Physics – Optics
Scientific paper
Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010spie.7732e..91a&link_type=abstract
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray. Edited by Arnaud, Monique; Murray, Stephen S.; Takahashi,
Physics
Optics
Scientific paper
In this paper we present the latest developments on the ruggedisation of the Silicon Pore Optics (SPO) mirror modules. SPO is one of the candidate technologies for producing the X-ray optics for the future space based Xray telescope, the International X-ray Observatory (IXO). To produce SPO mirror modules, Si mirrors are first bonded together using direct Si bonding to form a stack. These stacks are the glued into brackets, which then connect to the supporting optical bench by invar pins. The combination of brackets and invar pins now forms a full isostatic mount, and is rugged enough to allow the mirror module to survive the high loads of a launch. The mounting system furthermore allows for a certain level of manufacturing tolerances for the support structure, and ensures interchangeability of the mirror modules within one single ring of the optical bench. To prove this, a test interface has been designed and manufactured, on which a single, full fledged mirror module will be mounted to be exposed to environmental tests.
Ackermann Marcelo D.
Bavdaz Marcos
Collon Maximilien J.
Erhard Markus
Günther Ramses
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