| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.87 | 26.80 | 0.43 | 13.32 | -11.04 | 14.32 | 0.88 | 196.67 | 0.0891 | 256.2 | 164.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.39 | 0.00 | 0.69 | -9.42 | 19.45 | 6.01 | 249.50 | 0.1108 | 889.0 | 712.9 | |
| 0.00 | 4.59 | 0.00 | 2.28 | -9.38 | 17.88 | 4.44 | 243.80 | 0.0854 | 701.0 | 617.3 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -9.14 | 17.60 | 4.16 | 245.01 | 0.0794 | 905.0 | 747.2 | |
| 0.00 | 0.52 | 0.00 | 0.26 | -9.87 | 16.55 | 3.11 | 229.38 | 0.0707 | 522.0 | 525.0 | |
| 0.87 | 3.38 | 0.43 | 1.68 | -10.85 | 16.13 | 2.69 | 216.24 | 0.0784 | 1120.3 | 938.8 | |
| 0.00 | 1.65 | 0.00 | 0.82 | -11.30 | 15.11 | 1.66 | 201.94 | 0.0766 | 914.0 | 668.2 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -11.63 | 15.11 | 1.67 | 200.43 | 0.0820 | 733.0 | 579.3 | |
| 0.00 | 1.73 | 0.00 | 0.86 | -10.77 | 15.04 | 1.60 | 204.10 | 0.0676 | 934.0 | 797.2 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -11.06 | 14.68 | 1.24 | 197.68 | 0.0702 | 768.0 | 670.1 | |
| 0.00 | 1.82 | 0.00 | 0.90 | -11.83 | 11.03 | -2.41 | 152.80 | 0.0904 | -849.0 | -715.4 | |
| 0.00 | 3.21 | 0.00 | 1.60 | -12.25 | 10.51 | -2.93 | 150.21 | 0.1010 | -631.0 | -747.5 | |
| 0.00 | 2.69 | 0.00 | 1.34 | -12.45 | 10.36 | -3.09 | 149.96 | 0.1055 | -1013.0 | -763.5 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -12.66 | 10.29 | -3.15 | 150.44 | 0.1092 | -942.0 | -797.4 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -13.13 | 8.85 | -4.59 | 142.80 | 0.1296 | -836.0 | -666.9 | |
| 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. | |