Fig. 13
Upper panel: daily ratio of the number of RPC-MIP active spectra with cold electrons to all measured RPC-MIP active spectra (blue bars, left y-axis) and ratio of the number of RPC-MIP passive spectra with electric field emissions to all measured RPC-MIP passive spectra (red bars, right y-axis). The horizontal axis indicates the day of the year in 2016. Middle panel: cometocentric distance of Rosetta in km. Bottom panel: latitude (black line, left y-axis) and longitude (blue line, right y-axis) of Rosetta.
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