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Table A.3.

Type-III radio bursts and their properties (cf. Fig. 8, 9, 10). Radio bursts with fluxes above 10 SFU are highlighted in bold. The radio source position is noted with respect to the position of the AR, when the sources are projected to the solar surface from the LOFAR perspective. The propagation direction is in the same way the apparent movement on the solar disk with 0° as north, 180° as south, 90° as west and 270° as east.

Burst Phase Time UT Frequency Radio Radio source Propagation direction
at 70 MHz range [MHz] flux [SFU] position [50 MHz] [degree]
R10 pre-flare 08:32:30 80 - 40 .3 N 340
R20 pre-flare 08:34:49 80 - 35 .8 S 315 / 275 for 50 MHz
R30 pre-flare 08:35:28 80 - 32 2 N 315

R40 pre-flare 08:38:35 85 - 55 13 W LOS
R501 pre-flare 08:38:38 85 - 65 .6 W 315
R502 pre-flare 08:38:59 85 - 55 10 W 315
R503 pre-flare 08:39:07 85 - 48 25 W 330
R504 pre-flare 08:39:13 85 - 55 3 NW 315
R505 pre-flare 08:39:18 85 - 55 25 NW LOS / 290 for 50 MHz
R506 pre-flare 08:39:45 85 - 55 6 W 315
R507 pre-flare/first 08:40:13 85 - 50 3 W 315

R21 first 08:40:49 80 - 40 .6 W 270

R52 second 08:45:09 83 - 63 30 NW 315 / 0 for 40 MHz
65 - 38

R1g1 gradual 08:51:32 85 - 30 20 SE 355
R1g2 gradual 08:54:50 85 - 30 0.6 SE 30
R6g gradual 08:59:48 80 - 30 .4 LOS 330 / 80 for 80 MHz
R7g1 gradual 08:59:50 80 - 23 .3 LOS 325
R7g2 gradual 09:01:18 80 - 33 .4 SE 330

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