Paper
29 September 1999 Superpolishing and precision metrology on a metal mandrel and replicated segments for Constellation-X
Author Affiliations +
Abstract
We have superpolished a diamond-turned aluminum mandrel to an axial roughness of 0.34 nm rms. The mandrel is made to the Astro-E secondary mirror design for the 81st shell. Precision metrology at 100 mm to submicron scales has established the power spectral density of the mandrel and ultralightweight gold coated replicated segments. Predicted image quality of a set of optimally aligned replicated segments of this and a matching primary is substantially improved as compared to the flight mirrors for Astro-E. This approach using metal mandrels, superpolishing, and replicated ultralightweight foil mirrors, may represent a cost-effective approach to meeting the 15 arcsec half-energy width and weight requirements for the Constellation-X mission. Descriptions of the polishing apparatus, the precision metrology instruments, and the surface data analysis are presented. The general methods describe dare applicable to precision optics for both normal incidence and grazing incidence optics.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David A. Content, Timo T. Saha, Robert Petre, James J. Lyons III, Geraldine A. Wright, John J. Zaniewski, and Kai-Wing Chan "Superpolishing and precision metrology on a metal mandrel and replicated segments for Constellation-X", Proc. SPIE 3766, X-Ray Optics, Instruments, and Missions II, (29 September 1999); https://doi.org/10.1117/12.363647
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Metrology

Metals

Mirrors

Image segmentation

Polishing

Atomic force microscopy

Data modeling

RELATED CONTENT


Back to Top