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Fig. 2.

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Remote-sensing observations between 12 and 23 UT on 2024 July 16. (a): Soft X-ray flux measured by GOES-18. (b): Hard X-ray counts measured by SolO. (c): > 100 MeV γ-ray flux measured by Fermi-LAT. The dashed blue line marks the quiet-Sun background intensity (4.7 × 10−7 cm−2 s−1) reported in Ajello et al. (2021), and the shaded areas indicate the intervals where the Sun was outside the detector FoV. (d)–(g): Radio emission measured by PSP (d), SolO (e), STEREO-A (f), and Wind (g). The red arrow in panel f marks the end of the interplanetary type-II emission at 15:47 UT (1.4 MHz) according to the CDAW DH type-II burst catalog.

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