Paper
20 September 1989 Various Aspects Of Active Optics
Gerard Lemaitre
Author Affiliations +
Abstract
Optical telescopes of unprecedented size, high resolution optical arrays having large number of telescopes and more performant auxiliary instrumentations will be built by strongly applying the concept of active optics. Taking apart developments of adaptative optics relative to seeing compensation, the meaning of "active optics" must be considered as having at least three different senses i) maintaining, in situ, the best figure of the telescope optics during astronomical observations, ii) figuring highly aspheric optics and/or unaxisymmetric optics, and iii) modifying, in situ, the optical figure parameters as, for instance, the asphericity of a Cassegrain mirror for a better field optimization with respect to various focal instruments. This paper discusses some thoughts on these questions and presents some results and astronomical applications.
© (1989) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gerard Lemaitre "Various Aspects Of Active Optics", Proc. SPIE 1114, Active Telescope Systems, (20 September 1989); https://doi.org/10.1117/12.960838
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Cited by 14 scholarly publications.
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KEYWORDS
Mirrors

Telescopes

Active optics

Monochromatic aberrations

Astronomical imaging

Spherical lenses

Polishing

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