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Finite element analysis of carbon fibre composite adaptive mirrors

Abstract:
With the advent of the new generation of ground-based telescopes with primary sizes of 30-100 m, adaptive optics (AO) technology is in rapid development. One important area of research is that of integration of AO into the telescope's operation. A possible solution for this is the use of an adaptive secondary mirror. However, for a secondary of several meters in size, this presents many problems in choice of material, as well as design for the adaptive control. An active mirror prototype made out of a carbon fibre composite material (CFC) is under development at University College London in collaboration with QinetiQ and Cobham Composites. We present here results from finite element analysis of this mirror, as well as modelling results of an adaptive secondary mirror section as might be developed for the new class of telescopes. These results indicate that CFC could indeed present a viable alternative to more traditional deformable mirror materials.

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Publisher copy:
10.1117/12.552579

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
Proceedings of SPIE - The International Society for Optical Engineering More from this journal
Volume:
5490
Issue:
PART 3
Pages:
1591-1599
Publication date:
2004-01-01
DOI:
ISSN:
0277-786X


Language:
English
Keywords:
Pubs id:
pubs:455704
UUID:
uuid:44e4ae6c-e26b-4b06-9c5f-5d84a0fe3ac3
Local pid:
pubs:455704
Source identifiers:
455704
Deposit date:
2014-06-17
ARK identifier:

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