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Figure 3


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The CCDF of the SRB data set from 1996 to 2017. These events are plotted again in yellow in Figure 4 of Section 4. It is clear that the function is asymptotically decreasing towards 106 sfu. Saturation occurs on the RSTN instrument when the flux is larger than 106 sfu. There is currently not a global solar radio spectrometer network which is flux calibrated and which can measure above 106 sfu.

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