Fig. A.8
Comparison of gas density at the position of the Rosetta orbiter predicted by models with inhomogeneous (after four iterations) nucleus (green) and COPS measurements (red): in September 15–October 30, 2014 (top row), in October 8–12 (bottom row). Left panels: DSMC, right panels: EE. The bottom part of each panel shows cometocentric distance Δ, colatitude θSC, and phase angle α of the orbiter. The horizontal axis shows the date (yy-mm-dd).
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