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Progress in Earth and Planetary Science
Fig. 7 | Progress in Earth and Planetary Science

Fig. 7

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

Fig. 7

Diagonal elements of AKM and error ratio of dust model parameters. The left and right scales are for AKM and error ratio, respectively. Case 1, with all observation parameters listed in Table 5; case 2, without DSR; case 3, without aureole; case 4, without forward scattering; case 5 without backward scattering; and case 6, without color ratio. Averaging kernel closer to unity means that information from observations is more significant. Panels (a) - (g) show the relation between A ii / ε r,i and SZA for X 1 - X 7, respectively

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