| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.19 | 73.25 | 14.35 | 38.43 | -9.13 | 24.39 | 17.19 | 242.75 | 0.3293 | 568.7 | 360.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 3.61 | 0.67 | 1.92 | -8.93 | 26.57 | 19.37 | 246.47 | 0.3590 | 838.1 | 718.9 | |
| 3.52 | 5.69 | 1.87 | 3.02 | -8.68 | 26.46 | 19.26 | 247.00 | 0.3558 | 998.7 | 818.9 | |
| 22.05 | 45.45 | 11.62 | 23.93 | -8.93 | 25.43 | 18.23 | 245.23 | 0.3419 | 1110.5 | 637.7 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -8.72 | 24.87 | 17.67 | 245.16 | 0.3321 | 277.0 | 266.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -9.73 | 23.82 | 16.63 | 240.99 | 0.3239 | 845.0 | 699.7 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -10.26 | 23.33 | 16.14 | 238.84 | 0.3211 | 785.0 | 676.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -9.89 | 23.22 | 16.03 | 239.68 | 0.3164 | 819.0 | 670.6 | |
| 0.36 | 3.34 | 0.19 | 1.74 | -10.10 | 23.00 | 15.81 | 238.75 | 0.3151 | 1014.2 | 763.3 | |
| 0.00 | 4.52 | 0.00 | 2.33 | -9.19 | 20.51 | 13.32 | 237.16 | 0.2719 | -849.0 | -634.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -8.88 | 20.28 | 13.09 | 237.69 | 0.2658 | -821.0 | -630.9 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -9.46 | 20.20 | 13.01 | 235.69 | 0.2701 | -822.0 | -691.9 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -9.03 | 20.03 | 12.84 | 236.71 | 0.2637 | -891.0 | -763.2 | |
| 0.00 | 1.90 | 0.00 | 0.96 | -11.16 | 14.20 | 7.01 | 213.53 | 0.2176 | -788.0 | -522.0 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -12.65 | 13.48 | 6.29 | 207.43 | 0.2332 | -678.0 | -534.9 | |
| 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. | |