Fig. 1
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Distribution of the dynamic spectra directions (beams) within our observing FoV, overlaid on a NenuFAR broadband (30–78 MHz) Stokes I image of background astronomical radio sources. Each gray circle corresponds to a direction for the synthesized IQUV dynamic spectra. The dashed line represents the predicted path of STARLINK3647 across the FoV from 16:19:57 to 16:20:31 on 6 June 2024, calculated using TLE data.
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