| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.71 | 0.00 | 14.52 | 12.78 | 55.54 | -17.05 | 64.94 | 0.3147 | 240.3 | 260.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.62 | 14.09 | 67.08 | -5.51 | 34.22 | 0.1663 | -911.0 | -715.6 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 14.21 | 66.80 | -5.79 | 35.13 | 0.1707 | -875.0 | -710.1 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 14.80 | 63.10 | -9.49 | 46.74 | 0.2199 | -926.0 | -759.8 | |
| 0.00 | 2.02 | 0.00 | 1.02 | 10.35 | 62.36 | -10.23 | 67.25 | 0.1903 | -944.0 | -705.6 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 13.96 | 62.23 | -10.36 | 52.10 | 0.2223 | -877.0 | -684.5 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 13.69 | 58.07 | -14.52 | 61.38 | 0.2787 | 798.0 | 667.3 | |
| 0.00 | 2.54 | 0.00 | 1.31 | 13.13 | 57.41 | -15.19 | 64.17 | 0.2847 | 819.0 | 541.1 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 12.43 | 53.99 | -18.60 | 70.04 | 0.3329 | 904.0 | 757.8 | |
| 0.00 | 2.54 | 0.00 | 1.34 | 12.09 | 53.75 | -18.84 | 71.22 | 0.3350 | 954.0 | 740.2 | |
| 0.00 | 1.67 | 0.00 | 0.88 | 12.31 | 53.35 | -19.24 | 70.89 | 0.3423 | 885.0 | 746.5 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 12.42 | 52.82 | -19.77 | 71.01 | 0.3509 | 792.0 | 633.9 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 11.09 | 52.69 | -19.90 | 74.81 | 0.3477 | 691.0 | 525.8 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 9.10 | 51.68 | -20.91 | 80.85 | 0.3585 | 705.0 | 529.3 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 13.89 | 50.95 | -21.64 | 68.59 | 0.3862 | 721.0 | 566.5 | |
| 0.00 | 2.63 | 0.00 | 1.42 | 14.39 | 49.83 | -22.76 | 68.21 | 0.4053 | 794.0 | 707.5 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 14.40 | 49.19 | -23.40 | 68.66 | 0.4148 | 757.0 | 572.5 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 14.34 | 48.65 | -23.94 | 69.14 | 0.4225 | 700.0 | 550.5 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 7.40 | 46.84 | -25.75 | 85.92 | 0.4338 | -661.0 | -545.7 | |
| 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. | |