Paper
5 July 2016 E-ELT vibration modeling, simulation, and budgeting
Author Affiliations +
Proceedings Volume 10012, Integrated Modeling of Complex Optomechanical Systems II; 1001202 (2016) https://doi.org/10.1117/12.2200926
Event: Integrated Modeling of Complex Optomechanical Systems II, 2015, Varenna, Italy
Abstract
The E-ELT dynamical modeling toolkit is used extensively to understand the effect of vibrations from observatory equipments on the final performance of the telescope. The dynamical and control modeling toolkit uses the finite element model of the telescope structure and mirror units, the optical sensitivity and knowledge of the wavefront control correction capability to estimate the transmission of vibration from potential vibrational sources to the wavefront error. In addition, it helps i) to identify the sensitive optical units and sensitive vibrational sources and the frequency intervals they might affect most the wavefront error, ii) to perform design trade-offs, and iii) to derive subsystem specification requirements. In this paper, a vibration budgeting approach for the E-ELT using the modeling toolkit is presented.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
B. Sedghi, M. Müller, and G. Jakob "E-ELT vibration modeling, simulation, and budgeting", Proc. SPIE 10012, Integrated Modeling of Complex Optomechanical Systems II, 1001202 (5 July 2016); https://doi.org/10.1117/12.2200926
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Wavefronts

Telescopes

Error analysis

Mirrors

Interfaces

Adaptive optics

Motion models

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