| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.71 | 0.00 | 12.61 | 14.36 | 92.41 | -9.85 | 45.02 | 0.2196 | -62.5 | 290.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.70 | 9.40 | 101.69 | -0.57 | 10.67 | 0.0535 | -871.0 | -711.9 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 8.98 | 101.63 | -0.63 | 13.63 | 0.0465 | -983.0 | -772.8 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 9.49 | 100.84 | -1.42 | 24.43 | 0.0595 | -824.0 | -639.2 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 10.48 | 100.32 | -1.94 | 25.11 | 0.0790 | -896.0 | -727.0 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 10.38 | 98.67 | -3.59 | 41.49 | 0.0934 | -927.0 | -663.1 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 10.74 | 98.58 | -3.69 | 39.75 | 0.0992 | -830.0 | -698.5 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 10.61 | 97.78 | -4.48 | 46.10 | 0.1070 | -1026.0 | -858.3 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 17.52 | 92.87 | -9.39 | 38.69 | 0.2500 | 874.0 | 694.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 12.18 | 92.82 | -9.44 | 57.49 | 0.1911 | -861.0 | -653.2 | |
| 0.00 | 2.11 | 0.00 | 1.09 | 19.06 | 90.40 | -11.86 | 41.25 | 0.2959 | 926.0 | 730.6 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 16.32 | 89.33 | -12.93 | 50.82 | 0.2782 | 667.0 | 621.2 | |
| 0.00 | 7.38 | 0.00 | 3.77 | 13.50 | 89.44 | -12.82 | 59.65 | 0.2512 | 1373.0 | 1092.1 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 18.96 | 88.75 | -13.51 | 45.06 | 0.3135 | 832.0 | 703.1 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 25.02 | 84.30 | -17.96 | 40.76 | 0.4298 | 850.0 | 785.1 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 19.94 | 83.93 | -18.34 | 51.01 | 0.3822 | 759.0 | 561.2 | |
| 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. | |