Paper
22 October 1999 Optical calibration of the FUV spectrographic imager for the IMAGE mission
Serge LM Habraken, Yvette Houbrechts, Etienne Renotte, Marie-Laure Hellin, Anne Orban, Pierre P. Rochus, Stephen B. Mende, Harald U. Frey, Steve Geller, Joseph M. Stock
Author Affiliations +
Abstract
The FUV Spectrographic Imager for IMAGE is simultaneously imaging auroras at 1218 and 1358 angstrom. It is designed to efficiently reject the Lyman-(alpha) emission line at 1215.7 angstrom. This paper describes the optical calibration. The content is: 1) field of view calibration: detector pixels location with respect to the reference optical cube; distortion matrix used to computer the TDI. b) Radiometric calibration: detector response and linearity; instrument throughput according to its clear aperture and mirror reflection lost; response vs. wavelength and band-rejection certification.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Serge LM Habraken, Yvette Houbrechts, Etienne Renotte, Marie-Laure Hellin, Anne Orban, Pierre P. Rochus, Stephen B. Mende, Harald U. Frey, Steve Geller, and Joseph M. Stock "Optical calibration of the FUV spectrographic imager for the IMAGE mission", Proc. SPIE 3765, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy X, (22 October 1999); https://doi.org/10.1117/12.366529
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Cited by 3 scholarly publications.
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KEYWORDS
Sensors

Calibration

Monochromators

Mirrors

Imaging systems

Spectral resolution

Distortion

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