Table 1.
Flares with QPPs used in this study.
| Flare no. | Flare peak time (UT) | GOES class | QPP start time (UT) | QPP end time (UT) | Instrument | Period (s) |
|---|---|---|---|---|---|---|
| 008 | 2014-09-23 23:16:54 | M2.3 | 23:08:20 | 23:13:52 | GOES 0.5–4 Å |  |
| 010 | 2014-09-24 17:50:11 | C7.0 | 17:49:04 | 17:50:18 | GOES 1–8 Å |  |
| 010 | 2014-09-24 17:50:11 | C7.0 | 17:49:01 | 17:49:50 | DRGE |  |
| 049 | 2014-10-20 09:11:50 | M3.9 | 09:05:45 | 09:08:14 | GOES 0.5–4 Å |  |
| 052 | 2014-10-20 14:43:38 | C3.1 | 14:41:47 | 14:43:33 | GOES 1–8 Å |  |
| 054 | 2014-10-20 16:37:55 | M4.5 | 16:23:02 | 16:31:20 | GOES 1–8 Å |  |
| 056 | 2014-10-20 19:02:46 | M1.4 | 18:57:51 | 18:59:01 | GBM 25–50 keV |  |
| 058 | 2014-10-20 22:55:58 | M1.2 | 22:45:18 | 22:49:46 | GOES 0.5–4 Å |  |
| 068 | 2014-10-22 01:58:33 | M8.7 | 01:43:04 | 01:46:36 | GOES 0.5–4 Å |  |
| 072 | 2014-10-22 14:28:15 | X1.6 | 14:06:56 | 14:09:30 | GOES 1–8 Å |  |
| 072 | 2014-10-22 14:28:15 | X1.6 | 14:15:24 | 14:23:40 | GOES 0.5–4 Å |  |
| 079 | 2014-10-24 02:43:57 | C4.2 | 02:38:30 | 02:41:20 | NoRH |  |
| 081 | 2014-10-24 04:00:08 | C3.6 | 03:59:30 | 04:01:00 | NoRH |  |
| 085 | 2014-10-24 21:40:30 | X3.1 | 21:19:38 | 21:23:47 | GOES 0.5–4 Å |  |
| 092 | 2014-10-25 17:08:20 | X1.0 | 17:02:11 | 17:10:10 | GOES 0.5–4 Å |  |
| 098 | 2014-10-26 10:56:40 | X2.0 | 10:48:52 | 10:50:34 | GBM 25–50 keV |  |
| 104 | 2014-10-26 18:15:29 | M4.2 | 18:11:18 | 18:15:24 | GOES 0.5–4 Å |  |
| 105 | 2014-10-26 18:49:30 | M1.9 | 18:45:04 | 18:48:02 | GOES 1–8 Å |  |
| 106 | 2014-10-26 20:21:44 | M2.4 | 20:03:42 | 20:11:18 | GOES 0.5–4 Å |  |
| 117 | 2014-10-27 17:40:38 | M1.4 | 17:36:36 | 17:37:26 | GOES 1–8 Å |  |
| 161 | 2014-11-16 17:48:23 | M5.7 | 17:42:46 | 17:45:24 | GOES 0.5–4 Å |  |
| 177 | 2014-11-22 06:03:33 | C6.5 | 06:02:16 | 06:04:48 | GOES 0.5–4 Å |  |
Notes. The first column contains a numerical label for the flares (originally defined in Pugh et al. 2017b), the second column shows the time of the peak intensity of the flare in the GOES 1–8 Å waveband, the third column gives the GOES class, the fourth and fifth columns give the start and end times of the section of the flare where the QPP signal is most clearly visible in the power spectrum, the sixth column reports the instrument used to observe the QPP signal, and the seventh column lists the QPP period.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.