Paper
26 September 2011 Scanning Long-wave Optical Test System: a new ground optical surface slope test system
Author Affiliations +
Abstract
The scanning long-wave optical test system (SLOTS) is under development at the University of Arizona to provide rapid and accurate measurements of aspherical optical surfaces during the grinding stage. It is based on the success of the software configurable optical test system (SCOTS) which uses visible light to measure surface slopes. Working at long wave infrared (LWIR, 7-14 μm), SLOTS measures ground optical surface slopes by viewing the specular reflection of a scanning hot wire. A thermal imaging camera collects data while motorized stages scan the wire through the field. Current experiments show that the system can achieve a high precision at micro-radian level with fairly low cost equipment. The measured surface map is comparable with interferometer for slow optics. This IR system could be applied early in the grinding stage of fabrication of large telescope mirrors to minimize the surface shape error imparted during processing. This advantage combined with the simplicity of the optical system (no null optics, no high power carbon dioxide laser) would improve the efficiency and shorten the processing time.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Tianquan Su, Won Hyun Park, Robert E. Parks, Peng Su, and James H. Burge "Scanning Long-wave Optical Test System: a new ground optical surface slope test system", Proc. SPIE 8126, Optical Manufacturing and Testing IX, 81260E (26 September 2011); https://doi.org/10.1117/12.892666
Lens.org Logo
CITATIONS
Cited by 11 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Cameras

Mirrors

Optical testing

Sensors

Surface finishing

Long wavelength infrared

Optical scanning systems

RELATED CONTENT

Fabrication of the WIYN 3.5 m primary mirror producing...
Proceedings of SPIE (March 26 1992)
What Can Be Interferometered?
Proceedings of SPIE (January 16 1989)
Pre-launch optical tests of MODIS and MISR
Proceedings of SPIE (August 20 2008)
NOAO testing procedures for large optics
Proceedings of SPIE (March 26 1992)
Demonstration of an ion-figuring process
Proceedings of SPIE (November 01 1990)

Back to Top