| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.09 | 0.00 | 11.19 | 7.63 | 207.07 | -21.11 | 86.69 | 0.3592 | 168.4 | 292.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.55 | 8.09 | 211.24 | -16.94 | 84.78 | 0.2910 | -865.0 | -700.9 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 7.65 | 210.85 | -17.33 | 86.31 | 0.2972 | -735.0 | -595.8 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 6.52 | 210.41 | -17.77 | 90.06 | 0.3045 | -893.0 | -710.5 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 6.31 | 210.32 | -17.86 | 90.75 | 0.3061 | -906.0 | -739.8 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 6.55 | 208.78 | -19.40 | 89.78 | 0.3314 | -669.0 | -502.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 6.46 | 207.98 | -20.20 | 89.96 | 0.3445 | -818.0 | -556.7 | |
| 0.00 | 2.74 | 0.00 | 1.46 | 6.80 | 206.61 | -21.57 | 88.89 | 0.3667 | 913.0 | 751.9 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 7.06 | 206.47 | -21.71 | 88.16 | 0.3689 | 813.0 | 634.1 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 8.34 | 206.14 | -22.04 | 84.72 | 0.3745 | 837.0 | 738.7 | |
| 0.00 | 1.50 | 0.00 | 0.80 | 6.93 | 206.18 | -22.00 | 88.50 | 0.3736 | 887.0 | 602.5 | |
| 0.00 | 1.15 | 0.00 | 0.61 | 9.00 | 206.03 | -22.15 | 82.98 | 0.3768 | 661.0 | 576.8 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 8.81 | 205.94 | -22.24 | 83.48 | 0.3780 | 881.0 | 620.9 | |
| 0.00 | 2.82 | 0.00 | 1.51 | 8.35 | 205.61 | -22.57 | 84.75 | 0.3830 | 873.0 | 699.7 | |
| 0.00 | 1.59 | 0.00 | 0.85 | 8.14 | 205.56 | -22.62 | 85.31 | 0.3837 | 835.0 | 610.8 | |
| 0.00 | 2.29 | 0.00 | 1.23 | 8.46 | 205.37 | -22.81 | 84.49 | 0.3868 | 712.0 | 611.0 | |
| 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. | |