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- W262396169 abstract "Introduction: Planetary Fourier Spectrometer is working on orbit around Mars for more than one Martian year. More than 300 000 spectra were obtained for different seasons, locations and local times. Longwavelength channel of PFS covers a spectral range 300 – 1500 cm-1 (7-35 μm) with spectral resolution 1.8 cm-1 and allows retrieval of vertical temperature profiles from the surface up to 50-55 km. (Formisano et al., 2005). Vertical temperature profiles and aerosol opacity may be retrieved from a single spectrum on the day side, when the surface temperature is rather high. At night side the temperature is low and spectra have to be averaged. As well in the polar region we deal with spectra averaged over 2 10, so effective field of view increases up to 40-200 km respectively (Zasova et al.2005)" @default.
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- W262396169 date "2005-01-01" @default.
- W262396169 modified "2023-09-27" @default.
- W262396169 title "SEASONAL VARIATION OF THE STRUCTURE OF MARTIAN AT- MOSPHERE FROM PFS MARS EXPRESS DATA:WATER ICE CLOUDS ." @default.
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