Computer Science
Scientific paper
Jan 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2089..284a&link_type=abstract
Proc. SPIE Vol. 2089, p. 284-285, 9th International Conference on Fourier Transform Spectroscopy, John E. Bertie; Hal Wieser; Ed
Computer Science
Scientific paper
The Planetary Fourier Spectrometer (PFS) on board the Mars-94 mission is an infrared spectrometer optimized for studies of the Martian atmosphere. Moreover, the measurements of the instrument also will provide information about the surface composition and the surface- atmosphere interactions. The spectrometer consists of a dual Rotational Reflector Interferometer (RRI) covering two spectral ranges 220 - 1670 cm-1 (6 - 45 micrometers ) and 2080 - 8000 cm-1 (1.25 - 4.8 micrometers ) the long wavelength channel (LWC) and the short wavelength channel (SWC) respectively. Partial misalignment due to tolerance effects of real optical and mechanical elements are taken into account in an estimation of the spectral responsivity in comparison with the radiation of the Martian surface and atmosphere.
Arnold Gabriele
Formisano Vittorio
Hirsch Helmut
Moroz Vassili I.
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