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Fig. 12


Monte Carlo dust tail code simulations (red contours) compared to the OSIRIS NAC observations (black contours) for the input parameters derived from Rotundi et al. (2015) with a power-law exponent of the size distribution function of –3 and the terminal velocities being given by v(μ,t) = 1320(1−μ)0.96u(t) m s-1 (Model 2).

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