Fig. 1

Sketch of solar wind charge-exchange interactions (SWCX) at comet 67P for a heliocentric distance of about 2 AU. The upstream solar wind, composed of H+ and He2+ ions, experiences charge-changing collisions when impacting the comet’s neutral atmosphere, producing a mixture of charged states downstream of the collision. ENAs are depicted in pink. An increasingly deep blue color denotes a correspondingly denser atmosphere. SWCX plays a major role at and around the bow shock-like structure, depicted in shades of red, where the solar wind is heated and deflected.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.