Paper
13 April 1989 Diffraction Optical Modelling Of Far Infrared Spectrometers
Michel Saisse, Patrick Rabou
Author Affiliations +
Proceedings Volume 1013, Optical Design Methods, Applications and Large Optics; (1989) https://doi.org/10.1117/12.949363
Event: 1988 International Congress on Optical Science and Engineering, 1988, Hamburg, Germany
Abstract
At far Infrared wavelengths (45 to 180 micrometers) the energy losses by diffraction at the different optical surfaces of a spectrometer cannot be neglected. A specific optical software has been develooped to simulate the multiple diffraction effects existing in the Long Wavelength Spectrometer (LWS), one of the four scientific instruments of the ESA Infrared Satellite ISO. The optical design of the spectrometer is briefly described, the interest of the use of an off-axis aspherical grating for a compact and flexible design is demonstrated. The mathematical model based on the Fourier-Fraunhofer diffraction theory is explained. The diffraction effects due to the wavefront limitation, at the relevant levels, and the wavefront aberrations of the spectrometer are modelled. The main results are given and discussed. The emphasis is set on the study of the energy losses due to multiple diffractions. Finally this model has been used to optimise the LWS optics and to define tolerances for the manufacturing and the adjustment of the optical system.
© (1989) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michel Saisse and Patrick Rabou "Diffraction Optical Modelling Of Far Infrared Spectrometers", Proc. SPIE 1013, Optical Design Methods, Applications and Large Optics, (13 April 1989); https://doi.org/10.1117/12.949363
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KEYWORDS
Diffraction

Spectrometers

Mirrors

Sensors

Telescopes

Diffraction gratings

Fourier transforms

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