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Table 1.

Stationary type IV bursts (STIVB) and associated phenomena.

Date CME Flare Flare AR EUV loop STIVB Average Average
1st image onset peak location arcade onset polarisation log(TB)
[UT] [UT] [UT] [UT] [UT]
(1) (2) (3) (4) (5) (6) (7) (8) (9)
2000 Jul 14 10:54 10:03 10:24 N17 W11 10:28/10:38 HF: 10:26 164 MHz: 86%±8% 8.19 ± 0.13
(X5.7) LF: 10:38 237 MHz: 76%±7% 7.77 ± 0.21
327 MHz: 60%±7% 7.78 ± 0.41
432 MHz: 90%±3% 7.98 ± 0.41

2001 Oct 09 11:30 10:46 11:13 S30 E05 11:00/11:12 HF: 10:53 164 MHz: 67%±4% 8.41 ± 0.25
(M1.4) LF: 10:57 237 MHz: 82%±4% 8.17 ± 0.18
327 MHz: 46%±3% 7.88 ± 0.24
432 MHz: 77%±3% 7.65 ± 0.22

2007 May 19 13:24 12:50 13:02 N00 W05 12:49/12:52 HF: 12:49 151 MHz: 102%±6% 8.02 ± 0.06
(B9.5) LF: 13:03 237 MHz: 99%±2% 7.21 ± 0.06
327 MHz: 92%±3% 6.45 ± 0.06
432 MHz: 65%±9% 5.79 ± 0.09

2008 Apr 26 14:30 13:50 14:08 N10 E10 13:48/14:00 HF: 13:55 151 MHz: 84%±19% 5.98 ± 0.22
(B3.8) LF: 14:02 228 MHz: 57%±17% 5.64 ± 0.19
327 MHz: 24%±16% 5.53 ± 0.11
432 MHz: −6%±7% 5.59 ± 0.09

2010 Apr 03 10:34 08:50 10:00 S22 W29 09:48/10:00 HF: 09:50 151 MHz: 83%±12% 7.03 ± 0.11
(B7.4) (EIT) LF: < 10:05 237 MHz: 92%±7% 6.67 ± 0.10
09:54/10:14 327 MHz: 87%±19% 6.43 ± 0.13
(SWAP) 432 MHz: 88%±20% 6.59 ± 0.09

2012 Mar 04 11:00 10:29 10:52 N18 E54 10:32/10:48 HF: 10:38 151 MHz: 39%±24% 7.80 ± 0.35
(M2.0) LF: 10:50 228 MHz: 51%±20% 8.51 ± 0.33
327 MHz: 50%±14% 9.15 ± 0.46
432 MHz: 53%±15% 9.15 ± 0.50

2012 Jun 14 14:12 13:20 14:30 S17 W00 13:44/13:52 HF: 14:06 Eastern source (V <  0):
(M1.9) LF: 14:32 151 MHz: 71%±6% 9.24 ± 0.17
228 MHz: 88%±7% 9.06 ± 0.07
327 MHz: 78%±8% 8.74 ± 0.15
432 MHz: 64%±25% 8.49 ± 0.27
Western source (V >  0):
432 MHz: 96%±3% 8.45 ± 0.11

Notes. Contents: date (Col. 1), time of the first observation of the CME by the LASCO coronagraph (Col. 2), flare onset time and the flare class (GOES; Col. 3), flare peak (Col. 4), active region location (Col. 5), first appearance of the loop arcade in EUV images (Col. 6), stationary type IV burst (STIVB) onset (Col. 7), average of polarisation degree (Col. 8) and the logarithm of the brightness temperature (Col. 9) of the STIVB at different frequencies.

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