The ISEE-1 spacecraft carries a mass spectrometer for ions with E/Q ? 17 keV/e. On December 11, 1977, it traversed the equatorial magnetosphere in the prenoon and dawn sectors during the early recovery phase of a magnetic storm with peak DST=-125&ggr;. Along the dayside (inbound) leg O+ was comparable to or exceeded H+ in number density in the energy range 0.1 keV ? E ? 17 keV. The velocity distribution of O+ showed a characteristic dispersion, consistent with the ions being transported to the dayside from the dusk to midnight sector. The high-energy slope of the H+ and O+ distribution functions showing different radial dependence, with the slope of H+ being consistent with a harder component carrying most of the energy density. Along the nightside (outbound) leg the O+ density was very low outside of 5 RE, and most of the number density was due to the hard H+ component.