Fig. 12From: Feasibility of retrieving dust properties and total column water vapor from solar spectra measured using a lander camera on MarsSensitivities of water vapor observation parameters to TCWV and dust model parameters. Panels (a) - (d) show the relation between Δy(c w ) and SZA for D 2, D 3, S 2, and S 3, respectivelyBack to article page