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Table 1.

Coronal dimming and flare ribbon properties of the on-disc coronal dimmings from AR 13664.

N Day Start Flare FP Aϕ ϕ Arbn ϕrbn vCME Dimming
Location W m−2 1010 km2 1021 Mx 108 km2 1021 Mx (km s−1) Expansion
1 5 14:33 S20 E16 7.54E–06 0.78 ± 0.11 2.81 ± 0.48 0.62 ± 0.23 0.47 ± 0.12 623 South, north
2 5 18:34 S17 E21 1.07E–05 0.64 ± 0.09 2.77 ± 0.29 0.88 ± 0.35 0.47 ± 0.11 ... South
3 7 00:41 S18 E6 2.67E–05 0.75 ± 0.10 4.15 ± 0.51 1.23 ± 1.43 0.61 ± 0.25 484 South-east
4 7 11:40 S19 E0 2.49E–05 0.54 ± 0.09 4.25 ± 0.98 2.89 ± 0.94 1.94 ± 0.40 445 South
5 8 03:19 S18 W6 1.91E–05 0.82 ± 0.14 4.49 ± 0.67 1.53 ± 0.92 1.08 ± 0.39 812 South
6† 8 04:37 S19 W7 1.04E–04 1.46 ± 0.17 7.37 ± 0.86 8.95 ± 2.39 6.78 ± 1.27 1103 South
7† 8 11:13 S17 W8 8.60E–05 0.88 ± 0.11 4.91 ± 0.73 3.32 ± 1.30 1.91 ± 0.62 1321 South-east
8 8 19:15 S19 W19 2.08E–05 0.76 ± 0.12 10.14 ± 1.47 1.15 ± 0.73 0.78 ± 0.42 ... South
9† 8 21:12 S19 W21 1.00E–04 1.28 ± 0.20 13.11 ± 1.53 6.77 ± 4.23 4.00 ± 2.70 1304 South, north
10 9 06:03 S19 W23 2.35E–05 0.34 ± 0.05 2.84 ± 0.49 2.94 ± 1.08 2.23 ± 0.46 ... North, south
11† 9 08:45 S19 W22 2.24E–04 1.03 ± 0.15 8.55 ± 1.02 18.47 ± 4.50 12.59 ± 2.51 1963 South
12 9 11:50 S16 W33 3.15E–05 0.56 ± 0.10 3.31 ± 0.95 8.74 ± 2.07 4.10 ± 0.89 1036 South
13† 9 17:23 S16 W27 1.12E–04 1.65 ± 0.22 8.27 ± 2.13 10.20 ± 2.21 6.41 ± 1.15 1454 North, south
14† 10 06:27 S16 W33 3.95E–04 2.07 ± 0.25 6.83 ± 1.48 15.55 ± 3.21 11.11 ± 1.72 1249 North, south
15† 11 01:10 S16 W43 5.88E–04 3.08 ± 0.33 8.88 ± 1.17 24.24 ± 3.96 15.32 ± 2.10 1982 North, south
16 11 14:46 S14 W48 8.93E–05 1.21 ± 0.17 7.65 ± 2.46 15.18 ± 4.34 7.77 ± 1.63 1058 North

Notes. We list the day, start time, location, and peak SXR flux of the associated flare derived from the GOES flare catalogue. We list the magnetic dimming area (Aϕ), the total unsigned magnetic flux of the dimming (ϕ), the flare ribbon area (Arbn), and the flare ribbon flux (ϕrbn). In the ‘Dimming Expansion’ column we list the dimming expansion direction as described in Sect. 4.2. We list the maximum velocity of the associated CME (vCME) as given in Razquin et al. (2025). Events marked with a (†) are associated with a halo CME.

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