
Proceedings Paper
Design of a Fabry-Perot interferometer for the SO/PHI instrument on Solar OrbiterFormat | Member Price | Non-Member Price |
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Paper Abstract
We present our work on the spectral analyser of the Polarimetric and Helioseismic Imager (PHI) instrument to
be flown aboard ESA's Solar Orbiter mission. We detail the choices that were made to determine the concept
of the spectral analyser, a Lithium Niobate Fabry-Perot interferometer, and its characteristics, as to fulfil both
scientific needs and technical requirements. We will present the first experimental results - including stability,
repeatability, parallelism, spectral homogeneity and imaging capability - on an air-spaced piezoelectric-tunable
etalon, which is the backup solution for PHI.
Paper Details
Date Published: 12 July 2008
PDF: 10 pages
Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 701017 (12 July 2008); doi: 10.1117/12.788310
Published in SPIE Proceedings Vol. 7010:
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Jacobus M. Oschmann Jr.; Mattheus W. M. de Graauw; Howard A. MacEwen, Editor(s)
PDF: 10 pages
Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 701017 (12 July 2008); doi: 10.1117/12.788310
Show Author Affiliations
Clément Trosseille, Institut d’Astrophysique Spatiale, Univ. Paris-Sud 11 (France)
Thierry Appourchaux, Institut d’Astrophysique Spatiale, Univ. Paris-Sud 11 (France)
Thierry Appourchaux, Institut d’Astrophysique Spatiale, Univ. Paris-Sud 11 (France)
Jean-Jacques Fourmond, Institut d’Astrophysique Spatiale, Univ. Paris-Sud 11 (France)
Published in SPIE Proceedings Vol. 7010:
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Jacobus M. Oschmann Jr.; Mattheus W. M. de Graauw; Howard A. MacEwen, Editor(s)
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