The Near-Infrared Mapping Spectrometer (NIMS) is one of the four remote-sensing science instruments of the Galileo Orbiter scientific payload. The NIMS scientific objectives require operating the detector and optical subsystem at croygenic temperatures. The necessity of assembling, aligning, and testing the optics at room temperature and meeting design specifications at the cryogenic operating temperature (130 K) presented a set of challenging technical problems. A systematic approach to the development of athermalized mounts and supporting structures for optical components is described. A technique utilizing the visible spectral range and supplementary ray-trace information for alignment of an infrared instrument is presented. The optical subsystem point-spread function and spatial and spectral resolution were determined at room temperature using selected spectral and spatial targets. Based on thermal-distortion analyses of the structure and mounts, compensators ware selected, implemented, and verified at cryogenic temperatures. The selection of the compensator and the overall system performance were verified in a thermal vacuum chamber. Various external and internal calibration targets were used.
Near-infrared mapping spectrometer optical subsystem development and testing
Kurzwelliges Infrarotspektrometer fuer Kartographie: Entwicklung und Testen des optischen Teilsystems
Proc. of SPIE. Infrared Technology 9 ; 430 ; 313-324
1983
12 Seiten, 19 Bilder, 2 Tabellen, 5 Quellen
Aufsatz (Konferenz)
Englisch
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