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Progress in Earth and Planetary Science
Fig. 4 | Progress in Earth and Planetary Science

Fig. 4

From: Feasibility of retrieving dust properties and total column water vapor from solar spectra measured using a lander camera on Mars

Fig. 4

Transmittance of water vapor in the Martian atmosphere. Values are simulated with a wavelength resolution of 2 nm (FWHM) for volume concentrations of 100, 300, and 500 ppm. The blue band indicates the wavelength band around the absorption peak centered at 935 nm with a band width of 5 nm, and the two red bands indicate the wavelength band outside the absorption band centered at 935 and 972 nm with a band width of 5 nm

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