| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.17 | 21.97 | 1.28 | 12.85 | -18.44 | 239.62 | 20.88 | 219.47 | 0.5332 | 174.1 | 105.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 1.03 | -16.86 | 244.01 | 25.27 | 227.10 | 0.5598 | 754.0 | 538.5 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -17.00 | 243.44 | 24.69 | 226.26 | 0.5550 | 661.0 | 519.4 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -17.68 | 242.48 | 23.74 | 224.24 | 0.5519 | 800.0 | 663.2 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -17.17 | 242.14 | 23.39 | 224.50 | 0.5432 | 717.0 | 647.8 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -17.97 | 242.25 | 23.50 | 223.57 | 0.5524 | 591.0 | 485.6 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -18.03 | 242.04 | 23.30 | 223.25 | 0.5510 | 599.0 | 480.2 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -21.23 | 241.23 | 22.48 | 218.34 | 0.5768 | 418.0 | 363.7 | |
| 2.17 | 3.80 | 1.28 | 2.24 | -19.16 | 240.29 | 21.54 | 219.63 | 0.5459 | 923.0 | 749.1 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -18.26 | 238.76 | 20.02 | 218.72 | 0.5217 | 778.0 | 555.3 | |
| 0.00 | 2.08 | 0.00 | 1.21 | -20.08 | 237.14 | 18.40 | 214.26 | 0.5286 | -840.0 | -623.0 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -18.72 | 236.95 | 18.20 | 215.56 | 0.5108 | -170.0 | -259.7 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -18.48 | 236.82 | 18.08 | 215.66 | 0.5068 | -615.0 | -528.4 | |
| 0.00 | 2.17 | 0.00 | 1.23 | -17.40 | 236.17 | 17.43 | 216.01 | 0.4880 | -774.0 | -601.0 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -19.77 | 236.12 | 17.37 | 213.11 | 0.5164 | -714.0 | -565.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -18.45 | 233.71 | 14.96 | 210.78 | 0.4805 | -726.0 | -603.6 | |
| 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. | |