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Proceedings Paper

Alignment and performances of the FUV Spectrographic Imager for the IMAGE mission
Author(s): Serge LM Habraken; Yvette Houbrechts; Etienne Renotte; Claude A. J. Jamar; Stephen B. Mende; Harald U. Frey; Oswald H. W. Siegmund
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Paper 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.

Paper Details

Date Published: 10 November 1998
PDF: 11 pages
Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); doi: 10.1117/12.330301
Show Author Affiliations
Serge LM Habraken, Ctr. Spatial de Liege (Belgium)
Yvette Houbrechts, Ctr. Spatial de Liege (Belgium)
Etienne Renotte, Ctr. Spatial de Liege (Belgium)
Claude A. J. Jamar, Ctr. Spatial de Liege (Belgium)
Stephen B. Mende, Univ. of California/Berkeley (United States)
Harald U. Frey, Univ. of California/Berkeley (United States)
Oswald H. W. Siegmund, Univ. of California/Berkeley (United States)


Published in SPIE Proceedings Vol. 3445:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX
Oswald H. W. Siegmund; Mark A. Gummin, Editor(s)

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