| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.41 | 172.50 | 13.87 | 87.39 | 6.32 | 204.28 | -11.67 | 76.58 | 0.2074 | -558.6 | -379.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.50 | 7.80 | 210.45 | -5.50 | 52.83 | 0.1197 | -759.0 | -563.3 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 6.11 | 207.84 | -8.11 | 73.01 | 0.1473 | -767.0 | -512.7 | |
| 0.82 | 4.45 | 0.41 | 2.24 | 7.07 | 205.68 | -10.27 | 71.29 | 0.1876 | -1160.2 | -898.0 | |
| 24.78 | 148.53 | 12.53 | 75.06 | 6.23 | 204.80 | -11.15 | 76.67 | 0.1985 | -1434.5 | -472.0 | |
| 0.82 | 2.00 | 0.42 | 1.02 | 7.15 | 202.20 | -13.75 | 75.25 | 0.2450 | -1000.9 | -825.4 | |
| 0.45 | 1.72 | 0.23 | 0.88 | 5.71 | 201.73 | -14.22 | 81.37 | 0.2483 | 833.2 | 706.4 | |
| 0.54 | 2.54 | 0.28 | 1.30 | 6.16 | 201.69 | -14.26 | 79.57 | 0.2502 | 964.0 | 809.6 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 5.76 | 199.19 | -16.76 | 82.31 | 0.2909 | 821.0 | 621.2 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 8.47 | 197.40 | -18.55 | 74.60 | 0.3277 | 777.0 | 650.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 6.12 | 197.28 | -18.67 | 81.83 | 0.3230 | 835.0 | 660.2 | |
| 0.00 | 2.00 | 0.00 | 1.05 | 8.89 | 196.70 | -19.25 | 73.89 | 0.3405 | 708.0 | 366.0 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 5.86 | 196.80 | -19.15 | 82.76 | 0.3304 | 692.0 | 540.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 6.20 | 196.66 | -19.29 | 81.80 | 0.3333 | 686.0 | 525.2 | |
| 0.00 | 1.91 | 0.00 | 1.01 | 6.95 | 196.14 | -19.81 | 79.79 | 0.3433 | 771.0 | 640.8 | |
| 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. | |