Alignment and performances of the FUV Spectrographic Imager for the IMAGE mission

Details Alignment and performances of the FUV Spectrographic Imager for the IMAGE mission Alignment and performances of the FUV Spectrographic Imager for the IMAGE mission

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3445..416h&link_type=abstract

Proc. SPIE Vol. 3445, p. 416-426, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, Oswald H. Siegmund; Mark A. Gummin

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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