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Fig. 9 | Progress in Earth and Planetary Science

Fig. 9

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

Fig. 9

Non-diagonal elements of AKM (A ij  = ∂x r,i,/∂x j ) of dust model parameters. The lines with small symbols indicate the type of retrieved dust parameters (x r ), while the large circles indicate the type of true dust parameters (x). Panels (a) - (f) show the relation between A ij and SZA for cases 1-6, respectively. The definitions of cases 1–6 are the same as in Fig. 7. These graphs are useful for the examination of error propagation from one dust parameter to another (see text)

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