| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.05 | 213.96 | 21.33 | 113.90 | -11.71 | 178.72 | -11.43 | 148.11 | 0.3679 | 487.4 | 315.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.02 | 183.67 | 1.07 | 97.42 | -11.85 | 179.51 | -10.64 | 149.99 | 0.3628 | 853.7 | 436.2 | |
| 32.41 | -1.00 | 17.20 | -1.00 | -11.50 | 179.28 | -10.87 | 148.95 | 0.3600 | 1200.0 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -13.38 | 179.01 | -11.14 | 150.91 | 0.3884 | 692.0 | 492.0 | |
| 0.00 | 3.95 | 0.00 | 2.11 | -12.09 | 178.44 | -11.71 | 147.91 | 0.3752 | 576.0 | 635.7 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -12.41 | 177.14 | -13.01 | 145.60 | 0.3910 | -760.0 | -605.9 | |
| 0.00 | 2.64 | 0.00 | 1.42 | -12.51 | 176.82 | -13.33 | 145.10 | 0.3952 | -867.0 | -726.4 | |
| 1.84 | 4.39 | 1.00 | 2.37 | -12.71 | 176.59 | -13.57 | 144.93 | 0.3999 | -914.8 | -790.5 | |
| 0.00 | 3.51 | 0.00 | 1.94 | -14.25 | 174.10 | -16.06 | 142.55 | 0.4427 | -585.0 | -578.0 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -14.42 | 173.92 | -16.23 | 142.49 | 0.4464 | -650.0 | -561.4 | |
| 2.46 | 5.27 | 1.34 | 2.88 | -12.17 | 173.63 | -16.52 | 138.61 | 0.4223 | -941.4 | -772.2 | |
| 1.32 | 2.72 | 0.72 | 1.49 | -12.58 | 173.54 | -16.61 | 139.11 | 0.4281 | -1007.1 | -819.2 | |
| 0.00 | 1.67 | 0.00 | 0.92 | -13.23 | 173.30 | -16.85 | 139.70 | 0.4381 | -893.0 | -676.2 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -12.82 | 172.98 | -17.18 | 138.54 | 0.4368 | -619.0 | -497.6 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -12.41 | 172.23 | -17.92 | 136.68 | 0.4398 | -762.0 | -551.1 | |
| 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. | |