Dynamic and peak energy spectra of the electron events observed by the Solar Orbiter/EPD suite on 2021 August 24. (a) Dynamic spectrogram (EPT and STEP detectors). The data were smoothed by a running mean over 3 min. The magenta lines show the ideal dispersion for electrons injected at the earliest (solid lines) and latest (dotted lines) SRT times given for each event in Table 1. (b) Spectra of the differential electron flux at the maxima in each detector channel. A pre-event background taken 30 minutes before the first event was subtracted.