Fig. 11.
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Directivity fit on the peak fluxes measured during the 11 July 2020 event at different frequencies indicated with different colours. STEREO-A, WIND, Parker Solar Probe, and Solar Orbiter measurements are indicated by crosses and labelled as STA, WND, PSP, and SOLO respectively. The vertical lines show the position of the radio source in longitude as determined from the directivity fit.
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