Fig. B.1.
![image](/articles/aa/full_html/2024/06/aa49277-24/aa49277-24-fig10.jpg)
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Tracking the herringbone-like radio emission and type II radio bursts in the dynamic spectra. (a) Dynamic spectrum observed by ORFEES at 150–190 MHz between 11:01:10 and 11:01:50 UT. The points in the spectrum indicate a single reverse drifting structure and how the drift rate is determined. (b) Dynamic spectrum observed by STEREO-B/SWAVES and NDA at 1–80MHz between 11:00 and 11:25 UT.
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