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Table 2

Log-mean fluxes (in log 10 SFU) for the distributions show in Fig. 6 of type III bursts that are and are not interplanetary (have significant emission below 14 MHz).

Log-mean flux 164+173 MHz 237+228 MHz 327 MHz 411+408 MHz

IT3 2.0 ± 0.5 1.7 ± 0.4 1.6 ± 0.5 1.6 ± 0.6
No IT3 1.4 ± 0.5 1.5 ± 0.6 1.5 ± 0.6 1.5 ± 0.7

Notes. Values and errors are calculated from the first and second moments of the distributions. The log-mean is used to avoid biasing the results on the largest events.

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