Overview of the tailward pass of Venus by Solar Orbiter showing magnetic field magnitude (panel a), magnetic field vector in VSO coordinates (panel b), difference between the clock angles of the spacecraft and the solar wind convective electric field (panel c), sin²(θ) of the magnetic field and assumed radial bulk flow (panel d), |δB|/|B| (panel e), STEP Magnet channel total ion flux spectrogram (panel f), power spectral density of magnetic field perturbations (panel g), and ellipticity of the magnetic field (panel h). The local proton gyrofrequency is overplotted on panels g and h. Vertical lines denote current sheet crossings, and the purple bars in panel a mark traversals into the magnetotail (see text for criteria).