A new type of low energy (300 eV) population is absent, making the ion energy-time dispersion very weak. Third, this event does not seem to be related to either any solar wind density increase or southward/disturbed interplanetary magnetic field conditions. These observations suggest that this a more stagnant phenomenon, and we propose to call this a ''Stagnant Plasma Injection'' event. ¿ American Geophysical Union 1993