Table A.1
Sunspots used in this work.
Sunspot | Hemisphere | Start time | Duration (d, h, m) | Size (Mm × Mm) | Max. Amp. (°) |
(yyyy.mm.dd_hh:mm:ss UT) | |||||
|
|||||
11084 | South | 2010.06.26_21:00:00 | 11, 03, 00 | 43.8 × 40.0 | 0.48 |
11092 | North | 2010.07.28_18:00:00 | 11, 11, 48 | 52.9 × 52.9 | 0.37 |
11131 | North | 2010.12.02_10:36:00 | 11, 14, 00 | 61.9 × 61.9 | 0.58 |
11140 | North | 2010.12.31_10:00:00 | 11, 00, 00 | 58.9 × 58.9 | 0.52 |
11216 | South | 2011.05.16_04:24:00 | 11, 19, 24 | 41.5 × 41.5 | 0.39 |
11312 | North | 2011.10.04_15:00:00 | 12, 10, 24 | 55.1 × 55.1 | 0.58 |
11314 | North | 2011.10.11_15:00:00 | 07, 10, 48 | 65.7 × 65.7 | 1.01 |
11579 | North | 2012.09.25_09:48:00 | 09, 20, 36 | 42.3 × 42.3 | 0.69 |
11582 | South | 2012.09.27_07:24:00 | 10, 02, 24 | 46.1 × 46.1 | 0.66 |
11642 | South | 2013.01.01_03:00:00 | 09, 14, 24 | 40.0 × 40.0 | 0.56 |
11662 | North | 2013.01.23_23:24:00 | 09, 14, 12 | 54.4 × 47.6 | 1.03 |
11665 | North | 2013.01.29_07:00:00 | 10, 16, 48 | 43.8 × 43.8 | 0.86 |
11777 | South | 2013.06.20_14:00:00 | 09, 04, 00 | 45.3 × 45.3 | 0.79 |
11801 | North | 2013.07.23_13:36:00 | 09, 10, 12 | 38.5 × 38.5 | 0.84 |
11846 | South | 2013.09.17_02:00:00 | 11, 13, 00 | 49.8 × 49.8 | 1.05 |
11857 | South | 2013.10.02_10:00:00 | 09, 04, 48 | 38.5 × 27.5 | 0.97 |
11896 | North | 2013.11.10_22:00:00 | 11, 09, 36 | 43.8 × 43.8 | 0.78 |
11899 | North | 2013.01.13_09:00:00 | 10, 14, 48 | 69.5 × 66.1 | 0.59 |
11912 | South | 2013.12.02_12:00:00 | 11, 04, 48 | 43.0 × 38.5 | 0.43 |
12005 | North | 2014.03.12_13:00:00 | 11, 17, 48 | 50.6 × 50.6 | 0.77 |
12079 | North | 2014.06.01_12:00:00 | 08, 22, 48 | 30.9 × 30.9 | 0.39 |
12186 | South | 2014.10.07_18:36:00 | 11, 20, 12 | 48.3 × 55.9 | 0.53 |
12195 | North | 2014.10.24_02:00:00 | 08, 10, 48 | 84.2 × 84.6 | 0.85 |
12218 | North | 2014.11.24_22:00:00 | 10, 20, 24 | 43.8 × 43.8 | 0.48 |
12246 | North | 2014.12.22_08:00:00 | 11, 12, 00 | 41.5 × 26.4 | 0.54 |
Notes. The first column corresponds to the NOAA number of the active region associated with each sunspot. The second is the hemisphere where each sunspot was located. Third column is the time of the first frame used in our study. The time coverage (duration) is the fourth column, while the fifth column corresponds to the size of the field of view. Finally the last column represents the maximum oscillation amplitude, which was obtained by averaging the maximum amplitudes found with the circumference and the penumbral sector methods.
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