A corrector design using active vase mirrors that allows a fixed telescope to access a large region of the sky

Details A corrector design using active vase mirrors that allows a fixed telescope to access a large region of the sky A corrector design using active vase mirrors that allows a fixed telescope to access a large region of the sky

1997-02-14

arxiv.org/abs/astro-ph/9702122v1

Astronomy and Astrophysics

Astrophysics

Postscript file no figures included, 0.08 Megs, Complete paper can be obtained upon request from authors or from http://athe

Scientific paper

10.1364/AO.36.002114

We investigate whether a three-mirror system, having secondary and the tertiary mirrors with surfaces warped by Zernike polynomials generated by active vase mirrors, is suitable to do the corrections of a fixed parabolic mirror observing at large angles from the zenith. We obtain designs of correctors with remarkable images and control of the distortion of the field of the view contained within a field greater than 15 Deg.

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