Fig. 2
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Comparisons of the morphologies of AD Leo’s radio bursts observed on 2 December 2021 (a) and 3 December 2021 (c), with typical Jupiter S-bursts observed at the Nançay Decameter Array (Lamy et al. 2017; Mauduit et al. 2023) (b), and with Solar decameter spike bursts observed with the Huairou/NAOC solar spectrometer (Chernov et al. 2008) (d) and the NenuFAR low-frequency radio telescope (Zarka et al. 2020; Briand et al. 2022) (e).
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