Design and verification of the Far Ultraviolet Spectrographic Imager (FUV-SI) for the IMAGE mission

Details Design and verification of the Far Ultraviolet Spectrographic Imager (FUV-SI) for the IMAGE mission Design and verification of the Far Ultraviolet Spectrographic Imager (FUV-SI) for the IMAGE mission

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3445..427r&link_type=abstract

Proc. SPIE Vol. 3445, p. 427-438, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, Oswald H. Siegmund; Mark A. Gummin

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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.

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