| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.79 | 313.91 | 77.57 | 377.73 | -24.92 | 91.93 | -66.42 | 114.15 | 0.9116 | -140.6 | -50.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.46 | 7.76 | 1.57 | 8.33 | -24.06 | 95.41 | -62.95 | 113.43 | 0.8882 | 506.4 | 335.8 | |
| 9.48 | 112.19 | 9.88 | 119.94 | -22.94 | 96.22 | -62.14 | 112.23 | 0.8815 | 909.2 | 174.4 | |
| 1.29 | -2.00 | 1.37 | -2.00 | -23.36 | 95.72 | -62.63 | 112.67 | 0.8855 | 561.5 | 999999 | |
| 6.03 | -2.00 | 6.43 | -2.00 | -23.05 | 95.49 | -62.87 | 112.30 | 0.8870 | 591.1 | 999999 | |
| 1.38 | 9.91 | 1.51 | 10.87 | -23.86 | 94.71 | -63.64 | 113.15 | 0.8931 | -110.4 | -307.3 | |
| 0.00 | 2.41 | 0.00 | 2.60 | -23.33 | 95.11 | -63.25 | 112.58 | 0.8900 | 211.0 | 126.2 | |
| 0.00 | 0.60 | 0.00 | 0.73 | -26.11 | 91.71 | -66.64 | 115.43 | 0.9146 | -494.0 | -476.4 | |
| 7.93 | -2.00 | 8.82 | -2.00 | -23.25 | 94.07 | -64.28 | 112.42 | 0.8974 | 401.1 | 999999 | |
| 1.12 | 2.07 | 1.38 | 2.55 | -26.02 | 91.22 | -67.14 | 115.31 | 0.9177 | -631.6 | -529.0 | |
| 0.00 | 4.83 | 0.00 | 5.34 | -22.88 | 94.25 | -64.11 | 112.03 | 0.8960 | -472.0 | -349.4 | |
| 0.00 | 0.26 | 0.00 | 0.29 | -22.83 | 93.77 | -64.59 | 111.94 | 0.8993 | 322.0 | 276.7 | |
| 0.43 | 1.55 | 0.54 | 1.94 | -25.58 | 90.78 | -67.58 | 114.80 | 0.9202 | -643.8 | -586.2 | |
| 30.93 | 155.19 | 40.49 | 204.21 | -26.23 | 89.62 | -68.73 | 115.45 | 0.9274 | -591.2 | -139.7 | |
| 4.74 | 11.80 | 5.58 | 13.95 | -23.67 | 92.43 | -65.93 | 112.80 | 0.9089 | -614.9 | -245.8 | |
| 0.00 | 0.86 | 0.00 | 1.07 | -24.68 | 90.86 | -67.50 | 113.83 | 0.9194 | -214.0 | -279.1 | |
| 0.00 | 0.60 | 0.00 | 0.73 | -22.99 | 91.80 | -66.55 | 112.02 | 0.9128 | 187.0 | 189.3 | |
| 0.00 | 3.88 | 0.00 | 5.18 | -25.09 | 89.02 | -69.33 | 114.19 | 0.9305 | -559.0 | -493.5 | |
| 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. | |