Fig. 2From: Feasibility of retrieving dust properties and total column water vapor from solar spectra measured using a lander camera on MarsSensitivity of (a) DSR and (b–h) SSR to dust model parameters. DSR and SSR intensities for various values of dust model parameters (a: τ, b: τ, c: r eff, d: v eff, e: ρ A , f: m 0, g: k 0, h: z s ) calculated with a radiative transfer code (MODTRAN5) are plotted as functions of wavelength or scattering angleBack to article page