Paper
25 September 2008 Polishing and testing of the 3.5 m SiC M1 mirror of the Herschel space observatory of ESA
Tapio Korhonen, Perttu Keinanen, Mikko Pasanen, Aimo Sillanpaa
Author Affiliations +
Abstract
Herschel space observatory of ESA has a parabolic M1mirror of silicon carbide (SiC) with large diameter of 3.5 m, fast focal ratio of f/0.5 and extreme light-weighting to 25 kg/m2, which make the polishing of the mirror a very challenging task. Use of very high surface pressure is necessary to polish efficiently this hard material, which increases the risk of quilting effects to the shape of the only 2.5 mm thick front face of the mirror. In this paper we present descriptions of the testing and polishing methods used during Herschel M1 lapping and polishing to the specified surface shape accuracy < 1.5 μm rms and micro roughness <30 nm rms.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Tapio Korhonen, Perttu Keinanen, Mikko Pasanen, and Aimo Sillanpaa "Polishing and testing of the 3.5 m SiC M1 mirror of the Herschel space observatory of ESA", Proc. SPIE 7102, Optical Fabrication, Testing, and Metrology III, 710218 (25 September 2008); https://doi.org/10.1117/12.797645
Lens.org Logo
CITATIONS
Cited by 8 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Polishing

Profilometers

Surface finishing

Wavefronts

Silicon carbide

Optical testing

RELATED CONTENT

Fabrication and metrology study for M3M of TMT
Proceedings of SPIE (September 02 2014)
Large dimension optics
Proceedings of SPIE (September 20 2005)
Polishing and testing of the 1.5 m SiC M1 mirror...
Proceedings of SPIE (September 25 2008)

Back to Top