10 November 1998 Design and verification of the Far Ultraviolet Spectrographic Imager (FUV-SI) for the IMAGE mission
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The IMAGE FUV-SI is simultaneously imaging auroras at 121.8 nm and 135.8 nm. The spectrograph design challenge is the efficient rejection of the intense Lyman-alpha emission at 121.6 nm while passing its Doppler-shifted component at 121.8 nm. The FUV-SI opto-mechanical design, analysis integration, and verification of performances against environment are discussed in this paper. In absence of STM environmental constraints at subsystem levels are derived analytically from F.E.M. and used for pre-qualifying optical subsystems.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Etienne Renotte, Etienne Renotte, Serge LM Habraken, Serge LM Habraken, Pierre P. Rochus, Pierre P. Rochus, Marie-Laure Hellin, Marie-Laure Hellin, Anne Orban, Anne Orban, Isabelle Tychon, Isabelle Tychon, } "Design and verification of the Far Ultraviolet Spectrographic Imager (FUV-SI) for the IMAGE mission", Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); doi: 10.1117/12.330302; https://doi.org/10.1117/12.330302


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