| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.21 | 0.00 | 9.85 | -10.44 | 14.08 | 23.69 | 260.05 | 0.4023 | 214.2 | 283.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.64 | -9.48 | 19.50 | 29.11 | 263.45 | 0.4850 | 653.0 | 590.4 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -10.28 | 18.17 | 27.78 | 261.62 | 0.4654 | 703.0 | 513.7 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -9.57 | 18.00 | 27.61 | 263.13 | 0.4622 | 779.0 | 674.7 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -10.09 | 17.67 | 27.28 | 261.94 | 0.4577 | 685.0 | 493.1 | |
| 0.00 | 4.07 | 0.00 | 2.25 | -10.32 | 16.74 | 26.35 | 261.28 | 0.4437 | 931.0 | 744.3 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -9.46 | 16.23 | 25.84 | 263.18 | 0.4349 | 672.0 | 534.4 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -10.58 | 14.62 | 24.23 | 260.22 | 0.4111 | 785.0 | 556.3 | |
| 0.00 | 1.91 | 0.00 | 1.02 | -10.05 | 12.57 | 22.18 | 261.04 | 0.3779 | 857.0 | 728.5 | |
| 0.00 | 1.47 | 0.00 | 0.79 | -9.68 | 12.28 | 21.89 | 261.97 | 0.3728 | 863.0 | 778.5 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -11.01 | 11.95 | 21.56 | 258.30 | 0.3700 | -810.0 | -732.2 | |
| 0.00 | 1.39 | 0.00 | 0.73 | -11.62 | 11.02 | 20.63 | 256.24 | 0.3569 | -724.0 | -586.7 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -12.13 | 8.61 | 18.22 | 253.29 | 0.3206 | -825.0 | -742.4 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -11.59 | 7.81 | 17.42 | 254.40 | 0.3058 | -752.0 | -540.1 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -10.62 | 7.43 | 17.04 | 257.33 | 0.2965 | -818.0 | -705.6 | |
| 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. | |