Fig. 7.

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Solar radio noise storm observed on 2 November 2020. (a) In this mode 357 observation, a number of bright bursts can be seen at frequencies greater than 110 MHz (yellow in the dynamic spectrum). Here the data spans 2 h from 12:00 UTC and has a temporal resolution of 10 ms. (b) Zoom-in of panel a at 1 ms temporal resolution. A number of short duration SRBs are observed. The inset shows the sub-second variation of an individual burst in the noise storm, also at a temporal resolution of 1 ms.
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