| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.34 | 0.00 | 9.37 | -20.42 | 78.29 | -16.85 | 147.78 | 0.4948 | 541.4 | 494.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.82 | 0.00 | 0.96 | -15.00 | 86.29 | -8.86 | 155.48 | 0.3601 | 814.0 | 750.7 | |
| 0.00 | 2.08 | 0.00 | 1.13 | -17.94 | 84.30 | -10.84 | 154.42 | 0.4163 | 895.0 | 721.5 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -20.65 | 82.72 | -12.43 | 154.22 | 0.4650 | 681.0 | 493.6 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -20.85 | 82.61 | -12.54 | 154.22 | 0.4685 | 626.0 | 567.9 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -17.14 | 82.35 | -12.80 | 149.57 | 0.4198 | 874.0 | 657.7 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -20.05 | 79.93 | -15.21 | 148.77 | 0.4775 | 831.0 | 767.5 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -20.36 | 78.85 | -16.30 | 147.39 | 0.4903 | 666.0 | 521.8 | |
| 0.00 | 1.47 | 0.00 | 0.84 | -20.24 | 76.93 | -18.21 | 144.34 | 0.5050 | 379.0 | 447.3 | |
| 0.00 | 1.30 | 0.00 | 0.76 | -22.79 | 76.46 | -18.69 | 146.64 | 0.5393 | 356.0 | 401.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -20.62 | 75.85 | -19.30 | 143.25 | 0.5192 | 648.0 | 487.9 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -20.10 | 75.75 | -19.40 | 142.47 | 0.5141 | 417.0 | 426.6 | |
| 0.00 | 1.12 | 0.00 | 0.67 | -22.21 | 73.25 | -21.90 | 141.77 | 0.5601 | 284.0 | 316.6 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -25.57 | 68.83 | -26.32 | 140.67 | 0.6334 | 633.0 | 576.0 | |
| 0.00 | 0.86 | 0.00 | 0.60 | -28.33 | 63.18 | -31.97 | 138.49 | 0.7056 | -524.0 | -414.1 | |
| 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. | |