Fig. 2.

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Overview of the event observed in X-ray and radio. (a) GOES soft X-ray flux profile at 0.1–0.8 nm (1.5–12.4 keV) (black curves) and GBM/Fermi X-ray count rates in three energy bands between 6 and 25 keV (solid red curves). The GBM/Fermi X-ray count rates are the sum of the count rate recorded by the three detectors NaI00, NaI01, and NaI05. (b) STIX X-ray count rates in three energy bands between 6 and 28 keV (dotted blue lines) and NRH radio flux time profiles at 150.9 MHz (ruby) and 228.0 MHz (orange, the same colors as the colors of the NRH imaging contours shown later in the paper). The NRH radio flux profiles come from the full Sun. (c) ORFEES radio dynamic spectrum.
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