| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.50 | 26.60 | 0.81 | 14.14 | -9.20 | 9.20 | 20.92 | 259.98 | 0.3616 | 345.5 | 341.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.48 | -8.21 | 11.85 | 23.57 | 263.45 | 0.4001 | 669.0 | 577.7 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -8.16 | 11.68 | 23.40 | 263.56 | 0.3974 | 690.0 | 534.8 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -8.65 | 11.51 | 23.24 | 262.30 | 0.3953 | 691.0 | 588.9 | |
| 0.00 | 2.29 | 0.00 | 1.23 | -8.20 | 11.39 | 23.11 | 263.41 | 0.3927 | 729.0 | 658.7 | |
| 1.50 | 4.05 | 0.81 | 2.18 | -8.48 | 11.24 | 22.96 | 262.68 | 0.3907 | 1038.1 | 859.1 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -8.85 | 10.90 | 22.62 | 261.64 | 0.3858 | 863.0 | 699.6 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -8.71 | 10.69 | 22.42 | 261.96 | 0.3823 | 884.0 | 684.2 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -9.08 | 10.55 | 22.27 | 260.96 | 0.3806 | 891.0 | 775.9 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -12.28 | 10.33 | 22.05 | 252.59 | 0.3862 | -656.0 | -526.2 | |
| 0.00 | 3.17 | 0.00 | 1.68 | -7.83 | 9.47 | 21.19 | 264.10 | 0.3615 | 734.0 | 601.7 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -10.52 | 9.08 | 20.80 | 256.53 | 0.3605 | 747.0 | 626.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -10.34 | 9.00 | 20.72 | 256.98 | 0.3588 | 770.0 | 614.8 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -1.95 | 8.29 | 20.01 | 280.96 | 0.3498 | -15.0 | -3.3 | |
| 0.00 | 1.67 | 0.00 | 0.89 | -14.55 | 7.20 | 18.92 | 244.14 | 0.3504 | -3.0 | -3.0 | |
| 0.00 | 2.29 | 0.00 | 1.19 | -7.49 | 6.20 | 17.92 | 264.56 | 0.3079 | -880.0 | -629.8 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -7.50 | 5.73 | 17.45 | 264.42 | 0.3000 | -871.0 | -659.9 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -8.37 | 4.78 | 16.50 | 261.16 | 0.2857 | -770.0 | -639.1 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -15.64 | 3.03 | 14.75 | 235.45 | 0.2991 | 840.0 | 640.9 | |
| 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 | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |