Author
Saif, Babak N.Keski-Kuha, Ritva A.
Greenfield, Perry
North-Morris, Michael
Bluth, Marcel
Feinberg, Lee
Wyant, James C.
Park, Sang
Affiliation
Univ Arizona, James C Wyant Coll Opt SciIssue Date
2019-09-09
Metadata
Show full item recordPublisher
SPIE-INT SOC OPTICAL ENGINEERINGCitation
Saif, B., Keski-Kuha, R., Greenfield, P., North-Morris, M., Bluth, M., Feinberg, L., ... & Park, S. (2019, September). Picometer level spatial metrology for next generation telescopes. In UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts IX (Vol. 11115, p. 111150K). International Society for Optics and Photonics.Rights
© 2019 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Future space observatory missions require controlling wave front error and system alignment stability to picometer scale. Picometer stability performance demands precision knowledge of the mirror and metering structure materials to the same level. A high-speed electronic speckle pattern interferometer was designed and built to demonstrate measurements of both static and dynamic responses of picometer level amplitudes in mirror and structural materials subjected to very low energy disturbances. This paper summarizes the current status of tests to impart a dynamic disturbance of picometer scale and measure the response of specular and diffuse materials. The results show that subpicometer scale effects can be accurately measured in an open test environment outside a vacuum chamber.ISSN
0277-786XVersion
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2543034