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Fig. 5


Time series over three frequency channels where the J-burst is observed as the highest intensity peaks in the top panel compared to the evolution of the jet in AIA 171 Å (second panel), a B-class solar flare in GOES 1–8 Å (third panel), and RHESSI 3–6 and 6–12 keV channels (bottom panel). The flare seen in GOES and RHESSI light curves occurs in the southern hemisphere, while the jet and Type III bursts occurred in the northern hemisphere. The vertical dashed lines denote the time span of the dynamic spectra in Fig. 1b.

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