| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.03 | 80.46 | 12.19 | 40.74 | -4.56 | 30.56 | -2.00 | 171.35 | 0.2057 | 270.6 | 286.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.39 | 27.99 | 7.77 | 14.12 | -4.09 | 33.17 | 0.62 | 183.25 | 0.1904 | 1160.9 | 714.7 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -4.77 | 31.62 | -0.93 | 175.37 | 0.2024 | 918.0 | 748.1 | |
| 0.00 | 1.80 | 0.00 | 0.91 | -4.36 | 31.44 | -1.12 | 174.28 | 0.1958 | 1029.0 | 865.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -4.02 | 31.35 | -1.21 | 173.63 | 0.1901 | 1030.0 | 853.1 | |
| 0.00 | 2.88 | 0.00 | 1.46 | -4.73 | 31.32 | -1.24 | 173.86 | 0.2024 | 686.0 | 652.9 | |
| 0.00 | 0.90 | 0.00 | 0.45 | -3.90 | 31.11 | -1.45 | 172.27 | 0.1885 | 918.0 | 826.9 | |
| 2.16 | 16.74 | 1.09 | 8.45 | -4.15 | 30.68 | -1.88 | 170.26 | 0.1939 | 1032.3 | 801.2 | |
| 1.26 | 4.68 | 0.64 | 2.37 | -4.77 | 30.40 | -2.15 | 169.44 | 0.2052 | 897.2 | 721.3 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -5.58 | 29.33 | -3.22 | 165.38 | 0.2227 | -841.0 | -653.5 | |
| 2.52 | 8.46 | 1.28 | 4.28 | -4.43 | 29.10 | -3.46 | 162.84 | 0.2050 | -1135.6 | -876.2 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -5.89 | 29.03 | -3.53 | 164.43 | 0.2292 | -759.0 | -587.7 | |
| 0.81 | 4.23 | 0.41 | 2.14 | -4.16 | 28.91 | -3.64 | 161.58 | 0.2014 | -1074.4 | -780.2 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -4.78 | 28.85 | -3.71 | 162.21 | 0.2118 | -905.0 | -739.5 | |
| 0.00 | 1.98 | 0.00 | 1.02 | -6.58 | 23.86 | -8.70 | 146.89 | 0.2762 | -769.0 | -637.8 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -6.83 | 23.67 | -8.89 | 146.81 | 0.2815 | -724.0 | -628.4 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -5.45 | 22.49 | -10.07 | 140.45 | 0.2745 | -778.0 | -662.0 | |
| 0.00 | 1.26 | 0.00 | 0.65 | -6.70 | 22.31 | -10.25 | 142.69 | 0.2928 | -734.0 | -540.4 | |
| 1.89 | 1.89 | 1.00 | 1.00 | -10.00 | 21.02 | -11.53 | 145.54 | 0.3495 | -4.8 | 0.0 | |
| 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. | |