Pitch angle distributions of energetic electrons observed by SolO/EPT (top left), SolO/HET (top right), STEREO A/SEPT (bottom left), and Wind/3DP (bottom right). Top panels: sectored electron fluxs of ∼50 − 80 keV (bottom figures and top left figure) and 2.4 − 6.0 MeV (top right, HET) observed in the four viewing directions of the telescopes (in case of STEREO and SolO) or binned into eight sectors for Wind. Second panel: corresponding pitch angles covered by the different viewing directions or sectors, third panel: pitch angle distributions of the electrons (flux in color coding). Fourth panel: magnetic field magnitude and RTN components and bottom panel: first order anisotropy. The colored band on top of the magnetic field panel denotes the in situ magnetic field polarity with red (green) marking negative (positive) polarity and yellow denoting unclear polarity periods. We note the longer time period of the figure showing Wind data.