| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.89 | 198.59 | 18.96 | 99.32 | 6.22 | 204.25 | -7.30 | 70.31 | 0.1347 | -385.5 | -340.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.54 | 4.44 | 206.17 | -5.38 | 82.35 | 0.0947 | -913.0 | -688.8 | |
| 0.45 | 2.91 | 0.23 | 1.45 | 7.10 | 205.81 | -5.74 | 59.35 | 0.1159 | -1168.8 | -856.4 | |
| 24.62 | 156.26 | 12.29 | 77.99 | 6.18 | 205.02 | -6.53 | 69.23 | 0.1215 | -1433.3 | -429.3 | |
| 1.82 | -3.00 | 0.91 | -3.00 | 6.48 | 205.01 | -6.54 | 66.91 | 0.1235 | -1054.6 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 9.44 | 204.69 | -6.86 | 49.73 | 0.1551 | -809.0 | -675.5 | |
| 0.00 | 2.45 | 0.00 | 1.23 | 6.49 | 202.78 | -8.76 | 72.14 | 0.1598 | -1003.0 | -753.0 | |
| 0.91 | 3.54 | 0.46 | 1.78 | 6.95 | 202.59 | -8.96 | 69.83 | 0.1654 | -1142.9 | -857.9 | |
| 0.00 | 2.91 | 0.00 | 1.46 | 5.39 | 202.34 | -9.21 | 79.46 | 0.1629 | -929.0 | -796.1 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 7.37 | 202.02 | -9.53 | 68.63 | 0.1770 | -834.0 | -683.4 | |
| 0.55 | 3.54 | 0.27 | 1.78 | 6.15 | 201.52 | -10.03 | 76.07 | 0.1793 | 1090.2 | 836.0 | |
| 9.54 | 14.81 | 4.80 | 7.45 | 5.51 | 201.46 | -10.08 | 79.66 | 0.1779 | 1191.9 | 671.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 5.53 | 198.68 | -12.86 | 81.55 | 0.2250 | 866.0 | 753.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 8.21 | 198.14 | -13.41 | 70.85 | 0.2441 | 874.0 | 654.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 6.23 | 197.91 | -13.64 | 79.09 | 0.2397 | 881.0 | 702.7 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 5.70 | 197.42 | -14.13 | 81.54 | 0.2467 | 745.0 | 645.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 8.41 | 196.64 | -14.91 | 71.84 | 0.2691 | 884.0 | 729.6 | |
| 0.00 | 1.64 | 0.00 | 0.84 | 7.06 | 196.46 | -15.09 | 76.90 | 0.2664 | 900.0 | 732.4 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 7.06 | 196.30 | -15.24 | 77.03 | 0.2690 | 821.0 | 712.9 | |
| 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. | |