| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 48 | 310 | 26 | 172 | 14.87 | 4.10 | -17.66 | 40.67 | 0.4516 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 1 | 0 | 1 | 14.11 | 7.80 | -13.97 | 35.36 | 0.4063 | |
| 0 | 3 | 0 | 2 | 15.13 | 6.23 | -15.54 | 36.78 | 0.4339 | |
| 0 | 1 | 0 | 1 | 16.20 | 5.50 | -16.27 | 36.53 | 0.4540 | |
| 0 | 0 | 0 | 0 | 14.81 | 5.34 | -16.43 | 38.78 | 0.4385 | |
| 2 | 112 | 1 | 61 | 14.46 | 5.54 | -16.22 | 38.93 | 0.4322 | |
| 7 | -5 | 4 | -5 | 14.08 | 5.41 | -16.35 | 39.73 | 0.4290 | |
| 0 | 1 | 0 | 0 | 15.23 | 4.53 | -17.25 | 39.50 | 0.4516 | |
| 7 | 154 | 4 | 86 | 16.05 | 3.95 | -17.81 | 39.22 | 0.4667 | |
| 3 | -5 | 1 | -5 | 13.74 | 5.23 | -16.53 | 40.57 | 0.4267 | |
| 0 | 6 | 0 | 3 | 14.74 | 4.52 | -17.25 | 40.24 | 0.4458 | |
| 3 | -8 | 2 | -8 | 15.43 | 3.85 | -17.91 | 40.28 | 0.4605 | |
| 2 | -8 | 1 | -8 | 15.57 | 3.68 | -18.09 | 40.34 | 0.4640 | |
| 1 | -8 | 1 | -8 | 15.17 | 3.60 | -18.15 | 41.03 | 0.4600 | |
| 5 | -8 | 3 | -8 | 15.72 | 3.07 | -18.69 | 41.05 | 0.4716 | |
| 3 | -8 | 2 | -8 | 15.09 | 3.44 | -18.32 | 41.41 | 0.4607 | |
| 0 | 2 | 0 | 1 | 14.26 | 3.84 | -17.94 | 42.07 | 0.4473 | |
| 6 | -8 | 3 | -8 | 15.38 | 3.07 | -18.69 | 41.54 | 0.4678 | |
| 5 | -8 | 3 | -8 | 15.72 | 2.79 | -18.98 | 41.48 | 0.4746 | |
| 0 | 1 | 0 | 0 | 14.41 | 3.19 | -18.57 | 42.82 | 0.4557 | |
| 0 | 1 | 0 | 1 | 15.30 | 2.60 | -19.18 | 42.38 | 0.4719 | |
| 1 | -8 | 0 | -8 | 15.57 | 2.45 | -19.31 | 42.18 | 0.4763 | |
| 1 | 11 | 0 | 6 | 14.75 | 2.68 | -19.08 | 43.07 | 0.4648 | |
| 0 | 1 | 0 | 0 | 13.43 | 3.24 | -18.53 | 44.31 | 0.4444 | |
| 0 | 3 | 0 | 2 | 14.51 | 2.49 | -19.27 | 43.71 | 0.4642 | |
| 2 | 12 | 1 | 7 | 13.76 | 2.85 | -18.91 | 44.36 | 0.4522 | |
| 0 | 0 | 0 | 0 | 12.12 | 359.88 | -21.90 | 51.20 | 0.4698 | |
| 0 | 1 | 0 | 1 | 9.59 | 0.54 | -21.23 | 54.88 | 0.4383 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |