Temporal evolution of mass fluxes of the different accretion and ejection phenomena present in the system: mass accretion rate measured at the stellar surface (solid line), total mass outflow rate of magnetospheric ejections (dot-dashed line), mass flux fueling the MEs coming from the star only (long-dashed line), stellar wind outflow rate (dashed gray line), disk wind mass outflow rate (dotted line). The image refers to case C03. Time is given in units of rotation periods of the central star.