Inner heliospheric radial solar wind velocity in the ecliptic plane simulated using the WSA-ENLIL + Cone model provided by DONKI. The snapshots were taken at 2022 March 12 00:00 (left) and 2022 March 13 12:00 (right), corresponding to the time intervals of the ESP phase seen at Solar Orbiter and ACE. A SIR, denoted by the sharp transition between a slow solar wind stream (blue) and a faster stream (green), can be seen interacting with each spacecraft at the time of ICME passage.