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Table 1.

Characteristics of the studied type III radio bursts observed during the second PSP perihelion. These characteristics include the observed peak time by Wind (708 kHz), STEREO-A (725 kHz), and PSP (721.875 kHz) spacecraft; observed complexity in the time profile; and information about the associated coronal phenomena.

Event No. Date Observed peak time (UT) Associated Complexity of time profile PSP heliospheric
April 2019 Wind STA PSP phenomena Wind STA PSP distance (AU)
1 02 15:46 15:45 15:36 Jet N Y Y 0.184171
2 03 17:00 16:59 16:43 Jet N N Y 0.171613
3 03 19:00 18:59 18:43 Jet N Y Y 0.170892
4 03 22:34 22:33 22:26 Jet N N Y 0.169674
5 04 22:22 22:21 22:14 Jet N N Y 0.165906
6 05 01:24 01:23 01:22 Jet Y Y Y 0.165952
7 05 01:30 01:29 01:24 Jet Y Y Y 0.165953
8 05 17:06 17:05 16:58 Jet Y Y Y 0.168071
9 05 17:17 17:16 17:09 Jet Y Y Y 0.168113
10 05 20:08 20:07 20:01 Jet Y Y Y 0.168842
11 05 20:11 20:10 20:05 Jet Y Y Y 0.168883

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