Abstract. Day-time Pc 3-4 ($5±60 mHz) and nighttime Pi 2 ($5±20 mHz) ULF waves propagating down through the ionosphere can cause oscillations in the Doppler shift of HF radio transmissions that are correlated with the magnetic pulsations recorded on the ground. In order to examine properties of these correlated signals, we conducted a joint HF Doppler/ magnetometer experiment for two six-month intervals at a location near L = 1.8. The magnetic pulsations were best correlated with ionospheric oscillations from near the F region peak. The Doppler oscillations were in phase at two dierent altitudes, and their amplitude increased in proportion to the radio sounding frequency. The same results were obtained for the O-and X-mode radio signals. A surprising ®nding was a constant phase dierence between the pulsations in the ionosphere and on the ground for all frequencies below the local ®eld line resonance frequency, independent of season or local time. These observations have been compared with theoretical predictions of the amplitude and phase of ionospheric Doppler oscillations driven by downgoing Alfve n mode waves. Our results agree with these predictions at or very near the ®eld line resonance frequency but not at other frequencies. We conclude that the majority of the observations, which are for pulsations below the resonant frequency, are associated with downgoing fast mode waves, and models of the wave-ionosphere interaction need to be modi®ed accordingly.