Paper
26 September 2013 A tolerancing approach taking into account the interferometric alignment scheme of the EUCLID NISP space optics
Frank Grupp, Eric Prieto, Norbert Geis, Andreas Bode, Reinhard Katterloher, Christof Bodendorf, Martin Becker, Stephanie Bogner, Ralf Bender
Author Affiliations +
Abstract
The ESA/EUCLID satellite is equipped with two instruments that are simultaneously observing patches of < 0:5 square degree on the sky. The VIS visual light high spacial resolution imager and the NISP near infrared spectrometer and photometer are separated by a di-chroic beam splitter. The huge field of view, together with the enormous demands on the optical performance and in flight stability of the instruments and telescope lead to unique demands in post launch alignment. A very detailed, very well set up optical tolerance analysis is therefore one key point in the success of the mission. Design and alignment have to be optimized for best toleranced performance. This paper presents the baseline concept of the NISP instrument with its two observational modes being low resolution slit-less spectroscopy and three band J, H&K+ photometry. Special chapters deal with the alignment scheme and the derived tolerance approach which will be used towards the instrument PDR.
© (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Frank Grupp, Eric Prieto, Norbert Geis, Andreas Bode, Reinhard Katterloher, Christof Bodendorf, Martin Becker, Stephanie Bogner, and Ralf Bender "A tolerancing approach taking into account the interferometric alignment scheme of the EUCLID NISP space optics", Proc. SPIE 8860, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts VI, 88600G (26 September 2013); https://doi.org/10.1117/12.2023264
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KEYWORDS
Tolerancing

Computer generated holography

Space telescopes

Telescopes

Optical alignment

Galactic astronomy

Image quality

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