| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.75 | 0.00 | 12.91 | 8.42 | 28.37 | 17.82 | 277.17 | 0.3077 | -472.4 | -495.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.57 | 7.15 | 30.44 | 19.89 | 272.03 | 0.3393 | -679.0 | -601.5 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 10.51 | 30.60 | 20.05 | 281.85 | 0.3460 | -762.0 | -593.4 | |
| 0.00 | 4.32 | 0.00 | 2.27 | 7.10 | 30.21 | 19.66 | 271.87 | 0.3355 | -908.0 | -688.7 | |
| 0.00 | 3.96 | 0.00 | 2.08 | 7.02 | 29.92 | 19.37 | 271.62 | 0.3307 | -779.0 | -676.0 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 8.28 | 29.59 | 19.04 | 275.49 | 0.3257 | -895.0 | -690.4 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 7.65 | 29.30 | 18.75 | 273.58 | 0.3206 | -778.0 | -629.1 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 8.26 | 29.23 | 18.68 | 275.50 | 0.3198 | -780.0 | -555.2 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 8.63 | 28.96 | 18.41 | 276.74 | 0.3158 | -829.0 | -681.4 | |
| 0.00 | 2.97 | 0.00 | 1.55 | 8.46 | 28.82 | 18.27 | 276.20 | 0.3133 | -1104.0 | -912.4 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 8.47 | 28.59 | 18.05 | 276.28 | 0.3096 | -774.0 | -757.1 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 10.34 | 27.18 | 16.63 | 283.09 | 0.2903 | -855.0 | -604.8 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 10.03 | 23.53 | 12.98 | 284.73 | 0.2297 | 751.0 | 696.6 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 9.95 | 21.79 | 11.25 | 286.27 | 0.2010 | 884.0 | 706.7 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 13.93 | 19.49 | 8.94 | 309.50 | 0.1964 | 894.0 | 712.0 | |
| 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. | |