Radio dynamic spectra observed by both S/WAVES and Wind/WAVES from 2013 August 19 at 21:00 UT to 2013 August 20 at 04:00 UT. Both S/WAVES present coronal–IP type II radio emission, with fp and 2fp clearly present from ∼22:28 to ∼04:00 UT. Groups of (probably SA) type III bursts can be seen emerging from the type II, from ∼22:28 UT (labelled with an orange ‘1’) to ∼00:00 UT (orange ‘3’). Both type II and type III bursts are time related with the CME ejecting from AR6 (details given in main text). The orange number 2 indicates where fp and 2fp could possibly be further broken down into more bands. S/WAVES-A and Wind/WAVES present flare-related type III bursts at different times (green letters a to e), caused by the activity in AR2, AR3, and AR5, and S/WAVES-B observes some of these flare-related type III bursts lower in frequency, due to occultation (Table 3). Credit: Observatoire de Paris-Meudon.