Overview plot showing an example event from our list. The top panel shows the flux of all electron channels of HET and one electron channel of EPT for comparison. The black horizontal line shows the threshold of the E200 channel. The second subplot shows some of the proton channels of HET and one of EPT. Contamination might be seen here. Data from SWA are used in the third and fourth panels for the solar wind speed and the temperature and density. The MAG data are used for the fifth and sixth panels to show the different magnetic field values and the pitch angle of all viewing directions, respectively. In addition, the flux of the E200 channel is plotted alongside the pitch angels and is colour coded. The vertical black line shows the start time we find. The MAG data have a time resolution of 1 min and the other measurements have a time resolution of 10 min.