| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.54 | 48.90 | 5.70 | 26.31 | 4.66 | 157.62 | -22.89 | 82.03 | 0.3931 | 44.6 | 68.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.45 | 0.00 | 2.36 | 4.06 | 159.90 | -20.60 | 82.98 | 0.3552 | -1250.0 | -1011.3 | |
| 0.69 | 1.80 | 0.36 | 0.95 | 4.29 | 159.67 | -20.83 | 82.40 | 0.3594 | -882.9 | -705.8 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 4.23 | 159.45 | -21.05 | 82.63 | 0.3628 | -551.0 | -524.2 | |
| 0.00 | 1.46 | 0.00 | 0.77 | 4.08 | 159.20 | -21.30 | 83.12 | 0.3666 | -988.0 | -883.1 | |
| 0.00 | 1.80 | 0.00 | 0.96 | 4.40 | 159.00 | -21.50 | 82.30 | 0.3704 | -561.0 | -423.7 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 3.96 | 158.85 | -21.65 | 83.54 | 0.3721 | -708.0 | -412.6 | |
| 1.71 | 6.25 | 0.92 | 3.34 | 4.96 | 158.60 | -21.91 | 80.94 | 0.3780 | -858.6 | -260.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 3.48 | 158.48 | -22.02 | 84.90 | 0.3774 | -659.0 | -506.0 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 5.14 | 158.18 | -22.33 | 80.64 | 0.3852 | -593.0 | -345.7 | |
| 0.00 | 3.43 | 0.00 | 1.84 | 4.51 | 158.04 | -22.47 | 82.30 | 0.3861 | 931.0 | 791.5 | |
| 1.37 | 2.57 | 0.74 | 1.38 | 5.19 | 157.76 | -22.75 | 80.65 | 0.3920 | -701.6 | -454.3 | |
| 4.54 | 9.76 | 2.46 | 5.29 | 5.63 | 156.70 | -23.80 | 79.95 | 0.4097 | 1019.2 | 570.5 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 5.06 | 156.73 | -23.78 | 81.32 | 0.4081 | 880.0 | 815.1 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 5.00 | 156.57 | -23.94 | 81.51 | 0.4105 | 692.0 | 560.8 | |
| 0.00 | 3.68 | 0.00 | 2.00 | 3.96 | 156.18 | -24.33 | 84.13 | 0.4149 | 1015.0 | 787.1 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 4.04 | 155.82 | -24.69 | 84.00 | 0.4208 | 959.0 | 741.9 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 4.22 | 155.71 | -24.79 | 83.60 | 0.4226 | 578.0 | 577.0 | |
| 2.23 | 4.71 | 1.22 | 2.57 | 4.13 | 155.55 | -24.95 | 83.85 | 0.4250 | 931.5 | 670.0 | |
| 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. | |