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Fig. 2


Overview of the RPC magnetic field data and auxiliary data for the time interval 19 March to 19 April 2016, which are used to study the tail excursion. (AD) RPC MAG data Bx, By, Bz, Bm; (E) and (F) the cone-angle θcand clock-angle θcof the measured magnetic field; (G) sensor temperature; (H) radial distance R of Rosetta to comet 67P; (I) and (J) propagated solar wind tangential magnetic field Bsw and dynamic pressure Pdyn using Tao et al. (2005); and (K) clock angle of the solar wind magnetic field from OMNI shifted by 6 days.

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