| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.16 | 0.00 | 8.47 | -20.05 | 79.64 | -24.32 | 136.49 | 0.5619 | 704.9 | 620.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.65 | -20.89 | 85.35 | -18.61 | 144.61 | 0.5168 | 911.0 | 769.3 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -21.03 | 85.17 | -18.79 | 144.51 | 0.5200 | 591.0 | 552.6 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -16.90 | 84.73 | -19.23 | 138.42 | 0.4768 | 793.0 | 724.7 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -18.17 | 82.58 | -21.38 | 137.27 | 0.5125 | 601.0 | 440.4 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -20.32 | 81.94 | -22.02 | 139.33 | 0.5417 | 711.0 | 550.1 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -20.30 | 79.39 | -24.57 | 136.26 | 0.5664 | 743.0 | 669.9 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -20.55 | 78.82 | -25.14 | 135.95 | 0.5744 | 778.0 | 662.1 | |
| 0.00 | 1.12 | 0.00 | 0.68 | -20.42 | 78.74 | -25.23 | 135.69 | 0.5740 | 678.0 | 648.1 | |
| 0.00 | 1.38 | 0.00 | 0.84 | -20.26 | 77.56 | -26.40 | 134.23 | 0.5843 | 635.0 | 531.2 | |
| 0.00 | 1.04 | 0.00 | 0.63 | -20.05 | 77.00 | -26.96 | 133.38 | 0.5882 | 692.0 | 646.4 | |
| 0.00 | 1.47 | 0.00 | 0.90 | -20.23 | 76.47 | -27.50 | 133.08 | 0.5953 | 760.0 | 653.8 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -20.07 | 76.46 | -27.50 | 132.86 | 0.5939 | 775.0 | 680.4 | |
| 0.00 | 0.52 | 0.00 | 0.32 | -20.33 | 76.37 | -27.59 | 133.12 | 0.5971 | 618.0 | 541.5 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -20.69 | 75.62 | -28.34 | 132.84 | 0.6079 | 582.0 | 489.4 | |
| 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. | |