Paper
27 July 2016 NFIRAOS in 2015: engineering for future integration of complex subsystems
Author Affiliations +
Abstract
The Narrow Field InfraRed Adaptive Optics System (NFIRAOS) will be the first-light facility Adaptive Optics (AO) system for the Thirty Meter Telescope (TMT). NFIRAOS will be able to host three science instruments that can take advantage of this high performance system. NRC Herzberg is leading the design effort for this critical TMT subsystem. As part of the final design phase of NFIRAOS, we have identified multiple subsystems to be sub-contracted to Canadian industry. The scope of work for each subcontract is guided by the NFIRAOS Work Breakdown Structure (WBS) and is divided into two phases: the completion of the final design and the fabrication, assembly and delivery of the final product. Integration of the subsystems at NRC will require a detailed understanding of the interfaces between the subsystems, and this work has begun by defining the interface physical characteristics, stability, local coordinate systems, and alignment features. In order to maintain our stringent performance requirements, the interface parameters for each subsystem are captured in multiple performance budgets, which allow a bottom-up error estimate. In this paper we discuss our approach for defining the interfaces in a consistent manner and present an example error budget that is influenced by multiple subsystems.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jenny Atwood, David Andersen, Peter Byrnes, Adam Densmore, Joeleff Fitzsimmons, Glen Herriot, and Alexis Hill "NFIRAOS in 2015: engineering for future integration of complex subsystems", Proc. SPIE 9909, Adaptive Optics Systems V, 990934 (27 July 2016); https://doi.org/10.1117/12.2231813
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Interfaces

Optical alignment

Mirrors

Adaptive optics

Calibration

Thirty Meter Telescope

Wavefront sensors

Back to Top