Twelve-hour overview of the event, where magnetic fields and intensity-time energetic particle profiles are overlaid for the Solar Orbiter-Wind (left) and for the ACE-Wind observations. The fluxes are normalized to the maximum flux in each interval. From top to bottom, we show an example of high (top) and low (middle) energy particle intensity-time profiles and the magnetic field magnitude, scaled with the square of the heliocentric distance.