Fig. 6.

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In situ electron recordings by multiple observers. Energetic electron event observed by Solar Orbiter/EPT (a) and HET (b). The top panels of (a) and (b) show the intensities of 40–50 keV and 1.1–2.4 MeV electrons as observed by the four different sensors of the EPT and HET instruments. The second panels show the corresponding pitch-angle coverage, and the third panels show the pitch-angle-dependent intensities, with the intensity level indicated via colour coding. The bottom panels show the first-order anisotropies. Energetic electron event observed by STEREO-A/SEPT in the 45–55 keV energy channel (c) and Wind/3DP in the 50–82 keV channel (d). The panels have the same content as for (a) and (b), but (d) shows a longer time period.

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