Time series of the magnetic (left) and plasma (right) variables at Solar Orbiter. The shock is indicated with the vertical blue line. The green line denotes the passing of the magnetic ejecta. The blue and pink shades indicate the sheath and the regions of magnetic ejecta. The dynamic solar wind simulations, using the cone and spheromak CME models, are depicted in orange and green, respectively. The steady solar wind simulations with cone and spheromak CMEs are shown in red and purple.