| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.40 | 49.30 | 3.29 | 25.60 | 21.69 | 109.74 | 7.56 | 335.54 | 0.2977 | 434.7 | 512.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.70 | 25.72 | 113.37 | 11.18 | 332.64 | 0.3818 | 891.0 | 733.5 | |
| 1.58 | 1.66 | 0.82 | 0.86 | 20.04 | 112.22 | 10.04 | 325.98 | 0.2940 | -898.6 | -758.0 | |
| 0.00 | 2.63 | 0.00 | 1.36 | 20.20 | 112.01 | 9.82 | 326.86 | 0.2941 | -872.0 | -820.7 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 20.58 | 111.90 | 9.72 | 327.85 | 0.2983 | -807.0 | -638.9 | |
| 0.00 | 2.45 | 0.00 | 1.27 | 20.06 | 111.54 | 9.36 | 327.79 | 0.2879 | -1147.0 | -850.8 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 26.42 | 111.84 | 9.65 | 336.69 | 0.3812 | 694.0 | 561.1 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 26.26 | 111.45 | 9.27 | 337.34 | 0.3766 | 934.0 | 743.2 | |
| 0.00 | 6.04 | 0.00 | 3.23 | 26.49 | 111.40 | 9.22 | 337.70 | 0.3795 | 793.0 | 642.3 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 25.46 | 109.58 | 7.40 | 340.72 | 0.3537 | 859.0 | 660.7 | |
| 0.00 | 2.63 | 0.00 | 1.39 | 25.62 | 109.36 | 7.17 | 341.42 | 0.3550 | 856.0 | 701.3 | |
| 0.00 | 1.75 | 0.00 | 0.90 | 19.60 | 109.01 | 6.83 | 334.43 | 0.2608 | 851.0 | 636.7 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 19.45 | 108.91 | 6.73 | 334.49 | 0.2577 | 798.0 | 578.2 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 23.27 | 108.80 | 6.61 | 340.32 | 0.3156 | 912.0 | 722.0 | |
| 4.82 | 22.85 | 2.47 | 11.70 | 19.58 | 108.34 | 6.16 | 336.61 | 0.2557 | 1061.4 | 822.6 | |
| 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. | |