| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.17 | 64.51 | 16.41 | 47.39 | 17.12 | 19.53 | 45.13 | 293.48 | 0.7401 | -379.8 | -255.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.27 | 0.00 | 0.23 | 21.17 | 25.07 | 50.67 | 296.54 | 0.8085 | -478.0 | -417.7 | |
| 7.15 | 13.93 | 5.44 | 10.60 | 16.95 | 21.56 | 47.16 | 292.50 | 0.7615 | -566.3 | -244.2 | |
| 0.00 | 5.79 | 0.00 | 4.37 | 17.08 | 21.09 | 46.69 | 292.82 | 0.7569 | -716.0 | -594.4 | |
| 4.89 | 23.43 | 3.66 | 17.49 | 16.69 | 20.83 | 46.43 | 292.42 | 0.7530 | -710.8 | -539.2 | |
| 5.34 | -4.00 | 3.97 | -4.00 | 16.69 | 20.41 | 46.01 | 292.56 | 0.7486 | -861.6 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.69 | 19.16 | 21.02 | 46.62 | 295.48 | 0.7628 | 187.0 | 223.1 | |
| 0.00 | 0.63 | 0.00 | 0.46 | 16.85 | 19.19 | 44.79 | 293.20 | 0.7358 | -562.0 | -479.0 | |
| 2.17 | 2.99 | 1.54 | 2.12 | 16.92 | 17.61 | 43.21 | 293.88 | 0.7187 | -697.0 | -640.6 | |
| 0.00 | 1.18 | 0.00 | 0.83 | 17.24 | 17.40 | 43.00 | 294.39 | 0.7175 | -607.0 | -487.9 | |
| 0.00 | 1.45 | 0.00 | 1.02 | 17.05 | 17.30 | 42.90 | 294.17 | 0.7157 | -694.0 | -636.3 | |
| 0.00 | 1.36 | 0.00 | 0.95 | 17.01 | 16.94 | 42.54 | 294.27 | 0.7115 | -797.0 | -651.1 | |
| 0.00 | 0.54 | 0.00 | 0.38 | 17.14 | 16.85 | 42.45 | 294.48 | 0.7110 | -609.0 | -519.7 | |
| 0.00 | 0.72 | 0.00 | 0.49 | 16.92 | 15.08 | 40.68 | 294.93 | 0.6900 | 478.0 | 405.0 | |
| 0.00 | 1.00 | 0.00 | 0.68 | 16.54 | 14.90 | 40.50 | 294.49 | 0.6864 | 617.0 | 504.1 | |
| 2.62 | 7.69 | 1.80 | 5.27 | 17.91 | 15.05 | 40.65 | 296.30 | 0.6938 | 719.1 | 612.2 | |
| 0.00 | 1.63 | 0.00 | 1.13 | 18.97 | 15.15 | 40.75 | 297.69 | 0.6994 | 692.0 | 591.9 | |
| 0.00 | 1.00 | 0.00 | 0.68 | 19.77 | 13.78 | 39.38 | 299.46 | 0.6880 | 582.0 | 495.5 | |
| 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. | |