Notes. t_{_LW} is the approximate observation time of the Langmuir waves associated to the Type III bursts, given with the spacecraft (s/c) that recorded these Langmuir waves. The frequency at which each event was analysed for the purposes of examining the decay and rise times as a function of the observer’s location is given for each of the four spacecraft (f_{_PSP}, f_{_SOLO}, f_{_STA}, and f_{_WIND}). (...) indicates the lack of observation or lack of fitting output (due to a faint signal).