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. Author manuscript; available in PMC: 2020 Jul 22.
Published in final edited form as: Astron Astrophys. 2019 Sep 30;630:A30. doi: 10.1051/0004-6361/201833536

Fig. 3.

Fig. 3.

Top: post-outbound-equinox (8–10 July 2016) southern hemisphere time variation of the seven studied species scaled to the distance of Rosetta from the center of the nucleus (r2), and the corresponding sub-spacecraft longitude and latitude values (bottom). Species whose time variability trend together are illustrated with empty and filled markers.