Author/Authors :
Formisano، نويسنده , , V. and Encrenaz، نويسنده , , T. and Fonti، نويسنده , , S. and Giuranna، نويسنده , , M. De Grassi، نويسنده , , D. and Hirsh، نويسنده , , H. and Khatuntsev، نويسنده , , I. and Ignatiev، نويسنده , , N. and Lellouch، نويسنده , , E. and Maturilli، نويسنده , , A. and Moroz، نويسنده , , V. and Orleanski، نويسنده , , P. and Piccioni، نويسنده , , G. and Rataj، نويسنده , , M. and Saggin، نويسنده , , B. and Zasova، نويسنده , , L.، نويسنده ,
Abstract :
The evaluation of the planetary Fourier spectrometer performance at Mars is presented by comparing an average spectrum with the ISO spectrum published by Lellouch et al. [2000. Planet. Space Sci. 48, 1393.]. First, the average conditions of Mars atmosphere are compared, then the mixing ratios of the major gases are evaluated. Major and minor bands of CO2 are compared, from the point of view of features characteristics and bands depth. The spectral resolution is also compared using several solar lines. The result indicates that PFS radiance is valid to better than 1% in the wavenumber range 1800–4200 cm−1 for the average spectrum considered (1680 measurements). The PFS monochromatic transfer function generates an overshooting on the left-hand side of strong narrow lines (solar or atmospheric). The spectral resolution of PFS is of the order of 1.3 cm−1 or better. A large number of narrow features to be identified are discovered.
