| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.84 | 0.00 | 9.99 | -12.63 | 83.32 | -19.87 | 108.82 | 0.3509 | 279.8 | 311.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.93 | 0.00 | 0.98 | -12.56 | 90.98 | -12.21 | 117.19 | 0.2331 | 877.0 | 696.4 | |
| 0.00 | 1.93 | 0.00 | 0.99 | -11.34 | 89.38 | -13.81 | 110.09 | 0.2504 | 829.0 | 702.2 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -11.48 | 84.50 | -18.69 | 106.12 | 0.3284 | 799.0 | 703.5 | |
| 0.00 | 1.31 | 0.00 | 0.69 | -11.68 | 84.00 | -19.19 | 106.35 | 0.3370 | 998.0 | 884.0 | |
| 0.00 | 1.49 | 0.00 | 0.78 | -12.04 | 83.98 | -19.22 | 107.37 | 0.3388 | 725.0 | 578.7 | |
| 0.00 | 1.40 | 0.00 | 0.74 | -11.70 | 83.74 | -19.45 | 106.23 | 0.3411 | 633.0 | 561.9 | |
| 0.00 | 1.49 | 0.00 | 0.78 | -11.42 | 83.63 | -19.56 | 105.37 | 0.3419 | 765.0 | 711.6 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -11.28 | 83.19 | -20.01 | 104.72 | 0.3484 | 727.0 | 627.0 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -11.49 | 81.54 | -21.66 | 104.39 | 0.3750 | 642.0 | 537.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -14.50 | 78.80 | -24.40 | 110.20 | 0.4279 | -597.0 | -475.1 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -14.76 | 78.56 | -24.63 | 110.64 | 0.4325 | -641.0 | -584.9 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -14.85 | 78.38 | -24.81 | 110.71 | 0.4355 | -745.0 | -625.1 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -14.75 | 78.26 | -24.94 | 110.42 | 0.4369 | -531.0 | -379.2 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -14.86 | 77.97 | -25.23 | 110.49 | 0.4416 | -564.0 | -458.4 | |
| 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. | |