| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.11 | 40.54 | 6.96 | 28.19 | -11.05 | 11.82 | -45.01 | 98.40 | 0.7038 | 274.7 | 172.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 0.46 | -14.68 | 14.36 | -42.46 | 103.88 | 0.6751 | 629.0 | 510.9 | |
| 0.00 | 1.73 | 0.00 | 1.17 | -10.82 | 13.64 | -43.19 | 98.12 | 0.6814 | 684.0 | 502.2 | |
| 0.00 | 1.04 | 0.00 | 0.70 | -11.04 | 13.31 | -43.52 | 98.43 | 0.6856 | 667.0 | 513.9 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -10.85 | 13.30 | -43.53 | 98.16 | 0.6857 | 759.0 | 667.9 | |
| 0.43 | 1.47 | 0.29 | 1.00 | -10.95 | 13.07 | -43.76 | 98.30 | 0.6885 | 698.4 | 604.8 | |
| 7.69 | 14.35 | 5.23 | 9.76 | -10.27 | 13.15 | -43.67 | 97.31 | 0.6874 | 900.1 | 534.1 | |
| 0.00 | 3.98 | 0.00 | 2.75 | -10.84 | 12.16 | -44.67 | 98.12 | 0.6998 | 604.0 | 591.3 | |
| 0.00 | 1.47 | 0.00 | 1.03 | -10.28 | 11.49 | -45.33 | 97.30 | 0.7079 | 671.0 | 539.1 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -11.20 | 11.05 | -45.78 | 98.60 | 0.7133 | -486.0 | -371.4 | |
| 0.00 | 1.99 | 0.00 | 1.40 | -10.58 | 10.91 | -45.91 | 97.74 | 0.7149 | 698.0 | 519.7 | |
| 0.00 | 0.52 | 0.00 | 0.37 | -11.65 | 10.69 | -46.13 | 99.22 | 0.7177 | -593.0 | -540.2 | |
| 0.00 | 0.86 | 0.00 | 0.61 | -10.38 | 10.64 | -46.18 | 97.45 | 0.7181 | 521.0 | 410.9 | |
| 0.00 | 0.69 | 0.00 | 0.50 | -12.68 | 9.79 | -47.04 | 100.62 | 0.7288 | -661.0 | -578.8 | |
| 0.00 | 0.69 | 0.00 | 0.50 | -11.64 | 9.98 | -46.84 | 99.20 | 0.7261 | -751.0 | -651.9 | |
| 0.00 | 1.21 | 0.00 | 0.87 | -11.75 | 9.87 | -46.96 | 99.35 | 0.7275 | -755.0 | -626.4 | |
| 0.00 | 1.12 | 0.00 | 0.81 | -11.56 | 9.73 | -47.09 | 99.08 | 0.7290 | -603.0 | -507.8 | |
| 1.99 | 6.83 | 1.44 | 4.95 | -12.37 | 9.41 | -47.42 | 100.18 | 0.7330 | -666.9 | -551.1 | |
| 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. | |