| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 21.82 | 0.21 | 13.42 | 13.20 | 93.21 | 35.46 | 285.32 | 0.5868 | 201.3 | -7.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.36 | 10.93 | 101.74 | 43.99 | 279.36 | 0.6935 | -446.0 | -372.2 | |
| 0.00 | 5.26 | 0.00 | 3.58 | 10.95 | 101.41 | 43.66 | 279.42 | 0.6893 | -872.0 | -669.5 | |
| 0.00 | 0.96 | 0.00 | 0.63 | 6.88 | 98.56 | 40.81 | 273.37 | 0.6522 | -593.0 | -494.9 | |
| 0.00 | 1.49 | 0.00 | 0.94 | 7.49 | 96.30 | 38.55 | 274.26 | 0.6219 | -55.0 | -80.4 | |
| 0.00 | 1.40 | 0.00 | 0.88 | 10.68 | 95.43 | 37.68 | 279.49 | 0.6113 | -772.0 | -663.6 | |
| 0.00 | 1.05 | 0.00 | 0.65 | 11.92 | 94.89 | 37.14 | 281.61 | 0.6054 | -519.0 | -505.2 | |
| 0.35 | 1.58 | 0.21 | 0.97 | 11.11 | 93.89 | 36.14 | 280.40 | 0.5906 | 762.2 | 657.0 | |
| 0.00 | 0.35 | 0.00 | 0.22 | 21.91 | 94.86 | 37.10 | 297.49 | 0.6332 | 586.0 | 611.2 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 15.70 | 87.51 | 29.76 | 290.53 | 0.5123 | 564.0 | 406.1 | |
| 0.00 | 2.19 | 0.00 | 1.25 | 15.45 | 86.97 | 29.22 | 290.32 | 0.5038 | 828.0 | 760.8 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 19.77 | 85.29 | 27.54 | 299.52 | 0.5020 | 684.0 | 577.4 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 16.99 | 84.35 | 26.60 | 294.85 | 0.4738 | 722.0 | 562.7 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 21.92 | 84.49 | 26.74 | 304.04 | 0.5057 | 580.0 | 527.1 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 16.66 | 82.74 | 24.98 | 295.33 | 0.4495 | 880.0 | 648.9 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 16.84 | 82.14 | 24.39 | 296.16 | 0.4422 | 552.0 | 392.2 | |
| 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. | |