Fig. A.9
Comparison of relative abundances of H2O (top panels), CO (middle panels), and CO2 (bottom panels) at the position of the Rosetta orbiter predicted by the DSMC solution (green) with inhomogeneous (after four iterations) nucleus and COPS measurements (red): in September 15–October 30, 2014 (left panels), in October 8–12 (right panels).
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