Paper
10 July 2018 Final correction by Ion Beam Figuring of thin shells for X-ray telescopes
Author Affiliations +
Abstract
Future space X-ray mission concepts like STAR-X, AXIS and Lynx foresee optics with both high angular resolutions (HEW ~ 0.5 to 5 arcsec) and large collecting areas (~0.2-2.0 m2). These optics are very challenging to be produced and their manufacturing is under study. The Ion Beam Figuring (IBF) is one of the few techniques that is capable of correcting the residual manufacturing errors of the mirror shells and obtain the desired final optical figure. INAF-OABrera has two IBF facilities and is investigating the use of IBF on thin foils made by different materials, namely Silicon and Fused Silica. In this paper we describe the results obtained in a preliminary study on Silicon shells.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. Ghigo, S. Basso, M. Civitani, R. Gilli, G. Pareschi, B. Salmaso, G. Vecchi, and W. W. Zhang "Final correction by Ion Beam Figuring of thin shells for X-ray telescopes", Proc. SPIE 10706, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III, 107063I (10 July 2018); https://doi.org/10.1117/12.2313939
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications and 1 patent.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Ion beam finishing

Mirrors

Ion beams

Silicon

X-rays

X-ray optics

Aluminum

RELATED CONTENT

Aberration-free silicon pore x-ray optics
Proceedings of SPIE (September 26 2013)
ATHENA x-ray optics development and accommodation
Proceedings of SPIE (August 23 2021)
The ATHENA telescope and optics status
Proceedings of SPIE (August 29 2017)
Novel x-ray optics with Si wafers and formed glass
Proceedings of SPIE (June 13 2006)

Back to Top