| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.44 | 0.00 | 13.37 | 7.47 | 134.04 | 20.12 | 306.23 | 0.4240 | 342.4 | 345.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.47 | 0.00 | 0.84 | 5.11 | 141.14 | 27.22 | 293.67 | 0.4994 | -803.0 | -644.2 | |
| 0.00 | 1.81 | 0.00 | 1.02 | 4.35 | 139.50 | 25.59 | 293.62 | 0.4719 | -818.0 | -684.4 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 7.36 | 136.40 | 22.49 | 302.57 | 0.4520 | 788.0 | 580.3 | |
| 0.00 | 1.55 | 0.00 | 0.86 | 8.53 | 135.79 | 21.87 | 305.47 | 0.4543 | -885.0 | -686.6 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 8.45 | 135.46 | 21.55 | 305.75 | 0.4495 | -823.0 | -719.6 | |
| 0.00 | 2.59 | 0.00 | 1.41 | 6.98 | 134.23 | 20.31 | 304.60 | 0.4203 | 799.0 | 674.6 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 8.05 | 133.96 | 20.04 | 307.01 | 0.4268 | 551.0 | 521.0 | |
| 0.00 | 2.33 | 0.00 | 1.27 | 8.08 | 133.42 | 19.50 | 307.85 | 0.4204 | 1063.0 | 853.0 | |
| 0.00 | 2.42 | 0.00 | 1.32 | 8.27 | 133.34 | 19.42 | 308.32 | 0.4211 | 848.0 | 752.2 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 8.20 | 133.14 | 19.22 | 308.47 | 0.4180 | 1023.0 | 925.4 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 8.67 | 131.14 | 17.22 | 312.51 | 0.3988 | 704.0 | 599.2 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 8.01 | 130.73 | 16.81 | 311.94 | 0.3868 | 596.0 | 451.0 | |
| 0.00 | 2.25 | 0.00 | 1.21 | 8.19 | 130.68 | 16.76 | 312.39 | 0.3881 | 978.0 | 739.2 | |
| 0.00 | 2.94 | 0.00 | 1.57 | 7.26 | 130.48 | 16.56 | 310.90 | 0.3758 | 772.0 | 694.8 | |
| 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. | |