| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.12 | 44.31 | 2.61 | 22.66 | 8.45 | 195.61 | -9.48 | 40.08 | 0.2524 | -40.0 | 96.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.44 | 0.00 | 0.73 | 7.09 | 198.48 | -6.61 | 34.41 | 0.2031 | -935.0 | -685.1 | |
| 3.68 | 7.37 | 1.87 | 3.74 | 8.17 | 198.37 | -6.72 | 32.00 | 0.2195 | -1141.3 | -783.9 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 6.76 | 198.05 | -7.04 | 37.08 | 0.2027 | -919.0 | -679.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.67 | 197.65 | -7.44 | 33.44 | 0.2333 | -939.0 | -739.6 | |
| 0.72 | 4.67 | 0.37 | 2.38 | 8.46 | 197.50 | -7.59 | 34.49 | 0.2317 | -1104.0 | -911.0 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 8.40 | 197.10 | -7.99 | 36.03 | 0.2348 | -1052.0 | -804.9 | |
| 0.00 | 3.68 | 0.00 | 1.88 | 8.59 | 196.17 | -8.92 | 38.58 | 0.2471 | -894.0 | -755.6 | |
| 0.72 | 3.68 | 0.37 | 1.88 | 7.28 | 194.77 | -10.32 | 46.35 | 0.2467 | 1021.1 | 790.8 | |
| 0.00 | 4.58 | 0.00 | 2.36 | 9.26 | 194.22 | -10.87 | 42.46 | 0.2770 | 1103.0 | 848.4 | |
| 0.00 | 6.83 | 0.00 | 3.52 | 9.38 | 193.90 | -11.19 | 42.97 | 0.2821 | 695.0 | 682.9 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 8.46 | 193.40 | -11.69 | 46.58 | 0.2772 | 1052.0 | 879.6 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 7.63 | 193.36 | -11.73 | 48.96 | 0.2684 | 893.0 | 715.1 | |
| 0.00 | 1.89 | 0.00 | 0.97 | 8.65 | 193.17 | -11.92 | 46.63 | 0.2821 | 968.0 | 827.3 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 8.46 | 193.18 | -11.91 | 47.10 | 0.2799 | 944.0 | 754.0 | |
| 0.00 | 2.25 | 0.00 | 1.17 | 8.75 | 191.98 | -13.12 | 49.07 | 0.2982 | 668.0 | 600.8 | |
| 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. | |