| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.53 | 29.48 | 0.77 | 14.94 | 8.51 | 195.53 | -5.16 | 23.92 | 0.2145 | 40.5 | -94.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 2.25 | 0.23 | 1.13 | 8.20 | 198.65 | -2.05 | 10.78 | 0.1899 | -1237.6 | -1016.4 | |
| 0.00 | 2.96 | 0.00 | 1.49 | 7.09 | 198.44 | -2.26 | 13.19 | 0.1720 | -696.0 | -639.5 | |
| 1.08 | 4.58 | 0.54 | 2.31 | 8.54 | 197.73 | -2.97 | 14.97 | 0.1992 | -1122.4 | -837.4 | |
| 0.00 | 2.07 | 0.00 | 1.04 | 8.39 | 197.42 | -3.27 | 16.65 | 0.1981 | -989.0 | -820.8 | |
| 0.00 | 2.25 | 0.00 | 1.14 | 8.45 | 196.90 | -3.80 | 19.02 | 0.2019 | -1098.0 | -871.5 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 8.89 | 195.82 | -4.88 | 23.04 | 0.2155 | -822.0 | -645.5 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.96 | 195.20 | -5.49 | 25.47 | 0.2209 | -641.0 | -463.0 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 6.92 | 194.95 | -5.74 | 31.27 | 0.1923 | 858.0 | 624.5 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 7.54 | 194.42 | -6.27 | 31.88 | 0.2061 | 1005.0 | 703.7 | |
| 0.00 | 2.42 | 0.00 | 1.24 | 9.40 | 194.05 | -6.64 | 28.99 | 0.2365 | 962.0 | 746.0 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 11.42 | 193.48 | -7.21 | 27.12 | 0.2712 | 812.0 | 604.2 | |
| 0.00 | 2.07 | 0.00 | 1.05 | 7.79 | 193.34 | -7.36 | 35.40 | 0.2199 | 894.0 | 737.3 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 8.63 | 193.29 | -7.40 | 33.46 | 0.2320 | 803.0 | 593.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 8.51 | 193.17 | -7.52 | 34.19 | 0.2315 | 786.0 | 679.3 | |
| 0.00 | 2.87 | 0.00 | 1.48 | 9.70 | 190.41 | -10.28 | 39.86 | 0.2758 | 852.0 | 660.2 | |
| 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. | |