| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.65 | 34.25 | 6.28 | 17.10 | 7.80 | 345.16 | 5.64 | 276.77 | 0.1025 | 31.6 | -47.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.61 | 0.00 | 0.82 | 7.06 | 351.89 | 12.37 | 270.54 | 0.2136 | -875.0 | -670.0 | |
| 0.00 | 1.97 | 0.00 | 1.00 | 7.19 | 351.68 | 12.16 | 271.13 | 0.2099 | -868.0 | -695.1 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 8.40 | 350.37 | 10.85 | 277.56 | 0.1887 | -829.0 | -716.2 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 7.89 | 350.11 | 10.59 | 274.94 | 0.1835 | -795.0 | -661.3 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 7.12 | 349.35 | 9.82 | 270.67 | 0.1701 | -898.0 | -634.2 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 9.59 | 348.76 | 9.23 | 285.80 | 0.1652 | -759.0 | -607.6 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 7.02 | 346.66 | 7.14 | 269.70 | 0.1239 | -958.0 | -739.8 | |
| 3.23 | 5.38 | 1.61 | 2.68 | 8.40 | 345.70 | 6.18 | 282.26 | 0.1094 | -1136.1 | -788.0 | |
| 0.00 | 2.42 | 0.00 | 1.20 | 7.76 | 343.20 | 3.68 | 280.24 | 0.0650 | 1049.0 | 893.6 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 14.16 | 343.25 | 3.73 | 332.83 | 0.1389 | 739.0 | 471.8 | |
| 3.05 | 4.84 | 1.51 | 2.40 | 7.15 | 342.99 | 3.46 | 270.89 | 0.0602 | 1093.2 | 851.5 | |
| 6.37 | 8.79 | 3.16 | 4.36 | 6.76 | 342.40 | 2.88 | 263.22 | 0.0505 | 1051.2 | 730.1 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 7.19 | 341.73 | 2.21 | 272.19 | 0.0385 | 874.0 | 684.6 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 10.74 | 340.61 | 1.09 | 343.50 | 0.0663 | 723.0 | 550.6 | |
| 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. | |