Study of ISEE 2 fast plasma data reveals that many suprathermal ion events that in previous studies would have been identified as intermediate ion events are actually gyrating ion events. Of 190 apparently intermediate ion events selected on the basis of their signature in energy-time spectrograms, half are actually found to be gyrating ion events. Using a model bow shock, the shock geometries and spacecraft locations for the observed gyrating and intermediate ion events are compared and found to be quite similar. Both gyrating and intermediate ion events are found to be associated with upstream MHD-like wave activity. Most gyrating ion events are associated with large-amplitude, monochromatic, weakly compressive waves, whereas many intermediate ion events are associated with smaller-amplitude, nonmonochromatic, weakly compressive waves. Some intermediate ion events are found to have associated waves. Detailed study of the gyrating ion distributions reveals that the distributions are typically gyrotropic within ~4 RE of the bow shock, whereas at larger distances (up to ~10 RE) upstream from the shock the distributions are frequently ''gyrophase bunched.'' In light of these observational characteristics it is concluded that gyrating ion distributions are most likely generated both throuh coherent wave disruption of field-aligned beams and through reflection of solar wind ions off the shock.