Author/Authors :
Hirsch، نويسنده , , H. and Formisano، نويسنده , , V. D. Moroz، نويسنده , , V.I. and Arnold، نويسنده , , G. and Jurewicz، نويسنده , , A. and Michel، نويسنده , , G. and Lopez-Moreno، نويسنده , , J.J. and Piccioni، نويسنده , , G. and Cafaro، نويسنده , , N.، نويسنده ,
Abstract :
The Planetary Fourier Spectrometer (PFS) is intended for the mission Mars 96. It covers a wave-length 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 modified 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.
