| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.18 | 0.00 | 12.47 | 12.87 | 93.85 | 11.92 | 304.86 | 0.2593 | 93.1 | -55.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.61 | 25.81 | 91.02 | 9.09 | 337.00 | 0.3655 | 675.0 | 534.5 | |
| 0.00 | 2.89 | 0.00 | 1.55 | 9.44 | 104.10 | 22.17 | 279.54 | 0.3791 | -1090.0 | -860.4 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 22.17 | 85.26 | 3.33 | 348.87 | 0.2799 | 842.0 | 641.2 | |
| 0.00 | 2.63 | 0.00 | 1.39 | 9.37 | 102.83 | 20.90 | 279.75 | 0.3587 | 688.0 | 521.8 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 19.73 | 86.87 | 4.94 | 340.78 | 0.2473 | 845.0 | 582.8 | |
| 0.00 | 2.37 | 0.00 | 1.23 | 10.34 | 99.11 | 17.19 | 284.48 | 0.3015 | -1074.0 | -860.4 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 9.36 | 99.02 | 17.09 | 281.31 | 0.2970 | -735.0 | -537.0 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 15.49 | 89.32 | 7.39 | 322.30 | 0.2036 | 756.0 | 654.5 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 16.67 | 87.52 | 5.59 | 332.65 | 0.2039 | 769.0 | 619.5 | |
| 0.00 | 2.10 | 0.00 | 1.08 | 8.35 | 97.62 | 15.69 | 278.42 | 0.2717 | -893.0 | -738.7 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 14.77 | 86.98 | 5.05 | 330.01 | 0.1710 | 634.0 | 545.1 | |
| 0.00 | 1.84 | 0.00 | 0.93 | 14.66 | 87.08 | 5.16 | 329.14 | 0.1703 | 902.0 | 677.3 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 14.31 | 87.10 | 5.17 | 327.96 | 0.1654 | 866.0 | 650.7 | |
| 0.00 | 1.93 | 0.00 | 0.96 | 9.92 | 86.60 | 4.67 | 308.24 | 0.1026 | -958.0 | -763.8 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 8.74 | 88.18 | 6.25 | 291.80 | 0.1164 | -831.0 | -603.5 | |
| 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. | |