Table A.2
List of flares with a peak above the 95% confidence level in the power spectrum.
Flare no. | Start time | End time | Instrument | Method | Period (s) | References |
|
||||||
008* | 2014-09-23 23:08:20 | 2014-09-23 23:13:52 | GOES 0.5–4 Å | Regular |
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|
010* | 2014-09-24 17:49:04 | 2014-09-24 17:50:18 | GOES 1–8 Å | Rebinned (2) |
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2 |
010* | 2014-09-24 17:49:01 | 2014-09-24 17:49:50 | Vernov | Rebinned (2) |
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2 |
022 | 2014-10-17 05:23:18 | 2014-10-17 05:26:35 | NoRH | Rebinned (3) |
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|
024 | 2014-10-17 15:35:30 | 2014-10-17 15:37:54 | GOES 1–8 Å | Rebinned (2) |
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|
027 | 2014-10-18 01:04:10 | 2014-10-18 01:08:30 | NoRH | Rebinned (3) |
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|
029 | 2014-10-18 07:36:14 | 2014-10-18 07:48:48 | GOES 1–8 Å | Regular |
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1 |
030 | 2014-10-18 13:14:38 | 2014-10-18 13:15:52 | GOES 0.5–4 Å | Regular |
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|
035 | 2014-10-18 19:02:30 | 2014-10-18 19:06:58 | GOES 1–8 Å | Regular |
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2 |
037 | 2014-10-19 01:35:00 | 2014-10-19 01:43:00 | GOES 0.5–4 Å | Regular |
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|
037 | 2014-10-19 01:36:28 | 2014-10-19 01:42:42 | NoRH | Regular |
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|
038 | 2014-10-19 04:20:24 | 2014-10-19 04:24:56 | GOES 1–8 Å | Regular |
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|
038 | 2014-10-19 04:20:24 | 2014-10-19 04:24:56 | GOES 0.5–4 Å | Regular |
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|
038 | 2014-10-19 04:41:39 | 2014-10-19 04:50:00 | GOES 0.5–4 Å | Regular |
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|
049* | 2014-10-20 09:05:45 | 2014-10-20 09:08:14 | GOES 0.5–4 Å | Rebinned (3) |
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1 |
052* | 2014-10-20 14:41:47 | 2014-10-20 14:43:33 | GOES 1–8 Å | Regular |
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|
054* | 2014-10-20 16:23:02 | 2014-10-20 16:31:20 | GOES 1–8 Å | Regular |
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|
056* | 2014-10-20 18:57:51 | 2014-10-20 18:59:01 | Fermi 25–50 keV | Rebinned (3) |
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1, 2 |
056* | 2014-10-20 18:57:53 | 2014-10-20 18:59:02 | Vernov | Regular |
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1, 2 |
058* | 2014-10-20 22:45:18 | 2014-10-20 22:49:46 | GOES 1–8 Å | Rebinned (2) |
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1, 3 |
058* | 2014-10-20 22:45:18 | 2014-10-20 22:49:46 | GOES 0.5–4 Å | Rebinned (2) |
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1, 3 |
068* | 2014-10-22 01:43:04 | 2014-10-22 01:46:36 | GOES 1–8 Å | Regular |
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|
068* | 2014-10-22 01:43:04 | 2014-10-22 01:46:36 | GOES 0.5–4 Å | Regular |
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|
072* | 2014-10-22 14:06:55 | 2014-10-22 14:12:02 | Fermi 50–100 keV | Regular |
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5 |
072* | 2014-10-22 14:06:56 | 2014-10-22 14:09:30 | GOES 1–8 Å | Regular |
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5 |
072* | 2014-10-22 14:15:24 | 2014-10-22 14:23:40 | GOES 0.5–4 Å | Regular |
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5 |
079* | 2014-10-24 02:38:30 | 2014-10-24 02:41:20 | NoRH | Rebinned (2) |
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|
081* | 2014-10-24 03:59:30 | 2014-10-24 04:01:00 | NoRH | Rebinned (3) |
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|
085* | 2014-10-24 21:19:38 | 2014-10-24 21:23:47 | GOES 0.5–4 Å | Regular |
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|
092* | 2014-10-25 17:02:11 | 2014-10-25 17:10:10 | GOES 1–8 Å | Regular |
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1 |
092* | 2014-10-25 17:02:11 | 2014-10-25 17:10:10 | GOES 0.5–4 Å | Regular |
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1 |
098* | 2014-10-26 10:48:52 | 2014-10-26 10:50:34 | Fermi 25–50 keV | Regular |
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|
104* | 2014-10-26 18:11:18 | 2014-10-26 18:15:24 | GOES 0.5–4 Å | Regular |
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1 |
104* | 2014-10-26 18:12:40 | 2014-10-26 18:15:28 | Fermi 25–50 keV | Regular |
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1 |
105* | 2014-10-26 18:45:04 | 2014-10-26 18:48:02 | GOES 1–8 Å | Regular |
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1 |
106* | 2014-10-26 20:03:42 | 2014-10-26 20:11:18 | GOES 1–8 Å | Rebinned (2) |
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1 |
106* | 2014-10-26 20:03:42 | 2014-10-26 20:11:18 | GOES 0.5–4 Å | Rebinned (2) |
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1 |
106* | 2014-10-26 20:03:38 | 2014-10-26 20:09:02 | Fermi 25–50 keV | Regular |
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1 |
117* | 2014-10-27 17:36:36 | 2014-10-27 17:37:26 | GOES 1–8 Å | Regular |
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1 |
129 | 2014-10-29 09:58:00 | 2014-10-29 10:01:45 | EVE | Rebinned (2) |
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1 |
135 | 2014-10-29 21:21:33 | 2014-10-29 21:22:19 | Fermi 25–50 keV | Rebinned (3) |
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1, 2 |
135 | 2014-10-29 21:21:28 | 2014-10-29 21:22:52 | Vernov | Rebinned (3) |
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1, 2 |
138 | 2014-10-29 23:44:16 | 2014-10-29 23:45:48 | NoRH | Regular |
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|
140 | 2014-10-30 01:28:38 | 2014-10-30 01:30:30 | GOES 1–8 Å | Rebinned (2) |
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1, 3 |
141 | 2014-10-30 04:22:08 | 2014-10-30 04:28:00 | GOES 1–8 Å | Regular |
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1 |
142 | 2014-10-30 05:44:27 | 2014-10-30 05:45:45 | GOES 1–8 Å | Regular |
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|
142 | 2014-10-30 05:44:27 | 2014-10-30 05:45:43 | NoRH | Regular |
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|
147 | 2014-11-13 06:04:59 | 2014-11-13 06:07:15 | NoRH | Regular |
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|
152 | 2014-11-15 11:56:08 | 2014-11-15 12:02:58 | GOES 1–8 Å | Regular |
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1 |
152 | 2014-11-15 11:56:08 | 2014-11-15 12:02:58 | GOES 0.5–4 Å | Regular |
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1 |
152 | 2014-11-15 11:56:08 | 2014-11-15 12:02:58 | EVE | Regular |
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1 |
153 | 2014-11-15 20:42:57 | 2014-11-15 20:44:28 | GOES 0.5–4 Å | Rebinned (2) |
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1 |
161* | 2014-11-16 17:42:46 | 2014-11-16 17:45:24 | GOES 0.5–4 Å | Regular |
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|
177* | 2014-11-22 06:02:16 | 2014-11-22 06:04:48 | GOES 1–8 Å | Regular |
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|
177* | 2014-11-22 06:02:16 | 2014-11-22 06:04:48 | GOES 0.5–4 Å | Regular |
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Notes. The first column contains a numerical label for the flares (see also Table A.1), the second and third columns give the start and end times of the section of the flare where the QPP signal is most visible in the power spectrum, the fourth column is the instrument used, the fifth column is the type of power spectrum in which the signal was detected (the numbers for the rebinned power spectra refer to the number of frequency bins that were summed over, see Sect. 3), the sixth column is the QPP period, and finally the seventh column references other studies that find pulsations in the flare. Flare numbers marked with an asterisk indicate those that occurred while the active region was far enough away from the solar limb so that active region properties could be determined.
Reference. (1) Inglis et al. (2016); (2) Myagkova et al. (2016); (3) Cho et al. (2016); (5) Kuznetsov et al. (2016).
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