Solar Orbiter IP shock properties. Panel a shows M_A both computed from the MAG and SWA-PAS observations and M_A estimated from B according to Eq. (B.3). The shock geometry is shown in panel b and was computed from mixed-mode 3 if all data were available or from magnetic coplanarity if only MAG was available. The geocentric distance of each shock is shown in panel c and the compression ratios in panel d. Missing entries signify lack of data.