Onsets of the six events showing the hourly LETA range 1 proton rate in the top panels, the HFR and LFR radio data (second and third panels), and the magnetic field magnitude (black trace) and R (blue trace), T (green trace), N (red trace) components (bottom panels). Insets in the upper panels of each event show the solar source region during the related eruption as seen in STEREO-A/EUVI. The images were treated with a wavelet-based algorithm (Stenborg et al. 2008)to enhance the off-limb emission; full movies of the eruptions are available online.