作者: Michael J. Wolff , Michael D. Smith , R. Todd Clancy
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摘要: Near-infrared spectra returned by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM, [1]) on-board Orbiter (MRO) contain clear spectral signature of several atmospheric gases including carbon dioxide (CO2), water vapor (H2O), and monoxide (CO). Here we describe seasonal spatial mapping one full Martian year using CRISM spectra.