| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 29.99 | 0.00 | 14.93 | -10.67 | 14.79 | 2.45 | 215.91 | 0.0879 | 414.8 | 388.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.61 | -9.47 | 19.54 | 7.20 | 252.19 | 0.1304 | 916.0 | 666.6 | |
| 0.00 | 3.99 | 0.00 | 1.99 | -9.40 | 17.99 | 5.65 | 248.57 | 0.1048 | 862.0 | 689.5 | |
| 0.00 | 3.55 | 0.00 | 1.77 | -10.78 | 16.25 | 3.91 | 227.20 | 0.0916 | 1115.0 | 921.7 | |
| 0.00 | 2.86 | 0.00 | 1.42 | -10.16 | 16.18 | 3.84 | 232.23 | 0.0837 | 788.0 | 670.7 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -10.34 | 16.09 | 3.75 | 229.90 | 0.0845 | 894.0 | 699.5 | |
| 0.00 | 4.59 | 0.00 | 2.28 | -10.88 | 15.31 | 2.97 | 218.67 | 0.0817 | 881.0 | 783.4 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -10.79 | 15.07 | 2.72 | 216.99 | 0.0779 | 874.0 | 712.9 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -11.42 | 15.04 | 2.70 | 212.34 | 0.0866 | 834.0 | 702.1 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -11.00 | 14.73 | 2.39 | 211.98 | 0.0776 | 807.0 | 648.3 | |
| 0.00 | 0.61 | 0.00 | 0.30 | -10.94 | 13.92 | 1.57 | 202.65 | 0.0702 | 665.0 | 581.4 | |
| 0.00 | 1.21 | 0.00 | 0.60 | -6.30 | 13.42 | 1.08 | 311.49 | 0.0251 | 810.0 | 636.8 | |
| 0.00 | 0.52 | 0.00 | 0.26 | -11.72 | 11.00 | -1.34 | 163.58 | 0.0816 | -426.0 | -576.7 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -12.01 | 10.66 | -1.68 | 160.96 | 0.0883 | -902.0 | -719.9 | |
| 0.00 | 3.81 | 0.00 | 1.90 | -12.22 | 10.51 | -1.83 | 160.17 | 0.0927 | -903.0 | -759.0 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -12.43 | 10.39 | -1.96 | 159.74 | 0.0968 | -993.0 | -782.3 | |
| 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. | |