Paper
29 November 1979 Optical Design Of The ATMOS Fourier Transform Spectrometer
Irving R. Abel, Bruce R. Reynolds, J. B. Breckinridge, J. Pritchard
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Abstract
The optical system design of the ATMOS Fourier transform spectrometer to be operated from SpaceLab for the measurement of stratospheric trace molecules contains features which enable it to achieve the required fringe contrast of 80% and spectral resolution of .02 cm-1 (apodized) over a spectral range of 2-16 µm. In particular, the design for high performance and stability is based on the following key features, which alleviate to a substantial degree the usual requirements for alignment precision: 1. "cat's eye" mirror configuration in the two arms of the interferometer for retroreflection stability. 2. tilt-compensated system of beamsplitter, compensator and fold mirrors for wavefront directional stability. 3. paraboloidal "cat's eye" primary mirror for wavefront stability against shear. 4. rotable compensator for matching chromatic dispersion. 5. wedged refractive components to avoid channel spectra due to the Fabry-Perot effect.
© (1979) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Irving R. Abel, Bruce R. Reynolds, J. B. Breckinridge, and J. Pritchard "Optical Design Of The ATMOS Fourier Transform Spectrometer", Proc. SPIE 0193, Optical Systems in Engineering I, (29 November 1979); https://doi.org/10.1117/12.957867
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CITATIONS
Cited by 11 scholarly publications.
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KEYWORDS
Wavefronts

Mirrors

Eye

Sensors

Interferometers

Beam splitters

Retroreflectors

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