International Conference on Space Optics — ICSO 2016 2017
DOI: 10.1117/12.2296193
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Design study for an active metal mirror: sub-system of a correction chain for large UVOIR space telescopes

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Cited by 2 publications
(2 citation statements)
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References 8 publications
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“…In Europe, both the ESA [216] based on a DM designed by IOF, a Fibonacci distribution across the pupil, or mirror surface, was initially chosen after comparing it to alternative distributions for large UV-to-IR telescope applications [221]. Shown in Fig.…”
Section: Active Correctionmentioning
confidence: 99%
“…In Europe, both the ESA [216] based on a DM designed by IOF, a Fibonacci distribution across the pupil, or mirror surface, was initially chosen after comparing it to alternative distributions for large UV-to-IR telescope applications [221]. Shown in Fig.…”
Section: Active Correctionmentioning
confidence: 99%
“…Dimensional instabilities lead in general to a non-acceptable degradation of the optical performance of the system which has to be restored by dimensional stable materials and one or more compensation approaches. Thermal instabilities can be compensated using kinematic means [33,34], active/adaptive optics [35][36][37][38][39][40], or compensation optics [41,42]. While all aforementioned compensation approaches take place in a post-manufacturing stage or during the operation of the optical instrument, the subject of this article is compensation during manufacturing, possible when the static loads are known beforehand.…”
Section: Introductionmentioning
confidence: 99%