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Progress in Earth and Planetary Science
Fig. 11 | Progress in Earth and Planetary Science

Fig. 11

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

Fig. 11

a Sensitivity of dust observation parameters to the volume mixing ratio of fine mode dust (ρ F ). Parameter Δy represents the difference between the maximum and minimum values of the normalized observational parameters when ρ N is changed from 0 to 0.01. b Systematic error due to ignorance of bimodal size distribution. The systematic errors of the normalized dust model parameters are estimated from the differences between the observational parameters calculated with true (0.01) and wrong (0) values of the fine mode dust volume mixing ratio (ρ F )

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