Paper
1 December 1990 Telescope design of the CRISTA/SPAS experiment aboard the Space Shuttle
Author Affiliations +
Abstract
This paper presents details of the optical and mechanical layout of a cryogenically cooled IR-sensor named CRISTA (CRyogenic Infrared Spectrometers and Telescopes for the Atmosphere). The instrument is designed to analyze dynamical processes in the middle atmosphere. For this purpose, it measures IR emissions of several trace gases at the limb using three independent telescopes with high off axis rejection performance. CRISTA, integrated in the free-flyer ASTRO-SPAS, will be launched in 1993 by the Space Shuttle for a 9 day mission.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Peter Barthol, Klaus U. Grossmann, and Dirk Offermann "Telescope design of the CRISTA/SPAS experiment aboard the Space Shuttle", Proc. SPIE 1331, Stray Radiation in Optical Systems, (1 December 1990); https://doi.org/10.1117/12.22649
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Space telescopes

Spectrometers

Infrared telescopes

Mirrors

Sensors

Optical components

RELATED CONTENT

Optical design for the ATLAS multispectral scanner
Proceedings of SPIE (September 16 1992)
CRISTA: a cryogenic IR telescope with high spatial resolution
Proceedings of SPIE (September 30 1994)
TAUVEX: UV space telescope
Proceedings of SPIE (January 22 1993)
Very broad spectrum afocal telescope
Proceedings of SPIE (September 21 1998)

Back to Top