Combined instrument data for the ∼12 h flyby through the induced magnetotial and into the solar wind. (A) Low-pass filtered magnetic field data; (B) Location of the spacecraft in R_V; (C) The cone angle θ_c; (D) The clock angle ϕ_c; (E) The electron density determined from RPW (red) and SCP (black); (F) The time-energy spectrogram of the EPD-STEP instrument. The blue-shaded intervals indicate where the field has the direction of the upstream solar wind. The red-shaded intervals indicate significant structures in the magnetic field. The two dotted lines in the cone angle panel C at θ_c = 60° /120° show the solar wind θ_c, SW ≈ 120°. The vertical black dashed and dotted lines show X_VSO = 1 and ±1 R_V, respectively.