Overview of observations from the Venus flyby showing the magnetic field magnitude from MAG (panel a), MAG magnetic field vector in VSO coordinates (panel b), electron density estimate derived from RPW (panel c), STEP Magnet channel total ion flux spectrogram (panel d), and HET detector C high-gain channel GCR count rate (panel e). The bow shock is denoted by the vertical red line. The persistently high STEP count rate around 0.01 MeV is due to a well-understood instrumental background (Rodríguez-Pacheco et al. 2020).