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Proceedings Paper

Modeling a large submillimeter-wave observatory
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Paper Abstract

The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous increase in sensitivity in the submillimeter bands compared to existing observatories, provided it can establish and maintain excellent image quality. To accomplish this at a very low cost, it is necessary to conduct accurate engineering trades, including the most effective segment and wavefront sensing and control approach, to determine the best method for continuously maintaining wavefront quality in the operational environment. We describe an integrated structural/optical/controls model that provides accurate performance prediction. We also detail the analysis methods used to quantify critical design trades.

Paper Details

Date Published: 10 August 2010
PDF: 13 pages
Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 773326 (10 August 2010); doi: 10.1117/12.856493
Show Author Affiliations
John Z. Lou, Jet Propulsion Lab. (United States)
Andy Kissil, Jet Propulsion Lab. (United States)
Dave C. Redding, Jet Propulsion Lab. (United States)
Matt C Bradford, Jet Propulsion Lab. (United States)
Steve Padin, California Institute of Technology (United States)
David Woody, California Institute of Technology (United States)


Published in SPIE Proceedings Vol. 7733:
Ground-based and Airborne Telescopes III
Larry M. Stepp; Roberto Gilmozzi; Helen J. Hall, Editor(s)

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