10 November 1998 Alignment and performances of the FUV Spectrographic Imager for the IMAGE mission
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Abstract
The FUV Spectrometer Imager for IMAGE is designed to simultaneously take aurora images at 1218 and 1356 angstrom. This paper describes the alignment procedure and performance results. The Spectrograph alignment requires to efficiently reject the Lyman-(alpha) line at 1216 angstrom. The imager alignment requires to tune optical components until finest imaging.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Serge LM Habraken, Serge LM Habraken, Yvette Houbrechts, Yvette Houbrechts, Etienne Renotte, Etienne Renotte, Claude A. J. Jamar, Claude A. J. Jamar, Stephen B. Mende, Stephen B. Mende, Harald U. Frey, Harald U. Frey, Oswald H. W. Siegmund, Oswald H. W. Siegmund, } "Alignment and performances of the FUV Spectrographic Imager for the IMAGE mission", Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); doi: 10.1117/12.330301; https://doi.org/10.1117/12.330301
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