DOI:
10.1016/0032-0633(96)00062-1
Authors:
Hirsch H., Formisano V., Moroz V.I., Arnold G., Jurewicz A., Michel G., Lopez-Moreno J.J., Piccioni G., Cafaro N.
Journal:
Planetary and Space Science
Abstract:
The Planetary Fourier Spectrometer (PFS) is intended for the mission Mars 96. It covers a wavelength range of 1.25-5 and 6-45 μm with a spectral resolution of 2 cm-1 and a field of view (FOV) of 35 and 70 mrad, respectively. the instrument is a modiefied Michelson interferometer optimized for the study of the Martian atmosphere. Moreover, the PFS will provide information about the composition and properties of the Martian soil. Copyright © 1996 Elsevier Science Ltd.
URL:
https://ui.adsabs.harvard.edu/#abs/1996P&SS...44..889H/abstract