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1 October 1993 Infrared Space Observatory short-wavelength spectrometer
Mattheus WM de Graauw, Douwe A. Beintema, Willem Luinge, Jan J. Wijnbergen, Klaas J. Wildeman, G. Ploeger, J. Evers, Erick T. Young, Theo M. Kamperman, C. van Dijkhuizen, P. de Groene, M. Frericks, R. van der Linden, S. Czempiel, Helmut Feuchtgruber, Leo N. K. Haser, Reinhard O. Katterloher, F. Melzner, H. Spath, Jakob E. Stoecker, Huib Visser, Kees Smorenburg, H. van Agthoven
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Proceedings Volume 2019, Infrared Spaceborne Remote Sensing; (1993) https://doi.org/10.1117/12.157842
Event: SPIE's 1993 International Symposium on Optics, Imaging, and Instrumentation, 1993, San Diego, CA, United States
Abstract
The Short-Wavelength Spectrometer (SWS) for ISO operates in the wavelength range from 2.4 to 45 micrometers. It consists of two, almost identical, grating spectrometers that provide resolving powers varying between 1000 to 2000. In the wavelength region from 12 to 45 micrometers a much larger (>20.000) resolution can be obtained with a pair of Fabry-Perot interferometers. This paper describes the design of the SWS.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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Mattheus WM de Graauw, Douwe A. Beintema, Willem Luinge, Jan J. Wijnbergen, Klaas J. Wildeman, G. Ploeger, J. Evers, Erick T. Young, Theo M. Kamperman, C. van Dijkhuizen, P. de Groene, M. Frericks, R. van der Linden, S. Czempiel, Helmut Feuchtgruber, Leo N. K. Haser, Reinhard O. Katterloher, F. Melzner, H. Spath, Jakob E. Stoecker, Huib Visser, Kees Smorenburg, and H. van Agthoven "Infrared Space Observatory short-wavelength spectrometer", Proc. SPIE 2019, Infrared Spaceborne Remote Sensing, (1 October 1993); https://doi.org/10.1117/12.157842
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KEYWORDS
Sensors
Spectroscopy
Infrared spectroscopy
Spectral resolution
Fabry–Perot interferometry
Analytical research
Fabry–Perot interferometers
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