023