Optical properties of the Martian aerosols as derived from Imager for Mars Pathfinder midday sky brightness data

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Scientific paper

The data-model residuals exhibited, albeit weak, wavelength dependence (Table 2). This dependence can be interpreted as an indication that during the time the analyzed images were taken, the dust particle distribution was bimodal or that the Martian atmosphere contained a second component, possibly submicron ice particles, in the aerosol's population. Here we will present analysis of the data from the remaining 5 sols.

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