Fig. 6
Number density of solar wind protons together with their bulk velocity as a vector field a), and the magnetic field magnitude b). Cuts through y = 0 for the comet at 2.35 au, case five. The ambient solar wind number density is 0.9 cm-3, and the ambient magnetic field is 2.3 nT with a Parker spiral angle of 67°. The location of the comet is marked by black cross-hairs.
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