Abstract
Active optics methods were originally applied to the figuring of refractive Schmidt correctors. Further developments followed with the development of reflective correctors and reflective-diffractive correctors. The various ways to obtain each of the three corrector types are different.
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1.
The methods developed for refractive plate correctors have been called elastic relaxation figuring or more commonly stress figuring.
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2.
Two different methods are practicable for obtaining reflective correctors, namely stress figuring and in-situ stressing.
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3.
Starting from a plane or a spherical grating, there are also two methods of obtaining reflective aspherized gratings: duplication on an active submaster and then stressing and second duplication (more commonly used), or simple duplication and stressing.
The main feature of these methods is the inherent smoothness of the aspherized surface that is obtained directly from spherical or plane surfaces. This avoids the high spatial frequency errors which are a signature of the classical zonal retouch process. Active optics methods allow obtaining telescopes and astronomical instruments of the highest intrinsic image quality.
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Lemaitre, G. (2009). Schmidt Correctors and Diffraction Gratings Aspherized by Active Optics. In: Astronomical Optics and Elasticity Theory. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-68905-8_5
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