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An energetic ion (<i>E</i>&le;40) event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to three statistical bow shock position models, the Cluster spacecrafts are located at ~0.5 <i>R_e</i> from the shock and the averaged bow shock &theta;_<i>Bn0</i> is about ~30&deg;. The analysis of the three-dimensional angular distribution indicates that ions propagating roughly along the magnetic field direction are observed at the onset of the event. Later on, the angular distribution is gyrophase-bunched and the pitch-angle distribution is peaked at &alpha;₀~&theta;_<i>Bn0</i>, consistent with the specular reflection production mechanism. The analysis of the waves shows that they are left-handed in the spacecraft frame of reference (right-handed in the solar wind frame) and propagate roughly along the ambient magnetic field; we have found that they are in cyclotron-resonance with the field-aligned beam observed just upstream. Using properties of the waves and particles, we explain the observed particle flux-modulation in the context of &theta;_<i>Bn</i> changes at the shock caused by the convected ULF waves. We have found that the high count rates coincide with particles leaving the shock when &theta;_<i>Bn</i> angles are less than ~40&deg;, consistent with the specular reflection hypothesis as the production mechanism of ions.